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Results 1 - 63 of 63

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
JWST Imaging of Earendel, the Extremely Magnified Star at Redshift $z=6.2$. (arXiv:2208.09007v1 [astro-ph.GA])
- Volume 17, Issue 33 - article #4
- Brian Welch, Dan Coe, Erik Zackrisson, S.E. de Mink, Swara Ravindranath, Jay Anderson, Gabriel Brammer, Larry Bradley, Jinmi Yoon, Patrick Kelly, Jose M. Diego, Rogier Windhorst, Adi Zitrin, Paola Dimauro, Yolanda Jimenez-Teja, Abdurro'uf, Mario Nonino, Ana Acebron, Felipe Andrade-Santos, Roberto J. Avila, Matthew B. Bayliss, Alex Benitez, Tom Broadhurst, Rachana Bhatawdekar, Marusa Bradac, Gabriel Caminha, Wenlei Chen, Jan Eldridge, Ebraheem Farag, Michael Florian, Brenda Frye, Seiji Fujimoto, Sebastian Gomez, Alaina Henry, Tiger Y.-Y Hsiao, Taylor A. Hutchison, Bethan L. James, Meridith Joyce, Intae Jung, Gourav Khullar, Rebecca L. Larson, Guillaume Mahler, Nir Mandelker, Stephan McCandliss, Takahiro Morishita, Rosa Newshore, Colin Norman, Kyle O'Connor, Pascal A. Oesch, Masamune Oguri, et al. (13 additional authors not shown)
- http://arxiv.org/abs/2208.09007
Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-Faint Dwarf Galaxy in the Constellation Pegasus. (arXiv:2203.11788v1 [astro-ph.GA])
- Volume 17, Issue 12 - article #5
- W. Cerny, J. D. Simon, T. S. Li, A. Drlica-Wagner, A. B. Pace, C. E. Martınez-Vazquez, A. H. Riley, B. Mutlu-Pakdil, S. Mau, P. S. Ferguson, D. Erkal, R. R. Munoz, C. R. Bom, J. L. Carlin, D. Carollo, Y. Choi, A. P. Ji, D. Martınez-Delgado, V. Manwadkar, A. E. Miller, N. E. D. Noel, J. D. Sakowska, D. J. Sand, G. S. Stringfellow, E. J. Tollerud, A. K. Vivas, J. A. Carballo-Bello, D. Hernandez-Lang, D. J. James, J. L. Nilo Castellon, K. A. G. Olsen, A. Zenteno (DELVE Collaboration)
- http://arxiv.org/abs/2203.11788
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
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
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
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
EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with ?1.0 (Fe/O)? and 0.02 (O/H)? : Possible Traces of Super Massive (>300M?) Stars in Early Galaxies
- Volume 15, Issue 24 - article #7
- Takashi Kojima (1,2), Masami Ouchi (3,1,4), Michael Rauch (5), Yoshiaki Ono (1), Kimihiko Nakajima (3), Yuki Isobe (1,2), Seiji Fujimoto (6,7), Yuichi Harikane (3,8,1), Takuya Hashimoto (9), Masao Hayashi (3), Yutaka Komiyama (3), Haruka Kusakabe (10), Ji Hoon Kim (11,12), Chien-Hsiu Lee (13), Shiro Mukae (1,2), Tohru Nagao (14), Masato Onodera (11,15), Takatoshi Shibuya (16), Yuma Sugahara (17), Masayuki Umemura (18), Kiyoto Yabe (4) ((1) ICRR, (2) Univ. of Tokyo, (3) NAOJ, (4) Kavli IPMU, (5) Carnegie Observatory, (6) DAWN fellow, (7) Univ. of Copenhagen, (8) UCL, (9) TCHoU, (10) Observatoire de Geneve, (11) Subaru Telescope, (12) Metaspace, (13) NOAO, (14) Ehime Univ., (15) SOKENDAI, (16) Kitami Institute of Tech., (17) Waseda Univ., (18) Univ. of Tsukuba)
- http://arxiv.org/abs/2006.03831
The Sixth Data Release of the Radial Velocity Experiment (RAVE) -- II: Stellar Atmospheric Parameters, Chemical Abundances and Distances. (arXiv:2002.04512v1 [astro-ph.SR])
- Volume 15, Issue 7 - article #10
