Search - Segue Virtual Journal

Criteria:

Year:

2006	2007	2008	2009	2010	2011	2012	2013	2014	2015
2016	2017	2018	2019	2020	2021	2022	2023	2024

Results Per Page

(100 is the maximum results per page allowed.)

Boolean Operator
For Tags

Results 1 - 100 of 361

Select Page: 1 2 3 4 Next

APOKASC-3: The Third Joint Spectroscopic and Asteroseismic catalog for Evolved Stars in the Kepler Fields
- Volume 19, Issue 40 - article #1
- Marc H. Pinsonneault (Department of Astronomy, The Ohio State University, USA), Joel C. Zinn (Department of Physics, California State Long Beach, USA), Jamie Tayar (Department of Astronomy, University of Florida, USA), Aldo Serenelli (Institute of Space Sciences, ICE, CSIC, Spain, Institut d'Estudis Espacials de Catalunya, Spain), Rafael A. Garcia (Universite Paris Cite, CEA, CNRS, France), Savita Mathur (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain, Space Science Institute, USA), Mathieu Vrard (Department of Astronomy, The Ohio State University, USA, Observatoire de la Cote d'Azur CNRS, France), Yvonne P. Elsworth (School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark), Benoit Mosser (LESIA Observatoire de Paris Universite, PSL, CNRS, Sorbonne Universite, Universite de Paris, France), Dennis Stello (School of Physics, University of New South Wales, Australia, Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia, ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions, Australia), Keaton J. Bell (Department of Physics, Queens College, CUNY, USA), Lisa Bugnet (Institute of Science, Technology Austria), Enrico Corsaro (INAF, Osservatorio Astrofisico di Catania, Italy), Patrick Gaulme (Thuringer Landessternwarte, Germany, Department of Astronomy, New Mexico State University, USA), Saskia Hekker (Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark, Heidelberg University, Germany, Heidelberg Institute for Theoretical Studies, Germany), Marc Hon (Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, USA, Institute for Astronomy, University of Hawaii, USA), Daniel Huber (Institute for Astronomy, University of Hawaii, USA, SIfA, School of Physics, University of Sydney, Australia), Thomas Kallinger (Institute for Astronomy, University of Vienna, Austria), Kaili Cao (Center for Cosmology, AstroParticle Physics, Department of Physics, The Ohio State University, USA), Jennifer A. Johnson (Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics), Bastien Liagre (Universite Paris Cite, CEA, CNRS, France, Instituto de Astrofsica de Canarias, Spain, ENS Paris-Saclay, Universite Paris-Saclay, France), Rachel A. Patton (Department of Astronomy, The Ohio State University, USA, Center for Cosmology, AstroParticle Physics), Angela R. G. Santos (Instituto de Astrofisica e Ciencias do Espac{c}o, Universidade do Porto, Portugal), Sarbani Basu (Department of Astronomy, Yale University, USA), Paul G. Beck (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain), Timothy C. Beers (Dept. of Physics, Astronomy,, JINA Center for the Evolution of the Elements University of Notre Dame, USA), William J. Chaplin (School of Physics, Astronomy, University of Birmingham, UK, Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark), Katia Cunha (University of Arizona, Steward Observatory, USA, Observatorio Nacional, Sao Cristovao, Brazil), Peter M. Frinchaboy (Department of Physics, Astronomy, Texas Christian University, USA, Maunakea Spectroscopic Explorer, Canada-France-Hawaii-Telescope, USA), Leo Girardi (Osservatorio Astronomico di Padova, INAF, Italy), Diego Godoy-Rivera (Instituto de Astrofsica de Canarias, Spain, Departamento de Astrofisica Universidad de La Laguna, Spain), Jon A. Holtzman (Department of Astronomy, New Mexico State University, USA), Henrik Jonsson (Materials Science, Applied Mathematics, Malmo University, Sweden), Szabolcs Meszaros (ELTE Eotvos Lorand University, Gothard Astrophysical Observatory, Hungary, MTA-ELTE Lendulet Momentum Milky Way Research Group, Hungary), Claudia Reyes (School of Physics, University of New South Wales, Australia), Hans-Walter Rix (Max Planck Institute for Astronomy, Heidelberg, Germany), Matthew Shetrone (University of California Observatories, University of California Santa Cruz, USA), Verne V. Smith (NSFs NOIRLab, USA), Taylor Spoo (Department of Physics, Astronomy, Texas Christian University, USA), Keivan G. Stassun (Department of Physics, Astronomy, Vanderbilt University, USA), Ji Wang (Department of Astronomy, The Ohio State University, USA)
- https://arxiv.org/abs/2410.00102
The formation and disruption of globular cluster populations in simulations of present-day $L^ast$ galaxies with controlled assembly histories
- Volume 19, Issue 37 - article #3
- Oliver Newton (Astrophysics Research Institute, LJMU, Liverpool, UK, Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland), Jonathan J. Davies (Astrophysics Research Institute, LJMU, Liverpool, UK, University College London, UK), Joel Pfeffer (Swinburne University, Australia), Robert A. Crain (Astrophysics Research Institute, LJMU, Liverpool, UK), J. M. Diederik Kruijssen (Technical University of Munich, Germany, Cosmic Origins Of Life Research DAO, Germany), Andrew Pontzen (University College London, UK), Nate Bastian (Donostia International Physics Center, Guipuzkoa, Spain, Basque Foundation for Science, Bilbao, Spain)
- https://arxiv.org/abs/2409.04516
Metallicity relations in LMC and SMC from the slope of Red Giant Branch stars in globular clusters
- Volume 19, Issue 25 - article #3
- Saurabh Sharma (Aryabhatta Research Institute of Observational Sciences), Jura Borissova (Instituto de Fisica y Astronomia, Universidad de Valparaiso, Ave. Gran Bretana 1111, Valparaiso, Chile, Millennium Institute of Astrophysics, MAS, Chile)
- https://arxiv.org/abs/2406.09911
Metal-Poor Stars in the MW Disk: Resonant Cooling of Vertical Oscillations of Halo Stars in Barred Galaxies
- Volume 19, Issue 24 - article #3
- Xingchen Li (University of Kentucky), Isaac Shlosman (University of Kentucky,Theoretical Astrophysics, Osaka University), Daniel Pfenniger (University of Geneva), Clayton Heller (Georgia Southern University)
- https://arxiv.org/abs/2406.06716
Supernova Simulations
- Volume 19, Issue 13 - article #5
- Bernhard M"uller (School of Physics,Astronomy, Monash University)
- https://arxiv.org/abs/2403.18952
SkyMapper Southern Survey: Data Release 4
- Volume 19, Issue 6 - article #5
- Christopher A. OnkenResearch School of Astronomy, Astrophysics, Australian National University, Centre for Gravitational Astrophysics, Australian National University Christian WolfResearch School of Astronomy, Astrophysics, Australian National University, Centre for Gravitational Astrophysics, Australian National University Michael S. BessellResearch School of Astronomy, Astrophysics, Australian National University Seo-Won ChangAstronomy Program, Department of Physics, Astronomy, Seoul National University, SNU Astronomy Research Center, Seoul National University Lance C. LuvaulResearch School of Astronomy, Astrophysics, Australian National University John L. TonryInstitute for Astronomy, University of Hawaii Marc C. WhiteResearch School of Astronomy, Astrophysics, Australian National University Gary S. Da CostaResearch School of Astronomy, Astrophysics, Australian National University
- https://arxiv.org/abs/2402.02015
Did the Gaia Enceladus/Sausage merger form the Milky Way's bar?. (arXiv:2312.02318v1 [astro-ph.GA])
- Volume 18, Issue 47 - article #1
- Alex Merrow (1), Robert J. J. Grand (1), Francesca Fragkoudi (2), Marie Martig (1) ((1) Astrophysics Research Institute Liverpool John Moores University, (2) Department of Physics Durham University)
- http://arxiv.org/abs/2312.02318
Does the i-process operate at nearly solar metallicity?. (arXiv:2305.04189v1 [astro-ph.SR])
- Volume 18, Issue 19 - article #3
- D. Karinkuzhi (1,2), S. Van Eck (2), S. Goriely (2), L. Siess (2), A. Jorissen (2), A. Choplin (2), A. Escorza (3), S. Shetye (4), H. Van Winckel (5). ((1). Department of Physics, University of Calicut, Thenhipalam, Malappuram 673635, India (2). Institut d'Astronomie et d'Astrophysique, Universit'e Libre de Bruxelles (ULB) C.P. 226, B-1050 Bruxelles, Belgium (3). European Southern Observatory, Alonso de Córdova 3107, Vitacura, Casilla 19001, Santiago de Chile, Chile (4). Institute of Physics, Laboratory of Astrophysics, École polytechnique fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland (5).Instituut voor Sterrenkunde, KULeuven, Celestijnenlaan 200D, 3001 Leuven, Belgium)
- http://arxiv.org/abs/2305.04189
Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models. (arXiv:2303.15117v1 [astro-ph.SR])
- Volume 18, Issue 13 - article #7
- Nitesh Kumar (1), Anupam Bhardwaj (2), Harinder P. Singh (1), Susmita Das (3), Marcella Marconi (2), Shashi M. Kanbur (4), Philippe Prugniel (5) ((1) Department of Physics, Astrophysics, University of Delhi, Delhi 110007, India (2) INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, 80131, Naples, Italy (3) Konkoly Observatory, Research Centre for Astronomy, Earth Sciences, Eötvös Loránd Research Network (ELKH), Konkoly-Thege Miklós út 15-17, H-1121, Budapest, Hungary (4) Department of Physics, Earth Science, State University of New york at Oswego, Oswego, NY 13126, USA (5) Université de Lyon, Université Lyon 1, 69622 Villeurbanne, CRAL, Observatoire de Lyon, CNRS UMR 5574, 69561 Saint-Genis Laval, France)
- http://arxiv.org/abs/2303.15117
RR Lyrae mid-infrared Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity relations based on Gaia DR3 parallaxes. (arXiv:2301.03777v1 [astro-ph.GA])
- Volume 18, Issue 2 - article #2
- Joseph P. Mullen (1), Massimo Marengo (1, 2), Clara E. Martínez-Vázquez (3, 4), Brian Chaboyer (5), Giuseppe Bono (6, 7), Vittorio F. Braga (7, 8), Massimo Dall'Ora (9), Valentina D'Orazi (6, 10), Michele Fabrizio (7, 11), Matteo Monelli (8, 12), Frédéric Thévenin (13) ((1) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (2) Department of Physics, Florida State University, Tallahassee, FL, USA, (3) Gemini Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Hilo, HI, USA, (4) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile, (5) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA, (6) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy, (7) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (8) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (9) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (10) INAF-Osservatorio Astronomico di Padova, Padova, Italy, (11) Space Science Data Center, Roma, Italy, (12) Departmento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain, (13) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France)
- http://arxiv.org/abs/2301.03777
