Supernovae

References

Useful Links

References

[1-1]

Black Holes, White Dwarfs, and Neutron Stars: the Physics of Compact Objects, Shapiro, S. L., Teukolsky, S. A., John Wiley, 1983.

[1-2]

An Introduction to the Study of Stellar Structure, S. Chandrasekhar, University of Chicago Press, 1938.

[2-1]

Equation of State for Proto-Neutron Star, Gang Shen, arXiv:1202.5791, 2012.

[2-2]

Massive Stars and their Supernovae, Friedrich-Karl Thielemann, Raphael Hirschi, Matthias Liebendorfer, Roland Diehl, arXiv:1008.2144, 2010.

[2-3]

Diffuse supernova neutrinos at underground laboratories, Cecilia Lunardini, arXiv:1007.3252, 2010.

[2-4]

The Diffuse Supernova Neutrino Background, John F. Beacom, Ann. Rev. Nucl. Part. Sci. 60 (2010) 439, arXiv:1004.3311.

[2-5]

Low energy neutrino scattering measurements at future Spallation Source facilities, R. Lazauskas, C. Volpe, J. Phys. G37 (2010) 125101, arXiv:1004.0310.

[2-6]

Collective Neutrino Oscillations, Huaiyu Duan, George M. Fuller, Yong-Zhong Qian, Ann. Rev. Nucl. Part. Sci. 60 (2010), arXiv:1001.2799.

[2-7]

Search for CP violation in the lepton sector, Cristina Volpe, Prog. Part. Nucl. Phys. 64 (2010) 325-333, arXiv:0911.4314.

[2-8]

Neutrino flavour transformation in supernovae, Huaiyu Duan, James P Kneller, J. Phys. G36 (2009) 113201, arXiv:0904.0974.

[2-9]

The Gravitational Wave Signature of Core-Collapse Supernovae, Ott, Christian D., Class. Quant. Grav. 26 (2009) 063001, arXiv:0809.0695. .

[2-10]

The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries, M. Arnould, S. Goriely, K. Takahashi, Phys. Rept. 450 (2007) 97-213, arXiv:0705.4512.

[2-11]

Supernova neutrinos, from back of the envelope to supercomputer, Christian Y. Cardall, arXiv:astro-ph/0701831, 2007.

[2-12]

Theory of Core-Collapse Supernovae, H.-Th. Janka et al., Phys. Rept. 442 (2007) 38-74, arXiv:astro-ph/0612072.

[2-13]

The Supernova - Gamma-Ray Burst Connection, S. E. Woosley, J. S. Bloom, Ann. Rev. Astron. Astrophys. 44 (2006) 507-556, arXiv:astro-ph/0609142.

[2-14]

The Physics of Core-Collapse Supernovae, S. Woosley, H.-T. Janka, Nature Phys. 1 (2006) 147-154, arXiv:astro-ph/0601261.

[2-15]

The physics of dense hadronic matter and compact stars, Armen Sedrakian, Prog. Part. Nucl. Phys. 58 (2007) 168-246, arXiv:nucl-th/0601086.

[2-16]

Six Years of Chandra Observations of Supernova Remnants, Martin C. Weisskopf, John P. Hughes, arXiv:astro-ph/0511327, 2005.

[2-17]

Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae, Kei Kotake, Katsuhiko Sato, Keitaro Takahashi, Rept. Prog. Phys. 69 (2006) 971, arXiv:astro-ph/0509456.

[2-18]

Supernovae: Explosions in the Cosmos, Suresh, Paingalil Kunjan, Kumar, V. H. Satheesh, Science REPORTER (2005) Vol.42, arXiv:astro-ph/0504597.

[2-19]

Progenitors of Core-Collapse Supernovae, John J. Eldridge, arXiv:astro-ph/0502046, 2005.

[2-20]

Type Ia Supernovae and Cosmology, Alexei V. Filippenko, arXiv:astro-ph/0410609, 2004.

[2-21]

Relic neutrino background from cosmological supernovae, Shin'ichiro Ando, Katsuhiko Sato, New J. Phys. 6 (2004) 170, arXiv:astro-ph/0410061.

[2-22]

The Physics of Neutron Stars, J.M. Lattimer, M. Prakash, Science 304 (2004) 536-542, arXiv:astro-ph/0405262.

[2-23]

Astrophysical Neutrino Telescopes, A. B. McDonald et al., Rev. Sci. Instrum. 75 (2004) 293, arXiv:astro-ph/0311343.

[2-24]

Supernova Science at Spallation Neutron Sources, W. R. Hix, A. Mezzacappa, O. E. B. Messer, S. W. Bruenn, J. Phys. G29 (2003) 2523, arXiv:astro-ph/0310763.

[2-25]

Advances in r-Process Nucleosynthesis, John J. Cowan, Christopher Sneden, arXiv:astro-ph/0309802, 2003.

[2-26]

The Accelerating Universe and Dark Energy: Evidence from Type Ia Supernovae, A. V. Filippenko, Lect. Notes Phys. 646 (2004) 191, arXiv:astro-ph/0309739.

[2-27]

Supernova Neutrino-Nucleus Astrophysics, A. B. Balantekin, G. M. Fuller, J. Phys. G29 (2003) 2513, arXiv:astro-ph/0309519.

[2-28]

Shocks and Particle Acceleration in Supernova Remnants: Observational Features, Jacco Vink, arXiv:astro-ph/0304176, 2003.

[2-29]

Optical Light Curves of Supernovae, Bruno Leibundgut, Nicholas B.Suntzeff, arXiv:astro-ph/0304112, 2003.

[2-30]

Measuring Cosmology with Supernovae, Perlmutter, Saul, Schmidt, Brian P., Lect. Notes Phys. 598 (2003) 195-217, arXiv:astro-ph/0303428.

[2-31]

The Historical Supernovae, D. A. Green, F. R. Stephenson, arXiv:astro-ph/0301603, 2003.

[2-32]

The Origin of the Heavy Elements: Recent Progress in the Understanding of the r-Process, Yong-Zhong Qian, Prog. Part. Nucl. Phys. 50 (2003) 153, arXiv:astro-ph/0301422.

[2-33]

Physics of SNeIa and Cosmology, P. Hoeflich, C. Gerardy, E. Linder, H. Marion, arXiv:astro-ph/0301334, 2003.

[2-34]

Classification of Supernovae, Massimo Turatto, arXiv:astro-ph/0301107, 2003.

[2-35]

Explosion Mechanisms of Massive Stars, H.-Th. Janka et al., arXiv:astro-ph/0212314, 2002.

[2-36]

Absolute values of neutrino masses: Status and prospects, Bilenky, S. M., Giunti, C., Grifols, J. A., Masso, E., Phys. Rep. 379 (2003) 69-148, arXiv:hep-ph/0211462.

[2-37]

Neutrino-Matter Interaction Rates in Supernovae: The Essential Microphysics of Core Collapse, A. Burrows, T. A. Thompson, arXiv:astro-ph/0211404, 2002.

[2-38]

Supernova remnants and gamma-ray sources, Diego F. Torres, Gustavo E. Romero, Thomas M. Dame, Jorge A. Combi, Yousaf M. Butt, Phys. Rep. 382 (2003) 303, arXiv:astro-ph/0209565.

[2-39]

Observations and Theory of Supernovae, Wheeler, J. Craig, Am. J. Phys. 71 (2003) 11, arXiv:astro-ph/0209514.

[2-40]

The evolution and explosion of massive stars, S. E. Woosley, A. Heger, T. A. Weaver, Rev. Mod. Phys. 74 (2002) 1015-1071.

[2-41]

Element Synthesis in Stars, Thielemann, F. K. et al., Prog. Part. Nucl. Phys. 46 (2001) 5-22, arXiv:astro-ph/0101476.

[2-42]

Neutrino astronomy, Totsuka, Y., Rept. Prog. Phys. 55 (1992) 377-430.

[4-1]

Observational neutrino astrophysics, Koshiba, M., Phys. Rep. 220 (1992) 229-381.

[2-44]

Galactic and extragalactic supernova rates, van den Bergh, S., Tammann, G. A., Ann. Rev. Astron. Astrophys. 29 (1991) 363-407.

[2-45]

Supernova mechanisms, Bethe, H. A., Rev. Mod. Phys. 62 (1990) 801-866.

[2-46]

1987A: The greatest supernova since Kepler, V. Trimble, Rev. Mod. Phys. 60 (1988) 859-871.

[2-47]

The Physics of supernova explosions, Woosley, S. E., Weaver, T. A., Ann. Rev. Astron. Astrophys. 24 (1986) 205.

[2-48]

Supernovae. Part II: the aftermath, V. Trimble, Rev. Mod. Phys. 55 (1983) 511-563.

[2-49]

Supernovae. Part I: the events, V. Trimble, Rev. Mod. Phys. 54 (1982) 1183-1224.

[2-50]

Synthesis of the Elements in Stars, E. Margaret Burbidge, G. R. Burbidge, William A. Fowler, F. Hoyle, Rev. Mod. Phys. 29 (1957) 547.

[3-1]

Neutrinos and the stars, Georg Raffelt, arXiv:1201.1637, 2012. ISAPP School 'Neutrino Physics and Astrophysics', 26 July-5 August 2011, Villa Monastero, Varenna, Italy.

[3-2]

Neutrinos and core-collapse supernovae, Cristina Volpe, arXiv:1108.6285, 2011. XIV International Workshop on 'Neutrino Telescopes', March 15-18, 2011, Venice.

[3-3]

Physics and Astrophysics Opportunities with Supernova Neutrinos, Basudeb Dasgupta, PoS ICHEP2010 (2010) 294, arXiv:1005.2681. Electroweak Session of Rencontres de Moriond 2010.

[3-4]

Significance of neutrino cross-sections for astrophysics, A.B. Balantekin, AIP Conf. Proc. 1189 (2009) 11-15, arXiv:0909.0226. NUINT2009 (6th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region), May 18-22, 2009, Sitges, Barcelona, Spain.

[3-5]

Massive stars as thermonuclear reactors and their explosions following core collapse, Alak Ray, arXiv:0907.5407, 2009. Kodai School on Synthesis of Elements in Stars.

[3-6]

Opportunities for Neutrino Physics at the Spallation Neutron Source (SNS), Efremenko, Yu, Hix, W R, J. Phys. Conf. Ser. 173 (2009) 012006, arXiv:0807.2801. 2008 Carolina International Symposium on Neutrino Physics.

[3-7]

Physics of Supernovae: theory, observations, unresolved problems, D. K. Nadyozhin, arXiv:0804.4350, 2008. Baikal Young Scientists' International School (BAYSIS), 17-22 September 2007, Irkutsk, Russia.

[3-8]

Neutrinos from a core collapse supernova, Dighe, Amol, AIP Conf. Proc. 981 (2008) 75-79, arXiv:0712.4386. NuFact07.

[3-9]

Neutrino-driven explosions twenty years after SN1987A, Janka, H. -Th., Marek, A., Kitaura, F. -S., AIP Conf. Proc. 937 (2007) 144-154, arXiv:0706.3056. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.

[3-10]

Supernova neutrinos, Christian Y. Cardall, Nucl. Phys. Proc. Suppl. 168 (2007) 96-102, arXiv:astro-ph/0703334. NOW2006, Conca Specchiulla, Italy, September 9-16, 2006.

[3-11]

Supernova neutrino observations: What can we learn?, Georg G. Raffelt, Nucl. Phys. Proc. Suppl. 221 (2011) 218-229, arXiv:astro-ph/0701677. ]Neutrino 2006.

[3-12]

Supernova neutrino detection, K. Scholberg, Nucl. Phys. Proc. Suppl. 221 (2011) 248-253, arXiv:astro-ph/0701081. Neutrino 2006, Santa Fe.

[3-13]

Nuclear Astrophysics: CIPANP 2006, Haxton, W. C., AIP Conf. Proc. 870 (2006) 33-43, arXiv:nucl-th/0609006. CIPANP 2006.

[3-14]

Nucleosynthesis in neutrino heated matter: The vp-process and the r-process, G. Martinez-Pinedo et al., PoS NIC-IX (2006) 064, arXiv:astro-ph/0608490. NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006.

[3-15]

From progenitor to afterlife, Roger A. Chevalier, arXiv:astro-ph/0607422, 2006. 2006 STScI May Symposium on Massive Stars.

[3-16]

Supernova and GRB connection: Observations and Questions, Massimo Della Valle, AIP Conf. Proc. 836 (2006) 367-379, arXiv:astro-ph/0604110. 16th Annual October Astrophysics Conference in Maryland, "Gamma Ray Bursts in the Swift Era".

[3-17]

The Cosmic Stellar Birth and Death Rates, John F. Beacom, New Astron. Rev. 50 (2006) 561-565, arXiv:astro-ph/0602101. Astronomy with Radioactivities V, Clemson Univ., Sept. 2005.

[3-18]

Supernovae Shedding Light on Gamma-Ray Bursts, M. Della Valle, Nuovo Cim. 28C (2005) 563, arXiv:astro-ph/0504517. 4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004.

[3-19]

High Redshift Supernovae: Cosmological Implications, Nino Panagia, Nuovo Cim. B120 (2005) 667, arXiv:astro-ph/0502247. Vulcano Workshop 2004, Frontier Objects in Astrophysics and Particle Physics.

[3-20]

Supernova neutrino challenges, Christian Y. Cardall, Nucl. Phys. Proc. Suppl. 145 (2005) 295, arXiv:astro-ph/0502232. NOW2004, Conca Specchiulla (Otranto, Italy), September 11-17, 2004.

[3-21]

Supernova Neutrino Oscillations, Raffelt, Georg G., Phys. Scripta T121 (2005) 102, arXiv:hep-ph/0501049. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.

[3-22]

Physics of Supernovae, Nadyozhin, Dmitrij K., Imshennik, V. S., Int. J. Mod. Phys. A20 (2005) 6597, arXiv:astro-ph/0501002. 19th European Cosmic Ray Symposium (ECRS 2004), Florence, Italy, 30 Aug - 3 Sep 2004.

[3-23]

Supernova neutrino detection, Selvi, M., Nucl. Phys. Proc. Suppl. 145 (2005) 339-342.

[3-24]

Supernovae and Their Massive Star Progenitors, Alexei V. Filippenko, arXiv:astro-ph/0412029, 2004. Science Symposium on the Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.

[3-25]

Three-flavour effects and CP- and T-violation in neutrino oscillations, Evgeny Akhmedov, Phys. Scripta T121 (2005) 65, arXiv:hep-ph/0412029. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.

[3-26]

The Supernovae Associated with Gamma-Ray Bursts, Thomas Matheson, arXiv:astro-ph/0410668, 2004. Supernovae as Cosmological Lighthouses, Padua, 2004.

[3-27]

Stellar explosions: from supernovae to gamma-ray bursts, Konstantin Postnov, arXiv:astro-ph/0410349, 2004. ISCRA 14th School Neutrinos and Explosive Events in the Universe, Erice, Italy, July 2004.

[3-28]

Spectropolarimetry of Core-Collapse Supernovae, Douglas C. Leonard, Alexei V. Filippenko, arXiv:astro-ph/0409518, 2004. Supernovae as Cosmological Lighthouses, 16-19 June, Padua, Italy.

[3-29]

Supernova neutrinos: production, propagation and oscillations, Amol Dighe, Nucl. Phys. Proc. Suppl. 143 (2005) 449, arXiv:hep-ph/0409268. Neutrino 2004, Paris.

[3-30]

Neutrinos: "...annus mirabilis", A. Yu. Smirnov, arXiv:hep-ph/0402264, 2004. 2nd Int. Workshop on Neutrino oscillations in Venice (NOVE) December 3-5, 2003, Venice, Italy.

