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[SNO:2006dke]
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.
[Immler:2005ym]
Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C,
Stefan Immler et al.,
Astrophys. J. 632 (2005) 283,arXiv:astro-ph/0503678.
[Immler:2005vx]
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.
[Maund:2005nq]
SN Ib 1990I: Clumping and Dust in the Ejecta?,
Abouazza Elmhamdi et al.,
Astron. Astrophys. 426 (2004) 963-977,arXiv:astro-ph/0407145.
[Elmhamdi:2004he]
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.
[Chugai:2004gq]
XMM-Newton observation of Kepler's supernova remnant,
G. Cassam-Chenai et al.,
Astron.Astrophys. (2003),arXiv:astro-ph/0310687.
[Cassam-Chenai:2003lgh]
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.
[Alekseev:2002ji]
Search for supernova relic neutrinos at Super-Kamiokande,
M. Malek et al.(Super-Kamiokande),
Phys. Rev. Lett. 90 (2003) 061101,arXiv:hep-ex/0209028.
[Super-Kamiokande:2002hei]
The Asiago Supernova Catalogue - 10 years after,
R. Barbon, V. Buondi, E. Cappellaro, M. Turatto,
Astron. Astrophys. 139 (1999) 531-536. [Asiago-Supernova-Catalogue-AA139-1999]
Eleven Year Search for Supernovae with the IceCube Neutrino Observatory,
Robert Cross, Alexander Fritz, Spencer Griswold(IceCube),
PoS ICRC2019 (2020) 889,arXiv:1908.07249.
36th International Cosmic Ray Conference (ICRC 2019), Madison, WI, U.S.A. [Cross:2019jpb]
Improved Detection of Supernovae with the IceCube Observatory,
Lutz Kopke(IceCube),
J.Phys.Conf.Ser. 1029 (2018) 012001,arXiv:1704.03823.
8th international symposium on large TPCs for low-energy rare event detection, Paris, Dec. 5-7, 2016. [Kopke:2017req]
The core collapse supernova rate from 24 years of data of the Large Volume Detector,
G. Bruno, A. Molinario, W. Fulgione, C. Vigorito(LVD),
J.Phys.Conf.Ser. 888 (2017) 012256,arXiv:1701.06765.
XXV ECRS 2016. [Bruno:2017oxg]
The IceCube Neutrino Observatory Part V: Neutrino Oscillations and Supernova Searches,
M. G. Aartsen et al.(IceCube),
arXiv:1309.7008, 2013.33nd International Cosmic Ray Conference, Rio de Janeiro 2013. [IceCube:2013lje]
Supernova Detection in IceCube: Status and Future,
Ronald Bruijn(IceCube),
Nucl. Phys.B, Proc.Suppl.237-238 2013 (2013) 94-97,arXiv:1302.2040.
NOW 2012. [Bruijn:2013ibl]
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. [IceCube:2011vzz]
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. [Novoseltseva:2009cr]
Supernova Search with the AMANDA / IceCube Detectors,
Thomas Kowarik, Timo Griesel, Alexander Piegsa(Icecube),
arXiv:0908.0441, 2009.31st ICRC, Lodz, Poland, July 2009. [Kowarik:2009qr]
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. [Lennarz:2009xr]
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. [Stockdale:2007pe]
LVD highlights,
Marco Selvi et al.(LVD),
arXiv:hep-ex/0608061, 2006.Vulcano Workshop 2006 'Frontier Objects in Astrophysics and Particle Physics'. [Selvi:2006bi]
SNLS - the Supernova Legacy Survey,
C.J. Pritchet, SNLS(SNLS),
ASP Conf.Ser. (2004),arXiv:astro-ph/0406242.
Observing Dark Energy (NOAO/Tucson proceedings). [Pritchet:2004af]
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. [Hamuy:2002rz]
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. [Meikle:2002dn]
A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images,
Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko,
Publ.Astron.Soc.Pac. (2002),arXiv:astro-ph/0210347.
PASP (2003 Jan). [VanDyk:2002ry]
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. [Riello:2002hm]
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. [Napiwotzki:2002sa]
Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey,
A. Rest et al.,
Astrophys.J. 795 (2014) 44,arXiv:1310.3828.
[Rest:2013mwz]
Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample,
D. Scolnic et al.,
Astrophys.J. 795 (2014) 45,arXiv:1310.3824.