The Galactic Chemical Evolution of phosphorus observed with IGRINS. (arXiv:2210.04940v1 [astro-ph.SR])
- Volume 17, Issue 40 - article #10
- G. Nandakumar (1), N. Ryde (1), M. Montelius (2), B. Thorsbro (3), H. Jönsson (4), G. Mace (5) (1) Lund Observatory, Department of Astronomy, Theoretical Physics, Lund University, Box 43, SE-221 00 Lund, Sweden, (2) Kapteyn Astronomical Institute, University of Groningen, Landleven 12, NL-9747 AD Groningen, the Netherlands, (3) Department of Astronomy, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan, (4) Materials Science, Applied Mathematics, Malmö, University, SE-205 06 Malmö, Sweden, (5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX 78712, USA
- http://arxiv.org/abs/2210.04940
Milky Way's eccentric constituents with $Gaia$, APOGEE $&$ GALAH. (arXiv:2206.07744v1 [astro-ph.GA])
- Volume 17, Issue 24 - article #13
- G. C. Myeong (1), Vasily Belokurov (2, 3), David S. Aguado (4, 5), N. Wyn Evans (2), Nelson Caldwell (1), James Bradley (2) ((1) Harvard-Smithsonian Center for Astrophysics, (2) Institute of Astronomy, Cambridge University, (3) Center for Computational Astrophysics, Flatiron Institute, (4) Dipartimento di Fisica e Astrofisica, (5) INAF/Osservatorio Astrofisico di Arcetri)
- http://arxiv.org/abs/2206.07744
The chemical enrichment of the Milky Way disk evaluated using conditional abundances. (arXiv:2206.02772v1 [astro-ph.GA])
- Volume 17, Issue 23 - article #4
- Bridget Ratcliffe (1), Melissa Ness (2, 3) ((1) Department of Statistics, Columbia University, (2) Department of Astronomy, Columbia University, (3) Center for Computational Astrophysics, Flatiron Institute)
- http://arxiv.org/abs/2206.02772
The chemical composition of globular clusters in the Local Group. (arXiv:2112.00081v1 [astro-ph.GA])
- Volume 16, Issue 49 - article #10
- S. S. Larsen (1), P. Eitner (2,3), E. Magg (3), M. Bergemann (3,4), C. A. S. Moltzer (1), J. P. Brodie (5,7), A. J. Romanowsky (6,7), J. Strader (8) ((1) Department of Astrophysics/IMAPP, Radboud University, (2) Ruprecht-Karls-Universitaet, Heidelberg, (3) MPIA, Heidelberg, (4) Niels Bohr Academy, Niels Bohr Institute, Copenhagen, (5) Centre for Astrophysics, Supercomputing, Swinburne University, (6) Department of Physics, Astronomy, San Jose State Univ., (7) University of California Observatories, Santa Cruz, (8) Department of Physics, Astronomy, Michigan State University)
- http://arxiv.org/abs/2112.00081
SDSS-IV MaStar: Theoretical Atmospheric Parameters for the MaNGA Stellar Library. (arXiv:2111.05347v1 [astro-ph.GA])
- Volume 16, Issue 46 - article #7
- Lewis Hill (1), Daniel Thomas (1, 2), Claudia Maraston (1), Renbin Yan (3), Justus Neumann (1), Andrew Lundgren (1), Daniel Lazarz (3), Yan-Ping Chen (4), Michele Cappellari (5), Jon A. Holtzman (6), Julie Imig (6), Katia Cunha (7, 8), Guy Stringfellow (9), Dmitry Bizyaev (10, 11), David R. Law (12), Keivan G. Stassun (13), Niv Drory (14), Michael Merrifield (15), Timothy C. Beers (16) ((1) Institute of Cosmology, Gravitation, University of Portsmouth, UK, (2) School of Mathematics, Physics, University of Portsmouth, UK, (3) Department of Physics, Astronomy, University of Kentucky, USA, (4) New York University Abu Dhabi, Abu Dhabi, United Arab Emirates, (5) Department of Physics, University of Oxford, UK, (6) Department of Astronomy, New Mexico State University, USA, (7) Observatório Nacional/MCTIC, Brazil, (8) Steward Observatory, University of Arizona, USA, (9) Center for Astrophysics, Space Astronomy, University of Colorado, USA, (10) Apache Point Observatory, New Mexico State University, USA, (11) Sternberg Astronomical Institute, Moscow State niversity, Russia, (12) Space Telescope Science Institute, USA, (13) Vanderbilt University Physics, Astronomy Dept, USA, (14) McDonald Observatory, The University of Texas at Austin, USA, (15) School of Physics, Astronomy, University of Nottingham, UK, (16) Department of Physics, JINA Center for the Evolution of the Elements, University of Notre Dame, USA)
- http://arxiv.org/abs/2111.05347
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets. (arXiv:2111.01753v1 [astro-ph.EP])
- Volume 16, Issue 45 - article #9
- Robert F. Wilson (1, 2), Caleb I. Cañas (3, 4), Steven R. Majewski (1), Katia Cunha (5, 6), Verne V. Smith (7), Chad F. Bender (6), Suvrath Mahadevan (3, 4), Scott W. Fleming (8), Johanna Teske (9), Luan Ghezzi (10), Henrik Jönsson (11), Rachael L. Beaton (12, 13), Sten Hasselquist (14), Keivan Stassun (15), Christian Nitschelm (16), D. A. García-Hernández (17, 18), Christian R. Hayes (19), Jamie Tayar (20, 21) ((1) University of Virginia Department of Astronomy, (2) NASA Goddard Space Flight Center, (3) The Pennsylvania State University Department of Astronomy & Astrophysics, (4) The Pennsylvania State University Center for Exoplanets, Habitable Worlds, (5) Observatório Nacional, (6) Steward Observatory, (7) NSF's NOIRLab, (8) Space Telescope Science Institute, (9) Carnegie Earth, Planets Laboratory, (10) Universidade Federal do Rio de Janeiro, (11) Malmö University Materials Science, Applied Mathematics, (12) Princeton University Department of Astrophysical Sciences, (13) The Observatories of the Carnegie Institution for Science, (14) University of Utah Department of Physics & Astronomy, (15) Vanderbilt University Department of Physics, Astronomy, (16) Universidad de Antofagasta Centro de Astronomía, (17) Instituto de Astrofísica de Canarias, (18) Departamento de Astrofísica Universidad de La Laguna, (19) University of Washington Department of Astronomy, (20) University of Hawai'i at Manoa Institute for Astronomy, (21) University of Florida Department of Astronomy)
- http://arxiv.org/abs/2111.01753
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. (arXiv:2109.11600v1 [astro-ph.SR])
- Volume 16, Issue 40 - article #2
- Carlos Andrés Galarza (1), Simone Daflon (1), Vinicius M. Placco (2), Carlos Allende-Prieto (3, 4), Marcelo Borges Fernandes (1), Haibo Yuan (5), Carlos López-Sanjuan (6), Young Sun Lee (7), Enrique Solano (8), F. Jiménez-Esteban (8), David Sobral (9), Alvaro Alvarez Candal (1, 17), Claudio B. Pereira (1), Stavros Akras (10), Eduardo Martín (3, 8), Yolanda Jiménez Teja (16), Javier Cenarro (6), David Cristóbal-Hornillos (6), Carlos Hernández-Monteagudo (6), Antonio Marín-Franch (6), Mariano Moles (6), Jesús Varela (6), Héctor Vázquez Ramió, (6), Jailson Alcaniz (1), Renato Dupke (1, 13, 14, 15), Alessandro Ederoclite (11), Laerte Sodré, Jr. (11), Raul E. Angulo (12) ((1) Observatório Nacional - MCTI ON, Rio de Janeiro, Brazil, (2) NSF's NOIRLab, Tucson, AZ 85719, USA, (3) Instituto de Astrofísica de Canarias, Tenerife, Spain, (4) Universidad de La Laguna, Departamento de Astrofísica, Tenerife, Spain, (5) Department of Astronomy, Beijing Normal University, Beijing, People's Republic of China, (6) Centro de Estudios de Física del Cosmos de Aragón CEFCA, Unidad Asociada al CSIC, Teruel, Spain, (7) Department of Astronomy, Space Science, Chungnam National University, South Korea, (8) Departamento de Astrofísica, Centro de Astrobiología CSIC-INTA, ESAC Campus, Villanueva de la Cañada, Madrid, Spain, (9) Department of Physics, Lancaster University, Lancaster, UK, (10) Institute for Astronomy, Astrophysics, Space Applications, Remote Sensing, National Observatory of Athens, GR Penteli, Greece, (11) Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, São Paulo, Brazil, (12) Ikerbasque, Basque Foundation for Science, Bilbao, Spain, (13) Department of Astronomy, University of Michigan, Ann Arbor, MI USA, (14) Eureka Scientific Inc., Oakland, CA, USA, (15) Department of Physics, Astronomy, University of Alabama, Tuscaloosa, AL, USA, (16) Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía, Granada, Spain, (17) Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain)
- http://arxiv.org/abs/2109.11600
Dynamical model of the Milky Way using APOGEE and Gaia data. (arXiv:2106.05286v1 [astro-ph.GA])
- Volume 16, Issue 24 - article #2
- Maria Selina Nitschai (1), Anna-Christina Eilers (2), Nadine Neumayer (1), Michele Cappellari (3), Hans-Walter Rix (1) ((1) Max Planck Institute for Astronomy, (2) MIT Kavli Institute for Astrophysics, Space Research, (3) Sub-department of Astrophysics, Department of Physics, University of Oxford)
- http://arxiv.org/abs/2106.05286
On the Use of Field RR Lyrae as Galactic Probes. III. The $alpha$-element abundances. (arXiv:2104.08113v1 [astro-ph.GA])
- Volume 16, Issue 17 - article #2
- J. Crestani (1,2,3), V.F. Braga (3,4), M. Fabrizio (3,4), G. Bono (2,3), C. Sneden (5), G.W. Preston (6), I. Ferraro (3), G. Iannicola (3), M. Nonino (7), G. Fiorentino (3), F. Thévenin (8), B. Lemasle (9), Z. Prudil (8), A. Alves-Brito (1), G. Altavilla (3,4), B. Chaboyer (10), M. Dall'Ora (11), V. D'Orazi (12,13), C.K. Gilligan (10), E. Grebel (8), A.J. Koch-Hansen (9), H. Lala (9), M. Marengo (14), S. Marinoni (3,4), P.M. Marrese (3,4), C.E. Martínez-Vázquez (15), N. Matsunaga (16), M. Monelli (17), J.P. Mullen (14), J. Neeley (18), R. da Silva (3,4), P.B. Stetson (19), M. Salaris (20), J. Storm (21), E. Valenti (22), M. Zoccali (23,24) ((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil, (2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy, (3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (4) Space Science Data Center, Roma, Italy, (5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA, (6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy, (8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France, (9) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany, (10) Department of Physics, Astronomy, Dartmouth College, Hanover, USA, (11) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (12) INAF-Osservatorio Astronomico di Padova, Padova, Italy, (13) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia, (14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (15) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile, (16) Department of Astronomy, The University of Tokyo, Tokyo, Japan, (17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (18) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA, (19) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada, (20) Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK, (21) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany, (22) European Southern Observatory, Garching bei Munchen, Germany, (23) Instituto Milenio de Astrofísica, Santiago, Chile, (24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
- http://arxiv.org/abs/2104.08113
Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: I. Period-Fourier-Metallicity Relations for Fundamental Mode RR Lyrae. (arXiv:2103.09372v1 [astro-ph.SR])
- Volume 16, Issue 12 - article #5