[3-31]

Spectropolarimetric Observations of Supernovae, Alexei V. Filippenko, Douglas C. Leonard, arXiv:astro-ph/0312500, 2003. 3-D Signatures in Stellar Explosions, 10-13 June, 2003.

[3-32]

A Review of X-ray Observations of Supernova Remnants, Jacco Vink, Nucl. Phys. Proc. Suppl. 132 (2004) 21, arXiv:astro-ph/0311406. The restless high energy universe, Amsterdam, May 2003.

[3-33]

Neutrinos as astrophysical probes, F. Cavanna, M. L. Costantini, O. Palamara, F. Vissani, Surveys High Energ. Phys. 19 (2004) 35, arXiv:astro-ph/0311256. ICTP Summer School on Astroparticle Physics and Cosmology, Trieste, Italy, 17 June - 5 Jul 2002.

[3-34]

Supernova Spectra, M. Turatto, arXiv:astro-ph/0310837, 2003. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.

[3-35]

Observations of Type Ia Supernovae, and Challenges for Cosmology, W. Li, A. V. Filippenko, arXiv:astro-ph/0310529, 2003. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.

[3-36]

The Infrared Supernova Rate, F. Mannucci, G. Cresci, R. Maiolino, M. Della Valle, arXiv:astro-ph/0310210, 2003. IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.

[3-37]

Evidence from Type Ia Supernovae for an Accelerating Universe and Dark Energy, A. V. Filippenko, arXiv:astro-ph/0307139, 2003.

[3-38]

Neutrino Physics after KamLAND, Smirnov, Alexei Yu., arXiv:hep-ph/0306075, 2003. 4th Workshop on "Neutrino Oscillations and their Origin" (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Smirnov.pdf.

[3-39]

Cosmology with Supernovae, P. Ruiz-Lapuente, Astrophys. Space Sci. 290 (2004) 43, arXiv:astro-ph/0304108. JENAM 2002 (Porto, Portugal).

[3-40]

Review on the Observed and Physical Properties of Core Collapse Supernovae, Hamuy, Mario, arXiv:astro-ph/0301006, 2003. 2003 Aspen Summer Workshop on the Nuclear Physics of Core Collapse Supernovae, Aspen, Colorado, 26 May - 8 June 2003.

[3-41]

Supernova Neutrinos and Particle-Physics Applications, Raffelt, G., 2003. Lectures given at ISAPP 2003 - International School on AstroParticle Physics, 14-19 July 2003, Madonna di Campiglio, Italy. http://wwwth.mppmu.mpg.de/members/raffelt/mytalks/ISAPP3.pdf.

[3-42]

Bolometric Light Curves of Supernovae, Suntzeff, N. B., arXiv:astro-ph/0212561, 2002. From Twilight to Highlight - The Physics of Supernovae ESO/MPA/MPE Workshop, Garching, July 29 - 31, 2002.

[3-43]

Type Ia Supernova models: latest developments, Blinnikov, S., Sorokina, E., Astrophys. Space Sci. 290 (2004) 13, arXiv:astro-ph/0212530. JENAM-2002 meeting (Porto, Portugal, September, 3-8).

[3-44]

Neutrinos from supernovae, Choubey, Sandhya, Kar, Kamales, arXiv:hep-ph/0212326, 2002. INSA Proceedings.

[3-45]

Core Collapse and Then? The Route to Massive Star Explosions, H.-Th. Janka et al., arXiv:astro-ph/0212316, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.

[3-46]

Astrophysical and Cosmological Neutrinos, Raffelt, G. G., arXiv:hep-ph/0208024, 2002. International School of Physics "Enrico Fermi," CLII Course "Neutrino Physics," 23 July-2 August 2002, Varenna, Lake Como, Italy.

[3-47]

Neutrino masses in astroparticle physics, Raffelt, G. G., New Astron. Rev. 46 (2002) 699-708, arXiv:astro-ph/0207220. Dennis Sciama Memorial Volume of NAR.

[24-35]

Neutrinos from supernovae: experimental status and perspectives, Cei, Fabrizio, Int. J. Mod. Phys. A17 (2002) 1765-1776, arXiv:hep-ex/0202043. Second International Workshop on Matter, Anti-Matter and Dark Matter, Trento (Italy), 29-30 October 2001.

[3-49]

Physics with supernovae, Raffelt, Georg. G., Nucl. Phys. Proc. Suppl. 110 (2002) 254-267, arXiv:hep-ph/0201099. TAUP 2001: Topics in Astroparticle and Underground Physics, Assergi, Italy, 8-12 Sep 2001.

[3-50]

Supernovae : Theory, expected Rates, Energy Spectrum, Flavor Composition, Time Structure, Raffelt, G., 2002. Workshop on Large Detectors for proton decay, supernovae, and atmospheric neutrinos, and low energy neutrinos from high intensity beams, NNN02, CERN, 16-18 January 2002. http://muonstoragerings.cern.ch/NuWorkshop02/presentations/raffelt.ppt.

[3-51]

Supernova types and rates, Cappellaro, E., Turatto, M., arXiv:astro-ph/0012455, 2000.

[3-52]

Supernova and Cosmology, Signore, M., Puy, D., New Astron. Rev. 45 (2001) 409, arXiv:astro-ph/0010634.

[3-53]

Massive neutrinos in astrophysics, Raffelt, Georg G., Rodejohann, Werner, arXiv:hep-ph/9912397, 1999. 4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998.

[3-54]

Supernova 1987A - A review, Bhattacharya D., Bulletin of the Astronomical Society of India 16 (1988) 57-66. Astronomical Society of India, Meeting, 12th, Raipur, India, Dec. 1987.

[3-55]

Supernova models, S. E. Woosley, T. A. Weaver, New York Academy Sciences Annals 375 (1981) 357-380.

[3-56]

Evolution and explosion of massive stars, S. E. Woosley, T. A. Weaver, Ninth Texas Symposium on Relativistic Astrophysics. 335-357 (1980).

[4-1]

Observational neutrino astrophysics, Koshiba, M., Phys. Rep. 220 (1992) 229-381.

[4-2]

The number of neutrino species, Denegri, D., Sadoulet, B., Spiro, M., Rev. Mod. Phys. 62 (1990) 1.

[4-3]

1987A: The greatest supernova since Kepler, V. Trimble, Rev. Mod. Phys. 60 (1988) 859-871.

[5-1]

The Evolution of Low Mass Helium Stars towards Supernova Type I Explosion, Roni Waldman, Zalman Barkat, arXiv:astro-ph/0605692, 2006.

[5-2]

Supernova neutrino spectra and applications to flavor oscillations, Keil, Mathias Thorsten, arXiv:astro-ph/0308228, 2003.

[6-1]

Kepler's Supernova Remnant: The view at 400 Years, W. P. Blair, arXiv:astro-ph/0410081, 2004. 1604-2004: Supernovae as Cosmological Lighthouses.

[7-1]

The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae, Gaston Folatelli et al., Astron. J. 139 (2010) 120-144, arXiv:0910.3317.

[7-2]

Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations, K. Motohara et al., Astrophys. J. 652 (2006) L101-L104, arXiv:astro-ph/0610303.

[7-3]

The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey, A. Conley et al., Astron. J. 132 (2006) 1707-1713, arXiv:astro-ph/0607363.

[7-4]

Nonlinear Decline-Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities, Lifan Wang et al., Astrophys. J. 641 (2006) 50-69, arXiv:astro-ph/0512370.

[9-1]

The Supernova Legacy Survey: Measurement of , and from the First Year Data Set, P. Astier et al. (SNLS), Astron. Astrophys. 447 (2006) 31, arXiv:astro-ph/0510447.
From the abstract: With this data set, we have built a Hubble diagram extending to , with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: for a flat ; and for a flat cosmology with constant equation of state when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.

[9-2]

Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, Clocchiatti, A. et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.

[7-7]

Spectroscopy of twelve Type Ia supernovae at intermediate redshift, C. Balland et al., arXiv:astro-ph/0507703, 2005.

[9-3]

First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization, Chris J. Willott et al., Astrophys. J. 633 (2005) 630, arXiv:astro-ph/0507183.

[7-9]

Evidence for Spectropolarimetric Diversity in Type Ia Supernovae, Douglas C. Leonard et al., Astrophys. J. 632 (2005) 450, arXiv:astro-ph/0506470.

[7-10]

A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex, R. J. Foley et al., Astrophys. J. 626 (2005) L11, arXiv:astro-ph/0504481.

[9-4]

Restframe I-band Hubble diagram for type Ia supernovae up to redshift , Nobili, Serena et al. (Supernova Cosmology Project), arXiv:astro-ph/0504139, 2005.

[9-5]

Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Riess, Adam G. et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: .

[9-6]

The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Strolger, Louis-Gregory, Riess, Adam G., Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.

[9-7]

Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, Lidman, C. et al. (Supernova Cosmology Project), arXiv:astro-ph/0410506, 2004.

[9-8]

The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, Strolger, L. G. et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.

[9-9]

Type Ia supernova rate at a redshift of ~ 0.1, Blanc, Guillaume et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.

[9-10]

Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Garavini, Gabriele et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.

[9-11]

Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 607 (2004) 665, arXiv:astro-ph/0402512.
From the abstract: We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration.
...
A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at .
The data are consistent with the cosmic concordance model of (), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy.
For a flat Universe with a cosmological constant, we measure (equivalently, ). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find (and at the 95% confidence level) for an assumed static equation of state of dark energy, .
...
Our constraints are consistent with the static nature of and value of expected for a cosmological constant (i.e., , ), and are inconsistent with very rapid evolution of dark energy.

[9-12]

23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at , Brian J. Barris et al., Astrophys. J. 602 (2004) 571, arXiv:astro-ph/0310843.
From the abstract: This sample of 23 high-redshift supernovae includes 15 at , doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB []. Adopting the constraint that , we obtain best-fit values of (,)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation.

[9-13]

New Constraints on , , and from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Knop, Robert A. et al. (The Supernova Cosmology Project), Astrophys. J. 598 (2003) 102, arXiv:astro-ph/0309368.
From the abstract: We report measurements of , , and from eleven supernovae at - with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density (statistical) (identified systematics), or equivalently, a cosmological constant of (statistical) (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value . When the supernova results are combined with independent flat-universe measurements of from CMB and galaxy redshift distortion data, they provide a measurement of (statistical) (identified systematic), if is assumed to be constant in time. ... dark energy is required with .

[9-14]

Cosmological Results from High-z Supernovae, Tonry, John L. et al. (Supernova Search Team), Astrophys. J. 594 (2003) 1, arXiv:astro-ph/0305008.
From the abstract: The High- Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval . These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to , where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is , then , and . Including the constraint of a flat Universe, we find , independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range at 95% confidence. If we further assume that , we obtain at 95% confidence.

[7-22]

SN 2002cx: The Most Peculiar Known Type Ia Supernova, Weidong Li et al., Publ. Astron. Soc. Pac. 115 (2003) 453-473, arXiv:astro-ph/0301428.

[7-23]

Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el, Kevin Krisciunas et al., Astron. J. 125 (2003) 166, arXiv:astro-ph/0210327.

[7-24]

The Type la Supernova 2001V in NGC 3987, J. Vinko et al., Astron. Astrophys. 397 (2003) 115, arXiv:astro-ph/0210186.

[9-15]

The distant Type Ia supernova rate, Pain, R. et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.

[9-16]

The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Riess, Adam G. et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.

[9-17]

Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Perlmutter, S. et al. (Supernova Cosmology Project), Astrophys. J. 517 (1999) 565-586, arXiv:astro-ph/9812133.
From the abstract: The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation in the region of interest (). For a flat () cosmology we find (1 statistical) (identified systematics). The data are strongly inconsistent with a flat cosmology, the simplest inflationary universe model. An open, cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of %, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is Gyr for a flat cosmology.

[9-18]

Supernova Limits on the Cosmic Equation of State, Garnavich, Peter M. et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.

[9-19]

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Riess, Adam G. et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.

[8-1]

Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants, C. Badenes et al., arXiv:astro-ph/0506576, 2005. "Stellar end products" workshop, 13-15 April 2005, Granada, Spain.

[8-2]

The Fall 2004 SDSS Supernova Survey, Masao Sako et al. (The SDSS), eConf C041213 (2005) 1424, arXiv:astro-ph/0504455. 22nd Texas Symposium on Relativistic Astrophysics.

[9-1]

The Supernova Legacy Survey: Measurement of , and from the First Year Data Set, P. Astier et al. (SNLS), Astron. Astrophys. 447 (2006) 31, arXiv:astro-ph/0510447.
From the abstract: With this data set, we have built a Hubble diagram extending to , with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: for a flat model; and for a flat cosmology with constant equation of state when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.

[9-2]

Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, Clocchiatti, A. et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.

[9-3]

First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization, Chris J. Willott et al., Astrophys. J. 633 (2005) 630, arXiv:astro-ph/0507183.

[9-4]

Restframe I-band Hubble diagram for type Ia supernovae up to redshift , Nobili, Serena et al. (Supernova Cosmology Project), arXiv:astro-ph/0504139, 2005.

[9-5]

Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Riess, Adam G. et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: .

[9-6]

The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Strolger, Louis-Gregory, Riess, Adam G., Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.

[9-7]

Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, Lidman, C. et al. (Supernova Cosmology Project), arXiv:astro-ph/0410506, 2004.

[9-8]

The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, Strolger, L. G. et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.

[9-9]

Type Ia supernova rate at a redshift of ~ 0.1, Blanc, Guillaume et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.

[9-10]

Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Garavini, Gabriele et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.

[9-11]

Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 607 (2004) 665, arXiv:astro-ph/0402512.
From the abstract: We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration.
...
A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at .
The data are consistent with the cosmic concordance model of (), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy.
For a flat Universe with a cosmological constant, we measure (equivalently, ). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find (and at the 95% confidence level) for an assumed static equation of state of dark energy, .
...
Our constraints are consistent with the static nature of and value of expected for a cosmological constant (i.e., , ), and are inconsistent with very rapid evolution of dark energy.

[9-12]

23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at , Brian J. Barris et al., Astrophys. J. 602 (2004) 571, arXiv:astro-ph/0310843.
From the abstract: This sample of 23 high-redshift supernovae includes 15 at , doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB []. Adopting the constraint that , we obtain best-fit values of (,)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation.

[9-13]

New Constraints on , , and from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Knop, Robert A. et al. (The Supernova Cosmology Project), Astrophys. J. 598 (2003) 102, arXiv:astro-ph/0309368.
From the abstract: We report measurements of , , and from eleven supernovae at - with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density (statistical) (identified systematics), or equivalently, a cosmological constant of (statistical) (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value . When the supernova results are combined with independent flat-universe measurements of from CMB and galaxy redshift distortion data, they provide a measurement of (statistical) (identified systematic), if is assumed to be constant in time. ... dark energy is required with .

[9-14]

Cosmological Results from High-z Supernovae, Tonry, John L. et al. (Supernova Search Team), Astrophys. J. 594 (2003) 1, arXiv:astro-ph/0305008.
From the abstract: The High- Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval . These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to , where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is , then , and . Including the constraint of a flat Universe, we find , independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range at 95% confidence. If we further assume that , we obtain at 95% confidence.

[9-15]

The distant Type Ia supernova rate, Pain, R. et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.

[9-16]

The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Riess, Adam G. et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.

[9-17]

Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Perlmutter, S. et al. (Supernova Cosmology Project), Astrophys. J. 517 (1999) 565-586, arXiv:astro-ph/9812133.
From the abstract: The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation in the region of interest (). For a flat () cosmology we find (1 statistical) (identified systematics). The data are strongly inconsistent with a flat cosmology, the simplest inflationary universe model. An open, cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of %, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is Gyr for a flat cosmology.