[Scolnic:2013efb]
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.
[Folatelli:2009nm]
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.
[Motohara:2006tg]
The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey,
A. Conley et al.(SNLS),
Astron. J. 132 (2006) 1707-1713,arXiv:astro-ph/0607363.
[SNLS:2006vah]
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.
[Wang:2005bw]
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ 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 $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations. [SNLS:2005qlf]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications,
A. Clocchiatti et al.(High Z SN Search),
Astrophys. J. 642 (2006) 1-21,arXiv:astro-ph/0510155.
[HighZSNSearch:2005xhg]
Spectroscopy of twelve Type Ia supernovae at intermediate redshift,
C. Balland et al.,
Astron.Astrophys. (2005),arXiv:astro-ph/0507703.
[Balland:2005rw]
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.
[Willott:2005zr]
Evidence for Spectropolarimetric Diversity in Type Ia Supernovae,
Douglas C. Leonard et al.,
Astrophys. J. 632 (2005) 450,arXiv:astro-ph/0506470.
[Leonard:2005td]
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.
[Foley:2005qu]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$,
Serena Nobili et al.(Supernova Cosmology Project),
Astron.Astrophys. (2005),arXiv:astro-ph/0504139.
[SupernovaCosmologyProject:2005zcy]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant,
Adam G. Riess et al.,
Astrophys. J. 627 (2005) 579,arXiv:astro-ph/0503159. From the abstract:$H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$. [Riess:2005zi]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey,
Louis-Gregory Strolger, Adam G. Riess,
Astron. J. 131 (2006) 1629-1638,arXiv:astro-ph/0503093.
[Strolger:2005uk]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT,
C. Lidman et al.(Supernova Cosmology Project),
Astron.Astrophys. (2004),arXiv:astro-ph/0410506.
[SupernovaCosmologyProject:2004akn]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models,
L. G. Strolger et al.,
Astrophys. J. 613 (2004) 200-223,arXiv:astro-ph/0406546.
[Strolger:2004kk]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa,
Gabriele Garavini et al.(The Supernova Cosmology Project),
Mon. Not. Roy. Astron. Soc. 356 (2004) 456,arXiv:astro-ph/0404393.
[SupernovaCosmologyProject:2004yms]
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 $z=0.46 \pm 0.13$. The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), 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 $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$. ... Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy. [Ivanov:2004qa]
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$,
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 $z\geq0.7$, 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 [Go]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation. [Barris:2003dq]
New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST,
Robert A. Knop et al.(The Supernova Cosmology Project),
Astrophys. J. 598 (2003) 102,arXiv:astro-ph/0309368. From the abstract:We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ 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 $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$. [SupernovaCosmologyProject:2003dcn]
Cosmological Results from High-z Supernovae,
John L. Tonry et al.(Supernova Search Team),
Astrophys. J. 594 (2003) 1,arXiv:astro-ph/0305008. From the abstract:The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. 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 $ z\approx 1$, 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 $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence. [SupernovaSearchTeam:2003cyd]
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.
[Li:2003wja]
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el,
Kevin Krisciunas et al.,
Astron. J. 125 (2003) 166,arXiv:astro-ph/0210327.
[Krisciunas:2002rc]
The distant Type Ia supernova rate,
R. Pain et al.(Supernova Cosmology Project),
Astrophys. J. 577 (2002) 120,arXiv:astro-ph/0205476.
[SupernovaCosmologyProject:2002nuh]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 560 (2001) 49-71,arXiv:astro-ph/0104455.
[SupernovaSearchTeam:2001qse]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter 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 $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology. [SupernovaCosmologyProject:1998vns]
Supernova Limits on the Cosmic Equation of State,
Peter M. Garnavich et al.(Supernova Search Team),
Astrophys. J. 509 (1998) 74-79,arXiv:astro-ph/9806396.
[SupernovaSearchTeam:1998cav]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,
Adam G. Riess et al.(Supernova Search Team),
Astron. J. 116 (1998) 1009-1038,arXiv:astro-ph/9805201.
[SupernovaSearchTeam:1998fmf]
Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants,
C. Badenes et al.,
Mem.Soc.Ast.It. (2005),arXiv:astro-ph/0506576.