- Joseph P. Mullen (1), Massimo Marengo (1), Clara E. Martínez-Vázquez (2), Jillian R. Neeley (3), Giuseppe Bono (4, 5), Massimo Dall'Ora (6), Brian Chaboyer (7), Frédéric Thévenin (8), Vittorio F. Braga (5, 9), Juliana Crestani (4, 5,, 10), Michele Fabrizio (5, 9), Giuliana Fiorentino (5), Christina K. Gilligan (7), Matteo Monelli (11, 12), Peter B. Stetson (13) ((1) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (2) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile, (3) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA, (4) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy, (5) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (6) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (7) Department of Physics, Astronomy, Dartmouth College, Hanover, USA, (8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France, (9) Space Science Data Center, Roma, Italy, (10) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil, (11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (12) Departmento de Astrofísica, Universidad de La Laguna, La Laguna, Tenerife, Spain, (13) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada)
- http://arxiv.org/abs/2103.09372
R-process-rich stellar streams in the Milky Way. (arXiv:2102.00066v1 [astro-ph.SR])
- Volume 16, Issue 6 - article #5
- Maude Gull (1,2), Anna Frebel (2), Karina Hinojosa (2), Ian U. Roederer (3,4), Alexander P. Ji (5), Kaley Brauer ((1) Department of Astronomy, University of California Berkeley, Berkeley, CA USA, (2) Department of Physics & Kavli Institute for Astrophysics, Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA, (3) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA, (4) Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements (JINA-CEE), USA, (5) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA)
- http://arxiv.org/abs/2102.00066
On the Use of Field RR Lyrae as Galactic Probes. II. A new $Delta$S calibration to estimate their metallicity. (arXiv:2012.02284v1 [astro-ph.SR])
- Volume 15, Issue 50 - article #6
- J. Crestani (1,2,3), M. Fabrizio (3,4), V.F. Braga (3,4), C. Sneden (5), G.W. Preston (6), I. Ferraro (3), G. Iannicola (3), G. Bono (2,3), A. Alves-Brito (1), M. Nonino (7), V. D'Orazi (8,9), L. Inno (10), M. Monelli (11), J. Storm (12), G. Altavilla (3,4), B. Chaboyer (13), M. Dall'Ora (14), G. Fiorentino (3), C.K. Gilligan (13), E. Grebel (15), H. Lala (16), B. Lemasle (16), M. Marengo (17), S. Marinoni (3,4), P.M. Marrese (3,4), C.E. Martínez-Vázquez (18), N. Matsunaga (19), J.P. Mullen (17), J. Neeley (20), Z. Prudil (15), R. da Silva (3,4), P.B. Stetson (21), F. Thévenin (15), E. Valenti (22), A.R. Walker (18), M. Zoccali (23,24) ((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil, (2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy, (3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (4) Space Science Data Center, Roma, Italy, (5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA, (6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy, (8) INAF-Osservatorio Astronomico di Padova, Padova, Italy, (9) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia, (10) Università degli Studi di Napoli "Parthenope'', Napoli, Italy, (11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (12) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany, (13) Department of Physics, Astronomy, Dartmouth College, Hanover, USA, (14) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (15) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France, (16) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany, (17) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (18) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile, (19) Department of Astronomy, The University of Tokyo, Tokyo, Japan, (20) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA, (21) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada, (22) European Southern Observatory, Garching bei Munchen, Germany, (23) Instituto Milenio de Astrofísica, Santiago, Chile, (24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
- http://arxiv.org/abs/2012.02284
The Gaia spectrophotometric standard stars survey -- IV. Results of the absolute photometry campaign. (arXiv:2011.08625v2 [astro-ph.SR] UPDATED)
- Volume 15, Issue 48 - article #6
- G. Altavilla (1, 2), S. Marinoni (1, 2), E. Pancino (3, 2), S. Galleti (4), M. Bellazzini (4), N. Sanna (3), M. Rainer (3), G. Tessicini (4), J.M. Carrasco (5), A. Bragaglia (4), W.J. Schuster (6), G. Cocozza (4), M. Gebran (7), H. Voss (5), L. Federici (4), E. Masana (5), C. Jordi (5), M. Monguió, (5), A. Castro (8, 9), M.A. Peña-Guerrero (10), A. Pérez-Villegas (11, 6) ((1) INAF -- Osservatorio Astronomico di Roma, Italy, (2) Space Science Data Center -- ASI, Italy, (3) INAF -- Osservatorio Astrofisico di Arcetri, Italy, (4) INAF -- Osservatorio di Astrofisica e Scienza dello Spazio, Italy, (5) Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Spain, (6) Instituto de Astronomía, Universidad Nacional Autónoma de México, México, (7) Department of Physics, Astronomy, Notre Dame University-Louaize, Lebanon, (8) Observatorio Astronómico Nacional, Universidad Nacional Autónoma de México, México, (9) Consorcio de Investigación del Golfo de México, CICESE, México, (10) Space Telescope Science Institute, USA, (11) Universidade de São Paulo, IAG, Brazil)
- http://arxiv.org/abs/2011.08625
Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars. (arXiv:2010.13620v1 [astro-ph.SR])
- Volume 15, Issue 44 - article #6
- D. Karinkuzhi (1,2,3), S. Van Eck (2), S. Goriely (2), L. Siess (2), A. Jorissen (2), T. Merle (2), A. Escorza (2,4), T. Masseron (5,6) ((1). Department of Physics, Indian Institute of Science, Bangalore, India.560012, (2). Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium, (3). Department of Physics, Jnana Bharathi Campus, Bangalore University, Bangalore, India. 560056, (4). Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium, (5). Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain, (6). Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain)
- http://arxiv.org/abs/2010.13620
Preliminary Target Selection for the DESI Milky Way Survey (MWS). (arXiv:2010.11284v1 [astro-ph.GA])
- Volume 15, Issue 43 - article #4
- Carlos Allende Prieto (1, 2), Andrew P. Cooper (3), Arjun Dey (4), Boris T. Gänsicke (5), Sergey E. Koposov (6, 7, 8), Ting Li (9, 10), Christopher Manser (5), David L. Nidever (4, 11), Constance Rockosi (12, 13), Mei-Yu Wang (7, 14), David S. Aguado (8), Robert Blum (15), David Brooks (16), Daniel J. Eisenstein (17), Yutong Duan (18), Sarah Eftekharzadeh (19), Enrique Gaztañaga (20, 21), Robert Kehoe (22), Martin Landriau (23), Chien-Hsiu Lee (4), Michael E. Levi (23) Aaron M. Meisner (4), Adam D. Myers (24), Joan Najita (4), Knut Olsen (25), Nathalie Palanque-Delabrouille (26), Claire Poppett (23, 27), Francisco Prada (28), David J. Schlegel (23), Michael Schubnell (29), Gregory Tarlé, (29), Monica Valluri (30), Risa H. Wechsler (31, 32), Christophe Yèche (26) ((1) Instituto de Astrofísica de Canarias, (2) Universidad de La Laguna, (3) National Tsing Hua University. (4) NSF's NOIRLab, (5) Department of Physics, University of Warwick, (6) Institute for Astronomy, University of Edinburgh, (7) McWilliams Center for Cosmology, Carnegie Mellon University, (8) Institute of Astronomy, University of Cambridge, (9) Observatories of the Carnegie Institution for Science, (10) Department of Astrophysical Sciences, Princeton University, (11) Department of Physics, Montana State University, (12) Department of Astronomy, Astrophysics, University of California Santa Cruz, (13) University of California Observatories, (14) Department of Physics, Carnegie Mellon University, (15) Vera C. Rubin Observatory/NSF's NOIRLab, (16) Department of Physics, Astronomy, University College London, (17) Harvard-Smithsonian Center for Astrophysics, (18) Physics Department, Boston University, (19) Department of Physics, Astronomy, The University of Utah, (20) Institute of Space Sciences (ICE, CSIC), (21) Institut d' Estudis Espacials de Catalunya (IEEC), (22) Department of Physics, Southern Methodist University, (23) Lawrence Berkeley National Laboratory, (24) University of Wyoming, (25) Community Science, Data Center/NSF's NOIRLab, (26) IRFU, CEA, Université Paris-Saclay, (28) Instituto de Astrofisica de Andalucía, (29) Department of Physics, University of Michigan, (30) Department of Astronomy, University of Michigan, (31) Kavli Institute for Particle Astrophysics, Cosmology, Department of Physics, (32) SLAC National Accelerator Laboratory)
- http://arxiv.org/abs/2010.11284
The stochastic enrichment of Population II stars. (arXiv:2010.10532v1 [astro-ph.GA])
- Volume 15, Issue 43 - article #6
- Louise Welsh (1), Ryan Cooke (1), Michele Fumagalli (2,1) ((1) Centre for Extragalactic Astronomy, Durham University, (2) Physics department, University of Milano Bicocca)
- http://arxiv.org/abs/2010.10532
An extremely metal-deficient globular cluster in the Andromeda Galaxy. (arXiv:2010.07395v1 [astro-ph.GA])
- Volume 15, Issue 42 - article #1
- S. S. Larsen (1), A. J. Romanowsky (2,4), J. P. Brodie (3,4), A. Wasserman (4) ((1) Department of Astrophysics/IMAPP, Radboud University, Nijmegen, The Netherlands, (2) Department of Physics, Astronomy, San Jose State University, San Jose, CA, USA, (3) Centre for Astrophysics, Supercomputing, Swinburne University of Technology, Hawthorn, VIC, Australia, (4) University of California Observatories, University of California, Santa Cruz, CA, USA)
- http://arxiv.org/abs/2010.07395
Mergers of binary neutron star systems: a multi-messenger revolution. (arXiv:2009.12255v1 [astro-ph.HE])
- Volume 15, Issue 40 - article #9
- Elena Pian (1) ((1) INAF, Astrophysics, Space Science Observatory, Bologna, Italy)
- http://arxiv.org/abs/2009.12255
The First Stellar Parallaxes Revisited. (arXiv:2009.11913v1 [astro-ph.SR])
- Volume 15, Issue 40 - article #14
- Mark J. Reid (1), Karl M. Menten (2) ((1) Center for Astrophysics | Harvard & Smithsonian, (2) Max-Planck-Institut fuer Radioastronomie)
- http://arxiv.org/abs/2009.11913
Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine. (arXiv:2008.10136v1 [astro-ph.SR])
- Volume 15, Issue 35 - article #2
- A. A. Mura-Guzmán (1,2), D. Yong (1,2), C. Abate (3), A. Karakas (4,2), C. Kobayashi (5,2), H. Oh (6), S. Chun (6), G. Mace (7). ((1) Research School of Astronomy, Astrophysics, Australian National University, Australia, (2) ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia, (3) Deep Blue Srl, Rome, Italy, (4) School of Physics, Astronomy, Monash University, Australia, (5) Centre for Astrophysics Research, University of Hertfordshire, UK, (6) Korea Astronomy, Space Science Institute, Republic of Korea, (7) Department of Astronomy, McDonald Observatory, University of Texas at Austin, USA.)