[9-18]

Supernova Limits on the Cosmic Equation of State, Garnavich, Peter M. et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.

[9-19]

Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Riess, Adam G. et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.

[10-1]

Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program, R. Abbasi et al. (IceCube), arXiv:1111.7030, 2011.

[10-2]

An Extremely Luminous X-ray Outburst Marking the Birth of a Normal Supernova, A. M. Soderberg et al., Nature. 453 (2008) 469-474, arXiv:0802.1712.

[10-3]

Gamma-Ray Burst associated Supernovae: Outliers become Mainstream, E. Pian et al., Nature 442 (2006) 1011-1013, arXiv:astro-ph/0603530.

[10-4]

Discovery of 35 New Supernova Remnants in the Inner Galaxy, C. L. Brogan et al., Astrophys. J. 639 (2006) L25, arXiv:astro-ph/0601451.

[10-5]

Echoes from Ancient Supernovae in the Large Magellanic Cloud, A. Rest et al., arXiv:astro-ph/0510738, 2005.

[10-6]

Discovery of X-Ray Emission from Supernova 1970G with Chandra: Filling the Void between Supernovae and Supernova Remnants, Stefan Immler, K. D. Kuntz, Astrophys. J. 632 (2005) L99, arXiv:astro-ph/0506023.

[10-7]

Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C, Immler, Stefan et al., Astrophys. J. 632 (2005) 283, arXiv:astro-ph/0503678.

[10-8]

Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae, Justyn R. Maund, Stephen J. Smartt, Mon. Not. Roy. Astron. Soc. 360 (2005) 288, arXiv:astro-ph/0501323.

[10-9]

SN Ib 1990I: Clumping and Dust in the Ejecta?, Elmhamdi, Abouazza et al., Astron. Astrophys. 426 (2004) 963-977, arXiv:astro-ph/0407145.

[10-10]

The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope, Nikolai N. Chugai et al., Mon. Not. Roy. Astron. Soc. 352 (2004) 1213, arXiv:astro-ph/0405369.

[10-11]

XMM-Newton observation of Kepler's supernova remnant, G. Cassam-Chenai et al., arXiv:astro-ph/0310687, 2003.

[10-12]

The Asiago Supernova Catalogue - 10 years after, Barbon, R., Buondi, V., Cappellaro, E., Turatto, M., Astron. Astrophys. 139 (1999) 531-536.

[11-1]

The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova Searches, Ice Properties, R. Abbasi et al. (IceCube), arXiv:1111.2731, 2011. 32nd International Cosmic Ray Conference, Beijing 2011.

[11-2]

Low Energy Neutrino Astronomy in Super-Kamiokande, Michael Smy, arXiv:1110.0012, 2011. DPF 2011.

[11-3]

Search for neutrino bursts from core collapse supernovae at the Baksan Underground Scintillation Telescope, R.V. Novoseltseva et al., arXiv:0910.0738, 2009. 31 International Cosmic Ray Conference, Lodz, Poland, July 7-15, 2009.

[11-4]

Supernova Search with the AMANDA / IceCube Detectors, Thomas Kowarik, Timo Griesel, Alexander Piegsa (Icecube), arXiv:0908.0441, 2009. 31st ICRC, Lodz, Poland, July 2009.

[11-5]

Search for High Energetic Neutrinos from Supernova Explosions with AMANDA, Dirk Lennarz, Jan-Patrick Huls, Christopher Wiebusch (IceCube), arXiv:0907.4621, 2009. 31st ICRC, Lodz, Poland, July 2009.

[11-6]

Recent Type II Radio Supernovae, Christopher J. Stockdale et al., AIP Conf. Proc. 937 (2007) 264-268, arXiv:0708.1182. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.

[11-7]

LVD highlights, Marco Selvi et al. (LVD), arXiv:hep-ex/0608061, 2006. Vulcano Workshop 2006 "Frontier Objects in Astrophysics and Particle Physics".

[11-8]

SNLS - the Supernova Legacy Survey, C.J. Pritchet, SNLS Collaboration (SNLS), arXiv:astro-ph/0406242, 2004. Observing Dark Energy (NOAO/Tucson proceedings).

[11-9]

Evidence for Core Collapse in the Type Ib/c SN 1999ex, Mario Hamuy et al., arXiv:astro-ph/0212368, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.

[11-10]

The dusty type IIn Supernova 1998S, Peter Meikle et al., arXiv:astro-ph/0211144, 2002. ESO/MPA/MPE Workshop "From Twilight to Highlight: The Physics of Supernovae", Garching, Germany, 29-31 July 2002.

[11-11]

A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images, Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko, arXiv:astro-ph/0210347, 2002. PASP (2003 Jan).

[11-12]

An Intermediate Redshift Supernova Search at ESO: Reduction Tools and Efficiency Tests, M. Riello et al., arXiv:astro-ph/0210265, 2002. ESO/MPA/MPE Workshop "From Twilight to Highlight, The Physics of Supernovae", Garching, Jul 29-31, 2002.

[11-13]

Search for double degenerate progenitors of supernovae type Ia with SPY, R. Napiwotzki, H. Drechsel, U. Heber, C. Karl, E.-M. Pauli et al., others, others, others, others, others, others, others, others, others, others, arXiv:astro-ph/0210155, 2002. "White Dwarfs", Proc. XIII Workshop on White Dwarfs.

[12-1]

Supernova Relic Neutrino Search at Super-Kamiokande, K. Bays et al. (Super-Kamiokande), Phys. Rev. D85 (2012) 052007, arXiv:1111.5031.

[12-2]

IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae, R. Abbasi et al. (IceCube), arXiv:1108.0171, 2011.

[12-3]

Low Multiplicity Burst Search at the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 728 (2011) 83, arXiv:1011.5436.

[12-4]

A Search for Core-Collapse Supernovae using the MiniBooNE Neutrino Detector, A. A. Aguilar-Arevalo et al. (MiniBooNE), Phys. Rev. D81 (2010) 032001, arXiv:0910.3182.

[12-5]

Search for Supernova Neutrino Bursts at Super-Kamiokande, Ikeda, M., Takeda, A., Fukuda, Y., Vagins, M. R., Sakuda, M. (Super-Kamiokande), Astrophys. J. 669 (2007) 519-524, arXiv:0706.2283.

[12-6]

A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 653 (2006) 1545-1551, arXiv:hep-ex/0607010.

[12-7]

SNEWS: The SuperNova Early Warning System, P. Antonioli et al., New J. Phys. 6 (2004) 114, arXiv:astro-ph/0406214.

[12-8]

Twenty Years of Galactic Observations in Searching for Bursts of Collapse Neutrinos with the Baksan Underground Scintillation Telescope, E.N.Alexeyev, L.N.Alexeyeva, J. Exp. Theor. Phys. 95 (2002) 5, arXiv:astro-ph/0212499.

[12-9]

Search for supernova relic neutrinos at Super-Kamiokande, Malek, M. et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 061101, arXiv:hep-ex/0209028.

[13-1]

A "Missing" Supernova Remnant revealed by the 21-cm Line of Atomic Hydrogen, B-C Koo, J-h Kang, C.J. Salter, Astrophys. J. 643 (2006) L49-L52, arXiv:astro-ph/0604186.

[14-1]

A Search for Supernova Neutrinos with the Sudbury Neutrino Observatory, Jaret Heise, 2001. University of British Columbia, Vancouver BC, December 2001.

[15-1]

Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots, Per Groeningsson et al., arXiv:0810.2661, 2008.

[15-2]

Chandra HETG Spectra of SN 1987A at 20 years, Dewey, D., Zhekov, S. A., McCray, R., Canizares, C. R., arXiv:0802.2340, 2008.

[15-3]

Infrared Integral Field Spectroscopy of SN 1987A, Karina Kjaer et al., AIP Conf. Proc. 937 (2007) 76-80, arXiv:astro-ph/0703720.

[15-4]

Discovery of a nearby twin of SN1987A's nebula around the luminous blue variable HD168625: Was Sk-69 202 an LBV?, Nathan Smith, Astron. J. 133 (2007) 1034-1040, arXiv:astro-ph/0611544.

[15-5]

On the Progenitor of Supernova 1987A, M. Parthasarathy, David Branch, E. Baron, David J. Jeffery, arXiv:astro-ph/0611033, 2006.

[15-6]

Evolutionary Status of SNR 1987A at the Age of Eighteen, Sangwook Park et al., Astrophys. J. 646 (2006) 1001-1008, arXiv:astro-ph/0604201.

[15-7]

Coronal emission from the shocked circumstellar ring of SN 1987A, Per Groningsson et al., arXiv:astro-ph/0603815, 2006.

[15-8]

SN 1987A After 18 Years: Mid-Infrared GEMINI and SPITZER Observations of the Remnant, Patrice Bouchet et al., Astrophys. J. 650 (2006) 212-227, arXiv:astro-ph/0601495.

[15-9]

The reverse shock of SNR1987A at 18 years after outburst, Nathan Smith et al., Astrophys. J. 635 (2005) L41, arXiv:astro-ph/0510835.

[15-10]

Supernova Remnant 1987A: Opening the Future by Reaching the Past, Sangwook Park, Svetozar A. Zhekov, David N. Burrows, Richard McCray, Astrophys. J. 634 (2005) L73, arXiv:astro-ph/0510442.

[15-11]

Imaging of the Radio Remnant of SN 1987A at 12 mm Wavelength, R. N. Manchester et al., Astrophys. J. 628 (2005) L131, arXiv:astro-ph/0506475.

[15-12]

Chandra Observations of Shock Kinematics in Supernova Remnant 1987A, S.A. Zhekov et al., Astrophys. J. 628 (2005) L127, arXiv:astro-ph/0506443.

[15-13]

Limits from the Hubble Space Telescope on a Point Source in SN 1987A, G. J. M. Graves et al., Astrophys. J. 629 (2005) 944, arXiv:astro-ph/0505066.

[15-14]

A New View of the Circumstellar Environment of SN 1987A, Ben E. K. Sugerman et al., Astrophys. J. 627 (2005) 888, arXiv:astro-ph/0502268.

[15-15]

Supernova Remnant 1987A: The Latest Report from the Chandra X-Ray Observatory, Sangwook Park et al., Adv. Space Res. 35 (2005) 991-995, arXiv:astro-ph/0501561.

[15-16]

Constraints on the luminosity of the stellar remnant in SNR1987A, P. Shtykovskiy, A. Lutovinov, M. Gilfanov, R. Sunyaev, Astron. Lett. 31 (2005) 258, arXiv:astro-ph/0411731.

[15-17]

High Resolution Imaging of SN 1987A at 10 micron, P. Bouchet et al., Astrophys. J. 611 (2004) 394, arXiv:astro-ph/0312240.

[15-18]

The X-ray Remnant of SN1987A, Burrows, David N. et al., Astrophys. J. 543 (2000) L149-L152, arXiv:astro-ph/0009265.

[15-19]

Young Stellar Populations Around SN1987A, Panagia, Nino, Romaniello, Martino, Scuderi, Salvatore, Kirshner, Robert P., Astrophys. J. 539 (2000) 197-208, arXiv:astro-ph/0001476.

[15-20]

A Second Bright Source Detected Near SN1987A, Nisenson, Peter, Papaliolios, Costas, arXiv:astro-ph/9904109, 1999.

[15-21]

The X-ray lightcurve of SN 1987A, Hasinger, G., Aschenbach, B., Trumper, J., Astron. Astrophys. 312 (1996) L9-L12, arXiv:astro-ph/9606149.

[15-22]

The progenitor of SN 1987A - Spatially resolved ultraviolet spectroscopy of the supernova field, Sonneborn, George, Altner, Bruce, Kirshner, Robert P., Astrophys. J. 323 (1987) L35-L39.

[15-23]

Ultraviolet observations of SN 1987A, Kirshner, Robert P., Sonneborn, George, Crenshaw, D. Michael, Nassiopoulos, George E., Astrophys. J. 320 (1987) 602-608.

[16-1]

SN1987A: Revisiting the Data and the Correlation between Neutrino and Gravitational Detectors, P. Galeotti, G. V. Pallottino, G. Pizzella, arXiv:0810.3759, 2008. Vulcano Wokshop 2008, Frontier Objects in Astrophysics and Particle Physics, May 26-31.

[16-2]

Chandra Observations of Supernova 1987A, Sangwook Park et al., AIP Conf. Proc. 937 (2007) 43-50, arXiv:0704.0209. Supernova 1987A: 20 Years after Supernovae and Gamma-Ray Bursters, Aspen, CO, USA, Feb 19-23, 2007.

[16-3]

Supernova Remnant 1987A: High Resolution Images and Spectrum from Chandra Observations, Sangwook Park et al., arXiv:astro-ph/0511355, 2005. The X-Ray Universe 2005, Sept 26-30, 2005, El Escorial, Madrid, Spain.

[16-4]

A 2.14 ms Candidate Optical Pulsar in SN1987A, Middleditch, J. et al., arXiv:astro-ph/0010044, 2000. 5th CTIO/ESO Workshop and 1st CTIO/ESO/LCO Workshop: SN 1987A: Ten Years After, La Serena, Chile, 22-28 Feb 1997.

[17-1]

DETECTION OF THE NEUTRINO SIGNAL FROM SN1987A IN THE LMC USING THE INR BAKSAN UNDERGROUND SCINTILLATION TELESCOPE, Alekseev, E. N., Alekseeva, L. N., Krivosheina, I. V., Volchenko, V. I., Phys. Lett. B205 (1988) 209-214.

[17-2]

CHARACTERISTICS OF THE NEUTRINO EMISSION FROM SUPERNOVA SN1987A, Chudakov, A. E., Elensky, Ya. S., Mikheev, S. P., JETP Lett. 46 (1987) 373-377. [Pisma Zh. Eksp. Teor. Fiz. 46, 297 (1987)].

[17-3]

POSSIBLE DETECTION OF A NEUTRINO SIGNAL ON 23 FEBRUARY 1987 AT THE BAKSAN UNDERGROUND SCINTILLATION TELESCOPE OF THE INSTITUTE OF NUCLEAR RESEARCH, Alekseev, E. N., Alekseeva, L. N., Volchenko, V. I., Krivosheina, I. V., JETP Lett. 45 (1987) 589-592. [Pisma Zh. Eksp. Teor. Fiz. 45, 461-464 (1987)].

[18-1]

NEUTRINOS FROM SN1987A IN THE IMB DETECTOR, Van Der Velde, J. C. et al. (IMB), Nucl. Instrum. Meth. A264 (1988) 28-31.

[18-2]

ANGULAR DISTRIBUTION OF EVENTS FROM SN1987A, Bratton, C. B. et al. (IMB), Phys. Rev. D37 (1988) 3361.

[18-3]

OBSERVATION OF A NEUTRINO BURST IN COINCIDENCE WITH SUPERNOVA SN1987A IN THE LARGE MAGELLANIC CLOUD, Bionta, R. M. et al. (IMB), Phys. Rev. Lett. 58 (1987) 1494.

[19-1]

Observation in the Kamiokande-II detector of the neutrino burst from supernova SN1987A, Hirata, K. S. et al. (Kamiokande), Phys. Rev. D38 (1988) 448-458.

[19-2]

A search for high-energy neutrinos from SN1987a: first six months, Oyama, Y. et al. (Kamiokande), Phys. Rev. Lett. 59 (1987) 2604.

[19-3]

Observation of a neutrino burst from the supernova SN1987a, Hirata, K. et al. (Kamiokande), Phys. Rev. Lett. 58 (1987) 1490-1493.

[20-1]

Correlations between low-energy and high-energy pulses detected by the LSD installation under Mt. Blanc from 10 February 1987 to 1 July 1987, Dadykin, V. L. et al., JETP Lett. 56 (1992) 426-429.