"Stellar end products" workshop, 13-15 April 2005, Granada, Spain. [Badenes:2005kx]
Additional evidence for a pulsar wind nebula in the heart of SN 1987A from multi-epoch X-ray data and MHD modeling,
Emanuele Greco et al.,
Astrophys.J. 931 (2022) 132,arXiv:2204.06804.
[Greco:2022cto]
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.
[Koo:2006sr]
A 3D view of molecular hydrogen in Supernova 1987A,
J.Larsson, J. Spyromilio, C. Fransson, R. Indebetouw, M. Matsuura, F. J. Abellan, P. Cigan, H. Gomez, B. Leibundgut,
Astrophys.J. 873 (2019) 15,arXiv:1901.11235.
[Larsson:2019uwm]
Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
Astron.Astrophys. 492 (2008) 481,arXiv:0810.2661.
[Groeningsson:2008nc]
Chandra HETG Spectra of SN 1987A at 20 years,
D. Dewey, S. A. Zhekov, R. McCray, C. R. Canizares,
Astrophys.J. 676 (2008) L131,arXiv:0802.2340.
[Dewey:2008gy]
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.
[Smith:2006es]
On the Progenitor of Supernova 1987A,
M. Parthasarathy, David Branch, E. Baron, David J. Jeffery,
Bull.Astron.Soc.India (2006),arXiv:astro-ph/0611033.
[Parthasarathy:2006jr]
Evolutionary Status of SNR 1987A at the Age of Eighteen,
Sangwook Park et al.,
Astrophys. J. 646 (2006) 1001-1008,arXiv:astro-ph/0604201.
[Park:2006tg]
Coronal emission from the shocked circumstellar ring of SN 1987A,
Per Groningsson et al.,
Astron.Astrophys. (2006),arXiv:astro-ph/0603815.
[Groningsson:2006cb]
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.
[Bouchet:2006ff]
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.
[Park:2005qj]
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.
[Manchester:2005ti]
Chandra Observations of Shock Kinematics in Supernova Remnant 1987A,
S.A. Zhekov et al.,
Astrophys. J. 628 (2005) L127,arXiv:astro-ph/0506443.
[Zhekov:2005ni]
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.
[Graves:2005xy]
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.
[Sugerman:2005dk]
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.
[Park:2005ic]
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.
[Shtykovskiy:2004uj]
Young Stellar Populations Around SN1987A,
Nino Panagia, Martino Romaniello, Salvatore Scuderi, Robert P. Kirshner,
Astrophys. J. 539 (2000) 197-208,arXiv:astro-ph/0001476.
[Panagia:2000ga]
A Second Bright Source Detected Near SN1987A,
Peter Nisenson, Costas Papaliolios,
Astrophys.J. 518 (1999) L29,arXiv:astro-ph/9904109.
[Nisenson:1999qd]
The X-ray lightcurve of SN 1987A,
G. Hasinger, B. Aschenbach, J. Trumper,
Astron. Astrophys. 312 (1996) L9-L12,arXiv:astro-ph/9606149.
[Hasinger:1996rj]
Ultraviolet observations of SN 1987A,
Robert P. Kirshner, George Sonneborn, D. Michael Crenshaw, George E. Nassiopoulos,
Astrophys. J. 320 (1987) 602-608. [Kirshner-ApJ320-1987]
The progenitor of SN 1987A - Spatially resolved ultraviolet spectroscopy of the supernova field,
George Sonneborn, Bruce Altner, Robert P. Kirshner,
Astrophys. J. 323 (1987) L35-L39. [Kirshner-ApJ323-1987]
SN1987A: Revisiting the Data and the Correlation between Neutrino and Gravitational Detectors,
P. Galeotti, G. V. Pallottino, G. Pizzella,
Italian Phys.Soc.Proc. 98 (2009) 233-242,arXiv:0810.3759.
Vulcano Wokshop 2008, Frontier Objects in Astrophysics and Particle Physics, May 26-31. [Galeotti:2008wc]
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. [Park:2007nr]
Supernova Remnant 1987A: High Resolution Images and Spectrum from Chandra Observations,
Sangwook Park et al.,
ESA Spec.Publ. 604 (2006) 335,arXiv:astro-ph/0511355.