- http://arxiv.org/abs/2008.10136
Mapping the Galactic disk with the LAMOST and $Gaia$ Red clump sample: V: On the origin of the "young" [$alpha$/Fe]-enhanced stars. (arXiv:2008.10218v1 [astro-ph.GA])
- Volume 15, Issue 35 - article #5
- Weixiang Sun (1), Yang Huang (1), Haifeng Wang (1), Chun Wang (2,3), Meng Zhang (2,3), Xinyi Li (1), Bingqiu Chen (1), Huawei Zhang (2,3), Dandan Wei (4), Dengkai Jiang (4), Xiaowei Liu (1), ((1) South-Western Institute for Astronomy Research, Yunnan University, (2) Department of Astronomy, Peking University, (3) Kavli Institute for Astronomy, Astrophysics, Peking University, (4) Yunnan Observatories, Chinese Academy of Sciences)
- http://arxiv.org/abs/2008.10218
SkyMapper Southern Survey: Second Data Release (DR2). (arXiv:2008.10359v1 [astro-ph.IM])
- Volume 15, Issue 35 - article #6
- Christopher A. Onken (1), Christian Wolf (1), Michael S. Bessell (1), Seo-Won Chang (1), Gary S. Da Costa (1), Lance C. Luvaul (1), Dougal Mackey (1), Brian P. Schmidt (1), Li Shao (1, 2) ((1) Research School of Astronomy & Astrophysics, Australian National University, (2) Kavli Institute for Astronomy, Astrophysics, Peking University)
- http://arxiv.org/abs/2008.10359
The Initial Mass Function in the ELT era. (arXiv:2006.14997v1 [astro-ph.SR])
- Volume 15, Issue 27 - article #6
- Kieran Leschinski (1), João Alves (1) ((1) Department of Astrophysics, University of Vienna)
- http://arxiv.org/abs/2006.14997
Elemental Abundances in M31: Iron and Alpha Element Abundances in M31's Outer Halo
- Volume 15, Issue 24 - article #6
- Karoline M. Gilbert (1, 2), Jennifer Wojno (2), Evan N. Kirby (3), Ivanna Escala (3, 4), Rachael L. Beaton (4, 5, 6, 7), Puragra Guhathakurta (8), Steven R. Majewski (9) ((1) Space Telescope Science Institute, (2) Department of Physics & Astronomy, Johns Hopkins University, (3) California Institute of Technology, (4) Department of Astrophysical Sciences, Princeton University, (5) The Observatories of the Carnegie Institution for Science, (6) Hubble Fellow, (7) Carnegie-Princeton Fellow, (8) UCO/Lick Observatory, Department of Astronomy & Astrophysics, University of California Santa Cruz, (9) Department of Astronomy, University of Virginia)
- http://arxiv.org/abs/2006.05430
High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations. (arXiv:2006.06013v1 [astro-ph.SR])
- Volume 15, Issue 24 - article #9
- P. E. Nissen, J. Christensen-Dalsgaard, J. R. Mosumgaard, V. Silva Aguirre, E. Spitoni, K. Verma. (Stellar Astrophysics Centre, Department of Physics, Astronomy, Aarhus University, Denmark.)
- http://arxiv.org/abs/2006.06013
Hydrodynamics of core-collapse supernovae and their progenitors
- Volume 15, Issue 24 - article #10
- B. Müller (Monash University, School of Physics and Astronomy)
- http://arxiv.org/abs/2006.05083
Chronologically dating the early assembly of the Milky Way. (arXiv:2006.01783v1 [astro-ph.GA])
- Volume 15, Issue 23 - article #4
- Josefina Montalbán (1), John Ted Mackereth (1), Andrea Miglio (1, 2), Fiorenzo Vincenzo (3,4, 1), Cristina Chiappini (5), Gaël Buldgen (6), Benoît Mosser (7), Arlette Noels (8), Richard Scuflaire (8), Mathieu Vrard (4, 10), Emma Willett (1, 2), Guy R. Davies (1, 2), Oliver Hall (1, 2) Martin Bo Nielsen (1,2, 11), Saniya Khan (1, 2), Ben M. Rendle (1, 2), Walter E. van Rossem (1, 2), Jason W. Ferguson (9), William J. Chaplin (1, 2) ((1) School of Physics, Astronomy, University of Birmingham, UK, (2) SAC, Aarhus University, Denmark, (3) Center for Cosmology, AstroParticle Physics, The Ohio State University, USA, (4) Departement of Astronomy, The Ohio State University, USA, (5) Leibniz-Institut fur Astrophysik Potsdam, Germany, (6) Observatoire de Genève, Université de Genève, Switzerland, (7) LESIA, Observatoire de Paris, Université de Paris, France, (8) STAR Institute, University of Liège, Belgium, (9) Departement of Physics, Wichita State University, USA, (10) Instituto de Astrofśica e Ciências do Espaço, Universidade do Porto, Portugal, (11) Center for Space Science, NYUAD, New York University Abu Dhabi, United Arab Emirates)
- http://arxiv.org/abs/2006.01783
Helium Enhancement in the Metal Rich Red Giants of Omega Centauri. (arXiv:2005.06807v1 [astro-ph.SR])
- Volume 15, Issue 20 - article #3
- B. P. Hema (1), Gajendra Pandey (1), R. L. Kurucz (2), C. Allende Prieto (3), ((1) Indian Institute of Astrophysics, Koramangala II Block, Bengaluru, Karnataka, India (2) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA (3) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, Departamento de Astrofisica, Universidad de La Laguna, La Laguna, Tenerife, Spain)
- http://arxiv.org/abs/2005.06807
PypeIt: The Python Spectroscopic Data Reduction Pipeline. (arXiv:2005.06505v1 [astro-ph.IM])
- Volume 15, Issue 20 - article #5
- J. Xavier Prochaska (1, 2), Joseph F. Hennawi (3), Kyle B. Westfall (4), Ryan J. Cooke (5), Feige Wang (6), Tiffany Hsyu (1), Emanuele Paolo Farina (7) ((1) University of California, Santa Cruz, (2) Kavli Institute for the Physics, Mathematics of the Universe, (3) University of California, Santa Barbara, (4) University of California Observatories, (5) Durham University, UK, (6) Steward Observatory, University of Arizona, (7) Max Planck Institut fur Astrophysik)
- http://arxiv.org/abs/2005.06505
Omega Centauri: weak MgH-band in red giants directly trace the helium content. (arXiv:2004.09415v1 [astro-ph.SR])
- Volume 15, Issue 17 - article #6
- Arumalla B. S. Reddy (Indian Institute of Astrophysics, Koramangala, Bangalore, India)
- http://arxiv.org/abs/2004.09415
Production of Lithium in Primordial Supernovae. (arXiv:2002.04749v1 [astro-ph.SR])
- Volume 15, Issue 7 - article #7
- Alexander Heger (1), Stan Woosley (2) ((1) School of Physics, Astronomy, Monash University, Australia, (2) Department of Astronomy, Astrophysics, University of California at Santa Cruz, USA)
- http://arxiv.org/abs/2002.04749
Candidate Hypervelocity Red Clump Stars in the Galactic Bulge Found Using the VVV and Gaia Surveys. (arXiv:1912.02129v1 [astro-ph.GA])
- Volume 14, Issue 49 - article #3
- Alonso Luna (1, 2), Dante Minniti (2, 3, 4), Javier Alonso-García (3, 5) ((1) Instituto de Astronomía, Universidad Nacional Autónoma de México, México, (2) Depto. de Ciencias Físicas, Facultad de Ciencias Exactas, Universidad Andres Bello, Chile, (3) Millennium Institute of Astrophysics, Chile, (4) Vatican Observatory, Italy, (5) Centro de Astronomía (CITEVA), Universidad de Antofagasta, Chile)
- http://arxiv.org/abs/1912.02129
Identification of strontium in the merger of two neutron stars. (arXiv:1910.10510v1 [astro-ph.HE])
- Volume 14, Issue 43 - article #4
- Darach Watson (1, 2), Camilla J. Hansen (3), Jonatan Selsing (1, 2), Andreas Koch (4), Daniele B. Malesani (1, 2, 5), Anja C. Andersen (1), Johan P. U. Fynbo (1, 2), Almudena Arcones (6, 7), Andreas Bauswein (7, 8), Stefano Covino (9), Aniello Grado (10), Kasper E. Heintz (1, 2, 11), Leslie Hunt (12), Chryssa Kouveliotou (13, 14), Giorgos Leloudas (1, 5), Andrew Levan (15, 16), Paolo Mazzali (17, 18), Elena Pian (19) ((1) Niels Bohr Institute, University of Copenhagen, (2) Cosmic Dawn Center (DAWN), (3) Max-Planck-Institut für Astronomie, Heidelberg, (4) Zentrum für Astronomie der Universität Heidelberg, (5) DTU Space, Technical University of Denmark, (6) Institut für Kernphysik, Technische Universität Darmstadt, (7) GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, (8) Heidelberger Institut für Theoretische Studien, Heidelberg, (9) INAF / Brera Astronomical Observatory, Merate, (10) INAF-OACN, Naples, (11) Centre for Astrophysics, Cosmology, University of Iceland, (12) INAF - Osservatorio Astrofisico di Arcetri, Firenze, (13) Physics Department, the George Washington University, (14) Astronomy, Physics, Statistics Institute of Sciences (APSIS), Washington, DC, (15) Department of Astrophysics/IMAPP, Radboud University Nijmegen, (16) Department of Physics, University of Warwick, (17) Astrophysics Research Institute, Liverpool John Moores University, (18) Max-Planck Institute for Astrophysics, Garching, (19) INAF, Astrophysics, Space Science Observatory, Bologna)
- http://arxiv.org/abs/1910.10510
Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri. (arXiv:1906.08550v1 [astro-ph.SR])
- Volume 14, Issue 25 - article #2
- D. Magurno (1, 2, 3), C. Sneden (4), G. Bono (1, 2), V. F. Braga (5, 6), M. Mateo (7), S. E. Persson (8), G. Preston (8), F. Thevenin (9), R. da Silva (10), M. Dall'Ora (11), M. Fabrizio (2, 10), I. Ferraro (2), G. Fiorentino (12), G. Iannicola (2), L. Inno (13), M. Marengo (14), S. Marinoni (10), P. M. Marrese (10), C. E. Martinez-Vazquez (15), N. Matsunaga (16), M. Monelli (17), J. R. Neeley (18), M. Nonino (19), A. R. Walker (15) ((1) University of Roma Tor Vergata - Department of Physics - Roma - Italy, (2) INAF Osservatorio Astronomico di Roma - Monte Porzio Catone RM - Italy, (3) University of Bologna - Department of Physics, Astronomy - Bologna - Italy, (4) Department of Astronomy, McDonald Observatory - The University of Texas - Austin - TX - USA, (5) Instituto Milenio de Astrofisica - Santiago - Chile, (6) Departamento de Fisica - Facultad de Ciencias Exactas - Universidad Andres Bello - Las Condes - Santiago - Chile, (7) Department of Astronomy - University of Michigan - Ann Arbor - MI - USA, (8) Observatories of the Carnegie Institution for Science - Pasadena - CA 91101 - USA, (9) Universite de La Cote d'Azur - OCA - Laboratoire Lagrange CNRS - Nice Cedex - France, (10) SSDC - via del Politecnico snc - I-00133 Roma - Italy, (11) INAF Osservatorio Astronomico di Capodimonte - Salita Moiariello 16 - Napoli - Italy, (12) INAF Osservatorio Astronomico di Bologna - Via Ranzani 1 - Bologna - Italy, (13) Max Planck Institute fur Astronomie - Konigstuhl - Heidelberg - Germany, (14) Department of Physics, Astronomy - Iowa State University - Zaffarano - Ames - IA - USA, (15) Cerro Tololo Inter-American Observatory - National Optical Astronomy Observatory - Casilla - La Serena - Chile, (16) Department of Astronomy - The University of Tokyo - Hongo - Bunkyo-ku - Tokyo - Japan, (17) IAC - Instituto de Astrofsica de Canarias - Calle Via Lactea - La Laguna - Tenerife - Espana, (18) Department of Physics - Florida Atlantic University - Boca Raton - FL - USA, (19) INAF Osservatorio Astronomico di Trieste - Trieste - Italy)
- http://arxiv.org/abs/1906.08550
ACRONYM: Acronym CReatiON for You and Me. (arXiv:1903.12180v1 [astro-ph.IM])
- Volume 14, Issue 14 - article #1
- B. A Cook (1) ((1) Center for Astrophysics | Harvard & Smithsonian)
- http://arxiv.org/abs/1903.12180
Astro2020 Science White Paper: A Summary of Multimessenger Science with Galactic Binaries. (arXiv:1904.01601v1 [astro-ph.SR])
- Volume 14, Issue 14 - article #4
- Thomas Kupfer (Kavli Institute for Theoretical Physics), Mukremin Kilic (University of Oklahoma), Tom Maccarone (Texas Tech), Eric Burns (NASA Goddard), Chris L. Fryer (Los Alamos National Laboratory), Colleen A. Wilson-Hodge (NASA Marshall)