[20-2]

Coincidences among the data recorded by the Baksan, Kamioka and Mont Blanc underground neutrino detectors, and by the Maryland and Rome gravitational wave detectors during supernova SN1987A, Aglietta, M. et al., Nuovo Cim. C14 (1991) 171-193.

[20-3]

Correlation between the Maryland and Rome gravitational wave detectors and the Mont Blanc, Kamioka and IMB particle detectors during SN1987A, Aglietta, M. et al., Nuovo Cim. B106 (1991) 1257-1269.

[20-4]

Correlations of the low-energy pulses and muons recorded at the Mont Blanc LSD apparatus between 10 February and 1 July 1987, Dadykin, V. L. et al., Bull. Russ. Acad. Sci. Phys. 55 (1991) NO.4129.

[20-5]

Neutrino astrophysics and SN1987A, Aglietta, M. et al., Nuovo Cim. C13 (1990) 365-374.

[20-6]

ANALYSIS OF THE DATA RECORDED BY THE MONT BLANC NEUTRINO DETECTOR AND BY THE MARYLAND AND ROME GRAVITATIONAL WAVE DETECTORS DURING SN1987A, Aglietta, M. et al., Nuovo Cim. C12 (1989) 75-103.

[20-9]

NEUTRINO OBSERVATIONS FROM SUPERNOVA SN1987A, Galeotti, P. et al., Helv. Phys. Acta 60 (1987) 619-628.

[20-8]

DETECTION OF A RARE EVENT ON 23 FEBRUARY 1987 BY THE NEUTRINO RADIATION DETECTOR UNDER MONT BLANC, Dadykin, V. L. et al., JETP Lett. 45 (1987) 593-595.

[20-9]

NEUTRINO OBSERVATIONS FROM SUPERNOVA SN1987A, Galeotti, P. et al., Helv. Phys. Acta 60 (1987) 619-628.

[21-1]

Three-Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae, G C Jordan IV et al., (2007), arXiv:astro-ph/0703573.

[21-2]

Capturing the Fire: Flame Energetics and Neutronizaton for Type Ia Supernova Simulations, A. C. Calder et al., Astrophys. J. 656 (2007) 313-332, arXiv:astro-ph/0611009.

[21-3]

C+O detonations in thermonuclear supernovae: Interaction with previously burned material, A. Maier, J.C. Niemeyer, arXiv:astro-ph/0605293, 2006.

[21-4]

Type Ia supernova diversity in three-dimensional models, F. K. Roepke et al., arXiv:astro-ph/0506107, 2005.

[21-5]

Three-dimensional modeling of Type Ia supernovae - The power of late time spectra, Cecilia Kozma et al., arXiv:astro-ph/0504317, 2005.

[21-6]

The distributed burning regime in Type Ia supernova models, F. K. Roepke, W. Hillebrandt, Astron. Astrophys. 429 (2005) L29-L32, arXiv:astro-ph/0411667.

[21-7]

Three-Dimensional Delayed-Detonation Model of Type Ia Supernova, Vadim N. Gamezo, Alexei M. Khokhlov, Elaine S. Oran, Astrophys. J. 623 (2005) 337, arXiv:astro-ph/0409598.

[21-8]

Simulations of Turbulent Thermonuclear Burning in Type Ia Supernovae, W. Hillebrandt et al., arXiv:astro-ph/0405209, 2004.

[21-9]

Direct Numerical Simulations of Type Ia Supernovae Flames I: The Landau-Darrieus Instability, J. B. Bell et al., Astrophys. J. 606 (2004) 1029, arXiv:astro-ph/0311543.

[21-10]

Carbon Ignition in Type Ia Supernovae: An Analytic Model, S. E. Woosely, S. Wunsch, M. Kuhlen, arXiv:astro-ph/0307565, 2003.

[22-1]

Three-dimensional Modeling of Type Ia Supernova Explosions, F. K. Roepke, W. Hillebrandt, AIP Conf. Proc. 847 (2006) 190-195, arXiv:astro-ph/0610199. International Symposium of Origin of Matter and Evolution of Galaxies 2005.

[22-2]

Surface detonation in type Ia supernova explosions?, F. K. Roepke, S. E. Woosley, J. Phys. 46 (2006) 413-417, arXiv:astro-ph/0609691. SciDAC 2006 Meeting, Denver June 25-26 2006.

[22-3]

Numerical Simulations of Type Ia Supernova Explosions, Ropke, Friedrich K., Hillebrandt, W., Gieseler, M., Reinecke, M., Travaglio, C., arXiv:astro-ph/0609456, 2006. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, Germany, 2004.

[22-4]

Type Ia Supernovae: Simulations and Nucleosynthesis, E. F. Brown et al., arXiv:astro-ph/0505417, 2005. Nuclei in the Cosmos 8.

[22-5]

Thermonuclear supernova models, and observations of Type Ia supernovae, E. Bravo, C. Badenes, D. Garcia-Senz, Aip Conf. Proc. 797 (2005) 453, arXiv:astro-ph/0412155. Conference on Interacting Binaries: Accretion, Evolution and Outcomes, Cefalu, Italy, July 2004.

[23-1]

An Investigation into the Character of Pre-Explosion Core-Collapse Supernova Shock Motion, Adam Burrows, Joshua C. Dolence, Jeremiah W. Murphy, arXiv:1204.3088, 2012.

[23-2]

A New Monte Carlo Method for Time-Dependent Neutrino Radiation Transport, Ernazar Abdikamalov et al., arXiv:1203.2915, 2012.

[23-3]

Fully General Relativistic Simulations of Core-Collapse Supernovae with An Approximate Neutrino Transport, Kuroda, Takami, Kotake, Kei, Takiwaki, Tomoya, arXiv:1202.2487, 2012.

[23-4]

A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae II. Relativistic Explosion Models of Core-Collapse Supernovae, B. Mueller, H.-Th. Janka, A. Marek, arXiv:1202.0815, 2012.

[23-5]

Neutrino Transfer in Three Dimensions for Core-Collapse Supernovae. I. Static Configurations, Kohsuke Sumiyoshi, Shoichi Yamada, Astrophys. J. Supp. 199 (2012) 17, arXiv:1201.2244.

[23-6]

Neutrino spectra evolution during proto-neutron star deleptonization, T. Fischer, G. Martinez-Piedo, M. Hempel, M. Liebendorfer, Phys. Rev. D85 (2012) 083003, arXiv:1112.3842.

[23-7]

Is Strong SASI Activity the Key to Successful Neutrino-Driven Supernova Explosions?, Florian Hanke, Andreas Marek, Bernhard Mueller, Hans-Thomas Janka, arXiv:1108.4355, 2011.

[23-8]

Three-dimensional Hydrodynamic Core-Collapse Supernova Simulations for an Star with Spectral Neutrino Transport, Takiwaki, Tomoya, Kotake, Kei, Suwa, Yudai, Astrophys. J. 749 (2012) 98, arXiv:1108.3989.

[23-9]

Relativistic collapse and explosion of rotating supermassive stars with thermonuclear effects, Pedro J. Montero, Hans-Thomas Janka, Ewald Mueller, Astrophys. J. 749 (2012) 37, arXiv:1108.3090.

[23-10]

New equations of state in core-collapse supernova simulations, Matthias Hempel, Tobias Fischer, Jurgen Schaffner-Bielich, Matthias Liebendorfer, Astrophys. J. 748 (2012) 70, arXiv:1108.0848.

[23-11]

Parametrized 3D models of neutrino-driven supernova explosions: Neutrino emission asymmetries and gravitational-wave signals, E. Muller, H.-Th. Janka, A. Wongwathanarat, arXiv:1106.6301, 2011.

[23-12]

A Global Turbulence Model for Neutrino-Driven Convection in Core-Collapse Supernovae, Jeremiah W. Murphy, Casey Meakin, Astrophys. J. 742 (2011) 74, arXiv:1106.5496.

[23-13]

Effects of Rotation on Stochasticity of Gravitational Waves in Nonlinear Phase of Core-Collapse Supernovae, Kei Kotake, Wakana Iwakami Nakano, Naofumi Ohnishi, Astrophys. J. 736 (2011) 124, arXiv:1106.0544.

[23-14]

Solving the transport equation by the use of 6D spectral methods in spherical geometry, Silvano Bonazzola, Nicolas Vasset, arXiv:1104.5330, 2011.

[23-15]

Magnetic field amplification in collapsing, non-rotating stellar cores, Martin Obergaulinger, Hans-Thomas Janka, arXiv:1101.1198, 2011.

[23-16]

The revival of an explosion mechanism of massive stars - the quark hadron phase transition during the early post bounce phase of core collapse supernovae, T. Fischer et al., Astrophys. J. Supp. 194 (2011) 39, arXiv:1011.3409.

[23-17]

Induced Rotation in 3D Simulations of Core Collapse Supernovae: Implications for Pulsar Spins, E. Rantsiou, A. Burrows, J. Nordhaus, A. Almgren, Astrophys. J. 732 (2011) 57, arXiv:1010.5238.

[23-18]

Hydrodynamical Neutron Star Kicks in Three Dimensions, A. Wongwathanarat, H.-Th. Janka, E. Mueller, (2010), arXiv:1010.0167.

[23-19]

Formation of black hole and accretion disk in collapsar, Yuichiro Sekiguchi, Masaru Shibata, Astrophys. J. 737 (2011) 6, arXiv:1009.5303.

[23-20]

Results From Core-Collapse Simulations with Multi-Dimensional, Multi-Angle Neutrino Transport, Timothy D. Brandt, Adam Burrows, Christian D. Ott, Astrophys. J. 728 (2011) 8, arXiv:1009.4654.

[23-21]

An implementation of the microphysics in full general relativity : General relativistic neutrino leakage scheme, Yuichiro Sekiguchi, arXiv:1009.3358, 2010.

[23-22]

Stellar core collapse in full general relativity with microphysics - Formulation and Spherical collapse test -, Yuichiro Sekiguchi, Prog. Theor. Phys. 124 (2010) 331-379, arXiv:1009.3320.

[23-23]

Dynamical r-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input, A. Arcones, G. Martinez-Pinedo, Phys. Rev. C83 (2011) 045809, arXiv:1008.3890.

[23-24]

Nucleosynthesis-relevant conditions in neutrino-driven supernova outflows. II. The reverse shock in two-dimensional simulations, A. Arcones, H.-T. Janka, arXiv:1008.0882, 2010.

[23-25]

Production of Light Element Primary Process nuclei in neutrino-driven winds, A. Arcones, F. Montes, Astrophys. J. 731 (2011) 5, arXiv:1007.1275.

[23-26]

Dimension as a Key to the Neutrino Mechanism of Core-Collapse Supernova Explosions, J. Nordhaus, A. Burrows, A. Almgren, J. Bell, Astrophys. J. 720 (2010) 694-703, arXiv:1006.3792.

[23-27]

The Spiral Modes of the Standing Accretion Shock Instability in the Linear Phase, Rodrigo Fernandez, Astrophys. J. 725 (2010) 1563-1580, arXiv:1003.1730.

[23-28]

A new multi-dimensional general relativistic neutrino hydrodynamics code for core-collapse supernovae. I. Method and code tests in spherical symmetry, B. Mueller, H.-Th. Janka, H. Dimmelmeier, Astrophys. J. Suppl. 189 (2010) 104-133, arXiv:1001.4841.

[23-29]

A New Open-Source Code for Spherically-Symmetric Stellar Collapse to Neutron Stars and Black Holes, Evan O'Connor, Christian D. Ott, Class. Quant. Grav. 27 (2010) 114103, arXiv:0912.2393.

[23-30]

Gravitational waves from supernova matter, S. Scheidegger, S.C. Whitehouse, R. Kaeppeli, M. Liebendoerfer, Class. Quant. Grav. 27 (2010) 114101, arXiv:0912.1455.

[23-31]

Explosion geometry of a rotating 13 star driven by the SASI-aided neutrino-heating supernova mechanism, Yudai Suwa et al., Publ. Astron. Soc. Jap. 62 (2010) L49-L53, arXiv:0912.1157.

[23-32]

Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling, L. Huedepohl, B. Mueller, H.-Th. Janka, A. Marek, G.G Raffelt, Phys. Rev. Lett. 104 (2010) 251101, arXiv:0912.0260.

[23-33]

Three-Dimensional Simulations of Mixing Instabilities in Supernova Explosions, N.J. Hammer, H.-Th. Janka, E. Mueller, Astrophys. J. 714 (2010) 1371-1385, arXiv:0908.3474.

[23-34]

Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations, Fischer, T., Whitehouse, S. C., Mezzacappa, A., Thielemann, F. -K., Liebendorfer, M., (2009), arXiv:0908.1871.

[23-35]

A Model for Gravitational Wave Emission from Neutrino-Driven Core-Collapse Supernovae, Jeremiah W. Murphy, Christian D. Ott, Adam Burrows, Astrophys. J. 707 (2009) 1173-1190, arXiv:0907.4762.

[23-36]

Stochastic Nature of Gravitational Waves from Supernova Explosions with Standing Accretion Shock Instability, Kei Kotake, Wakana Iwakami, Naofumi Ohnishi, Shoichi Yamada, Astrophys. J. 697 (2009) L133-L136, arXiv:0904.4300.

[23-37]

Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae, Wakana Iwakami, Kei Kotake, Naofumi Ohnishi, Shoichi Yamada, Keisuke Sawada, Astrophys. J. 700 (2009) 232-242, arXiv:0811.0651.

[23-38]

Systematic thermal reduction of neutronization in core-collapse supernovae, A.F. Fantina, P. Donati, P.M. Pizzochero, Phys. Lett. B676 (2009) 140-145, arXiv:0811.0456.

[23-39]

The neutrino signal from protoneutron star accretion and black hole formation, T. Fischer, S.C. Whitehouse, A. Mezzacappa, F.-K. Thielemann, M. Liebendorfer, arXiv:0809.5129, 2008.

[23-40]

Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae, Marek, A., Janka, H. -Th., Mueller, E., arXiv:0808.4136, 2008.

[23-41]

GRB production and SN signatures in slowly rotating collapsars, Diego Lopez-Camara, William H. Lee, Enrico Ramirez-Ruiz, Astrophys. J. 692 (2009) 804-815, arXiv:0808.0462.

[23-42]

Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. II. progenitor dependence, K. Sumiyoshi, S. Yamada, H. Suzuki, arXiv:0808.0384, 2008.

[23-43]

Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism, Murphy, Jeremiah W., Burrows, Adam, arXiv:0805.3345, 2008.

[23-44]

2D Multi-Angle, Multi-Group Neutrino Radiation-Hydrodynamic Simulations of Postbounce Supernova Cores, Christian D. Ott, Adam Burrows, Luc Dessart, Eli Livne, Astrophys. J. 685 (2008) 1069, arXiv:0804.0239.

[23-45]

Relativistic Radiation Magnetohydrodynamics in Dynamical Spacetimes: Numerical Methods and Tests, Brian D. Farris, Tsz Ka Li, Yuk Tung Liu, Stuart L. Shapiro, Phys. Rev. D78 (2008) 024023, arXiv:0802.3210.

[23-46]

Special Relativistic Simulations of Magnetically-dominated Jets in Collapsing Massive Stars, Tomoya Takiwaki, Kei Kotake, Katsuhiko Sato, Astrophys. J. 691 (2009) 1360-1379, arXiv:0712.1949.

[23-47]

Neutrinos from Fallback onto Newly Formed Neutron Stars, Fryer, Chris L., Astrophys. J. 699 (2009) 409-420, arXiv:0711.0551.