The X-Ray Universe 2005, Sept 26-30, 2005, El Escorial, Madrid, Spain. [Park:2005vu]
A 2.14 ms Candidate Optical Pulsar in SN1987A,
J. Middleditch 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. [Middleditch:2000it]
DETECTION OF THE NEUTRINO SIGNAL FROM SN1987A IN THE LMC USING THE INR BAKSAN UNDERGROUND SCINTILLATION TELESCOPE,
E. N. Alekseev, L. N. Alekseeva, I. V. Krivosheina, V. I. Volchenko,
Phys. Lett. B205 (1988) 209-214. [Alekseev:1988gp]
POSSIBLE DETECTION OF A NEUTRINO SIGNAL ON 23 FEBRUARY 1987 AT THE BAKSAN UNDERGROUND SCINTILLATION TELESCOPE OF THE INSTITUTE OF NUCLEAR RESEARCH,
E. N. Alekseev, L. N. Alekseeva, V. I. Volchenko, I. V. Krivosheina,
JETP Lett. 45 (1987) 589-592.[Pisma Zh. Eksp. Teor. Fiz. 45, 461-464 (1987)]. [Alekseev:1987ej]
CHARACTERISTICS OF THE NEUTRINO EMISSION FROM SUPERNOVA SN1987A,
A. E. Chudakov, Ya. S. Elensky, S. P. Mikheev,
JETP Lett. 46 (1987) 373-377.[Pisma Zh. Eksp. Teor. Fiz. 46, 297 (1987)]. [Chudakov:1987my]
OBSERVATION OF A NEUTRINO BURST IN COINCIDENCE WITH SUPERNOVA SN1987A IN THE LARGE MAGELLANIC CLOUD,
R. M. Bionta et al.(IMB),
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Supernova Neutrino Scattering off Gadolinium Even Isotopes in Water Cherenkov Detectors,
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JCAP 1809 (2018) 029,arXiv:1808.01677.
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Constraints on differential Shapiro delay between neutrinos and photons from IceCube-170922A,
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Eur.Phys.J. C79 (2019) 185,arXiv:1807.05201.
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On Possibility of Determining Neutrino Mass Hierarchy by the Charged-Current and Neutral-Current Events of Supernova Neutrinos in Scintillation Detectors,
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Eur.Phys.J. C79 (2019) 131,arXiv:1807.05170.
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High-Energy Emission from Interacting Supernovae: New Constraints on Cosmic-Ray Acceleration in Dense Circumstellar Environments,
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Astrophys.J. 874 (2019) 80,arXiv:1807.01460.
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JUNO Sensitivity to Resonant Absorption of Galactic Supernova Neutrinos by Dark Matter,
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Sensitivity of the PICO-500 Bubble Chamber to Supernova Neutrinos Through Coherent Nuclear Elastic Scattering,
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Astropart.Phys. 105 (2019) 25-30,arXiv:1806.01417.
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The $\nu$ process in the light of an improved understanding of supernova neutrino spectra,
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Astrophys.J. 865 (2018) 143,arXiv:1805.10231.
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Astrophys.J. 866 (2018) 105,arXiv:1804.03947.
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Measuring the supernova unknowns at the next-generation neutrino telescopes through the diffuse neutrino background,
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JCAP 1805 (2018) 066,arXiv:1804.03157.
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Neutrino Signals of Core-Collapse Supernovae in Underground Detectors,
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Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background,
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JCAP 1806 (2018) 019,arXiv:1803.04541.
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Neutrino flavor transformation in supernova as a probe for nonstandard neutrino-scalar interactions,
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Phys.Rev. D97 (2018) 103018,arXiv:1803.04504.
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Survey of astrophysical conditions in neutrino-driven supernova ejecta nucleosynthesis,
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Astrophys.J. 855 (2018) 135,arXiv:1802.00737.
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Neutrino-nucleon scattering in the neutrino-sphere,
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Phys.Rev. C98 (2018) 015802,arXiv:1801.07077.
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The gravitational wave signal from core-collapse supernovae,
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Astrophys.J. 861 (2018) 10,arXiv:1801.01914.
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What can we learn on supernova neutrino spectra with water Cherenkov detectors?,
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JCAP 1804 (2018) 040,arXiv:1712.05584.
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JCAP 1809 (2018) 002,arXiv:1712.03836.
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Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements,
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Astrophys.J. 856 (2018) 35,arXiv:1712.00021.