- http://arxiv.org/abs/1904.01601
HST resolves stars in a tiny body falling on the dwarf galaxy DDO 68. (arXiv:1904.01986v1 [astro-ph.GA])
- Volume 14, Issue 14 - article #6
- F. Annibali (1), M. Bellazzini (1), M. Correnti (2), E. Sacchi (2), M. Tosi (1), M. Cignoni (3), A. Aloisi (2), D. Calzetti (4), L. Ciotti (5), F. Cusano (1), J. Lee (6), C. Nipoti (5) ((1) INAF-Astrophysics, Space Science Observatory, Bologna, Italy (2) Space Telescope Science Institute, Baltimore, USA (3) Dipartimento di Fisica, Universita' di Pisa, Italy (4) Department of Astronomy, University of Massachusetts-Amherst, USA (5) Dipartimento di Fisica e Astronomia, Universita' di Bologna, Italy (6) Caltech-IPAC, USA)
- http://arxiv.org/abs/1904.01986
The Fornax 3D project: Thick disks in a cluster environment. (arXiv:1904.01260v1 [astro-ph.GA])
- Volume 14, Issue 14 - article #11
- F. Pinna (1, 2), J. Falcón-Barroso (1, 2), M. Martig (3), L. Coccato (4), E. M. Corsini (5, 6), P.T. de Zeeuw (7, 8), D.A. Gadotti (4), E. Iodice (9), R. Leaman (10), M. Lyubenova (4), I. Martín-Navarro (11, 10), L. Morelli (12, 6), M. Sarzi (13), G. van de Ven (14, 4), S. Viaene (15, 16), R.M. McDermid (17, 18) ((1) Instituto de Astrofísica de Canarias, (2) Depto. Astrofísica, Universidad de La Laguna, (3) Astrophysics Research Institute, Liverpool John Moores University, (4) European Southern Observatory, (5) Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova, (6) INAF-Osservatorio Astronomico di Padova, (7) Sterrewacht Leiden, Leiden University, (8) Max-Planck-Institut fuer extraterrestrische Physik, (9) INAF-Osservatorio Astronomico di Capodimonte, (10) Max-Planck Institut fuer Astronomie, (11) University of California Observatories, (12) Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama, (13) Armagh Observatory, Planetarium, (14) Department of Astrophysics, University of Vienna, (15) Sterrenkundig Observatorium, Universiteit Gent, (16) Centre for Astrophysics Research, University of Hertfordshire, (17) Department of Physics, Astronomy, Macquarie University, (18) Australian Astronomical Observatory)
- http://arxiv.org/abs/1904.01260
The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees. (arXiv:1902.11265v1 [astro-ph.GA])
- Volume 14, Issue 9 - article #7
- K. Kuijken (1), C. Heymans (2), A. Dvornik (1), H. Hildebrandt (3,4), J.T.A. de Jong (5), A.H. Wright (4), T. Erben (4), M. Bilicki (1,6), B. Giblin (2), H.-Y. Shan (4,7), F. Getman (8), A. Grado (8), H. Hoekstra (1), L. Miller (9), N. Napolitano (10,8), M. Paolilo (11), M. Radovich (12), P. Schneider (4), W. Sutherland (13), M. Tewes (4), C. Tortora (14), E.A. Valentijn (5), G.A. Verdoes Kleijn (5) ((1) Leiden Observatory, (2) SUPA, Edinburgh, (3) Astronomisches Inst., Bochum, (4) Argelander Inst., Bonn, (5) Kapteyn Astronomical Inst., Groningen, (6) Ctr. For Theoretical Physics, Polish Academy of Sciences, Warsaw, (7) Shanghai Astronomical Observatory, (8) INAF Capodimonte, (9) Dept. of Physics, Oxford, (10) School of Physics, Astronomy, Sun Yat-sen University, Guangzhou, (11) Dept. of Physics, Univ. Federico II, Naples, (12) INAF Padua, (13) School of Physics, Astronomy, Queen Mary University, London, (14) INAF Arcetri)
- http://arxiv.org/abs/1902.11265
Mapping the stellar age of the Milky Way bulge with the VVV. I. The method. (arXiv:1902.01695v1 [astro-ph.GA])
- Volume 14, Issue 6 - article #2
- F. Surot (1, 4), E. Valenti (1), S. L. Hidalgo (2, 3), M. Zoccali (4, 5), E. Sökmen (2, 3), M. Rejkuba (1, 6), D. Minniti (5, 7, 8), O. A. Gonzalez (9), S. Cassisi (10, 11), A. Renzini (12), A. Weiss (13) ((1) European Southern Observatory, (2) Instituto de Astrofísica de Canarias, (3) Department of Astrophysics University of La Laguna, (4) Instituto de Astrofísica Pontificia Universidad Católica de Chile, (5) Millennium Institute of Astrophysics, (6) Excellence Cluster Universe, (7) Departamento de Ciencias Físicas Universidad Andrés Bello, (8) Vatican Observatory, (9) Institute for Astronomy University of Edinburgh, (10) INAF - Astronomical Observatory of Abruzzo, (11) INFN, (12) INAF - Osservatorio Astronomico di Padova, (13) Max-Planck-Institut für Astrophysik)
- http://arxiv.org/abs/1902.01695
Variable stars in Terzan 5: additional evidence of multi-age and multi-iron stellar populations. (arXiv:1812.04325v1 [astro-ph.GA])
- Volume 13, Issue 50 - article #5
- L. Origlia (1), A. Mucciarelli (2,1), G. Fiorentino (1), F.R. Ferraro (2,1), E. Dalessandro (1), B. Lanzoni (2,1), R.M. Rich (3), D. Massari (4), R.R. Contreras (5,6), N. Matsunaga (7)- (1 INAF-OAS, Bologna, Italy, 2 Bologna University, Italy, 3 UCLA, USA, 4 University of Groningen, The Netherlands, 5 Millennium Institute of Astrophysics, Santiago, Chile, 6 Pontificia Universidad Catolica de Chile, Santiago, Chile, 7 University of Tokyo, Japan)
- http://arxiv.org/abs/1812.04325
On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $omega$ Centauri as a first test case. (arXiv:1811.07069v1 [astro-ph.SR])
- Volume 13, Issue 47 - article #2
- G. Bono (1, 2), G. Iannicola (2), V.F. Braga (3, 4), I. Ferraro (2), P.B. Stetson (5), D. Magurno (1), N. Matsunaga (6), R.L. Beaton (7), R. Buonanno (8), B. Chaboyer (9), M. Dall'Ora (10), M. Fabrizio (2, 11), G. Fiorentino (12), W.L. Freedman (13,7), C.K. Gilligan (9), B.F. Madore (7), M. Marconi (10), M. Marengo (14), S. Marinoni (2, 11), P. Marrese (2, 11), C.E. Martinez-Vazquez (15), M. Mateo (16), M. Monelli (17, 18), J.R. Neeley (19), M. Nonino (20), C. Sneden (21), F. Thevenin (22), E. Valenti (23), A.R. Walker (15) ((1) Department of Physics, Università di Roma Tor Vergata, Roma, Italy, (2) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (3) Instituto Milenio de Astrofisica, Santiago, Chile, (4) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile, (5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria BC, Canada, (6) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Nagano Japan, (7) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (8) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy, (9) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA, (10) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (11) SSDC, Roma, Italy, (12) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy, (13) Department of Astronomy, Astrophysics, University of Chicago, Chicago, IL, USA, (14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (15) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile, (16) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA, (17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (18) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain, (19) Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA, (20) INAF-Osservatorio Astronomico di Trieste, Trieste, Italy, (21) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA, (22) Universite de Nice Sophia-antipolis, CNRS, Observatoire de la Cote d'Azur, Laboratoire Lagrange, Nice, France, (23) European Southern Observatory, Garching bei Munchen, Germany)
- http://arxiv.org/abs/1811.07069
GAIA Cepheid parallaxes and 'Local Hole' relieve $H_0$ tension. (arXiv:1810.02595v1 [astro-ph.CO])
- Volume 13, Issue 41 - article #6
- Tom Shanks, Lucy Hogarth, Nigel Metcalfe (Department of Physics, Durham University, UK)
- http://arxiv.org/abs/1810.02595
Local disc model in view of Gaia DR1 and RAVE data. (arXiv:1810.00814v1 [astro-ph.GA])
- Volume 13, Issue 40 - article #5
- K. Sysoliatina (1), A. Just (1), I. Koutsouridou (2), E.K. Grebel (1), G. Kordopatis (8), M. Steinmetz (10), O. Bienaymé, (9), B.K. Gibson (3), J. Navarro (7), W. Reid (5,6), G. Seabroke (4) ((1) Astronomisches Rechen-Institut, Heidelberg, Germany, (2) Observatoire de Paris, France, (3) E.A. Milne Centre for Astrophysics, University of Hull, UK, (4) Mullard Space Science Laboratory, University College London, UK, (5) Department of Physics, Astronomy, Macquarie University, Sydney, Australia, (6) Western Sydney University, Australia, (7) Senior CIfAR Fellow, University of Victoria, Canada, (8) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France, (9) Observatoire astronomique de Strasbourg, Université de Strasbourg, France, (10) Leibniz Institut für Astrophysik Potsdam, Germany)
- http://arxiv.org/abs/1810.00814
The faint end of the Centaurus A satellite luminosity function. (arXiv:1809.05103v1 [astro-ph.GA])
- Volume 13, Issue 38 - article #9
- D. Crnojević, (1,2), D. J. Sand (3), P. N. Bennet (2), S. Pasetto (4,1), K. Spekkens (5), N. Caldwell (6), P. Guhathakurta (7), B. McLeod (6), A. Seth (8), J. D. Simon (4), J. Strader (9), E. Toloba (10) ((1) University of Tampa, Tampa, FL, USA, (2) Department of Physics & Astronomy, Texas Tech University, Lubbock, TX, USA, (3) Department of Astronomy, Steward Observatory, University of Arizona, Tucson, AZ, USA, (4) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (5) Department of Physics & Space Science, Royal Military College of Canada, Kingston, Ontario, Canada, (6) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA, (7) Department of Astronomy & Astrophysics, University of California Santa Cruz, CA, USA, (8) Department of Physics, Astronomy, University of Utah, Salt Lake City, UT, USA, (9) Department of Physics, Astronomy, Michigan State University, East Lansing, MI, USA, (10), Department of Physics, University of the Pacific, Stockton, CA, USA)
- http://arxiv.org/abs/1809.05103
Structure and kinematics of Type II Cepheids in the Galactic bulge based on near-infrared VVV data. (arXiv:1808.10838v1 [astro-ph.GA])
- Volume 13, Issue 36 - article #9
- V.F. Braga (1,2), A. Bhardwaj (3), R. Contreras Ramos (1,4), D. Minniti (1,2,5), G. Bono (6,7), R. de Grijs (8,9), J.H. Minniti (4,10), M. Rejkuba (11) ((1) Instituto Milenio de Astrofísica, Santiago, Chile, (2) Departamento de Física, Facultad de Ciencias Exactas, Universidad Andrés Bello, Santiago, Chile, (3) Kavli Institute for Astronomy, Astrophysics, Peking University, China, (4) Pontificia Universidad Católica de Chile, Instituto de Astrofísica, Macul, Chile, (5) Vatican Observatory, Italy, (6) Department of Physics, Università di Roma Tor Vergata, Italy, (7) INAF-Osservatorio Astronomico di Roma, Italy, (8) Department of Physics, Astronomy, Macquarie University, Balaclava Road, Sydney, Australia, (9) International Space Science Institute--Beijing, Zhongguancun, China, (10) European Southern Observatory, Santiago, Chile, (11) European Southern Observatory, Garching, Germany)
- http://arxiv.org/abs/1808.10838
The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS) I: A Pilot Study of the stellar populations in NGC 2298 and NGC 3201. (arXiv:1808.05271v1 [astro-ph.GA])
- Volume 13, Issue 34 - article #4