[23-48]

Three-Dimensional Simulations of Standing Accretion Shock Instability in Core-Collapse Supernovae, Wakana Iwakami, Kei Kotake, Naofumi Ohnishi, Shoichi Yamada, Keisuke Sawada, arXiv:0710.2191, 2007.

[23-49]

Magnetohydrodynamics of Neutrino-Cooled Accretion Tori around a Rotating Black Hole in General Relativity, M. Shibata, Y. Sekiguchi, R. Takahashi, (2007), arXiv:0709.1766.

[23-50]

Ascertaining the Core Collapse Supernova Mechanism: An Emerging Picture?, A. Mezzacappa, S.W. Bruenn, J.M. Blondin, W.R. Hix, O.E.B. Messer, (2007), arXiv:0709.1484.

[23-51]

Gravitational waves from 3D MHD core collapse simulations, S.Scheidegger, T.Fischer, M.Liebendoerfer, arXiv:0709.0168, 2007.

[23-52]

Delayed neutrino-driven supernova explosions aided by the standing accretion-shock instability, A. Marek, H.-Th. Janka, Astrophys. J. 694 (2009) 664-696, arXiv:0708.3372.

[23-53]

Multi-Dimensional Simulations for Early Phase Spectra of Aspherical Hypernovae: SN 1998bw and Off-Axis Hypernovae, Masaomi Tanaka, Keiichi Maeda, Paolo A. Mazzali, Ken'ichi Nomoto, arXiv:0708.3242, 2007.

[23-54]

Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence, K. Sumiyoshi, S. Yamada, H. Suzuki, Astrophys. J. 667 (2007) 382-394, arXiv:0706.3762.

[23-55]

Numerical Study on Stellar Core Collapse and Neutrino Emission: Probe into the Spherically Symmetric Black Hole Progenitors with 3 - 30Msun Iron Cores, Ken'ichiro Nakazato, Kohsuke Sumiyoshi, Shoichi Yamada, Astrophys. J. 666 (2007) 1140-1151, arXiv:0705.4350.

[23-56]

Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core, L. Scheck, H.-Th. Janka, T. Foglizzo, K. Kifonidis, Astron. Astrophys. 477 (2008) 931, arXiv:0704.3001.

[23-57]

Magnetorotational Collapse of Population III Stars, Yudai Suwa, Tomoya Takiwaki, Kei Kotake, Katsuhiko Sato, Publ. Astron. Soc. Jap. 59 (2007) 771-785, arXiv:0704.1945.

[23-58]

Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation, Adam Burrows et al., Astrophys. J. 664 (2007) 416-434, arXiv:astro-ph/0702539.

[23-59]

Supernova Nucleosynthesis in Population III 13 - 50 Stars and Abundance Patterns of Extremely Metal-Poor Stars, Nozomu Tominaga, Hideyuki Umeda, Ken'ichi Nomoto, Astrophys. J. 660 (2007) 516-540, arXiv:astro-ph/0701381.

[23-60]

Nucleosynthesis-relevant conditions in neutrino-driven supernova outflows. I. Spherically symmetric hydrodynamic simulations, A. Arcones, H.-Th. Janka, L. Scheck, arXiv:astro-ph/0612582, 2006.

[23-61]

Features of the Acoustic Mechanism of Core-Collapse Supernova Explosions, A. Burrows et al., Astrophys. J. 655 (2007) 416-433, arXiv:astro-ph/0610175.

[23-62]

Collapsars in Three Dimensions, Gabriel Rockefeller, Christopher L. Fryer, Hui Li, arXiv:astro-ph/0608028, 2006.

[23-63]

A Numerical Algorithm for Modeling Multigroup Neutrino-Radiation Hydrodynamics in Two Spatial Dimensions, F. Douglas Swesty, Eric S. Myra, arXiv:astro-ph/0607281, 2006.

[23-64]

Multi-Dimensional Simulations of the Accretion-Induced Collapse of White Dwarfs to Neutron Stars, Luc Dessart et al., Astrophys. J. 644 (2006) 1063-1084, arXiv:astro-ph/0601603.

[23-65]

Multidimensional Supernova Simulations with Approximative Neutrino Transport I. Neutron Star Kicks and the Anisotropy of Neutrino-Driven Explosions in Two Spatial Dimensions, L. Scheck, K. Kifonidis, H.-Th. Janka, E. Mueller, arXiv:astro-ph/0601302, 2006.

[23-66]

Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars, Buras, R., Janka, Hans-Thomas, Rampp, M., Kifonidis, K., Astron. Astrophys. 457 (2005) 281-308, arXiv:astro-ph/0512189.

[23-67]

Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae, F.S. Kitaura, H.-Th. Janka, W. Hillebrandt, Astron. Astrophys. 450 (2006) 345-350, arXiv:astro-ph/0512065.

[23-68]

Non-Spherical Core-Collapse Supernovae II. Late-Time Evolution of Globally Anisotropic Neutrino-Driven Explosions and Implications for SN 1987A, K. Kifonidis et al., arXiv:astro-ph/0511369, 2005.

[23-69]

A New Mechanism for Core-Collapse Supernova Explosions, Burrows, Adam, Livne, Eli, Dessart, Luc, Ott, Christian, Murphy, Jeremiah, Astrophys. J. 640 (2006) 878-890, arXiv:astro-ph/0510687.

[23-70]

Gravitational Collapse and Neutrino Emission of Population III Massive Stars, Nakazato, Ken'ichiro, Sumiyoshi, Kohsuke, Yamada, Shoichi, Astrophys. J. 645 (2006) 519-533, arXiv:astro-ph/0509868.

[23-71]

Numerical Analysis on Standing Accretion Shock Instability with Neutrino Heating in the Supernova Cores, Naofumi Ohnishi, Kei Kotake, Shoichi Yamada, Astrophys. J. 641 (2006) 1018-1028, arXiv:astro-ph/0509765.

[23-72]

Neutrino-driven convection versus advection in core collapse supernovae, T. Foglizzo, L. Scheck, H.-Th. Janka, Astrophys. J. 652 (2006) 1436-1450, arXiv:astro-ph/0507636.

[23-73]

Core-Collapse Very Massive Stars: Evolution, Explosion, and Nucleosynthesis of Population III 500 - 1000 Stars, T. Ohkubo et al., Astrophys. J. 645 (2006) 1352-1372, arXiv:astro-ph/0507593.

[23-74]

Two-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 star, Buras, Robert, Rampp, M., Janka, H. -Th., Kifonidis, K., Astron. Astrophys. 447 (2006) 1049-1092, arXiv:astro-ph/0507135.

[23-75]

Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state, K. Sumiyoshi et al., Astrophys. J. 629 (2005) 922, arXiv:astro-ph/0506620.

[23-76]

Core Collapse via Coarse Dynamic Renormalization, Andras Szell, David Merritt, Ioannis G. Kevrekidis, Phys. Rev. Lett. 95 (2005) 081102, arXiv:astro-ph/0504546.

[23-77]

Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations, A. Marek et al., Astron. Astrophys. 445 (2006) 273, arXiv:astro-ph/0502161.

[23-78]

Effects of rotation on the revival of a stalled shock in supernova explosions, T. Yamasaki, S. Yamada, Astrophys. J. 623 (2005) 1000, arXiv:astro-ph/0412625.

[23-79]

Anisotropies in the Neutrino Fluxes and Heating Profiles in Two-dimensional, Time-dependent, Multi-group Radiation Hydrodynamics Simulations of Rotating Core-Collapse Supernovae, R. Walder et al., Astrophys. J. 626 (2005) 317, arXiv:astro-ph/0412187.

[23-80]

Nuclear Input for Core-collapse Models, G. Martinez-Pinedo, M. Liebendoerfer, D. Frekers, Nucl. Phys. A777 (2006) 395-423, arXiv:astro-ph/0412091.

[38-96]

Neutrino Opacities in Nuclear Matter, Adam Burrows, Sanjay Reddy, Todd A. Thompson, Nucl. Phys. A777 (2006) 356-394, arXiv:astro-ph/0404432.

[23-82]

Fluid Stability Below the Neutrinospheres of Supernova Progenitors and the Dominant Role of Lepto-Entropy Fingers, S. W. Bruenn, E. A. Raley, A. Mezzacappa, arXiv:astro-ph/0404099, 2004.

[23-83]

Two-dimensional, Time-dependent, Multi-group, Multi-angle Radiation Hydrodynamics Test Simulation in the Core- Collapse Supernova Context, Livne, Eli, Burrows, Adam, Walder, Rolf, Lichtenstadt, Itamar, Thompson, Todd A., Astrophys. J. 609 (2004) 277, arXiv:astro-ph/0312633.

[23-84]

Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods, M. Liebendoerfer, M. Rampp, H.-Th. Janka, A. Mezzacappa, Astrophys. J. 620 (2005) 840, arXiv:astro-ph/0310662.
From the abstract: Accurate neutrino transport has been built into spherically symmetric simulations of stellar core collapse and postbounce evolution. The results of such simulations agree that spherically symmetric models with standard microphysical input fail to explode by the delayed, neutrino-driven mechanism.

[23-85]

Core-Collapse Supernova Mechanism - Importance of Rotation, A. Odrzywolek, M. Kutschera, M. Misiaszek, K. Grotowski, arXiv:astro-ph/0310047, 2003.

[23-86]

3-Dimensional Core-Collapse, Fryer, Chris L., Warren, Michael S., Astrophys. J. 601 (2004) 391-404, arXiv:astro-ph/0309539.

[23-87]

Pulsar Recoil by Large-Scale Anisotropies in Supernova Explosions, Scheck, L., Plewa, T., Janka, Hans-Thomas, Kifonidis, K., Mueller, E., Phys. Rev. Lett. 92 (2004) 011103, arXiv:astro-ph/0307352.

[23-88]

Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae, M. Limongi, A. Chieffi, Astrophys. J. 592 (2003) 404, arXiv:astro-ph/0304185.

[23-89]

Improved Models of Stellar Core Collapse and Still no Explosions: What is Missing?, R. Buras, M. Rampp, H.-Th. Janka, K. Kifonidis, Phys. Rev. Lett. 90 (2003) 241101, arXiv:astro-ph/0303171.

[23-90]

Electron capture rates on nuclei and implications for stellar core collapse, Langanke, K. et al., Phys. Rev. Lett. 90 (2003) 241102, arXiv:astro-ph/0302459.

[23-91]

Non-spherical Core Collapse Supernovae I. Neutrino-Driven Convection, Rayleigh-Taylor Instabilities, and the Formation and Propagation of Metal Clumps, K. Kifonidis, T. Plewa, H.-Th. Janka, E. Mueller, Astron. Astrophys. 408 (2003) 621, arXiv:astro-ph/0302239.

[23-92]

Shock breakout in core-collapse supernovae and its neutrino signature, Thompson, Todd A., Burrows, Adam, Pinto, Philip A., Astrophys. J. 592 (2003) 434, arXiv:astro-ph/0211194.

[23-93]

Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae, J. M. Blondin, A. Mezzacappa, C. DeMarino, Astrophys. J. 584 (2003) 971, arXiv:astro-ph/0210634.

[23-94]

A finite difference representation of neutrino radiation hydrodynamics for spherically symmetric general relativistic supernova simulations, Liebendoerfer, M. et al., Astrophys. J. Suppl. 150 (2004) 263, arXiv:astro-ph/0207036.

[23-95]

Modeling Core-Collapse Supernovae in Three Dimensions, Fryer, C.L., Warren, M.S., Astrophys. J. 574 (2002) L65-L68, arXiv:astro-ph/0206017.

[23-96]

Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations, M. Rampp, H.-T. Janka, Astron. Astrophys. 396 (2002) 361, arXiv:astro-ph/0203101.

[23-97]

NewtonPlus: Approximate Relativity for Supernova Simulations, Cardall, Christian Y., Mezzacappa, Anthony, Liebendorfer, Matthias, arXiv:astro-ph/0106105, 2001.

[23-98]

Spherical collapse of supermassive stars: neutrino emission and gamma-ray bursts, Felix Linke, Jose A. Font, Hans-Thomas Janka, E. Mueller, Philippos Papadopoulos, arXiv:astro-ph/0103144, 2001.

[23-99]

General Relativistic Effects in the Core Collapse Supernova Mechanism, Bruenn, S. W., De Nisco, K. R., Mezzacappa, A., Astrophys. J. 560 (2001) 326, arXiv:astro-ph/0101400.

[23-100]

Conservative General Relativistic Radiation Hydrodynamics in Spherical Symmetry and Comoving Coordinates, Liebendorfer, Matthias, Mezzacappa, Anthony, Thielemann, Friedrich-Karl, Phys. Rev. D63 (2001) 104003, arXiv:astro-ph/0012201.

[23-101]

Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae, H.-Th. Janka, Astron. Astrophys. 368 (2000) 527-560, arXiv:astro-ph/0008432.

[23-102]

Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport, Liebendorfer, Matthias et al., Phys. Rev. D63 (2001) 103004, arXiv:astro-ph/0006418.
From the article: We investigate the confluence of (i) matter and radiation in a deeper effective gravitational potential, (ii) a GR core hydrodynamic structure that acts as a more intense neutrino source, and (iii) an increased heating efficiency obtained from accurate three-flavor Boltzmann neutrino transport. However, we find that the combination of these ingredients does not result in a supernova explosion. Our model shares this outcome with recent simulations that investigated a subset of these issues (Rampp and Janka [23-103], Mezzacappa and others [23-104], Bruenn and others [23-99]).

[23-103]

Spherically symmetric simulation with Boltzmann neutrino transport of core collapse and post-bounce evolution of a 15 solar mass star, Rampp, Markus, Janka, H. Thomas, Astrophys. J. 539 (2000) L33-L36, arXiv:astro-ph/0005438.

[23-104]

The Simulation of a Spherically Symmetric Supernova of a 13 Solar Mass Star with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism, Mezzacappa, Anthony et al., Phys. Rev. Lett. 86 (2001) 1935-1938, arXiv:astro-ph/0005366.
From the abstract: In this model, a supernova explosion is not obtained.

[23-105]

A new algorithm for supernova neutrino transport and some applications, Burrows, A., Young, T., Pinto, P., Eastman, R., Thompson, T. A., Astrophys. J. 539 (2000) 865-887.

[23-106]

Future detection of supernova neutrino burst and explosion mechanism, Totani, T., Sato, K., Dalhed, H. E., Wilson, J. R., Astrophys. J. 496 (1998) 216-225, arXiv:astro-ph/9710203.
From the abstract: We mainly discuss the detectability of the signatures of the delayed explosion mechanism in the time evolution of the luminosity and spectrum.

[23-107]

An investigation of neutrino-driven convection and the core collapse supernova mechanism using multigroup neutrino transport, Mezzacappa, A. et al., arXiv:astro-ph/9612107, 1996.

[23-108]

On the nature of core collapse supernova explosions, Burrows, Adam, Hayes, John, Fryxell, Bruce A., Astrophys. J. 450 (1995) 830, arXiv:astro-ph/9506061.

[23-109]

Neutrino Emission from Type II Supernovae: The First 100 Milliseconds, E. Myra, A. Burrows, Astrophys. J. 364 (1989) 222.

[23-110]

The Hydrodynamic Behavior of Supernovae Explosions, S. A. Colgate, R. H. White, Astrophys. J. 143 (1966) 626-681.

[24-1]

Exploding SNe with jets: time-scales, Oded Papish, Noam Soker, arXiv:1204.2560, 2012. IAU Symposium No. 279, 2012.

[24-2]

General Relativistic Explosion Models of Core-Collapse Supernovae, Bernhard Mueller, Andreas Marek, Hans-Thomas Janka, Harald Dimmelmeier, arXiv:1112.1920, 2011.