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Intermediate-Mass-Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions,
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Astrophys.J. 856 (2018) 18,arXiv:1710.10372.
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A physical model of mass ejection in failed supernovae,
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On the Possibility to Determine Neutrino Mass Hierarchy via Supernova Neutrinos with Short-Time Characteristics,
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Chin.Phys. C43 (2019) 095102,arXiv:1709.09453.
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Measuring the Progenitor Mass and Dense Circumstellar Material of Type II Supernovae,
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Astrophys.J. 858 (2018) 15,arXiv:1709.04928.
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Neutrinos from beta processes in a presupernova: probing the isotopic evolution of a massive star,
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Astrophys.J. 851 (2017) 6,arXiv:1709.01877.
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Astrophys.J. 851 (2017) 95,arXiv:1708.08356.
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Measuring the neutron star compactness and binding energy with supernova neutrinos,
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JCAP 1711 (2017) 036,arXiv:1708.00760.
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The Neutrino Signal From Pair Instability Supernovae,
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JCAP 1801 (2018) 025,arXiv:1706.02175.
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JCAP 1711 (2017) 031,arXiv:1705.02122.
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Neutrino intensity interferometry: Measuring proto-neutron star radii during core-collapse supernovae,
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The Nickel Mass Distribution of Normal Type II Supernovae,
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Pre-supernova neutrino emissions from ONe cores in the progenitors of core-collapse supernovae: are they distinguishable from those of Fe cores?,
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Neutrino Nucleosynthesis of radioactive nuclei in supernovae,
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Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos,
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The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields,
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Astrophys.J. 801 (2015) 90,arXiv:1409.0540.
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Study of Gamow-Teller transitions in isotopes of titanium within the quasi particle random phase approximation,
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Astrophys.Space Sci. 352 (2014) 645-663,arXiv:1408.4886.
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How many nucleosynthesis processes exist at low metallicity?,
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Inverse Prob. 30 (2014) 114008,arXiv:1407.7549.
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Resolving neutrino mass hierarchy from supernova (anti)neutrino-nucleus reactions,
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Supernova Relic Neutrinos and the Supernova Rate Problem: Analysis of Uncertainties and Detectability of ONeMg and Failed Supernovae,
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Spectrum of Supernova Neutrinos in Ultra-pure Scintillators,
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JCAP 1407 (2014) 051,arXiv:1402.6953.
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J. Phys. G41 (2014) 044005,arXiv:1312.0434.
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Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves,
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Mon.Not.Roy.Astron.Soc. 441 (2014) 733,arXiv:1308.4710.
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Observing the Next Galactic Supernova,
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Natal Kicks of Stellar-Mass Black Holes by Asymmetric Mass Ejection in Fallback Supernovae,
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Mon.Not.Roy.Astron.Soc. 434 (2013) 1355,arXiv:1306.0007.
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RAA 13 (2013) 1063-1074,arXiv:1305.1755.
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Revisiting the Triangulation Method for Pointing to Supernova and Failed Supernova with Neutrinos,
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Could a reported 2007 analysis of Super-Kamiokande data have missed a detectable supernova signal from Andromeda?,
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Tomography of Massive Stars from Core Collapse to Supernova Shock Breakout,
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Probing the Structure of Jet Driven Core-Collapse Supernova and Long Gamma Ray Burst Progenitors with High Energy Neutrinos,
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Probing Dark Energy via Neutrino and Supernova Observatories,
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On the relative frequencies of core-collapse supernovae sub-types: the role of progenitor metallicity,
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The First Supernova Explosions in the Universe,
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Detecting the Neutrino Mass Hierarchy with a Supernova at IceCube,
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JCAP 0306 (2003) 005,arXiv:hep-ph/0303210.
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Astrophys. J. 592 (2003) 1035,arXiv:astro-ph/0302015.
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Effects of the Sound Speed of Quintessence on the Microwave Background and Large Scale Structure,
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Phys. Rev. D67 (2003) 103509,arXiv:astro-ph/0301284.
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Astrophys. J. 594 (2003) 390,arXiv:astro-ph/0301120.
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Astropart. Phys. 20 (2003) 189,arXiv:astro-ph/0212195.
