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The Origin of the Heavy Elements: Recent Progress in the Understanding of the r-Process,
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A Primer on Eulerian Computational Fluid Dynamics for Astrophysics,
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Theoretical Modelling of Early Massive Black Holes,
Marta Volonteri,
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Measures of luminous and dark matter in galaxies across time,
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Pulsations in binary stars - a short review,
Simon J. Murphy,
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Unveiling the quasar main sequence: illuminating the complexity of active galactic nuclei and their evolution,
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Venus Phosphine: Updates and lessons learned,
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Characterizing Exoplanetary Atmospheres: New Views on Exoplanet Composition and Chemistry,
Jonathan J. Fortney,
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Galaxy groups as the ultimate probe of AGN feedback,
Dominique Eckert, Fabio Gastaldello, Ewan O'Sullivan, Alexis Finoguenov, Marisa Brienza(X-GAP),
Galaxies 12 (2024) 24,arXiv:2403.17145.
AGN on the beach, Tropea, Italy, 10-15 September 2023. [Eckert:2024ryi]
The Cepheid Extragalactic Distance Scale: Past, Present and Future,
Wendy L. Freedman, Barry F. Madore,
IAU Symp. 376 (2022) 1-14,arXiv:2308.02474.
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Analyzing Astronomical Data with Machine Learning Techniques,
Mohammad H. Zhoolideh Haghighi,
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Introduction of Machine Learning for Astronomy (Hands-on Workshop),
Yu Wang, Rahim Moradi, Mohammad H. Zhoolideh Haghighi, Fatemeh Rastegarnia,
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Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map,
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EPJ Quant.Technol. 9 (2022) 30,arXiv:2201.07789.
Community Workshop on Cold Atoms in Space and corresponding Road-map. [Alonso:2022oot]
Main ways in which stars influence the climate and surface habitability of their planets,
Martin Turbet, Franck Selsis,
arXiv:2104.06391, 2021.Evry Schatzman School 2019 'Interactions star-planet'. [2104.06391]
Selected Chapters on Active Galactic Nuclei as Relativistic Systems,
Vladimir Karas, Jiri Svoboda, Michal Zajacek,
arXiv:1901.06507, 2019.Summer School on Relativistic Accretion: Theoretical Models and Their Application to Observations (ZARM, Bremen, 26-30 September 2016). [Karas:2019lju]
Current State of Astrophysical Opacities: A White Paper,
A.E. Lynas-Gray et al.,
ASP Conf.Ser. 515 (2018) 301,arXiv:1804.06804.
Second Workshop on Astrophysical Opacities, Kalamazoo, Michigan, USA: 2017 August 1st - 4th. [Lynas-Gray:2018eru]
Theory of Stellar Oscillations,
Margarida S. Cunha,
arXiv:1711.01236, 2017.IVth Azores International Advanced School in Space Sciences on 'Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds', Horta, Azores Islands, Portugal, July 2016. [1711.01236]
Radio Pulsars: The Neutron Star Population $\text{\&}$ Fundamental Physics,
Victoria M. Kaspi, Michael Kramer,
arXiv:1602.07738, 2016.26th Solvay Conference on Physics on Astrophysics and Cosmology. [Kaspi:2016jkv]
Ground-based Observations of the Solar Sources of Space Weather (Invited Review),
Astrid M. Veronig, Werner Potzi,
arXiv:1602.02721, 2016.Coimbra Solar Physics Meeting 2015. [1602.02721]
The Kinematics of Star Formation: Theory and Observation in the Gaia Era,
Nicholas J. Wright,
arXiv:1512.06854, 2015.RAS Specialist Discussion meeting, January 2015. [1512.06854]
From Interstellar Clouds to Stars,
Jonathan C. Tan,
arXiv:1512.00920, 2015.6th Zermatt ISM Symposium: Conditions and Impact of Star Formation From Lab to Space. [1512.00920]
Asteroseismology of Exoplanet Host Stars,
Daniel Huber,
arXiv:1511.07441, 2015.Focus Meeting 17 at the IAU General Assembly in Hawaii, August 2015. [1511.07441]
From Theory to Observations and viceversa: theoretical uncertainties and observational constraints,
Santi Cassisi,
EAS Publ.Ser. 65 (2014) 17,arXiv:1312.5968.
$23^rd$ Evry Schatzman School on Stellar Astrophysics, 'The Ages of Stars', Roscoff (France), 2013. [Cassisi:2013yua]
Galaxy formation,
Joseph Silk, Arianna Di Cintio, Irina Dvorkin,
Proc.Int.Sch.Phys.Fermi 186 (2014) 137-187,arXiv:1312.0107.
Post-Planck Cosmology, Ecole de Physique des Houches, Les Houches, July 8-Aug 2, 2013. [Silk:2013xca]
Neutron rich matter, neutron stars, and their crusts,
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J. Phys. Conf. Ser. 312 (2012) 042003,arXiv:1008.0402.
International Nuclear Physics Conference 2010, Vancouver, Ca. [Horowitz:2012za]
Searching for the First Galaxies,
Steven L. Finkelstein,
ASP Conf.Ser. 432 (2010) 33,arXiv:1004.0001.