[24-3]

Studies of Stellar Collapse and Black Hole Formation with the Open-Source Code GR1D, Christian D. Ott, Evan O'Connor, AIP Conf. Proc. 1269 (2010) 166-173, arXiv:1011.0005. OMEG10 Symposium, Osaka, Japan, March 8-10, 2010.

[24-4]

Mechanisms of Core-Collapse Supernovae & Simulation Results from the CHIMERA Code, Bruenn, S. W. et al., AIP Conference Proceedings 1111 (2009) 593-601, arXiv:1002.4909. Probing Stellar Populations Out To The Distant Universe: Cefalu 2008.

[24-5]

Computational Models of Stellar Collapse and Core-Collapse Supernovae, C. D. Ott et al., J. Phys. Conf. Ser. 180 (2009) 012022, arXiv:0907.4043. DOE/SciDAC 2009.

[24-6]

Nucleosynthesis Calculations from Core-Collapse Supernovae, Fryer, Christopher L. et al. (The NuGrid), arXiv:0811.4648, 2008. 10th Symposium on Nuclei in the Cosmos (NIC X), July 27 - August 1 2008, Mackinack Island, Michigan, USA.

[24-7]

Supernova explosions and the birth of neutron stars, H.-Th. Janka, A. Marek, B. Mueller, L. Scheck, AIP Conf. Proc. 983 (2008) 369-378, arXiv:0712.3070. 40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More, August 12-17, 2007, McGill Univ., Montreal, Canada.

[24-8]

Nuclear physics with spherically symmetric supernova models, M. Liebendoerfer, T. Fischer, C. Frohlich, F.-K. Thielemann, S. Whitehouse, J. Phys. G35 (2008) 014056, arXiv:0708.4296. NPA III, Dresden 2007.

24-9.

, 2010.

[24-10]

Multi-Dimensional Explorations in Supernova Theory, Adam Burrows, Luc Dessart, Christian D. Ott, Eli Livne, Phys. Rept. 442 (2007) 23-37, arXiv:astro-ph/0612460. Centennial Festschrift for Hans Bethe, 2006.

[24-11]

Collapse and black hole formation in magnetized, differentially rotating neutron stars, Branson C. Stephens et al., Class. Quant. Grav. 24 (2007) S207-S220, arXiv:gr-qc/0610103. New Frontiers in Numerical Relativity, the Albert Einstein Institute, Potsdam, July 17-21, 2006.

[24-12]

Efficient approximations of neutrino physics for three-dimensional simulations of stellar core collapse, M. Liebendoerfer, U.-L. Pen, C. Thompson, PoS NIC-IX (2006) 132, arXiv:astro-ph/0609651. Nuclei in the Cosmos IX, Geneva, June 25-30.

[24-13]

Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae, Kei Kotake, Naofumi Ohnishi, Shoichi Yamada, Katsuhiko Sato, J. Phys. Conf. Ser. 31 (2006) 95, arXiv:astro-ph/0511826. Third 21COE Symposium : Astrophysics as Interdisciplinary Science, Waseda University, Japan, September 1-3, 2005.

[24-14]

Toward Five-dimensional Core-collapse Supernova Simulations, Christian Y. Cardall et al., J. Phys. Conf. Ser. 16 (2005) 390, arXiv:astro-ph/0510706. SciDAC 2005, Scientific Discovery through Advanced Computing, San Francisco, CA, 26-30 June 2005.

[24-15]

The Long Term: Six-dimensional Core-collapse Supernova Models, Christian Y. Cardall, Alexei O. Razoumov, Eirik Endeve, Anthony Mezzacappa, arXiv:astro-ph/0510704, 2005. Open Issues in Understanding Core Collapse Supernovae, National Institute for Nuclear Theory, University of Washington, 22-24 June 2004.

[24-16]

Multigroup Models of the Convective Epoch in Core Collapse Supernovae, F. Douglas Swesty, Eric S. Myra, J. Phys. Conf. Ser. 16 (2005) 380, arXiv:astro-ph/0507294. SciDAC 2005, San Francisco, CA, USA, 26-30 June 2005.

[24-17]

An approach toward the successful supernova explosion by physics of unstable nuclei, K. Sumiyoshi et al., Nucl. Phys. A758 (2005) 63, arXiv:astro-ph/0506619. Nuclei in the Cosmos 8.

[24-18]

Issues with Core-Collapse Supernova Progenitor Models, Stephen W. Bruenn, arXiv:astro-ph/0506313, 2005. Workshop on Open Issues in Understanding Core Collapse Supernovae, Seattle, Washington, 22-24 June 2004.

[24-19]

Magnetic Fields in Core Collapse Supernovae: Possibilities and Gaps, J. Craig Wheeler, Shizuka Akiyama, arXiv:astro-ph/0412382, 2004. INT workshop "Open Issues in Understanding Core Collapse Supernovae," Seattle, 2004.

[24-20]

Neutrino-Driven Supernovae: an Accretion Instability in a Nuclear Physics Controlled Environment, Janka, Hans-Thomas et al., Nucl. Phys. A758 (2005) 19, arXiv:astro-ph/0411347. 8th Symposium on Nuclei in the Cosmos, Vancouver, BC, Canada, 19-23 Jul 2004.

[24-21]

Magnetorotational supernova simulations, S.G. Moiseenko, G.S. Bisnovatyi-Kogan, N.V. Ardeljan, arXiv:astro-ph/0410330, 2004. International Conference "1604-2004 Supernovae as Cosmological Lighthouses" (Padova, Italy, June 16-19, 2004).

[24-22]

The Core Collapse Supernova Mechanism: Current Models, Gaps, and the Road Ahead, Anthony Mezzacappa, arXiv:astro-ph/0410085, 2004. Supernovae as Cosmological Lighthouses, Padua, Italy, June 16-19, 2004.

[24-23]

Early Spectra of Supernovae, E. Baron, Peter Nugent, David Branch, Peter H. Hauschildt, arXiv:astro-ph/0409659, 2004. 1604-2004 Supernovae As Cosmological Lighthouses, San Francisco.

[24-24]

Rotating Core Collapse and Bipolar Supernova Explosions, Burrows, Adam, Walder, Rolf, Ott, Christian D., Livne, Eli, arXiv:astro-ph/0409035, 2004. Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.

[24-25]

Understanding Core-Collapse Supernovae, Adam Burrows, arXiv:astro-ph/0405427, 2004. Twelfth Workshop on "Nuclear Astrophysics," a Tribute to an Explosive Astrophysicist, Wolfgang Hillebrandt, on the occasion of his 60th Birthday, Ringberg Castle, Lake Tegernsee, Germany, March 22 - 27, 2004.

[24-26]

Core-Collapse Supernovae: Modeling between Pragmatism and Perfectionism, H.-Th. Janka et al., arXiv:astro-ph/0405289, 2004. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004.

[24-27]

Fifty-Nine Reasons for a Supernova to not Explode, M. Liebendoerfer, arXiv:astro-ph/0405029, 2004. 12th Workshop on "Nuclear Astrophysics", Ringberg Castle, March 22-27, 2004.

[39-31]

An Approach to Neutrino Radiative Transfer in Supernova Simulations, Christian Y. Cardall, arXiv:astro-ph/0404401, 2004. Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003.

[24-29]

Synthetic Spectrum Methods for Three-Dimensional Supernova Models, R. C. Thomas, arXiv:astro-ph/0310619, 2003. "3-D Signatures in Stellar Explosions", Austin, Texas.

[39-36]

Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions, H. Madokoro, T. Shimizu, Y. Motizuki, arXiv:astro-ph/0310481, 2003. IAU Colloquium 192, SUPERNOVAE (10 years of SN1993J), Valencia, Spain.

[24-31]

Topics in Core-Collapse Supernova Theory, A. Burrows, C. D. Ott, C. Meakin, arXiv:astro-ph/0309684, 2003. 3-D Signatures in Stellar Explosions: A Workshop honoring J. Craig Wheeler's 60th birthday, June 10-13, 2003, Austin, Texas, USA.

[24-32]

The Status of Core-collapse Supernova Simulations, C. Y. Cardall, arXiv:astro-ph/0212438, 2002. 4th International Workshop on the Identification of Dark Matter (IDM2002), York, England 2-6 September 2002.

[24-33]

The Mechanism of Core-Collapse Supernova Explosions: A Status Report, A. Burrows, T. A. Thompson, arXiv:astro-ph/0210212, 2002. ESO/MPA/MPE Workshop (an ESO Astrophysics Symposium) "From Twilight to Highlight: The Physics of Supernovae", Garching bei Munchen, Germany, July 29-31, 2002.

[24-34]

The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models, Liebendorfer, M. et al., arXiv:astro-ph/0203260, 2002. 11th Workshop on Nuclear Astrophysics, Ringberg Caste, Lake Tegernsee, Germany, 11-16 Feb 2002.

[24-35]

Neutrinos from supernovae: experimental status and perspectives, Cei, F., Int. J. Mod. Phys. A17 (2002) 1765-1776, arXiv:hep-ex/0202043. Second International Workshop on Matter, Anti-Matter and Dark Matter, Trento (Italy), 29-30 October 2001.

[24-36]

Toward a Standard Model of Core Collapse Supernovae, Mezzacappa, A., arXiv:astro-ph/0010580, 2000. Nuclei in the Cosmos 2000, University of Aarhus, Aarhus, Denmark, June 27-July 1, 2000.

[25-1]

Anisotropic Thermal Conduction in Supernova Remnants: Relevance to Hot Gas Filling Factors in the Magnetized ISM, David A. Tilley, Dinshaw S. Balsara, Astrophys. J. 645 (2006) L49-L52, arXiv:astro-ph/0604117.

[26-1]

Magneto-rotationally driven Supernovae as the origin of early galaxy r-process elements?, Christian Winteler et al., (2012), arXiv:1203.0616.

[26-2]

Inferring Core-Collapse Supernova Physics with Gravitational Waves, Logue, J., Ott, C.D., Heng, I.S., Kalmus, P., Scargill, J., arXiv:1202.3256, 2012.

[26-3]

The primary cosmic ray spectrum in supernova remnants from very high energy gamma-ray data, F.L. Villante, F. Vissani, Phys. Rev. D76 (2007) 125019, arXiv:0707.0471.

[26-4]

Bayesian Single-Epoch Photometric Classification of Supernovae, Dovi Poznanski, Dan Maoz, Avishay Gal-Yam, Astron. J. 134 (2007) 1285-1297, arXiv:astro-ph/0610129.

[26-5]

A Probabilistic Approach to Classifying Supernovae Using Photometric Information, Natalia V. Kuznetsova, Brian M. Connolly, Astrophys. J. 659 (2007) 530-540, arXiv:astro-ph/0609637.

[26-6]

Remarks on Super-Novae and Cosmic Rays, W. Baade, F. Zwicky, Phys. Rev. 46 (1934) 76-77.

[27-1]

The Supernova Gamma-Ray Burst Connection, Stan Woosley, Alexander Heger, AIP Conf. Proc. 836 (2006) 398-407, arXiv:astro-ph/0604131. AIP Conf. Proc. "Gamma Ray Bursts in the Swift Era".

[28-1]

The Cosmic Core-collapse Supernova Rate does not match the Massive-Star Formation Rate, Shunsaku Horiuchi et al., Astrophys. J. 738 (2011) 154-169, arXiv:1102.1977.

[28-2]

The supernova rate in local galaxy clusters, F. Mannucci et al., Mon. Not. Roy. Astron. Soc. 383 (2008) 1121-1130, arXiv:0710.1094.

[28-3]

On the Rates of Gamma Ray Bursts and Type Ib/c Supernovae, Dafne Guetta, Massimo Della Valle, Astrophys. J. Lett. 657 (2007) L73-L76, arXiv:astro-ph/0612194.

[28-4]

Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate, Keren Sharon et al., Astrophys. J. 660 (2007) 1165-1175, arXiv:astro-ph/0610228.

[28-5]

Cosmic Supernova Rates and the Hubble Sequence, F. Calura, F. Matteucci, Astrophys. J. 652 (2006) 889-901, arXiv:astro-ph/0607674.

[28-6]

A new formulation of the Type Ia SN rate and its consequences on galactic chemical evolution, F. Matteucci et al., Mon. Not. Roy. Astron. Soc. 372 (2006) 265-275, arXiv:astro-ph/0607504.

[28-7]

Rates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies, M. Sullivan et al., Astrophys. J. 648 (2006) 868-883, arXiv:astro-ph/0605455.

[38-77]

The diffuse supernova neutrino flux, star formation rate and SN1987A, Lunardini, Cecilia, Astropart. Phys. 26 (2006) 190-201, arXiv:astro-ph/0509233.

[28-9]

New Estimates of the Solar-Neighborhood Massive-Stars Birthrate and the Galactic Supernova Rate, Reed, B. Cameron, Astronomical J. 130 (2005) 1652-1657, arXiv:astro-ph/0506708.

[38-90]

The concordance cosmic star formation rate: Implications from and for the supernova neutrino and gamma ray backgrounds, Strigari, Louis E., Beacom, John F., Walker, Terry P., Zhang, Pengjie, JCAP 0504 (2005) 017, arXiv:astro-ph/0502150.

[28-11]

The supernova rate per unit mass, Mannucci, Filippo et al., Astron. Astrophys. 433 (2005) 807-814, arXiv:astro-ph/0411450.

[28-12]

Death rate of massive stars at redshift , Cappellaro, Enrico et al., arXiv:astro-ph/0407216, 2004.

[28-13]

High Redshift Supernova Rates, Dahlen, Tomas et al., Astrophys. J. 613 (2004) 189-199, arXiv:astro-ph/0406547.

[28-14]

Formation rates of core collapse SNe and GRBs, Robert G. Izzard, Enrico Ramirez-Ruiz, Christopher A. Tout, Mon. Not. Roy. Astron. Soc. 348 (2004) 1215, arXiv:astro-ph/0311463.

[28-15]

The Type-Ia Supernova Rate in z < 1 Galaxy Clusters: Implications for Progenitors and the Source of Cluster Iron, D. Maoz, A. Gal-Yam, Mon. Not. Roy. Astron. Soc. 347 (2004) 951, arXiv:astro-ph/0309797.

[28-16]

The Redshift Distribution of Type-Ia Supernovae: Constraints on Progenitors and Cosmic Star Formation History, A. Gal-Yam, D. Maoz, Mon. Not. Roy. Astron. Soc. 347 (2004) 942, arXiv:astro-ph/0309796.

[28-17]

The infrared supernova rate in starburst galaxies, F. Mannucci et al., Astron. Astrophys. 401 (2003) 519, arXiv:astro-ph/0302323.

[28-18]

A new determination of supernova rates and a comparison with indicators for galactic star formation, Cappellaro, E., Evans, R., Turatto, M., Astron. Astrophys. 351 (1999) 459-466, arXiv:astro-ph/9904225.

[28-19]

Why are supernovae in our Galaxy so frequent?, Dragicevich, P. M., Blair, D. G., Burman, R. R, Mon. Not. Roy. Astron. Soc. 302 (1999) 693-699.

[28-20]

Constraints from Al Measurements on the Galaxy's Recent Global Star Formation Rate and Core Collapse Supernovae Rate, Timmes, F. X., Diehl, R., Hartmann, D. H., arXiv:astro-ph/9701242, 1997.

[28-21]

The rate of Supernovae from the combined sample of five searches, Cappellaro, E. et al., Astron. Astrophys. 322 (1997) 431-441, arXiv:astro-ph/9611191.

[28-22]

The Galactic supernova rate, Tammann, G. A., Loeffler, W., Schroder, A., Astrophys. J. Suppl. 92 (1994) 487-493.

[28-23]

"Guest stars", sample completeness and the local supernova rate, Strom, R. G., Astron. Astrophys. 288 (1994) L1-L4.