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Asymmetric Explosions of Thermonuclear Supernovae,
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Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant,
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SN1999E: Another piece in the SN-GRB connection puzzle,
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Mirror model for sterile neutrinos,
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The high energy gamma-ray emission expected from Tycho's supernova remnant,
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Peculiar, Low Luminosity Type II Supernovae: Low Energy Explosions in Massive Progenitors?,
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What Can Be Learned with a Lead-Based Supernova-Neutrino Detector?,
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Bulk neutrinos and core collapse supernovae,
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Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background,
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Tomography of the Earth's Core Using Supernova Neutrinos,
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Astropart. Phys. 19 (2003) 755,arXiv:hep-ph/0207238.
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Neutrino oscillation mechanism for pulsar kicks revisited,
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Spectrum of the Supernova Relic Neutrino Background and Evolution of Galaxies,
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Lepton flavor violating New Physics and supernova explosion,
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Neutrinos in Extra Dimensions and Supernovae,
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Supernova neutrinos, LSND and MiniBooNE,
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Phys. Rev. D79 (2009) 025011,arXiv:0901.1069.
[Haghighat:2009pv]
Improved analysis of SN1987A antineutrino events,
G. Pagliaroli, F. Vissani, M.L. Costantini, A. Ianni,
Astropart.Phys. 31 (2009) 163-176,arXiv:0810.0466.
[Pagliaroli:2008ur]
How much can we learn from SN1987A events? Or: An analysis with a two-Component model for the antineutrino signal,
F. Vissani, G. Pagliaroli,
arXiv:0807.1301, 2008. [Vissani:2008ac]
Bounds on large extra dimensions from photon fusion process in SN1987A,
V. H. Satheeshkumar, P. K. Suresh,
JCAP 0806 (2008) 011,arXiv:0805.3429.
[Satheeshkumar:2008fb]
SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels,
Leonard S. Kisslinger, Sandip Pakvasa,
arXiv:0802.1689, 2008. [Kisslinger:2008rx]
Statistical analysis of neutrino events from SN1987A neutrino burst: estimation of the electron antineutrino mass,
B. I. Goryachev,
arXiv:0709.4627, 2007. [Goryachev:2007xg]
Unparticle constraints from SN1987A,
Steen Hannestad, Georg Raffelt, Yvonne Y. Y. Wong,
Phys. Rev. D76 (2007) 121701,arXiv:0708.1404.
[Hannestad:2007ys]
Supernovae as Probes of Extra Dimensions,
V. H. Satheesh Kumar, P. K. Suresh, P. K. Das,
AIP Conf. Proc. 939 (2007) 258-262,arXiv:0706.3551.
[SatheeshKumar:2007gb]
High resolution spectroscopy of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
Astron.Astrophys. (2007),arXiv:astro-ph/0703788.
[Groeningsson:2007nh]
Neutrino Spectrum from SN 1987A and from Cosmic Supernovae,
Hasan Yuksel, John F. Beacom,
Phys. Rev. D76 (2007) 083007,arXiv:astro-ph/0702613.
[Yuksel:2007mn]
Magnetic field in supernova remnant SN 1987A,
E.G. Berezhko, L.T. Ksenofontov,
Astrophys. J. 650 (2006) L59-L62,arXiv:astro-ph/0608586.
[Berezhko:2006vv]
Is there a problem with low energy SN1987A neutrinos?,
Maria Laura Costantini, Aldo Ianni, Giulia Pagliaroli, Francesco Vissani,
JCAP 0705 (2007) 014,arXiv:astro-ph/0608399.
[Costantini:2006xd]
Constraints on neutrino mixing angle $\theta_{13}$ and Supernova neutrino fluxes from the LSD neutrino signal from SN1987A,
Oleg Lychkovskiy,
arXiv:hep-ph/0604113, 2006. [Lychkovskiy:2006yw]
Lower neutrino mass bound from SN1987A data and quantum geometry,
G. Lambiase, G. Papini, R. Punzi, G. Scarpetta,
Class. Quant. Grav. 23 (2006) 1347-1358,arXiv:gr-qc/0512154.
[Lambiase:2005ui]
New analysis of the SN 1987A neutrinos with a flexible spectral shape,
Alessandro Mirizzi, Georg G. Raffelt,
Phys. Rev. D72 (2005) 063001,arXiv:astro-ph/0508612.