Frank N. Bash Symposium 2009: New Horizons in Astronomy. [Finkelstein:2010ip]
High Energy Phenomena In The Universe,
Arnon Dar,
arXiv:0906.0973, 2009.44th Rencontre De Moriond on High Energy Phenomena In The Universe, La Thuile, Italy, February 1-8, 2009. [Dar:2009tv]
Science with the new generation high energy gamma- ray experiments,
M. Alvarez et al.,
Frascati Phys.Ser. 45 (2007) pp.1-328,arXiv:0712.1548.
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Lessons from Surveys of The Galaxy,
Rosemary F.G. Wyse,
Mem. Soc. Ast. It. 77 (2006) 1036-1049,arXiv:astro-ph/0701832.
Exploiting Large Surveys for Galactic Astronomy, XXVI General Assembly of the IAU, Prague 2006. [Wyse:2006ehh]
1st Workshop of Astronomy and Astrophysics for Students,
N.R. Napolitano, M. Paolillo,
arXiv:astro-ph/0701577, 2007.1st Workshop of Astronomy and Astrophysics for Students, Naples, Italy, April 19-20, 2006. [Napolitano:2007te]
Massive Black Holes: formation and evolution,
Martin J. Rees, Marta Volonteri,
IAU Symp. 238 (2007) 51,arXiv:astro-ph/0701512.
IAU Symp. 238, 'Black Holes: from stars to galaxies - across the range of masses'. [Rees:2007nc]
The Star Formation History of the Universe,
Andrew M. Hopkins,
ASP Conf.Ser. (2006),arXiv:astro-ph/0611283.
At the Edge of the Universe, October 2006, Sintra, Portugal. [Hopkins:2006pr]
Conference Summary: Astronomy Perspective of Astro-Statistics,
Ofer Lahav,
ASP Conf.Ser. (2006),arXiv:astro-ph/0610713.
Statistical Challenges in Modern Astronomy IV, 2007. [Lahav:2006jt]
Astrophysical Probes of Fundamental Physics,
C.J.A.P. Martins,
arXiv:astro-ph/0610665, 2006.ESO Precision Spectroscopy in Astrophysics. [Martins:2006br]
General Relativity effects and line emission,
Giorgio Matt,
Astron. Nachr. 88 (2006) 789-796,arXiv:astro-ph/0610224.
ESAC Workshop 'Variable and broad lines around black holes'. [Matt:2006zx]
Observations of solar-like oscillations,
Timothy R. Bedding, Hans Kjeldsen,
ESA Spec.Publ. 624 (2006) 25,arXiv:astro-ph/0609770.
SOHO 18 / GONG 2006 / HELAS conference, 'Beyond the Spherical Sun: a new era of helio- and asteroseismology', 7-11 August 2006, Sheffield, England. [Bedding:2006aa]
TeV Astrophysics, A Review,
Wei Cui,
arXiv:astro-ph/0608042, 2006.Vulcano Workshop 2006 'Frontier Objects in Astrophysics and Particle Physics'. [Cui:2006jm]
Understanding Galaxy Formation and Evolution,
V. Avila-Reese,
arXiv:astro-ph/0605212, 2006.IV Mexican School of Astrophysics, July 18-25, 2005. [Avila-Reese:2006pwa]
Dense plasmas in astrophysics: from giant planets to neutron stars,
G. Chabrier, D. Saumon, A. Potekhin,
J. Phys. A39 (2006) 4411,arXiv:astro-ph/0511803.
Strongly Coupled Coulomb Systems, Moscow June 2005. [Potekhin:2005ey]
Binaries as Astrophysical Laboratories: Open Questions,
Ignasi Ribas,
ASP Conf.Ser. (2005),arXiv:astro-ph/0511433.
Pecs PhD Conference on 'Astrophysics of Variable Stars'. [Ribas:2005eq]
Trust but verify: The case for astrophysical black holes,
Scott A. Hughes,
eConf C0507252 (2005) L006,arXiv:hep-ph/0511217.
2005 SLAC Summer Institute. [Hughes:2005wj]
Trends in Space Astronomy and Cosmic Vision 2015-2025,
Catherine Turon et al.,
ESA Spec.Publ. 588 (2005) 53,arXiv:astro-ph/0510809.
2005 ESLAB Symposium 'Trends in Space Science and Cosmic Vision 2020', ESTEC, 19-21 April 2005. [Turon:2005cg]
Early Stage of Galaxy Formation,
Y. Taniguchi et al.,
IAU Symp. (2005),arXiv:astro-ph/0510601.
4 pages with 1 table, Invited Review IAU The 9th Asian Pacific Regional Meeting. [Taniguchi:2005tn]
Radio Spectroscopy of Active Galactic Nuclei,
A.P. Lobanov,
Mem.Soc.Ast.It. (2005),arXiv:astro-ph/0507665.
5th Serbian Conference on Spectral Line Shapes in Astrophysics. [Lobanov:2005mn]
Cepheids, Eclipsing Binaries and the Distance Scale: from the Galaxy to the Local Group,
Lucas M. Macri,
ASP Conf.Ser. (2005),arXiv:astro-ph/0507648.
Cozumel meeting on Resolved Stellar Populations. [Macri:2005kv]
Numerical simulations of quasar absorbers,
Tom Theuns,
IAU Symp. (2005),arXiv:astro-ph/0507570.