[28-24]

The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity, Cappellaro, E. et al., Astron. Astrophys. 273 (1993) 383, arXiv:astro-ph/9302017.

[28-25]

How rare are supernovae?, van den Bergh, S., Comments on Astrophys. 17 (1993) 125-130.

[28-26]

High rate for Type IC supernovae, Muller, Richard A. et al., Astrophys. J. 384 (1992) L9-L13.

[28-27]

The rate of stellar collapses in the galaxy, Ratnatunga, Kavan U., van den Bergh, Sidney, Astrophys. J. 343 (1989) 713-717.

[29-1]

Supernova Remnants - Part One - Historical Events, Strom, R. G., 1990. NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, Erice, Sicily, Italy, September 5-17, 1988, p. 253.

[29-2]

Supernova statistics and related problems, Tammann, G. A., 1982. Supernovae: a Survey of Current Research, Cambridge, England, June 29-July 10, 1981, p. 371-403.

[30-1]

Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations, Alejandro Ferrero, Brett Altschul, Phys. Rev. D82 (2010) 123002, arXiv:1008.4769.

[30-2]

On variations of the brightness of type Ia supernovae with the age of the host stellar population, Brendan K. Krueger et al., Astrophys. J. 719 (2010) L5-L9, arXiv:1007.0910.

[38-18]

Probing thermonuclear supernova explosions with neutrinos, A. Odrzywolek, T. Plewa, arXiv:1006.0490, 2010.

[30-4]

Comparison of Recent SnIa datasets, J. C. Bueno Sanchez, S. Nesseris, L. Perivolaropoulos, JCAP 0911 (2009) 029, arXiv:0908.2636.

[30-5]

Like vs. Like: Strategy and Improvements in Supernova Cosmology Systematics, Linder, Eric V., Phys. Rev. D79 (2009) 023509, arXiv:0812.0370.

[30-6]

Implications of Two Type Ia Supernova Populations for Cosmological Measurements, Devdeep Sarkar, Alexandre Amblard, Asantha Cooray, Daniel E. Holz, (2008), arXiv:0806.3267.

[30-7]

Luminosity Indicators in the UV Spectra of Type Ia Supernovae, Ryan J. Foley, Alexei V. Filippenko, Saurabh W. Jha, arXiv:0803.1181, 2008.

[30-8]

Determining the Type, Redshift, and Age of a Supernova Spectrum, Stephane Blondin, John L. Tonry, Astrophys. J. 666 (2007) 1024-1047, arXiv:0709.4488.

[30-9]

Evidence for short-lived SN Ia progenitors, Eric Aubourg et al., PoS SUPERNOVA (2007) 017, arXiv:0707.1328.

[30-10]

The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology, Neill, James D., Hudson, Michael J., Conley, Alex, Astrophys. J. 661 (2007) L123, arXiv:0704.1654.

[30-11]

A Model-Independent Photometric Redshift Estimator for Type Ia Supernovae, Yun Wang, Astrophys. J. 654 (2007) L123, arXiv:astro-ph/0609639.

[30-12]

Lightcurves of Type Ia Supernovae from Near the Time of Explosion, Arti Garg et al., Astron. J. 133 (2007) 403-419, arXiv:astro-ph/0608639.

[30-13]

Cosmological Implications of the Second Parameter of Type Ia Supernovae, Philipp Podsiadlowski et al., arXiv:astro-ph/0608324, 2006.

[30-14]

Sensitivity and figures of merit for dark energy supernovae surveys, J.-M. Virey, A. Ealet, arXiv:astro-ph/0607589, 2006.

[30-15]

A possible interrelation between the estimated luminosity distances and internal extinctions of type Ia supernovae, L.G. Balazs et al., Astron. J. 327 (2006) 917, arXiv:astro-ph/0607369.

[30-16]

A New Method to Calibrate the Magnitudes of Type Ia Supernovae at Maximum Light, Jose Luis Prieto, Armin Rest, Nicholas B. Suntzeff, Astrophys. J. 647 (2006) 501-512, arXiv:astro-ph/0603407.

[30-17]

The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects In Dark Energy Surveys from SNe Ia at z>2, Adam G Riess, Mario Livio, Astrophys. J. 648 (2006) 884-889, arXiv:astro-ph/0601319.

[30-18]

Supernova constraints on models of neutrino dark energy, Li, Hong, Feng, Bo, Xia, Jun-Qing, Zhang, Xinmin, Phys. Rev. D73 (2006) 103503, arXiv:astro-ph/0509272.

[30-19]

Light Curves of Microlensed Type Ia Supernovae, Hamed Bagherpour, R. Kantowski, David Branch, Dean Richardson, arXiv:astro-ph/0411622, 2004.

[30-20]

Probing Dark Energy with Supernovae : Bias from the time evolution of the equation of state, J.-M. Virey et al., Phys. Rev. D70 (2004) 043514, arXiv:astro-ph/0403285.

[30-21]

The Cellular Burning Regime in Type Ia Supernova Explosions - II. Flame Propagation into Vortical Fuel, F. K. Roepke, W. Hillebrandt, J. C. Niemeyer, Astron. Astrophys. 421 (2004) 783, arXiv:astro-ph/0312203.

[30-22]

Testing the running of the cosmological constant with Type Ia Supernovae at high z, C. Espana-Bonet, P. Ruiz-Lapuente, I. L. Shapiro, J. Sola, JCAP 0402 (2004) 006, arXiv:hep-ph/0311171.

[30-23]

Could There Be A Hole In Type Ia Supernovae?, D. Kasen, P. Nugent, R. C. Thomas, L. Wang, Astrophys. J. 610 (2004) 876, arXiv:astro-ph/0311009.

[30-24]

Spectroscopic detection of Type Ia Supernovae in the Sloan Digital Sky Survey, D. S. Madgwick, P. Hewett, D. Mortlock, L. Wang, Astrophys. J. 599 (2003) L33, arXiv:astro-ph/0310887.

[30-25]

On Variations in the Peak Luminosity of Type Ia Supernovae, F. X. Timmes, Edward F. Brown, J. W. Truran, Astrophys. J. 590 (2003) L83, arXiv:astro-ph/0305114. 4 pages, 1 figure, to appear in ApJL. Uses emulateapj.cls (included).

[30-26]

Effects of Systematic Uncertainties on the Supernova Determination of Cosmologial Parameters, Alex G. Kim, Eric V. Linder, Ramon Miquel, Nick Mostek, Mon. Not. Roy. Astron. Soc. 347 (2004) 909, arXiv:astro-ph/0304509.

[30-27]

The intrinsic colour dispersion in Type Ia supernovae, S.Nobili, A.Goobar, R.Knop, P.Nugent, Astron. Astrophys. 404 (2003) 901, arXiv:astro-ph/0304240.

[30-28]

Future Type Ia Supernova Data as Tests of Dark Energy from Modified Friedmann Equations, Yun Wang, Katherine Freese, Paolo Gondolo, Matthew Lewis, Astrophys. J. 594 (2003) 25, arXiv:astro-ph/0302064.

[30-29]

A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy, Padmanabhan, T., Choudhury, T. Roy, Mon. Not. Roy. Astron. Soc. 344 (2003) 823, arXiv:astro-ph/0212573.

[30-30]

Current and future supernova constraints on decaying cosmologies, Alcaniz, J. S., Maia, J. M. F., Phys. Rev. D67 (2003) 043502, arXiv:astro-ph/0212510.

[30-31]

The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology, M. Sullivan et al. (Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 340 (2003) 1057, arXiv:astro-ph/0211444.

[30-32]

A Precise distance indicator: Type Ia supernova multicolor light curve shapes, Riess, Adam G., Press, William H., Kirshner, Robert P., Astrophys. J. 473 (1996) 88, arXiv:astro-ph/9604143.

[31-1]

Type Ia supernova diversity: Standardizing the candles, T. M. Davis, J. B. James, B. P. Schmidt, A. G. Kim, AIP Conf. Proc. 924 (2007) 330-335, arXiv:astro-ph/0701904. Cefalu 2006, The multicoloured landscape of compact objects and their explosive origins.

[31-2]

Progenitors of Type Ia Supernovae: Circumstellar Interaction, Rotation, and Steady Hydrogen Burning, Ken'ichi Nomoto et al., Asp Conf. Ser. 342 (2005) 105, arXiv:astro-ph/0603432. 1604-2004: Supernovae as Cosmological Lighthouses.

[32-1]

Evaluating nuclear physics inputs in core-collapse supernova models, Eric J. Lentz, W. Raphael Hix, Mark L. Baird, O. E. Bronson Messer, Anthony Mezzacappa, arXiv:1101.0156, 2011. 5 pages, 2 figures, presented at Nuclei in the Cosmos XI, Heidelberg, Germany.

[32-2]

Black Hole Formation in Failing Core-Collapse Supernovae, Evan O'Connor, Christian D. Ott, Astrophys. J. 730 (2011) 70, arXiv:1010.5550.

[32-3]

mu->e gamma decay versus mu->eee bound and lepton flavor violating processes in supernova, Oleg Lychkovskiy, Mikhail Vysotsky, arXiv:1010.1694, 2010.

[32-4]

Cooling rates of neutron stars and the young neutron star in the Cassiopeia A supernova remnant, Dmitry G. Yakovlev, Wynn C. G. Ho, Peter S. Shternin, Craig O. Heinke, Alexander Y. Potekhin, Mon. Not. Roy. Astron. Soc. 411 (2011) 1977-1988, arXiv:1010.1154.

[32-5]

Statistical description of complex nuclear phases in supernovae and proto-neutron stars, Ad. R. Raduta, F. Gulminelli, Phys. Rev. C82 (2010) 065801, arXiv:1009.2226.

[32-6]

Gravitational Waves from Core Collapse Supernovae, Yakunin, Konstantin N et al., Class. Quant. Grav. 27 (2010) 194005, arXiv:1005.0779.

[32-7]

Gravitational-Wave Signatures in Magnetically-driven Supernova Explosions, Tomoya Takiwaki, Kei Kotake, Astrophys. J. 743 (2011) 30, arXiv:1004.2896.

[32-8]

Impact of Quarks and Pions on Dynamics and Neutrino Signal of Black Hole Formation in Non-rotating Stellar Core Collapse, Ken'ichiro Nakazato, Kohsuke Sumiyoshi, Shoichi Yamada, Astrophys. J. 721 (2010) 1284-1294, arXiv:1001.5084.

[38-24]

The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse, S. Scheidegger, R. Kaeppeli, S. C. Whitehouse, T. Fischer, M. Liebendoerfer, arXiv:1001.1570, 2010.

[38-25]

Detecting the QCD phase transition in the next Galactic supernova neutrino burst, Basudeb Dasgupta et al., Phys. Rev. D81 (2010) 103005, arXiv:0912.2568.

[38-27]

Reconstructing the supernova bounce time with neutrinos in IceCube, Halzen, Francis, Raffelt, Georg G., Phys. Rev. D80 (2009) 087301, arXiv:0908.2317.

[32-12]

Fingerprints of a Local Supernova, Oliver Manuel, Hilton Ratcliffe, arXiv:0905.0684, 2009.

[32-13]

Astrophysical Implications of Equation of State for Hadron-Quark Mixed Phase: Compact Stars and Stellar Collapses, Ken'ichiro Nakazato, Kohsuke Sumiyoshi, Shoichi Yamada, Phys. Rev. D77 (2008) 103006, arXiv:0804.0661.

[38-57]

Neutrino-Induced Gamma-Ray Emission from Supernovae, Yu Lu, Yong-Zhong Qian, Phys. Rev. D76 (2007) 103002, arXiv:0709.0501.

[32-15]

Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field, Troy A. Porter, Igor V. Moskalenko, Andrew W. Strong, Astrophys. J. 648 (2006) L29-L32, arXiv:astro-ph/0607344.

[38-69]

Neutrino signatures of supernova turbulence, Alexander Friedland, Andrei Gruzinov, arXiv:astro-ph/0607244, 2006.

[38-70]

Probing Dark Energy via Neutrino and Supernova Observatories, Lawrence J. Hall, Hitoshi Murayama, Michele Papucci, Gilad Perez, arXiv:hep-ph/0607109, 2006.

[38-71]

Supernova Neutrinos: The Accretion Disk Scenario, G. C. McLaughlin, R. Surman, Phys. Rev. D75 (2007) 023005, arXiv:astro-ph/0605281.

[32-19]

Towards a Cosmological Hubble Diagram for Type II-P Supernovae, Peter Nugent et al., Astrophys. J. 645 (2006) 841-850, arXiv:astro-ph/0603535.

[32-20]

TeV Gamma-Rays from Old Supernova Remnants, Ryo Yamazaki et al., Mon. Not. Roy. Astron. Soc. 371 (2006) 1975-1982, arXiv:astro-ph/0601704.

[32-21]

The supernova rate-velocity dispersion relation in the interstellar medium, Sami Dib, Eric Bell, Andreas Burkert, Astrophys. J. 638 (2006) 797, arXiv:astro-ph/0506339.

[32-22]

Iron Needles in Supernova Remnants?, Gomez, H L, Dunne, L, Eales, S, Gomez, E, Edmunds, M, arXiv:astro-ph/0505557, 2005.

[44-100]

Exploiting the neutronization burst of a galactic supernova, M. Kachelriess et al., Phys. Rev. D71 (2005) 063003, arXiv:astro-ph/0412082.

[32-24]

Extracting clean supernova spectra, S. Blondin, J. R. Walsh, B. Leibundgut, G. Sainton, Astron. Astrophys. 431 (2005) 757, arXiv:astro-ph/0410406.

[32-25]

Type IIP Supernovae as Cosmological Probes: A SEAM Distance to SN 1999em, E. Baron, Peter Nugent, David Branch, Peter H. Hauschildt, Astrophys. J. 616 (2004) L91, arXiv:astro-ph/0410153.

[32-26]

Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae, J. Pruet et al., Astrophys. J. 623 (2005) 325, arXiv:astro-ph/0409446.

[32-27]

The Progenitors of Core-Collapse Supernovae, J. J. Eldridge, C. A. Tout, Mon. Not. Roy. Astron. Soc. 353 (2004) 87, arXiv:astro-ph/0405408.

[32-28]

Viscosity and Rotation in Core-Collapse Supernovae, Todd A. Thompson, Eliot Quataert, Adam Burrows, Astrophys. J. 620 (2005) 861, arXiv:astro-ph/0403224.

[32-29]

Analytic Solutions for the Evolution of Radiative Supernova Remnants, R. Bandiera, O. Petruk, Astron. Astrophys. 419 (2004) 419, arXiv:astro-ph/0402598.

[32-30]

Redshift Accuracy Requirements for Future Supernova and Number Count Surveys, Dragan Huterer, Alex Kim, Lawrence M. Krauss, Tamara Broderick, Astrophys. J. 615 (2004) 595, arXiv:astro-ph/0402002.

[32-31]

The Nearby Supernova Factory, Wood-Vasey, W. M. et al., New Astron. Rev. 48 (2004) 637, arXiv:astro-ph/0401513.

[32-32]

Core-collapse supernovae and gravitational waves, Cardall, Christian Y., Nucl. Phys. Proc. Suppl. 138 (2005) 436, arXiv:astro-ph/0401060.

[32-33]

Asphericity Effects in Supernovae, P. Hoeflich, C. Gerardy, R. Quimby, arXiv:astro-ph/0312587, 2003.

[32-34]

Low-mass supernovae in the early Galactic halo: source of the double r/s-process enriched halo stars?, Albert A. Zijlstra, Mon. Not. Roy. Astron. Soc. 348 (2004) L23, arXiv:astro-ph/0312481.

[32-35]

The consequences of nuclear electron capture in core collapse supernovae, W. R. Hix et al., Phys. Rev. Lett. 91 (2003) 201102, arXiv:astro-ph/0310883.