[Mirizzi:2005tg]
The Three-Dimensional Circumstellar Environment of SN 1987A,
Ben E. K. Sugerman et al.,
Astrophys. J. Suppl. 159 (2005) 60-99,arXiv:astro-ph/0502378.
[Sugerman:2005dr]
The Light Curve of Supernova 1987A: The Structure of the Presupernova and Radioactive Nickel Mixing,
V. P. Utrobin,
Astron. Lett. 30 (2004) 293,arXiv:astro-ph/0406410.
[Utrobin:2004rt]
SN1987A and the properties of neutrino burst,
Maria Laura Costantini, Aldo Ianni, Francesco Vissani,
Phys. Rev. D70 (2004) 043006,arXiv:astro-ph/0403436.
[Costantini:2004ry]
Neutrinos from SN1987A: flavor conversion and interpretation of results,
C. Lunardini, A. Yu. Smirnov,
Astropart. Phys. 21 (2004) 703,arXiv:hep-ph/0402128.
[Lunardini:2004bj]
A Rotating Collapsar and Possible Interpretation of the LSD Neutrino Signal from SN 1987A,
V.S. Imshennik, O.G. Ryazhskaya,
Astron. Lett. 30 (2004) 14,arXiv:astro-ph/0401613.
[Imshennik:2004iya]
Supernova 1987A did not test the neutrino mass hierarchy,
V. Barger, D. Marfatia, B. P. Wood,
Phys. Lett. B532 (2002) 19-28,arXiv:hep-ph/0202158.
[Barger:2002px]
SN1987A and the status of oscillation solutions to the solar neutrino problem,
M. Kachelriess, A. Strumia, R. Tomas, J. W. F. Valle,
Phys. Rev. D65 (2002) 073016,arXiv:hep-ph/0108100.
[Kachelriess:2001sg]
Bayesian analysis of neutrinos observed from supernova SN 1987A,
Thomas J. Loredo, Don Q. Lamb,
Phys. Rev. D65 (2002) 063002,arXiv:astro-ph/0107260. From the abstract:We present a Bayesian analysis of the energies and arrival times of the neutrinos from supernova SN 1987A detected by the Kamiokande II, IMB, and Baksan detectors, and find strong evidence for two components in the neutrino signal: a long time scale component from thermal Kelvin-Helmholtz cooling of the nascent neutron star, and a brief ($\sim 1$ s), softer component similar to that expected from emission by accreting material in the delayed supernova scenario. In the context of this model, we show that the data constrain the electron antineutrino rest mass to be less than 5.7~eV with 95% probability. [Loredo:2001rx]
Neutrinos from SN1987A, Earth matter effects and the LMA solution of the solar neutrino problem,
C. Lunardini, A. Yu. Smirnov,
Phys. Rev. D63 (2001) 073009,arXiv:hep-ph/0009356.
[Lunardini:2000sw]
SN1987A: A testing ground for the KARMEN anomaly,
I. Goldman, R. Mohapatra, S. Nussinov,
Phys. Lett. B481 (2000) 151-159,arXiv:hep-ph/9912465.
[Goldman:1999hg]
Contact interactions involving right-handed neutrinos and SN 1987A,
J. A. Grifols, E. Masso, R. Toldra,
Phys. Rev. D57 (1998) 2005-2008,arXiv:hep-ph/9707531.
[Grifols:1997iy]
Gamma rays from SN1987A due to pseudoscalar conversion,
J. A. Grifols, E. Masso, R. Toldra,
Phys. Rev. Lett. 77 (1996) 2372-2375,arXiv:astro-ph/9606028.
[Grifols:1996id]
Gamma-rays and the decay of neutrinos from SN1987A,
Andrew H. Jaffe, Michael S. Turner,
Phys. Rev. D55 (1997) 7951-7959,arXiv:astro-ph/9601104.
[Jaffe:1995sw]
Constraints to the decays of Dirac neutrinos from SN1987A,
Scott Dodelson, Joshua A. Frieman, Michael S. Turner,
Phys. Rev. Lett. 68 (1992) 2572-2575. [Dodelson:1992tv]
comment on 'constraints on the majoron interactions from the supernova SN1987A.',
Y. Aharonov, F. T. Avignone, S. Nussinov,
Phys. Rev. D39 (1989) 985. [Aharonov:1989ik]