Probing Galaxies through Quasar Absorption Lines. [Theuns:2005jd]
Ongoing Space Physics - Astrophysics Connections,
David Eichler,
Adv.Space Res. 38 (2006) 16,arXiv:astro-ph/0503350.
Critical Phenomena in the Solar System, Ein-Boqeq, March, 2004. [Eichler:2005te]
Nuclear Astrophysics,
Carl R. Brune,
arXiv:astro-ph/0502588, 2005.Lake Louise Winter Institute 2004 on Fundamental Interactions (LL WI 2004), Lake Louise, Alberta, Canada, 15-21 Feb 2004. [Brune:2005ee]
Outstanding Problems in Particle Astrophysics,
Thomas K. Gaisser,
arXiv:astro-ph/0501195, 2005.14th International School of Cosmic Ray Astrophysics: 'Neutrinos and Explosive Events in the Universe', July, 2004. [Gaisser:2005tu]
Concluding Remarks: Gaia and Astrophysics in 2015-2020,
Tim de Zeeuw,
ESA Spec.Publ. 576 (2005) 729,arXiv:astro-ph/0412429.
Symposium 'The Three-dimensional Universe with Gaia', 4-7 October 2004, Observatoire de Paris-Meudon, France. [deZeeuw:2004mc]
Interstellar dust: what is it, how does it evolve, and what are its observational consequences?,
Eli Dwek,
Aip Conf. Proc. 761 (2005) 103,arXiv:astro-ph/0412344.
'The Spectral Energy Distribution of Gas-Rich Galaxies: Confronting Models with Data', Heidelberg, 4-8 Oct. 2004. [Dwek:2004ad]
Where Are We Now, and Where Are We Going? Perspectives on Cosmic Abundances,
Timothy C. Beers,
ASP Conf.Ser. (2004),arXiv:astro-ph/0411751.
'Cosmic abundances as records of stellar evolution and nucleosynthesis', ASP conf. series. [Beers:2004ad]
The Chandra X-Ray Observatory: Observations of Neutron Stars,
Martin C. Weisskopf,
arXiv:astro-ph/0411243, 2004.NATO ASI - The Electromagnetic Spectrum of Neutron Stars: June 7-18, 2004, Marmaris, Turkey. [Weisskopf:2004qm]
Exploring the Universe beyond the Photon Window,
Luis A. Anchordoqui,
Acta Phys. Polon. B36 (2005) 495,arXiv:astro-ph/0410087.
XXXIV International Symposium on Multiparticle Dynamics, Sonoma County, California, July 26 - August 1, 2004. [Anchordoqui:2004pf]
Deep Field Surveys - A Radio View,
M.A. Garrett,
EAS Publ.Ser. 15 (2005) 73,arXiv:astro-ph/0409197.
JENAM-2003 Symposium, 'Radio Astronomy at 70: from Karl Jansky to microjansky,' Budapest, Hungary, 27-30 August 2003. [Garrett:2004wp]
The role of interactions,
H. R. Schmitt,
IAU Symp. 222 (2004) 395,arXiv:astro-ph/0407590.
'The Interplay among Black Holes, Stars and ISM in Galactic Nuclei,' IAU 222 (Gramado, Brazil). [Schmitt:2004fp]
The Current Status of Primary Distance Indicators,
Michael Feast,
ASP Conf.Ser. 329 (2005) 241,arXiv:astro-ph/0405440.
Nearby Large-Scale Structures and the Zone of Avoidance. [Feast:2004rx]
Astroparticle Physics,
I. I. Tkachev,
arXiv:hep-ph/0405168, 2004.2003 European School of High-Energy Physics, Tsakhkadzor, Armenia, 24 August - 6 September 2003. [Tkachev:2004ee]
The Solar Galactic Environment,
P. C. Frisch,
Aip Conf. Proc. 719 (2004) 404,arXiv:astro-ph/0405167.
3rd Annual IGPP-UCR Astrophysics Conference: Physics of the Outer Heliosphere. [Frisch:2004fx]
Pulsar astrophysics : the glitch phenomenon,
J.E. Horvath, Sao Paulo,
Int. J. Mod. Phys. D13 (2004) 1327,arXiv:astro-ph/0404324.
First International Workshop on Astronomy and Relativistic Astrophysics (Olinda, Brazil, October 2003). [Horvath:2004xm]
Galactic Structure,
Rosemary F.G. Wyse,
arXiv:astro-ph/0402636, 2004.2003 May Symposium, Space Telescope Science Institute, `The Local Group as an Astrophysical Laboratory'. [Wyse:2004nr]
Microquasars,
M. Ribo,
ASP Conf.Ser. (2004),arXiv:astro-ph/0402134.
'Future Directions in High Resolution Astronomy: A Celebration of the 10th Anniversary of the VLBA', June 8-12, 2003, Socorro, New Mexico, USA. [Ribo:2004if]
A Review of the Current Status of Follow-Up Techniques to Study Known Extrasolar Planets,
David Charbonneau,
IAU Symp. 219 (2004) 367,arXiv:astro-ph/0312252.