- Stephanie Monty (1,2), Thomas H. Puzia (3), Bryan W. Miller (4), Eleazar R. Carrasco (4), Mirko Simunovic (5), Mischa Schirmer (4,6), Peter B. Stetson (7), Santi Cassisi (8), Kim A. Venn (1), Aaron Dotter (9), Paul Goudfrooij (10), Sibilla Perina (11), Peter Pessev (12), Ata Sarajedini (13), Matthew A. Taylor (5) ((1) Department of Physics, Astronomy, University of Victoria, Canada, (2) Research School of Astronomy, Astrophysics, Australian National University, Australia, (3) Institute of Astrophysics, Pontificia Universidad Catolica de Chile, Santiago, Chile, (4) Gemini Observatory/AURA, Southern Operations Center, Chile, (5) Gemini Observatory, USA, (6) Max-Planck-Institut fuer Astronomie, Germany, (7) Herzberg Astronomy, Astrophysics, National Research Council Canada, Canada, (8) INAF - Astronomical Observatory of Abruzzo, Italy, (9) Harvard-Smithsonian Center for Astrophysics, USA, (10) Space Telescope Science Institute, USA, (11) INAF - Astronomical Observatory of Torino, Italy, (12) Gran Telescopio Canarias, Instituto de Astrofisica de Canarias, Universidad de La Laguna, Spain, (13) Department of Astronomy, University of Florida, 211 Bryant Space Science Center Gainesville, FL, USA)
- http://arxiv.org/abs/1808.05271
When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic. (arXiv:1807.06332v1 [astro-ph.SR])
- Volume 13, Issue 29 - article #16
- D. Karinkuzhi (1), S. Van Eck (1), A. Jorissen (1), S. Goriely (1), L. Siess (1), T. Merle (1), A. Escorza (1, 2), M. Van der Swaelmen (1), H.M.J. Boffin (3), T. Masseron (4,5), S. Shetye (1,2), B. Plez (6) ((1). Institute of Astronomy, Astrophysics, University of Brussels, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium. (2) Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium. (3) ESO, Karl Schwarzschild Strasse 2, D-85748 Garching bei Munchen, Germany. (4) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain. (5) Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain. (6) Laboratoire Univers et Particules de Montpellier, Universite Montpellier, CNRS, 34095, Montpellier Cedex 05, France.)
- http://arxiv.org/abs/1807.06332
Dwarf Galaxies with Ionizing Radiation Feedback. I: Escape of Ionizing Photons. (arXiv:1210.3361v5 [astro-ph.GA] UPDATED)
- Volume 13, Issue 11 - article #2
- Ji-hoon Kim (1,2), Mark R. Krumholz (1), John H. Wise (3), Matthew J. Turk (4), Nathan J. Goldbaum (1), Tom Abel (2) ((1) University of California, Santa Cruz, (2) Kavli Institute for Particle Astrophysics, Cosmology, Stanford University, (3) Georgia Institute of Technology, (4) Columbia University)
- http://arxiv.org/abs/1210.3361
The local rotation curve of the Milky Way based on SEGUE and RAVE data. (arXiv:1802.07658v1 [astro-ph.GA])
- Volume 13, Issue 8 - article #12
- K. Sysoliatina (1), A. Just (1), O. Golubov (2,3,4), Q.A. Parker (5,6), E.K. Grebel (1), G. Kordopatis (17), T. Zwitter (15), J. Bland-Hawthorn (14), B.K. Gibson (8), A. Kunder (16), U. Munari (7), J. Navarro (12), W. Reid (10,11), G. Seabroke (9), M.Steinmetz (18), F. Watson (13) ((1) Astronomisches Rechen-Institut, Heidelberg, Germany, (2) Schools of Physics, Technology, Karazin Kharkiv National University, Kharkiv, Ukraine, (3) Institute of Astronomy, Karazin Kharkiv National University, Kharkiv, Ukraine, (4) Department of Aerospace Engineering Sciences, University of Colorado at Boulder, USA, (5) Department of Physics, the University of Hong Kong, China, (6) The Laboratory for Space Research, the university of Hong Kong, China, (7) INAF Astronomical Observatory of Padova, Italy, (8) E.A. Milne Centre for Astrophysics, University of Hull, UK, (9) Mullard Space Science Laboratory, University College London, UK, (10) Department of Physics, Astronomy, Macquarie University, Sydney, Australia, (11) Western Sydney University, Australia, (12) Senior CIfAR Fellow, University of Victoria, Canada, (13) Australian Astronomical Observatory (14) Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia, (15) Faculty of Mathematics, Physics, University of Ljubljana, Slovenia, (16) Saint Martin's University, Lacey, USA, (17) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France, (18) Leibniz Institut für Astrophysik Potsdam, Germany)
- http://arxiv.org/abs/1802.07658
The Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations. (arXiv:1802.07319v1 [astro-ph.GA])
- Volume 13, Issue 8 - article #14
- S. L. Hidalgo (1, 2), A. Pietrinferni (3), S. Cassisi (3), M. Salaris (4), A. Mucciarelli (5, 6), A. Savino (4, 7), A. Aparicio (1, 2), V. Silva Aguirre (8), K. Verma (8) ((1) Instituto de Astrofísica de Canarias, (2) Department of Astrophysics of University of La Laguna, (3) INAF-Osservatorio Astronomico d'Abruzzo, (4) Astrophysics Research Institute Liverpool John Moores University, (5) Dipartimento di Fisica e Astronomia - Universitá a degli Studi di Bologna, (6) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, (7) Kapteyn Astronomical Institute University of Groningen, (8) Stellar Astrophysics Centre Department of Physics, Astronomy Aarhus University)
- http://arxiv.org/abs/1802.07319
On the RR Lyrae stars in globulars: V. the complete Near-Infrared (JHKs) census of omega Centauri RR Lyrae variables. (arXiv:1802.03578v1 [astro-ph.SR])
- Volume 13, Issue 7 - article #7
- V. F. Braga (1, 2, 3, 4), P. B. Stetson (5), G. Bono (3, 6), M. Dall'Ora (7), I. Ferraro (6), G. Fiorentino (8), G. Iannicola (6), M. Marconi (7), M. Marengo (9), A. J. Monson (10), J. Neeley (9), S. E. Persson (10), R. L. Beaton (10), R. Buonanno (3, 11), A. Calamida (12), M. Castellani (6), E. Di Carlo (11), M. Fabrizio (4), W. L. Freedman (13), L. Inno (14), B. F. Madore (10), D. Magurno (3), E. Marchetti (15), S. Marinoni (4), P. Marrese (4), N. Matsunaga (16), D. Minniti (1, 2, 17), M. Monelli (18), M. Nonino (19), A. M. Piersimoni (11), A. Pietrinferni (11), P. Prada-Moroni (20, 21), L. Pulone (6), R. Stellingwerf (22), E. Tognelli (20, 21), A. R. Walker (23), E. Valenti (15), M. Zoccali (1, 24) ((1) Instituto Milenio de Astrofisica, Santiago, Chile, (2) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile, (3) Department of Physics, Università di Roma Tor Vergata, Roma, Italy, (4) SSDC, Roma, Italy, (5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria, Canada, (6) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy, (7) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy, (8) INAF-Osservatorio Astronomico di Bologna, Bologna, Italy, (9) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA, (10) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (11) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy, (12) National Optical Astronomy Observatory, Tucson AZ, USA, (13) Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA, (14) Max Planck Institute for Astronomy, Heidelberg, Germany, (15) European Southern Observatory, Garching bei Munchen, Germany, (16) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Kiso-machi, Japan, (17) Vatican Observatory, Vatican City State, Italy, (18) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain, (19) INAF, Osservatorio Astronoico di Trieste, Trieste, Italy, (20) INFN, Sezione di Pisa, Pisa, Italy, (21) Dipartimento di Fisica "Enrico Fermi", Università di Pisa, Pisa, Italy, (22) Stellingwerf Consulting, Huntsville, AL, USA, (23) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile, (24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
- http://arxiv.org/abs/1802.03578
Mixture Models in Astronomy. (arXiv:1711.11101v1 [astro-ph.IM])
- Volume 12, Issue 48 - article #5
- Michael A. Kuhn (1,2), Eric D. Feigelson (3,1) ((1) Millennium Institute of Astrophysics, (2) Universidad de Valparaíso, (3) Pennsylvania State University)
- http://arxiv.org/abs/1711.11101
Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions. (arXiv:1705.03642v1 [astro-ph.SR])
- Volume 12, Issue 19 - article #2
- T. Mishenina (1), M. Pignatari (2,3,6), B.Cot'e (3,4,5,6), F.-K. Thielemann (7), C. Soubiran (8), N. Basak (1), T. Gorbaneva (1), S.A. Korotin (1,9), V.V. Kovtyukh (1), B. Wehmeyer (7), S. Bisterzo (3,10,11), C. Travaglio (3,10,11), B.K. Gibson (2,6), C. Jordan (2,6), A. Paul (4), C. Ritter (3,6), F. Herwig (3,6) ((1) Astronomical Observatory, Odessa National University,, Isaac Newton Institute of Chile, Odessa branch, Odessa, Ukraine, (2) E.A. Milne Centre for Astrophysics, University of Hull, (3) The NuGrid Collaboration, (4) Department of Physics, Astronomy, University of Victoria, (5) National Superconducting Cyclotron Laboratory, Michigan State University, (6) Joint Institute for Nuclear Astrophysics Center for the Evolution of the Elements, (7) Department of Physics, University of Basel, (8) Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux - CNRS, B18N, allée Geoffroy Saint-Hilaire, (9) Crimean Astrophysical Observatory, (10) INAF, Astrophysical Observatory Turin, Strada Osservatorio 20, (11) B2FH Association)
- http://arxiv.org/abs/1705.03642
Chemical characterization of the globular cluster NGC 5634 associated to the Sagittarius dwarf spheroidal galaxy. (arXiv:1701.03116v1 [astro-ph.SR])
- Volume 12, Issue 2 - article #1
- Eugenio Carretta (1), Angela Bragaglia (1), Sara Lucatello (2), Valentina D'Orazi (2,3,4), Raffaele G. Gratton (2), Paolo Donati (1,5), Antonio Sollima (1), Chris Sneden (6) ((1) INAF-Osservatorio Astronomico di Bologna, (2) INAF-Osservatorio Astronomico di Padova, (3) Dept. of Physics, Astronomy, Macquarie Univ., (4) Monash Centre for Astrophysics, (5) DIFA, Universita' di Bologna, (6) Dept. of Astronomy, McDonald Observatory, The University of Texas, Austin, USA)
- http://arxiv.org/abs/1701.03116
Pan-STARRS Photometric and Astrometric Calibration. (arXiv:1612.05242v1 [astro-ph.IM])
- Volume 11, Issue 51 - article #5
- Eugene. A. Magnier (1), Edward. F. Schlafly (2,3), Douglas P. Finkbeiner (4,5), J. L. Tonry (1), B. Goldman (6), S. Röser (7), E. Schilbach (7), K. C. Chambers (1), H. A. Flewelling (1), M. E. Huber (1), P. A. Price (8), W. E. Sweeney (1), C. Z. Waters (1), L. Denneau (1), P. Draper (9), K. W. Hodapp (1), R. Jedicke (1), R.-P. Kudritzki (1), N. Metcalfe (9), C. W. Stubbs (10), R. J. Wainscoast (1) ((1) UH Institute for Astronomy, (2) Lawrence Berkeley National Laboratory, (3) Hubble Fellow, (4) ITC Harvard-Smithsonian Center for Astrophysics, (5) Department of Physics Harvard University, (6) Max Planck Institute for Astronomy, (7) Astronomisches Rechen-Institut Zentrum für Astronomie der Universität Heidelberg, (8) Department of Astrophysical Sciences Princeton University, (9) Department of Physics Durham University, (10) Harvard-Smithsonian Center for Astrophysics)
- http://arxiv.org/abs/1612.05242
On the dearth of ultra-faint extremely metal poor galaxies. (arXiv:1612.00273v1 [astro-ph.GA])
- Volume 11, Issue 49 - article #8
- J. Sanchez Almeida (1, 2), M. E. Filho (1, 2,, 3), C. Dalla Vecchia (1, 2), E. D. Skillman (4) ((1) Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, (2) Departamento de Astrofisica, Universidad de La Laguna, (3) SIM/FEUP, Porto, Portugal, (4) Minnesota Institute for Astrophysics, School of Physics, Astronomy, University of Minnesota, Minneapolis, USA.)