- Matthias Steinmetz, Guillaume Guiglion, Paul J. McMillan, Gal Matijevic, Harry Enke, Georges Kordopatis, Tomaz Zwitter, Marica Valentini, Cristina Chiappini, Luca Casagrande, Jennifer Wojno, Borja Anguiano, Olivier Bienayme, Albert Bijaoui, James Binney, Donna Burton, Paul Cass, Patrick de Laverny, Kristin Fiegert, Kenneth Freeman, Jon P. Fulbright, Brad K. Gibson, Gerard Gilmore, Eva K. Grebel, Amina Helmi, Andrea Kunder, Ulisse Munari, Julio F. Navarro, Quentin Parker, Gregory R. Ruchti, Alejandra Recio-Blanco, Warren Reid, George M. Seabroke, Alessandro Siviero, Arnaud Siebert, Milorad Stupar, Fred Watson, Mary E.K. Williams, Rosemary F.G. Wyse, Friedrich Anders, Teresa Antoja, Joss Bland-Hawthorn, Diego Bossini, Rafael A. Garcia, Ismael Carrillo, William J. Chaplin, Yvonne Elsworth, Benoit Famaey, et al. (13 additional authors not shown)
- http://arxiv.org/abs/2002.04512
Detection and characterisation of oscillating red giants: first results from the TESS satellite. (arXiv:1912.07604v1 [astro-ph.SR])
- Volume 14, Issue 51 - article #2
- Víctor Silva Aguirre, Dennis Stello, Amalie Stokholm, Jakob R. Mosumgaard, Warrick Ball, Sarbani Basu, Diego Bossini, Lisa Bugnet, Derek Buzasi, Tiago L. Campante, Lindsey Carboneau, William J. Chaplin, Enrico Corsaro, Guy R. Davies, Yvonne Elsworth, Rafael A. García, Patrick Gaulme, Oliver J. Hall, Rasmus Handberg, Marc Hon, Thomas Kallinger, Liu Kang, Mikkel N. Lund, Savita Mathur, Alexey Mints, Benoit Mosser, Zeynep Çelik Orhan, Thaíse S. Rodrigues, Mathieu Vrard, Mutlu Yıldız, Joel C. Zinn, Sibel Örtel, Paul G. Beck, Keaton J. Bell, Zhao Guo, Chen Jiang, James S. Kuszlewicz, Charles A. Kuehn, Tanda Li, Mia S. Lundkvist, Marc Pinsonneault, Jamie Tayar, Margarida S. Cunha, Saskia Hekker, Daniel Huber, Andrea Miglio, Mario J. P. F. G. Monteiro, Ditte Slumstrup, et al. (31 additional authors not shown)
- http://arxiv.org/abs/1912.07604
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
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
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
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
The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS. (arXiv:1804.05869v1 [astro-ph.SR])
- Volume 13, Issue 16 - article #10
- S. Buder (1), K. Lind (1,2), M. K. Ness (3,4), M. Asplund (5,6), L. Duong (5), J. Lin (5), J. Kos (7), L. Casagrande (5,6), J. Bland-Hawthorn (7,6), A. R. Casey (8), G. M. De Silva (9, 7), V. D'Orazi (10), K. C. Freeman (5), G. F. Lewis (7), S. L. Martell (11), K. J. Schlesinger (5), S. Sharma (7,6), J. D. Simpson (9), D. B. Zucker (12,9), T. Zwitter (13), K. Cotar (13), A. Dotter (14), M. R. Hayden (7,6), E. A. Hyde (15), P. R. Kafle (16), D. M. Nataf (17), T. Nordlander (5,6), W. Reid (15,12), H.-W. Rix (1), A. Skuladottir (1), D. Stello (11,18,7,6), Y.-S. Ting (19,20,21), G. Traven (13), R. F. G. Wyse (17) ((1) MPIA Heidelberg, (2) Uppsala University, (3) Columbia University New York, (4) CCA New York, (5) RSAA/MSO Canberra, (6) ASTRO-3D Australia, (7) SIfA Sydney, (8) Monash University, (9) AAO North Ryde, (10) INAF Padova, (11) UNSW Sydney, (12) Macquarie University Sydney, (13) University of Ljubljana, (14) Harvard/CfA Cambridge, (15) Western Sydney University, (16) University of Western Australia, (17) Johns Hopkins University Baltimore, (18) Aarhus University, (19) IAS Princeton, (20) Princeton University, (21) Carnegie Observatories Pasadena)
- http://arxiv.org/abs/1804.05869
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
- Volume 13, Issue 16 - article #12