IAU Symposium 219: Stars as Suns: Activity, Evolution, and Planets. [Charbonneau:2003sp]
A Review of the Distance and Structure of the Large Magellanic Cloud,
David R. Alves,
New Astron. Rev. 48 (2004) 659,arXiv:astro-ph/0310673.
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Magnetised Neutron Stars : An Overview,
Ashok Goyal,
arXiv:hep-ph/0306116, 2003.Workshop on High magnetic field and neutron star, Havana, April 2003. [Goyal:2003su]
The Phenomena of High Energy Astrophysics,
R. D. Blandford,
ASP Conf. Ser. (2003),arXiv:astro-ph/0302226.
High Energy Processes and Phenomena in Astrophysics, IAU Symposium 214. [Blandford:2003fg]
Captain Cook, the Terrestrial Planet Finder and the Search for Extraterrestrial Intelligence,
Charles Beichman,
IAU Symp.213 (2002),arXiv:astro-ph/0212336.
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Microlensing Searches for Extrasolar Planets: Current Status and Future Prospects,
B. Scott Gaudi,
ASP Conf.Ser. (2002),arXiv:astro-ph/0207533.
ASP Conference Series: Scientific Frontiers in Research on Extrasolar Planets. [Gaudi:2002mn]
The Matter-Antimatter Asymmetry of the Universe,
F. W. Stecker,
arXiv:hep-ph/0207323, 2002.XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002. [Stecker:2002tb]
Nuclear and High-Energy Astrophysics,
Fridolin Weber,
arXiv:astro-ph/0207053, 2002.VIII International Workshop on Hadron Physics, April 14-19, 2002, Rio Grande do Sul, Brazil. [Weber:2002de]
Exploration of possible signals beyond special relativity using high-energy astroparticle physics,
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Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies,
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Astrophys. J. 904 (2020) 51,arXiv:2009.11525.
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Blazar Radio and Optical Survey (BROS): A catalog of blazar candidates showing flat radio spectrum and their optical identification in Pan-STARRS1 Surveys,
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Astrophys.J. 901 (2020) 3,arXiv:2008.00038.
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Planck intermediate results. XLII. Large-scale Galactic magnetic fields,
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Parallax of Galactic Cepheids from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope: The Case of SS Canis Majoris,
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The XXL Survey: XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters,
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Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz,
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Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck clusters,
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Planck Intermediate Results II: Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters,
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GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end,
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The Fourth Data Release of the Sloan Digital Sky Survey,
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Lithium and Lithium Depletion in Halo Stars on Extreme Orbits,
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Astrophys. J. 633 (2005) 398,arXiv:astro-ph/0507625.
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Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation,
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The DEEP2 Redshift Survey: The Galaxy Luminosity Function to z ~ 1,
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Early SPI/INTEGRAL measurements of galactic 511 keV line emission from positron annihilation,
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The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging,
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The Torino Observatory Parallax Program: White Dwarf Candidates,
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The Hubble Space Telescope WFPC2 B-Band Parallel Survey: A Study of Galaxy Morphology for 18 < B < 27 mag,
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SDSS Catalog of Stars in the Draco Dwarf Spheroidal Galaxy,
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Nucleosynthesis results from INTEGRAL,
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A Catalogue of infrared star clusters and stellar groups,
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ASTRO-F - Super IRAS - The All Sky Infra-Red Survey,
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Limits from the grave: resurrecting Hitomi for decaying dark matter and forecasting leading sensitivity for XRISM,
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A Deep Chandra Catalog of X-ray Point Sources toward the Galactic Center,
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X-ray Source Population in the Elliptical Galaxy NGC 720 with Chandra,
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The Chandra Deep Field-North Survey. XVI. The X-ray properties of moderate-luminosity Active Galaxies at $z > 4$,
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Chandra Evidence for a Flattened, Triaxial Dark Matter Halo in the Elliptical Galaxy NGC 720,
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Studying the Nearby Universe with Chandra,
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Precise measurement of the $^7\mathrm{Be}(p,gamma)^8\mathrm{B}$ S-factor,
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Precise measurement of cross section of 3He(3He,2p)4He by using He-3 doubly charged beam,
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The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars,
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Neutrinos as a new tool to characterise the Milky Way Centre,
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Neutrino imaging of the Galactic Centre and Millisecond Pulsar Population,
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Contrast Loss from Astrophysical Backgrounds in Space-Based Matter-Wave Interferometers,
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Studying the mass sensitivity of air-shower observables using simulated cosmic rays,
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DIAPHANE: a Portable Radiation Transport Library for Astrophysical Applications,
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Bayesian Inference from Observations of Solar-Like Oscillations,
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2dFGRS and SDSS Galaxy Group Density Profiles,
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Lyman Alpha Flux Power Spectrum and Its Covariance,
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Cosmological Three-Point Function: Testing The Halo Model Against Simulations,
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Pioneer anomaly? Gravitational pull due to the Kuiper belt,
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The Millennium Galaxy Catalogue: the space density and surface brightness distribution(s) of galaxies,
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A Strong Test of Electro-Weak Theory using Pulsating DB White Dwarf Stars as Plasmon Neutrino Detectors,
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The Imprint of the Cosmic Dark Ages on the Near Infrared Background,
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Light Elements in Main Sequence Stars: Li, Be, B, C, O,
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Population synthesis in astrophysics,
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Phys. Usp. 50 (2007) 1123-1146,arXiv:astro-ph/0411792.