- http://arxiv.org/abs/1612.00273
Chemical analysis of a carbon-enhanced very metal-poor star: CD-27 14351. (arXiv:1611.01637v1 [astro-ph.SR])
- Volume 11, Issue 46 - article #4
- Drisya Karinkuzhi (1), Aruna Goswami (1), Thomas Masseron (2) ((1) Indian Institute of Astrophysics, Koramangala, Bangalore 560034, (2) Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK)
- http://arxiv.org/abs/1611.01637
On the RR Lyrae stars in globulars: IV. $omega$ Centauri Optical UBVRI Photometry. (arXiv:1609.04916v1 [astro-ph.SR])
- Volume 11, Issue 39 - article #12
- V. F. Braga (1, 2), P. B. Stetson (3), G. Bono (1, 4), M. Dall'Ora (5), I. Ferraro (4), G. Fiorentino (6), L. M. Freyhammer (7), G. Iannicola (4), M. Marengo (8), J. Neeley (8), E. Valenti (9), R. Buonanno (1, 10), A. Calamida (11), M. Castellani (4), R. da Silva (4, 2), S. Degl'Innocenti (12, 13), A. Di Cecco (10), M. Fabrizio (10, 2), W. L. Freedman (14), G. Giuffrida (4, 2), J. Lub (15), B. F. Madore (16), M. Marconi (5), S. Marinoni (4, 2), N. Matsunaga (17), M. Monelli (18), S. E. Persson (16), A. M. Piersimoni (10), A. Pietrinferni (10), P. Prada-Moroni (12, 13), L. Pulone (4), R. Stellingwerf (19), E. Tognelli (12, 13), A. R. Walker (20) ((1) Department of Physics, Università di Roma Tor Vergata (2) ASDC (3) NRC-Herzberg, Dominion Astrophysical Observatory (4) INAF-Osservatorio Astronomico di Roma (5) INAF-Osservatorio Astronomico di Capodimonte (6) INAF-Osservatorio Astronomico di Bologna (7) Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire (8) Department of Physics, Astronomy, Iowa State University (9) European Southern Observatory (10) INAF-Osservatorio Astronomico di Teramo (11) National Optical Astronomy Observatory (12) INFN, Sezione di Pisa (13) Dipartimento di Fisica Enrico Fermi, Università di Pisa (14) Department of Astronomy & Astrophysics, University of Chicago (15) Sterrewacht Leiden, Leiden University (16) The Observatories of the Carnegie Institution for Science (17) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo (18) Instituto de Astrofísica de Canarias (19) Stellingwerf Consulting (20) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory)
- http://arxiv.org/abs/1609.04916
The evolution of the Milky Way: New insights from open clusters. (arXiv:1609.02619v1 [astro-ph.GA])
- Volume 11, Issue 38 - article #10
- Arumalla B. S. Reddy (1), David L. Lambert (1), Sunetra Giridhar (2) ((1) W.J. McDonald Observatory, Department of Astronomy, The University of Texas at Austin (2) Indian Institute of Astrophysics)
- http://arxiv.org/abs/1609.02619
Shaken and Stirred: The Milky Way's Dark Substructures. (arXiv:1609.01718v1 [astro-ph.GA])
- Volume 11, Issue 37 - article #13
- Till Sawala (1), Pauli Pihajoki (1), Peter H. Johansson (1), Carlos S. Frenk (2), Julio F. Navarro (3), Kyle A. Oman (3), Simon D. M. White (4) ((1) University of Helsinki, Finland (2) Institute for Computational Cosmology, University of Durham, UK (3) University of Victoria, Canada (4) Max-Planck Institute for Astrophysics, Garching, Germany)
- http://arxiv.org/abs/1609.01718
Abundance analysis of s-process enhanced barium stars. (arXiv:1608.06734v1 [astro-ph.SR])
- Volume 11, Issue 35 - article #2
- Upakul Mahanta (1,2), Drisya Karinkuzhi (3), Aruna Goswami (3), Kalpana Duorah (2) ((1). Department of Physics, Bajali College, Pathsala, Assam, 781325, India, (2). Department of Physics, Gauhati University, Guwahati 781014, Assam, India, (3). Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India)
- http://arxiv.org/abs/1608.06734
The Age and Distance of the Kepler Open Cluster NGC 6811 from an Eclipsing Binary, Turnoff Star Pulsation, and Giant Asteroseismology. (arXiv:1608.03917v1 [astro-ph.SR])
- Volume 11, Issue 34 - article #7
- Eric L. Sandquist (San Diego State University), J. Jessen-Hansen (Aarhus University), Matthew D. Shetrone (McDonald Observatory), Karsten Brogaard (Aarhus University), Soren Meibom (Harvard-Smithsonian Center for Astrophysics), Marika Leitner (Humboldt State University), Dennis Stello (Sydney Institute for Astronomy), Hans Bruntt (Aarhus University), Victoria Antoci (Aarhus University), Jerome A. Orosz (San Diego State University), Frank Grundahl (Aarhus University), Soren Frandsen (Aarhus University)
- http://arxiv.org/abs/1608.03917
Open journals that piggyback on arXiv gather momentum
- Volume 11, Issue 6 - article #18
- Peer-review platforms built around online pre-print repositories spread to astrophysics.
- Nature - Volume: 530, Issue: 7588
- 8-124
The extended halo of Centaurus A: uncovering satellites, streams and substructures
- Volume 10, Issue 46 - article #17
- D. Crnojević, (1), D. J. Sand (1), K. Spekkens (2), N. Caldwell (3), P. Guhathakurta (4), B. McLeod (3), A. Seth (5), J. Simon (6), J. Strader (7), E. Toloba (1,4) ((1) Department of Physics, Texas Tech University, Lubbock, TX, USA, (2) Department of Physics, Royal Military College of Canada, Kingston, Ontario, Canada, (3) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA, (4) UCO/Lick Observatory, University of California, Santa Cruz, CA, USA, (5) Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA, (6) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (7) Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Dec
- arXiv:1512.05366 [pdf, ps, other]
Subaru/HDS study of CH stars: elemental abundances for stellar neutron-capture process studies
- Volume 10, Issue 40 - article #15
- Aruna Goswami (1), Wako Aoki (2), Drisya Karinkuzhi (1) ((1) Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India (2) National Astronomical Observatory, Mitaka, Tokyo, 181-8588 Japan)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 30 Oct
- arXiv:1510.07814 [pdf, ps, other]
Resolving the extended stellar halos of nearby galaxies: the wide-field PISCeS survey
- Volume 10, Issue 38 - article #7
- D. Crnojević, (1), D. J. Sand (1), N. Caldwell (2), P. Guhathakurta (3), B. McLeod (2), A. Seth (4), J. D. Simon (5), J. Strader (6), E. Toloba (1,3) ((1) Texas Tech University, Physics Department, Lubbock, TX, USA, (2) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA, (3) UCO/Lick Observatory, University of California, Santa Cruz, CA, USA, (4) Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA, (5) Observatories of the Carnegie Institution for Science, Pasadena, CA, USA, (6) Michigan State University, Department of Physics and Astronomy, East Lansing, MI, USA)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 16 Oct
- arXiv:1510.03487 [pdf, ps, other]
Post first dredge-up [C/N] ratio as age indicator. Theoretical calibration
- Volume 10, Issue 35 - article #3
- Maurizio Salaris (1), Adriano Pietrinferni (2), Anna M. Piersimoni (2), Santi Cassisi (2,3) ((1) Astrophysics Research Institute, Liverpool John Moores University, United Kingdom, (2) INAF-Osservatorio Astronomico di Collurania, Italy, (3) Instituto de Astrofisica de Canarias, La Laguna, Spain)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 25 Sep
- arXiv:1509.06904 [pdf, ps, other]
Inclusion of Horizontal Branch stars in the derivation of star formation histories of dwarf galaxies: the Carina dSph
- Volume 10, Issue 34 - article #2
- Alessandro Savino (1 and 2), Maurizio Salaris (1), Eline Tolstoy (2) ((1) Astrophysics Research Institute, Liverpool John Moores University, (2) Kapteyn Astronomical Institute, University of Groningen)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Sep
- arXiv:1509.04929 [pdf, other]
Discovery of low-metallicity stars in the central parsec of the Milky Way
- Volume 10, Issue 25 - article #23
- Tuan Do (1 and 2), Wolfgang Kerzendorf (3 and 4), Nathan Winsor (1 and 5), Morten Støstad (3), Mark R. Morris (2), Jessica R. Lu (6), Andrea M. Ghez (2) ((1) Dunlap Institute, University of Toronto, (2) Physics and Astronomy Department, UCLA, (3) Department of Astronomy, University of Toronto, (4) ESO, (5) Grenfell Campus, Memorial University of Newfoundland, (6) IfA, University of Hawaii)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 3 Jul
- arXiv:1506.07891 [pdf, other]
Chemical abundances of giant stars in NGC 5053 and NGC 5634, two globular clusters associated with the Sagittarius dwarf Spheroidal galaxy?