- S. Buder (1,2), M. Asplund (3,4), L. Duong (3), J. Kos (5), K. Lind (1,6), M. K. Ness (7,8), S. Sharma (5,4), J. Bland-Hawthorn (5,4), A. R. Casey (9), G. M. De Silva (10,5), V. D'Orazi (11), K. C. Freeman (3), G. F. Lewis (5), J. Lin (3,4), S. L. Martell (12), K. J. Schlesinger (3), J. D. Simpson (10), D. B. Zucker (13,10), T. Zwitter (14), A. M. Amarsi (1), B. Anguiano (15), D. Carollo (16), K. Cotar (14), P. L. Cottrell (9,17), G. Da Costa (3), X. D. Gao (1), M. R. Hayden (5,4), J. Horner (18), M. J. Ireland (3), P. R. Kafle (19), U. Munari (20), D. M. Nataf (21), T. Nordlander (3,4), Dennis Stello (12,22,4), Y.-S. Ting (23,24,25), G. Traven (14), F. Watson (10,26), R. A. Wittenmyer (18), R. F. G. Wyse (21), D. Yong (3), J. C. Zinn (27), M. Zerjal (3) ((1) MPIA Heidelberg, (2) IMPRS HD, (3) RSAA/MSO Canberra, (4) ASTRO-3D Australia, (5) SIfA Sydney, (6) Uppsala University, (7) Columbia University New York, (8) CCA New York (9) Monash University, (10) AAO North Ryde, (11) INAF Padova, (12) UNSW Sydney, (13) Macquarie University Sydney, (14) University of Ljubljana, (15) University of Virginia, (16) INAF Turin, (17) University of Canterbury, (18) University of Southern Queensland, (19) University of Western Australia, (20) INAF Padova, (21) Johns Hopkins University Baltimore, (22) Aarhus University, (23) IAS Princeton, (24) Princeton University, (25) Carnegie Observatories Pasadena, (26) Western Sydney University, (27) The Ohio State University)
- http://arxiv.org/abs/1804.06041
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
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
Behavior of Abundances in Chemically Peculiar Dwarf and Subgiant A-Type Stars: HD 23193 and HD 170920. (arXiv:1801.00492v1 [astro-ph.SR])
- Volume 13, Issue 1 - article #2
- Tolgahan Kılıçoğlu, Şeyma Çalışkan, Kübraözge Ünal
- http://arxiv.org/abs/1801.00492
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
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
Abundance analysis of the supergiant stars HD 80057 and HD 80404 based on their UVES Spectra
- Volume 10, Issue 46 - article #3
- Taner Tanrıverdi, Özgür Baştürk
- arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Dec
- arXiv:1512.03762 [pdf, ps, other]
Chemical composition of intermediate mass stars members of the M6 (NGC 6405) open cluster
- Volume 10, Issue 39 - article #5
- Tolgahan Kılıçoğlu, Richard Monier, Jacques Richer, Luca Fossati, Berahitdin Albayrak
- arXiv.org - Astrophysics - Volume: 2015, Issue: 23 Oct
- arXiv:1510.05385 [pdf, ps, other]
Affordable échelle spectroscopy with a 60 cm telescope
- Volume 10, Issue 33 - article #11
- T. Pribulla, Z. Garai, Ľ. Hambálek, V. Kollár, R. Komžík, E. Kundra, J. Nedoroščík, M. Sekeráš, and M. Vaňko
- Astronomische Nachrichten - Volume: 336, Issue: 7
- Abstract PDF(417K)PDF(417K)References Request Permissions
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]
Population III Stars in I Zw 18
- Volume 10, Issue 15 - article #6
- Sally Heap (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA), Jean-Claude Bouret (Aix Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, UMR 7326, 13388, Marseille, France), Ivan Hubeny (University of Arizona, USA)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 17 Apr
- arXiv:1504.02742 [pdf]
Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)
- Volume 10, Issue 7 - article #13
- The origin of lithium is key to understanding the enrichment history of the Universe, now the classical nova V339 Del (Nova Delphini 2013) reveals that nova explosions could have been contributing to the recent rapid increase of the amount of lithium in the Universe.