Helmholtz International Summer School and Workshop on Hot points in Astrophysics and Cosmology. [Popov:2004gw]
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Eur. Phys. J. C40 (2005) 15,arXiv:astro-ph/0410407.
42nd course of the international school of subnuclear physics, 'How and where to go beyond the standard model', Erice, Aug. 29 - Sep. 7, 2004. [Sandin:2004kb]
Parity Violation in Astrophysics,
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Eur. Phys. J. A24S2 (2005) 167,arXiv:nucl-th/0410074.
PAVI04 conference in Grenoble, France. [Horowitz:2004pc]
Conference Summary: AGN Physics with the Sloan Digital Sky Survey,
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From Reference Frames to Relativistic Experiments: Absolute and Relative Radio Astrometry,
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JENAM meeting in Budapest, 27-30 August 2003. [Fomalont:2004db]
AGN Unification: An Update,
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ASP Conf.Ser. (2003),arXiv:astro-ph/0312545.
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Evidence for the Black Hole Event Horizon,
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Astron.Geophys. (2003),arXiv:astro-ph/0310692.
George Darwin Lecture presented at the Royal Astronomical Society, London, 13 December 2002. [Narayan:2003fy]
Astrophysical constraints on hypothetical variability of fundamental constants,
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Lect. Notes Phys. 648 (2004) 151,arXiv:astro-ph/0309817.
302 WE-Heraeus-Seminar on Astrophysics, Clocks and Fundamental Constants (16-18 June 2003: Bad Honnef, Germany). [Levshakov:2003fa]
Cosmic rays, stellar evolution, and supernova physics,
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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. [Biermann:2003et]
TeV Blazars - Observations and Models,
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New Astron. Rev. 48 (2004) 367,arXiv:astro-ph/0309443.
'2nd VERITAS Symposium on TeV Astrophysics of Extragalactic Sources', April 24-26, 2003, Chicago. [Krawczynski:2003sw]
Strange Quark Matter in Neutron Stars? - New Results from Chandra and XMM,
Markus H. Thoma, Joachim Truemper, Vadim Burwitz,
J. Phys. G30 (2004) S471,arXiv:astro-ph/0305249.
SQM 2003. [Thoma:2003xq]
White Dwarf Rotation: Observations and Theory,
Steven D. Kawaler,
arXiv:astro-ph/0301539, 2003.IAU Symposium #215 - Stellar Rotation (November 2002). [Kawaler:2003sr]
The First Sources of Light,
Volker Bromm, Abraham Loeb,
Aip Conf. Proc. 666 (2003) 73,arXiv:astro-ph/0301406.
13th Annual October Astrophysics Conference in Maryland, 'The Emergence of Cosmic Structure', College Park, October 2002. [Bromm:2003rx]
$\alpha$:a constant that is not a constant?,
B. Ricci G. Fiorentini,
arXiv:astro-ph/0207390, 2002.ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics, Garching bei Munchen, Germany March 4-7, 2002. [Fiorentini:2002kx]
LeHaMoC: a versatile time-dependent lepto-hadronic modeling code for high-energy astrophysical sources,
S. I. Stathopoulos, M. Petropoulou, G. Vasilopoulos, A. Mastichiadis,
Astron.Astrophys. 683 (2024) A225,arXiv:2308.06174.
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Hard X-ray emission from blazars associated with high-energy neutrinos,
A. V. Plavin, R. A. Burenin, Y. Y. Kovalev, A. A. Lutovinov, A. A. Starobinsky, S. V. Troitsky, E. I. Zakharov,
JCAP 05 (2024) 133,arXiv:2306.00960.
[Plavin:2023wsb]
The early evolution of magnetar rotation - II. Rapidly rotating magnetars: Implications for Gamma-Ray Bursts and Super Luminous Supernovae,
Tejas Prasanna, Matthew S. B. Coleman, Matthias J. Raives, Todd A. Thompson,
Mon.Not.Roy.Astron.Soc. 526 (2023) 3141-3155,arXiv:2305.16412.
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Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta,
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Class.Quant.Grav. 34 (2017) 154001,arXiv:1612.04829.
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Microphysical dissipation, turbulence and magnetic fields in hyper-accreting discs,
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Mon.Not.Roy.Astron.Soc. 391 (2008) 922,arXiv:0807.3547.
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Why is the Zel'dovich Approximation so Accurate?,
A. Yoshisato, M. Morikawa, N. Gouda, H. Mouri,
Astrophys. J. 637 (2006) 555,arXiv:astro-ph/0510107.
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Gravitational Structure Formation,
Francesco Sylos Labini, Thierry Baertschiger,
arXiv:astro-ph/0511655, 2005.'Few-Body Problem: Theory and Computer Simulations A Workshop in celebration of the 60th Birthday of Professor Mauri Valtonen. [Labini:2005ma]
Nonextensive statistical effects on nuclear astrophysics and many-body problems,
A. Lavagno, P. Quarati,
arXiv:nucl-th/0504080, 2005.X Convegno su Problemi di Fisica Nucleare Teorica. [Lavagno:2005ge]
The neutron decay anomaly, neutron stars and dark matter,
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Phys.Rev.D 110 (2024) 083003,arXiv:2403.08666.