[32-36]

Towards Gravitational Wave Signals from Realistic Core Collapse Supernova Models, E. Mueller et al., Astrophys. J. 603 (2004) 221, arXiv:astro-ph/0309833.

[32-37]

Theoretical Light Curves of Type II-P SNe and Applications to Cosmology, A. Chieffi et al., Mon. Not. Roy. Astron. Soc. 345 (2003) 111, arXiv:astro-ph/0306629.

[32-38]

Nucleosynthesis in Black-Hole-Forming Supernovae and Abundance Patterns of Extremely Metal-Poor Stars, K. Nomoto et al., Prog. Theor. Phys. Suppl. 151 (2003) 44, arXiv:astro-ph/0306412. 12 pages, 9 figures. To appear in 'Carnegie Observatories Astrophysics Series, Vol. 4: Origin and Evolution of the Elements, 2003, eds. A. McWilliam and M. Rauch (Pasadena: Carnegie Observatories).

[32-39]

Nucleosynthesis of Light Elements and Heavy r-Process Elements through the nu-Process in Supernova Explosion, T. Yoshida, M. Terasawa, T. Kajino, K. Sumiyoshi, Astrophys. J. 600 (2004) 204, arXiv:astro-ph/0305555.

[32-40]

On the relative frequencies of core-collapse supernovae sub-types: the role of progenitor metallicity, Nikos Prantzos, Samuel Boissier, Astron. Astrophys. 406 (2003) 259, arXiv:astro-ph/0305376.

[32-41]

The First Supernova Explosions in the Universe, Volker Bromm, Naoki Yoshida, Lars Hernquist, Astrophys. J. 596 (2003) L135, arXiv:astro-ph/0305333.

[32-42]

Jets and Black Holes in Hypernova Explosions, K. Maeda, K. Nomoto, Prog. Theor. Phys. Suppl. 151 (2003) 211, arXiv:astro-ph/0305183.

[32-43]

A Two-Component Model for the Light Curves of Hypernovae, K. Maeda et al., Astrophys. J. 593 (2003) 931, arXiv:astro-ph/0305182.

[32-44]

Supernovae and Light Neutralinos: SN1987A Bounds on Supersymmetry Revisited, Dreiner, H. K., Hanhart, C., Langenfeld, U., Phillips, D. R., Phys. Rev. D68 (2003) 055004, arXiv:hep-ph/0304289.

[32-45]

Bipolar Supernova Explosions: Nucleosynthesis and Implication on Abundances in Extremely Metal-Poor Stars, K. Maeda, K. Nomoto, Astrophys. J. 598 (2003) 1163, arXiv:astro-ph/0304172.

[32-46]

Light curves and luminosities as indicators of mass in type IIP supernovae, Elmhamdi, A., Chugai, N. N., Danziger, I. J., Astron. Astrophys. 404 (2003) 1077-1086, arXiv:astro-ph/0304144.

[32-47]

Supernova and neutron-star limits on large extra dimensions reexamined, S.Hannestad, G.G.Raffelt, Phys. Rev. D67 (2003) 125008, arXiv:hep-ph/0304029.

[32-48]

Stellar Sources for Heavy r-Process Nuclei, Y.-Z. Qian, G. J. Wasserburg, arXiv:astro-ph/0301461, 2003.

[32-49]

Did Egret Detect Distant Supernova Remnants?, Diego F. Torres et al., Adv. Space Res. 33 (2004) 450, arXiv:astro-ph/0301424.

[32-50]

Gamma-Ray Lines from Asymmetric Supernovae, A. L. Hungerford, C. L. Fryer, M. S. Warren, Astrophys. J. 594 (2003) 390, arXiv:astro-ph/0301120.

[60-4]

How Massive Single Stars End their Life, A. Heger et al., Astrophys. J. 591 (2003) 288, arXiv:astro-ph/0212469.

[32-52]

Asymmetric Explosions of Thermonuclear Supernovae, C. R. Ghezzi, E. M. de Gouveia Dal Pino, J. E. Horvath, Mon. Not. Roy. Astron. Soc. 348 (2004) 451, arXiv:astro-ph/0211605.

[32-53]

Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant, Masamune Oguri, Yozo Kawano, Mon. Not. Roy. Astron. Soc. 338 (2003) L25-L29, arXiv:astro-ph/0211499.

[32-54]

SN1999E: Another piece in the SN-GRB connection puzzle, L. Rigon et al., Mon. Not. Roy. Astron. Soc. 340 (2003) 191, arXiv:astro-ph/0211432.

[32-55]

Massive galaxy clusters as gravitational telescopes for distant supernovae, Christofer Gunnarsson, Ariel Goobar, Astron. Astrophys. 405 (2003) 859, arXiv:astro-ph/0211401.

[32-56]

Ozone Depletion from Nearby Supernovae, Neil Gehrels et al., Astrophys. J. 585 (2003) 1169, arXiv:astro-ph/0211361.

[32-57]

The high energy gamma-ray emission expected from Tycho's supernova remnant, H.J. Voelk, E.G. Berezhko, L.T. Ksenofontov, G.P. Rowell, Astron. Astrophys. 396 (2002) 649, arXiv:astro-ph/0210176.

[32-58]

Peculiar, Low Luminosity Type II Supernovae: Low Energy Explosions in Massive Progenitors?, L. Zampieri et al., Mon. Not. Roy. Astron. Soc. 338 (2003) 711, arXiv:astro-ph/0210171.

[32-59]

Gravitational Lensing Magnification and Time Delay Statistics for Distant Supernovae, Masamune Oguri, Yasushi Suto, Edwin L. Turner, Astrophys. J. 583 (2003) 584, arXiv:astro-ph/0210107.

[32-60]

Photometry and Spectroscopy of the Type IIP SN 1999em from Outburst to Dust Formation, Elmhamdi, A. et al., Mon. Not. Roy. Astron. Soc. 338 (2003) 939-956, arXiv:astro-ph/0209623.

[32-61]

Observed and Physical Properties of Core-Collapse Supernovae, Hamuy, Mario, Astrophys. J. 582 (2003) 905, arXiv:astro-ph/0209174.

[32-62]

Seeing double: strong gravitational lensing of high- redshift supernovae, Holz, Daniel E., Astrophys. J. 556 (2001) L71, arXiv:astro-ph/0104440.

[32-63]

Gravitational collapse of rotating stellar cores and supernovae, Sato, K., Shimizu, T. M., Yamada, S., Nucl. Phys. A606 (1996) 118-136.

[32-64]

Gravitational radiation from rotational collapse of a supernova core, Yamada, S., Sato, K., Astrophys. J. 450 (1995) 245-252.

[32-65]

The absolute magnitudes of Type IA supernovae, Phillips, M. M., Astrophys. J. 413 (1993) L105-L108.

[32-66]

Convective instability in hot bubble in a delayed supernova explosion, Yamada, Shoichi, Shimizu, Tetsuya, Sato, Katsuhiko, Prog. Theor. Phys. 89 (1993) 1175-1182.

[32-67]

Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovae, Nomoto, K., Thielemann, F.K., Yokoi, K., Astrophys. J. 286 (1984) 644-658.

[33-1]

Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star, Men-Quan Liu, Ye-Fei Yuan, arXiv:1005.1845, 2010. Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, Beijing, P. R. China.

[33-2]

Probing the Core-Collapse Supernova Mechanism with Gravitational Waves, C. D. Ott, Class. Quant. Grav. 26 (2009) 204015, arXiv:0905.2797. 13th Gravitational Wave Data Analysis Workshop.

[33-3]

Spectral Modeling of Type II Supernovae, E. Baron, AIP Conf. Proc. 924 (2007) 350-357, arXiv:astro-ph/0611545. The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations.

[33-4]

Time-dependence Effects in Photospheric-Phase Type II Supernova Spectra, Luc Dessart, John Hillier, arXiv:astro-ph/0610136, 2006. The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations, Cefalu, Sicily, June 11-24, 2006.

[33-5]

Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars, Marco Limongi, Alessandro Chieffi, arXiv:astro-ph/0507340, 2005. 6IAU Symp. No. 228 "From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution".

[33-6]

SN/GRB connection: a statistical approach with BATSE and Asiago Catalogues, S. Valenti et al., Nuovo Cim. 28C (2005) 633, arXiv:astro-ph/0505052. 4th workshop on Gamma Ray Bursts in the Afterglow Era, Rome, 2004.

[33-7]

Supernova search at intermediate z. II. Host galaxy morphology, J. Mendez et al., arXiv:astro-ph/0502397, 2005. 1604-2004: Supernovae as Cosmological Lighthouses.

[33-8]

Supernova search at intermediate z. I. Spectroscopic analysis, G. Altavilla et al., arXiv:astro-ph/0502395, 2005. 1604-2004: Supernovae as Cosmological Lighthouses.

[33-9]

Supernova Rates in Galaxy Clusters, Dan Maoz, arXiv:astro-ph/0501492, 2005. 1604-2004: Supernovae as Cosmological Lighthouses.

[33-10]

Searching for Progenitors of Core-Collapse Supernovae, Schuyler D. Van Dyk, arXiv:astro-ph/0501363, 2005. 1604-2004: Supernovae as Cosmological Lighthouses.

[33-11]

IMF variations and their implications for Supernovae numbers, C. Weidner, P. Kroupa, Proc. Sci. BDMH2004 (2004) 063, arXiv:astro-ph/0412114. "Baryons in Dark Matter Halos", Novigrad, Croatia, October 5-9, 2004.

[33-12]

The Evolution of Supernovae in the Winds of Massive Stars, Vikram Dwarkadas, arXiv:astro-ph/0403195, 2004. Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts.

[39-34]

Neutron Star Kicks and Supernova Asymmetry, Dong Lai, arXiv:astro-ph/0312542, 2003. 3D Signatures of Stellar Explosion, a workshop honoring J.C. Wheeler's 60th Birthday.

[33-14]

Low frequency radio and X-ray properties of core-collapse supernovae, A. Ray, P. Chandra, F. Sutaria, S. Bhatnagar, arXiv:astro-ph/0311419, 2003. IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", April 2003, Valencia, Spain.

[33-15]

Expected Changes of Supernovae with Redshift due to Evolution of their Progenitors, I. Dominguez et al., arXiv:astro-ph/0311140, 2003. IAU Colloquium 192, "Supernovae (10 years of 1993J)", Valencia, Spain 22-26 April 2003.

[33-16]

44Ti radioactivity in young supernova remnants: Cas A and SN 1987A, Y. Motizuki, S. Kumagai, New Astron. Rev. 48 (2004) 69, arXiv:astro-ph/0311080. "Astronomy with Radioactivities IV", Seeon, Germany, June 2003.

[33-17]

Supernova Statistics, E. Cappellaro, R. Barbon, M. Turatto, arXiv:astro-ph/0310859, 2003. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.

[33-18]

Type Ia Supernovae: Spectroscopic Surprises, D. Branch, arXiv:astro-ph/0310685, 2003. 3-D Signatures of Stellar Explosions: A Workshop Honoring J. Craig Wheeler's 60th Birthday.

[33-19]

Understanding Type II Supernovae, L. Zampieri, M. Ramina, A. Pastorello, arXiv:astro-ph/0310057, 2003. IAU Colloquium 192, "Supernovae (10 years of 1993J)", Valencia, Spain 22-26 April 2003.

[33-20]

Observational Properties of Type II Plateau Supernovae, A. Pastorello et al., arXiv:astro-ph/0310056, 2003. IAU Colloquium 192, "Supernovae (10 years of 1993J)", Valencia, Spain 22-26 April 2003.

[33-21]

Cosmic rays, stellar evolution, and supernova physics, P. L. Biermann, New Astron. Rev. 48 (2004) 41, arXiv:astro-ph/0309810. "Astronomy With Radioactivities IV - Filling the Sensitivty Gap in MEV Astronomy", Seeon Conference, Bavaria, Germany, May 2003.

[33-22]

mass in type IIP SNe: Light curves and H-alpha luminosities diagnostics, Elmhamdi, Abouazza, Chugai, N. N., Danziger, I. J., arXiv:astro-ph/0309286, 2003. IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.

[33-23]

Supernova Explosions from Accretion Disk Winds, Andrew I. MacFadyen, arXiv:astro-ph/0301425, 2003. "From Twilight to Highlight - The Physics of Supernovae" ESO/MPA/MPE Workshop, Garching July 2002.

[60-3]

Presupernova Evolution of Rotating Massive Stars and the Rotation Rate of Pulsars, A. Heger, S. E. Woosley, N. Langer, H. C. Spruit, arXiv:astro-ph/0301374, 2003. IAU 215 "Stellar Rotation".

[33-25]

Supernovae, Gamma-Ray Bursts, and Stellar Rotation, S. E. Woosley, A. Heger, arXiv:astro-ph/0301373, 2003. IAU 215 "Stellar Rotation".

[33-26]

Circumstellar Interaction Around Supernovae, Roger A. Chevalier, arXiv:astro-ph/0301368, 2003. "From Twilight to Highlight - The Physics of Supernovae" ESO/MPA/MPE Workshop, Garching July 2002.

[33-27]

Observable Effects of Shocks in Compact and Extended Presupernovae, Blinnikov, S. et al., arXiv:astro-ph/0212569, 2002. ESO/MPA/MPE Workshop "From Twilight to Highlight: The Physics of Supernovae", Garching, July 2002.

[33-28]

Light Curves of Type Ia Supernovae as a Probe for an Explosion Model, Sorokina, Elena, Blinnikov, Sergey, arXiv:astro-ph/0212527, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.

[33-29]

The Mechanism of Core-Collapse Supernovae and the Ejection of Heavy Elements, H.-Th. Janka, R. Buras, M. Rampp, Nucl. Phys. A718 (2003) 269, arXiv:astro-ph/0212317. NIC7, Fuji-Yoshida, Japan, July 8-12, 2002.

[33-30]

X-ray emission of young SN Ia remnants as a probe for an explosion model, D.I.Kosenko, E.I.Sorokina, S.I.Blinnikov, P. Lundqvist, arXiv:astro-ph/0212188, 2002. 34th COSPAR Sci. Assembly, Houston, 10-19 october 2002.

[33-31]

Energy exchange inside SN ejecta and light curves of SNe Ia, E.I.Sorokina, S.I.Blinnikov, arXiv:astro-ph/0212187, 2002. 11th Workshop on "Nuclear Astrophysics", Ringberg Castle, Tegernsee, Germany, February 11-16, 2002.

[33-32]

Magnetic Field in Supernovae, Shizuka Akiyama, J. Craig Wheeler, arXiv:astro-ph/0211458, 2002. conference "Core Collapse of Massive Stars".

[33-33]

Variety in Supernovae, Turatto, Massimo, Benetti, Stefano, Cappellaro, Enrico, arXiv:astro-ph/0211219, 2002. ESO / MPA / MPE Workshop: From Twilight to Highlight: The Physics of Supernovae, Garching, Germany, 29-31 June 2002.

[33-34]

Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae, Domingo Garcia-Senz, Eduardo Bravo, Nucl. Phys. A718 (2003) 563, arXiv:astro-ph/0210339. "Nuclei in the Cosmos VII" 2002.

[33-35]

Neutron Stars, Pulsars and Supernova Remnants: concluding remarks, Pacini, F., arXiv:astro-ph/0208563, 2002. Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef.

[33-36]

Core-collapse supernova simulations: Variations of the input physics, M. Rampp, R. Buras, H.-Th. Janka, G. Raffelt, arXiv:astro-ph/0203493, 2002. Proceedings of the 11th Workshop on "Nuclear Astrophysics" held at Ringberg Castle, February 11-16, 2002.