- Volume 10, Issue 18 - article #5
- L. Sbordone (1,2), L. Monaco (3,4), C. Moni Bidin (5), P. Bonifacio (6), S. Villanova (7), M. Bellazzini (8), R. Ibata (9), M. Chiba (10), D. Geisler (7), E. Caffau (6), S. Duffau (1,2) ((1) Millennium Institute for Astrophysics, Chile, (2) Pontificia Universidad Catolica de Chile, Santiago, Chile, (3) European Southern Observatory, Santiago, Chile, (4) Departamento de Ciencias Fisicas, Universidad Andres Bello, Santiago, Chile, (5) Instituto de Astronomia, Universidad Catolica del Norte, Antofagasta, Chile (6) GEPI, Observatoire de Paris, PSL Resarch University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cite, Meudon, France, (7) Departamento de Astronomia, Universidad de Concepcion, Concepcion, Chile, (8) INAF-Osservatorio Astronomico di Bologna, Bologna, Italy, (9) Observatoire Astronomique de Strasbourg, Universite de Strasbourg, CNRS, Strasbourg, France, (10) Astronomical Institute, Tohoku University, Sendai, Japan)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 8 May
- arXiv:1505.01487 [pdf, other]
Understanding AGB evolution in Galactic bulge stars from high-resolution infrared spectroscopy
- Volume 10, Issue 18 - article #18
- S. Uttenthaler (1), J. A. D. L. Blommaert (2,3), P. R. Wood (4), T. Lebzelter (1), B. Aringer (5,1), M. Schultheis (6), N. Ryde (7) ((1) University of Vienna, Department of Astrophysics, (2) Department of Physics and Astrophysics, Vrije Universiteit Brussel, (3) Instituut voor Sterrenkunde, KU Leuven, (4) Research School of Astronomy and Astrophysics, Australian National University, (5) Department of Physics and Astronomy G. Galilei, University of Padova, (6) Laboratoire Lagrange, Université de Nice Sophia Antipolis, (7) Lund Observatory, Sweden)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 8 May
- arXiv:1505.01425 [pdf, ps, other]
Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
- Volume 10, Issue 16 - article #3
- Oliver Just (1,2), Andreas Bauswein (3), Ricard Ardevol Pulpillo (1,4), Stephane Goriely (5), H.-Thomas Janka (1) ((1) MPI Astrophysics, Garching, (2) MPPC, (3) Univ. Thessaloniki, (4) Physik Dept., TUM, Garching, (5) ULB Brussels)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 24 Apr
- arXiv:1504.05448 [pdf, other]
TOPoS: II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies
- Volume 10, Issue 16 - article #19
- P. Bonifacio (1), E. Caffau (1,2), M. Spite (2), M. Limongi (3,4), A. Chieffi (5), R.S. Klessen (6,7,8), P. François (1,9), P. Molaro (10), H. G. Ludwig (2,1), S. Zaggia (11), F. Spite (1), B. Plez (12), R. Cayrel (1), N. Christlieb (2), P.C. Clark (13,6), S.C.O. Glover (6), F. Hammer (1), A. Koch (2), L. Monaco (14,15), L. Sbordone (16,17), M. Steffen (18,1) ((1) GEPI, Observatoire de Paris, (2) ZAH-LSW, (3) INAF - OA Roma, (4) Kavli IPMU, Univ. Tokyo (5) INAF - IASFC, (6) ZAH-ARI, (7) Kavli, IPAC, Stanford Univ., (8) Dep A&A Univ, Calfornia, (9) UPJV, Univ. Picardie, (10) INAF - OA Trieste, (11) INAF- OA Padova, (12) LUPM, Univ. Montpellier, (13) School of Physics and Astronomy, Cardiff Univ. (14) ESO, (15) DCF - Univ. A. Bello, (16) MAS, (17) PUC - Chile, (18) Leibniz-Institut AIP)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 24 Apr
- arXiv:1504.05963 [pdf, ps, other]
Nucleosynthesis of heavy elements in gamma ray bursts
- Volume 10, Issue 13 - article #7
- Agnieszka Janiuk, Bartlomiej Kaminski (Center for Theoretical Physics, PAS)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 3 Apr
- arXiv:1504.00145 [pdf, ps, other]
Kinematics and Velocity Ellipsoid of the Solar Neighborhood White Dwarfs
- Volume 10, Issue 10 - article #8
- W. H. Elsanhoury, M. I. Nouh, H. I. Abdel-Rahman (Department of Astronomy, National Research Institute of Astronomy and Geophysics, Cairo, Egypt)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 13 Mar
- arXiv:1503.03595 [pdf]
The VLT Survey Telescope ATLAS
- Volume 10, Issue 7 - article #9
- T. Shanks (1), N. Metcalfe (1), B. Chehade (1), J.R. Findlay (1), M.J. Irwin (2), E. Gonzalez-Solares (2), J.R. Lewis (2), A. Kupcu Yoldas (2), R.G.Mann (3), M.A. Read (3), E.T.W. Sutorius (3), S. Voutsinas (3) ((1) Dept of Physics, Durham University, UK, (2) Institute of Astronomy, University of Cambridge, UK (3) Institute for Astronomy, University of Edinburgh, UK)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 20 Feb
- arXiv:1502.05432 [pdf, other]
Chemical Abundances of the Highly Obscured Galactic Globular Clusters 2MASS GC02 and Mercer 5
- Volume 10, Issue 5 - article #1
- Francisco Penaloza (Universidad de Valparaiso), Peter Pessev (Instituto de Astrofisica de Canarias; Gran Telescopio de Canarias), Sergio Vasquez (Pontifica Universidad Catolica de Chile; Milenium Institute of Astrophysics), Jura Borissova, Radostin Kurtev (Universidad de Valparaiso; Milenium Institute of Astrophysics), Manuela Zoccali (Pontifica Universidad Catolica de Chile; Milenium Institute of Astrophysics)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 6 Feb
- arXiv:1502.01627 [pdf, ps, other]
The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk
- Volume 10, Issue 5 - article #9
- Chiara Battistini (1), Thomas Bensby (1) ((1) Lund Observatory, Department of Astronomy and Theoretical Physics, Lund, Sweden)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 6 Feb
- arXiv:1502.01152 [pdf, other]
Chemical analysis of CH stars - II: atmospheric parameters and elemental abundances
- Volume 9, Issue 25 - article #3
- Drisya Karinkuzhi (1,2), Aruna Goswami (1) ((1) Indian Institute of Astrophysics, Koramangala (2) Department of physics, Bangalore university)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 12 Dec
- arXiv:1412.3548 [pdf, ps, other]
A search for open cluster Cepheids in the Galactic plane
- Volume 9, Issue 23 - article #11
- Xiaodian Chen (1,2,3), Richard de Grijs (1,2), Licai Deng (3) ((1) Kavli Institute for Astronomy and Astrophysics, Peking University (2) Department of Astronomy, Peking University (3) Key Laboratory for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Oct
- arXiv:1410.4489 [pdf, ps, other]
High-Resolution Spectroscopy of Extremely Metal-Poor Stars from SDSS/SEGUE: II. Binary Fraction
- Volume 9, Issue 23 - article #17
- Wako Aoki (1), Takuma Suda (1), Timothy C. Beers (3), Satoshi Honda (4) ((1) National Astronomical Observatory of Japan, (2) Joint Institute for Nuclear Astrophysics, (3) University of Hyogo)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 17 Oct
- arXiv:1410.2674 [pdf, ps, other]
Chemical analysis of CH stars - I: atmospheric parameters and elemental abundances
- Volume 9, Issue 23 - article #28
- Drisya Karinkuzhi (1,2), Aruna Goswami (1) ((1) Indian Institute of Astrophysics, Koramangala, India (2) Department of physics, Bangalore university, Jnana Bharathi Campus, Karnataka, India)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 3 Oct
- arXiv:1410.0111 [pdf, ps, other]
Nitrogen abundances and multiple stellar populations in the globular clusters of the Fornax dSph
- Volume 9, Issue 22 - article #42
- S. S. Larsen (1), J. P. Brodie (2), F. Grundahl (3), J. Strader (4) ((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen, The Netherlands, (2) UCO/Lick Observatory, UC Santa Cruz, USA, (3) Stellar Astrophysics Centre, Aarhus University, Denmark, (4) Department of Physics and Astronomy, Michigan State University, USA)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 5 Sep
- arXiv:1409.0541 [pdf, other]
Improved Estimates of the Milky Way's Stellar Mass and Star Formation Rate from Hierarchical Bayesian Meta-Analysis
- Volume 9, Issue 20 - article #5
- Timothy C. Licquia (1,2), Jeffrey A. Newman (1,2) ((1) University of Pittsburgh, (2) Pittsburgh Particle physics, Astrophysics, and Cosmology Center (PITT PACC))
- arXiv.org - Astrophysics - Volume: 2014, Issue: 11 Jul
- arXiv:1407.1078 [pdf, ps, other]
Searching for Dust around Hyper Metal-Poor Stars
- Volume 9, Issue 20 - article #9
- Kim A. Venn (University of Victoria), Thomas H. Puzia (Institute of Astrophysics, PUC), Mike Divell (University of Victoria), Stephanie Cote (NRC Herzberg Institute of Astrophysics), David L. Lambert (McDonald Observatory, University of Texas, Austin), Else Starkenburg (University of Victoria)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 11 Jul
- arXiv:1407.1449 [pdf, other]
The Milky Way as a High Redshift Galaxy: The Importance of Thick Disk Formation in Galaxies
- Volume 9, Issue 20 - article #24
- Matthew D. Lehnert (1), Paola Di Matteo (2), Misha Haywood (2), Owain N. Snaith (3) ((1) Institut d'Astrophysique de Paris, (2) GEPI, Observatoire de Paris, (3) Department of Physics & Astronomy, University of Alabama)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 13 Jun
- arXiv:1406.3039 [pdf, ps, other]
Stellar Variability in the VVV Survey: An Update
- Volume 9, Issue 20 - article #96
- M. Catelan (1,2), I. Dekany (2,1), M. Hempel (1,2), D. Minniti (1,2) ((1) Pontificia Universidad Catolica de Chile, (2) Millennium Institute of Astrophysics)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 27 Jun
- arXiv:1406.6727 [pdf, ps, other]
Stellar Mergers Are Common
- Volume 9, Issue 19 - article #6
- C.S. Kochanek (1), Scott M. Adams (1), Krzysztof Belczynski (2,3) ((1) Department of Astronomy and the Center for Cosmology and AstroParticle Physics, The Ohio State University, (2) Astronomical Observatory, Warsaw University, (3) Center for Gravitational Wave Astronomy, University of Texas at Brownsville)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 9 May
- arXiv:1405.1042 [pdf, other]
Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621
- Volume 9, Issue 18 - article #6
- Rolf-Peter Kudritzki (1), Miguel A. Urbaneja (2), Fabio Bresolin (1), Matthew. W. Hosek Jr (1), Norbert Przybilla (2) ((1) Institute for Astronomy, University of Hawaii (2) Institute for Astro- and Particle Physics, University of Innsbruck)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 2 May
- arXiv:1404.7244 [pdf, ps, other]

Results 1 - 100 of 361

Select Page: 1 2 3 4 Next
RSS Feed of This Search