[Bastero-Gil:2024kjo]
Is there a black hole in the center of the Sun?,
Matthew E. Caplan, Earl P. Bellinger, Andrew D. Santarelli,
Astrophys. Space Sci. 369 (2024) 8,arXiv:2312.07647.
[Caplan:2023ddo]
Solar Evolution Models with a Central Black Hole,
Earl P. Bellinger, Matt E. Caplan, Taeho Ryu, Deepika Bollimpalli, Warrick H. Ball, Florian Kuhnel, R. Farmer, S. E. de Mink, J\orgen Christensen-Dalsgaard,
Astrophys. J. 959 (2023) 113,arXiv:2312.06782.
[Bellinger:2023wou]
Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop,
James Gurian, Donghui Jeong, Boyuan Liu,
Astrophys.J. 963 (2024) 33,arXiv:2309.05758.
[Gurian:2023ctu]
The Jeans mass and the origin of the knee in the IMF,
I. A. Bonnell, C. J. Clarke, M. R. Bate,
Mon. Not. Roy. Astron. Soc. 368 (2006) 1296,arXiv:astro-ph/0603444.
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Galaxy Star-Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey,
Percy Gomez et al.(The SDSS),
Astrophys. J. 584 (2003) 210,arXiv:astro-ph/0210193.
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Stellar Neutrino Emission Across The Mass-Metallicity Plane,
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Astrophys.J.Suppl. 270 (2024) 5,arXiv:2310.13142.
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Cumulative physical uncertainty in modern stellar models I. The case of low-mass stars,
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A&A, 549, A50 (2013),arXiv:1211.0706.
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The chemical composition of White Dwarfs as a test of convective efficiency during core He-burning,
Oscar Straniero, Inma Dominguez, Gianluca Imbriani, Luciano Piersanti,
Astrophys. J. 583 (2003) 878,arXiv:astro-ph/0210191.
[Straniero:2002pf]
Continuum Equations for Stellar Dynamics,
Edward A. Spiegel, Jean-Luc Thiffeault,
arXiv:astro-ph/0210185, 2002.Chateau de Mons meeting in honour of Douglas Gough's 60th birthday. [Spiegel:2002nz]
Probing the equation of state of neutron stars using neutrino oscillations,
Siddhartha Bandyopadhyay, Golam Mortuza Hossain,
Phys.Rev.D 111 (2025) 065009,arXiv:2409.16232.
[Bandyopadhyay:2024uld]
Emergent nucleosynthesis from a 1.2 second long simulation of a black-hole accretion disk,
T. M. Sprouse, K. A. Lund, J. M. Miller, G. C. McLaughlin, M. R. Mumpower,
Astrophys.J. 962 (2024) 79,arXiv:2309.07966.
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Viscous hydrodynamic evolution of neutron star merger accretion disks: a code comparison,
Rodrigo Fernandez, Oliver Just, Zewei Xiong, Gabriel Martinez-Pinedo,
Phys.Rev.D 110 (2024) 023001,arXiv:2307.02554.
[Fernandez:2023vxj]
Anomaly induced cooling of Neutron Stars: A Standard Model contribution,
Sabyasachi Chakraborty, Aritra Gupta, Miguel Vanvlasselaer,
JCAP 10 (2023) 030,arXiv:2306.15872.
[Chakraborty:2023wgl]
Isospin Equilibration in Neutron Star Mergers,
Mark G. Alford, Alexander Haber, Ziyuan Zhang,
Phys.Rev.C 109 (2024) 055803,arXiv:2306.06180.
[Alford:2023gxq]
Nucleation rate of color superconducting droplets in protoneutron stars,
T. A. S. do Carmo, G. Lugones, A. G. Grunfeld,
J. Phys. G40 (2013) 035201,arXiv:1301.3483.
to appear in J. Phys. G. [Carmo:2013fr]
The importance of cooling in triggering the collapse of hypermassive neutron stars,
Vasileios Paschalidis, Zachariah B. Etienne, Stuart L. Shapiro,
Phys. Rev. D86 (2012) 064032,arXiv:1208.5487.
[Paschalidis:2012ff]
The impact of magnetic field on the thermal evolution of neutron stars,
Deborah N. Aguilera, Jose A. Pons, Juan A. Miralles,
Astrophys. J. 673 (2008) L167,arXiv:0712.1353.
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Neutron Star Observations: Prognosis for Equation of State Constraints,
James M. Lattimer, Maddapa Prakash,
Phys. Rept. 442 (2007) 109-165,arXiv:astro-ph/0612440.
[Lattimer:2006xb]
Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition,
Sanjib Gupta et al.,
Astrophys. J. 662 (2007) 1188-1197,arXiv:astro-ph/0609828.
[Gupta:2006fd]
Towards a self-consistent relativistic model of the exterior gravitational field of rapidly rotating neutron stars,
Matthias Stute, Max Camenzind,
Mon. Not. Roy. Astron. Soc. 336 (2002) 831,arXiv:astro-ph/0301466.
[Stute:2002mqa]
Effects of Differential Rotation on the Maximum Mass of Neutron Stars,
Nicholas D. Lyford, Thomas W. Baumgarte, Stuart L. Shapiro,
Astrophys. J. 583 (2003) 410,arXiv:gr-qc/0210012.
[Lyford:2002ip]
The Neutron Star and Black Hole Initial Mass Function,
F. X. Timmes, S. E. Woosley, Thomas A. Weaver,
Astrophys. J. 457 (1996) 834,arXiv:astro-ph/9510136.
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Entropy, Disequilibrium and Complexity in Compact Stars: An information theory approach to understand their Composition,
Marcio G B de Avellar, Jorge E Horvath,
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Neutron Stars in a Chiral Model with Finite Temperature,
V. Dexheimer, S. Schramm, H. Stoecker,
J. Phys. G35 (2008) 014060,arXiv:0708.0502.
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Neutron star cooling,
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Nucl. Phys. A752 (2005) 590,arXiv:astro-ph/0409751.
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Physical Processes in Strong Magnetic Fields of Neutron Stars,
Alice K. Harding,
arXiv:astro-ph/0304120, 2003.Pulsars, AXPs and SGRs Observed with BeppoSAX and Other Observatories, Marsala, Sicily, Sept. 2002. [Harding:2003cx]
Role of symmetry energy at subnuclear densities in protoneutron star crusts,
Ken'ichiro Nakazato, Hajime Togashi, Kohsuke Sumiyoshi, Hideyuki Suzuki,
arXiv:2508.16120, 2025. [Nakazato:2025czl]
Weak interaction rates of sd-shell Urca pairs in stellar environment using a shell-model approach,
Shweta Sharma, Praveen C. Srivastava, Toshio Suzuki,
Phys. Rev. C 112 (2025) 015806,arXiv:2508.05456.
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$f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping,
Nilaksha Barman, Debarati Chatterjee,
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New Skyrme parametrizations to describe finite nuclei and neutron star matter with realistic effective masses. II. Adjusting the spin-dependent terms,
Mingya Duan, Michael Urban,
Phys.Rev.C 112 (2025) 045808,arXiv:2501.03411.
[Duan:2025hyo]
Ab initio calculation of the $^3$He$(\alpha,\gamma)^7$Be astrophysical S factor with chiral two- and three-nucleon forces,
M. C. Atkinson, K. Kravvaris, S. Quaglioni, P. Navratil,
Phys.Lett.B 860 (2025) 139189,arXiv:2409.09515.
[Atkinson:2024zrm]
Investigating the crust of neutron stars with neural-network quantum states,
Bryce Fore, Jane Kim, Morten Hjorth-Jensen, Alessandro Lovato,
Commun.Phys. 8 (2025) 108,arXiv:2407.21207.
[Fore:2024exa]
Spin response of neutron matter in ab initio approach,
J. E. Sobczyk, W. Jiang, A. Roggero,
Phys.Rev.Lett. 134 (2025) 192701,arXiv:2407.20986.
[Sobczyk:2024hdl]
Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction,
T. R. Routray, S. Sahoo, X. Vinas, D. N. Basu, M. Centelles,
J.Phys.G 51 (2024) 085203,arXiv:2404.05910.
[Routray:2024kgv]
Antineutrino Opacity in Neutron Stars in the Models Constrained by Recent Terrestrial Experiments and Astrophysical Observations,
Parada T. P. Hutauruk,
Astronomy 3 (2024) 240-254,arXiv:2311.09986.
[Hutauruk:2023nqc]
Production of $p$-nuclei from $r$-process seeds: the $\nu r$-process,
Zewei Xiong, Gabriel Martinez-Pinedo, Oliver Just, Andre Sieverding,
Phys.Rev.Lett. 132 (2024) 192701,arXiv:2305.11050.
[Xiong:2023uyb]
Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities,
Ken'ichiro Nakazato, Hideyuki Suzuki,
Astrophys.J. 878 (2019) 25,arXiv:1905.00014.
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Shell-model computed cross sections for charged-current scattering of astrophysical neutrinos off $^{40}$Ar,
Joel Kostensalo, Jouni Suhonen, K. Zuber,
Phys. Rev. C97 (2018) 034309. [Kostensalo:2018kgh]
Nuclear pasta in hot dense matter and its implications for neutrino scattering,
Alessandro Roggero, Jerome Margueron, Luke F. Roberts, Sanjay Reddy,
Phys.Rev. C97 (2018) 045804,arXiv:1710.10206.
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Effect of electric field of the electrosphere on photon emission from quark stars,
B.G. Zakharov,
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Neutron-Rich Nuclei and Neutron Stars: A New Accurately Calibrated Interaction for the Study of Neutron-Rich Matter,
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A model of the internal structure of Titan: first results,
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Cosmic ray feedback in hydrodynamical simulations of galaxy formation,
Martin Jubelgas, Volker Springel, Torsten A. Ensslin, Christoph Pfrommer,
Astron.Astrophys. (2006),arXiv:astro-ph/0603485.
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Cosmic ray physics in calculations of cosmological structure formation,
Torsten A. Ensslin, Christoph Pfrommer, Volker Springel, Martin Jubelgas,
Astron. Astrophys. 473 (2007) 41-57,arXiv:astro-ph/0603484.
[Ensslin:2006mt]
The spin period - eccentricity relation of double neutron stars: evidence for weak supernova kicks?,
J D M Dewi, Ph Podsiadlowski, O R Pols,
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Formation of an evanescent proto-neutron star binary and the origin of pulsar kicks,
Ira Wasserman Monica Colpi,
Astrophys. J. 581 (2002) 1271,arXiv:astro-ph/0207327.
[Colpi:2002cu]
Jet Formation in Black Hole Accretion Systems II: Numerical Models,
Jonathan C. McKinney,
Astrophys.J. (2005),arXiv:astro-ph/0506369.
[McKinney:2005zy]
Jet Formation in Black Hole Accretion Systems I: Theoretical Unification Model,
Jonathan C. McKinney,
Astrophys.J. (2005),arXiv:astro-ph/0506368.
[McKinney:2005zx]
Korean Nova Records in A.D. 1073 and A.D. 1074: R Aquarii,
Hong-Jin Yang, Myeong-Gu Park, Se-Hyung Cho, Changbom Park,
Astron. Astrophys. 435 (2005) 207,arXiv:astro-ph/0501331.
[Yang:2005ny]
Solar Oblateness from Archimedes to Dicke,
Costantino Sigismondi, Pietro Oliva,
Adv.Theor.Math.Phys. 9 (2005) 129-172,arXiv:physics/0501083.
[Isenberg:2005xp]
Halley of 87 BC on the Coins of Armenian King Tigranes?,
V.G.Gurzadyan, R.Vardanyan,
Phys. Rev. D71 (2005) 017301,arXiv:physics/0405073.
[Latimer:2004hd]
Digitatio and Scientific Exploitation of the Italian and Vatican Astronomical Plate Archives,
Cesare Barbieri et al.,
Exper. Astron. 15 (2003) 29,arXiv:astro-ph/0401200.
[Barbieri:2003dxm]
History of Astrophysics in Antarctica - A Brief Overview,
Balthasar T. Indermuehle, Michael G. Burton, Sarah T. Maddison,
ASP Conf.Ser. (2003),arXiv:astro-ph/0309124.
[Indermuehle:2003te]
What do astrophysics and the world's oldest profession have in common?,
Martin Lopez-Corredoira,
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Galactic Gradients, Postbiological Evolution and the Apparent Failure of SETI,
Milan M. Cirkovic, Robert J. Bradbury,
New Astron. 11 (2006) 628-639,arXiv:astro-ph/0506110.
[Cirkovic:2005rt]
Too Early? On the Apparent Conflict of Astrobiology and Cosmology,
Milan M. Cirkovic,
Biol. Phil. 21 (2006) 369-379,arXiv:astro-ph/0505006.
[Cirkovic:2005me]
"Permanence" - An Adaptationist Solution to Fermi's Paradox?,
Milan M. Cirkovic,
J.Br.Interplanet.Soc. 58 (2005) 62,arXiv:astro-ph/0408521.
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The Road Less Traveled: Non-traditional Ways of Communicating Astronomy with the Public,
Michael J. West,
arXiv:physics/0508183, 2005.Communicating Astronomy with the Public 2005. [West:2005mq]
The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope,
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JCAP 08 (2025) 034,arXiv:2503.00636.
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Synergies of THESEUS with the large facilities of the '30s and GO opportunities,
P. Rosati et al.,
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The THESEUS space mission: science goals, requirements and mission concept,
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ESA Voyage 2050 white paper - Faint objects in motion: the new frontier of high precision astrometry,
F. Malbet et al.,
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Galaxy Evolution and Cosmology with the Square Kilometre Array,
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The LXeGRIT Compton Telescope Prototype: Current Status and Future Prospects,
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Liverpool Telescope 2: a new robotic facility for time domain astronomy in 2020+,
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High-energy Astrophysics and the Virtual Observatory,
P. Padovani,
Astron.Astrophys. (2005),arXiv:astro-ph/0507594.
Workshop 'Multifrequency Behaviour of High Energy Cosmic Sources', Vulcano, Italy, May 2005. [Padovani:2005pv]
The South Pole Telescope,
SPT(The SPT),
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Accelerator Experiments for Astrophysics,
J. S. T. Ng,
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When you wish upon a star: Future developments in astronomical VLBI,
M. A. Garrett,
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Toward Ultra Short Gamma Ray Burst Ground Based Detection, SGARFACE status,
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Prospects for High Energy Studies of Pulsars with the AGILE Gamma-Ray Telescope,
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Optimising GAIA: How do we meet the science challenge?,
G. Gilmore,
ASP Conf.Ser. (2002),arXiv:astro-ph/0212027.
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Scientific goals of the UKIRT Infrared Deep Sky Survey,
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The Extra-Solar Planet Imager (ESPI),
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ASP Conf.Ser. 294 (2003) 633,arXiv:astro-ph/0210046.
P.A.S.P. Proceedings of Carnegie Meeting on Scientific Frontiers in Research on Extrasolar Planets. [Nisenson:2002yh]
It is possible to perform a cross search between the various pages of Neutrino Unbound.
This is useful if you want to show the common elements that appear
in the listings of two (or more) different topics or experiments.