- Nature - Volume: 518, Issue: 7539
- 276-450
The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
- Volume 10, Issue 1 - article #8
- Shadab Alam (1), Franco D. Albareti (2), Carlos Allende Prieto (3,4), F. Anders (5), Scott F. Anderson (6), Brett H. Andrews (7,8), Eric Armengaud (9), Éric Aubourg (10), Stephen Bailey (11), Julian E. Bautista (10), Rachael L. Beaton (12,13), Timothy C. Beers (14), Chad F. Bender (15,16) Andreas A. Berlind (17), Florian Beutler (11), Vaishali Bhardwaj (6,11), Jonathan C. Bird (17), Dmitry Bizyaev (18,19), Cullen H. Blake (20), Michael R. Blanton (21), Michael Blomqvist (22), John J. Bochanski (6,23), Adam S. Bolton (24), Jo Bovy (25,26), A. Shelden Bradley (18), W. N. Brandt (15,27), D. E. Brauer (5), J. Brinkmann (18), Peter J. Brown (28), Joel R. Brownstein (24), Angela Burden (29), Etienne Burtin (9), Nicolás G. Busca (30,31,10), Zheng Cai (32), Diego Capozzi (29), Aurelio Carnero Rosell (30,31), et al. (238 additional authors not shown)
- arXiv.org - Astrophysics - Volume: 2015, Issue: 9 Jan
- arXiv:1501.00963 [pdf, other]
The exclusion of a significant range of ages in a massive star cluster
- Volume 9, Issue 25 - article #53
- Hubble Space Telescope observations of the stellar cluster NGC 1651, which is approximately two billion years old, show that the colour–brightness distribution of stars old enough to have left the main sequence can be explained only by a single-age population, despite having a feature usually interpreted to indicate an age spread of more than 300 million years.
- Nature - Volume: 516, Issue: 7531
- 290-444
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. I. Overview of the Project and Detection of Multiple Stellar Populations
- Volume 9, Issue 23 - article #26
- G. Piotto (1,2), A. P. Milone (3), L. R. Bedin (2), J. Anderson (4), I. R. King (5), A. Marino (3), D. Nardiello (1,2), A. Aparicio (6,7), B. Barbuy (8), A. Bellini (4), T. M. Brown (4), S. Cassisi (10), A. Cunial (1,2), E. Dalessandro (11), F. D'Antona (12), F. R. Ferraro (11), S. Hidalgo (6,7), B. Lanzoni (11), M. Monelli (6,7), S. Ortolani (1,2), A. Renzini (2), M. Salaris (13), A. Sarajedini (14), R. P. van der Marel (4), E. Vesperini (15), M. Zoccali (16,17) ((1) UNIPD, (2) INAF-OAPd, (3) ANU, (4) STScI, (5) Univ.Washington, (6) IAC, (7) Dip.Astroph. La Laguna, (8) IAG, (9) INAF-OATe, (10) SFSU, (11) UNIBO, (12) INAF-OABo, (13) Liverpool John Moores University, (14) UFL, (15) Univ.Indiana, (16) PUC, (17) MIA, Chile)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 24 Oct
- arXiv:1410.4564 [pdf, ps, other]
Synthetic biology: Engineering explored
- Volume 9, Issue 19 - article #17
- A simulation that starts 12 million years after the Big Bang and traces 13 billion years of cosmic evolution yields a reasonable population of elliptical and spiral galaxies, reproduces the observed distribution of galaxies in clusters and the characteristics of hydrogen on large scales, and at the same time matches the ‘metal’, and hydrogen content of galaxies on small scales.
- Nature - Volume: 509, Issue: 7499
- 136-254
Constraints on the Galactic bar from the Hercules stream as traced with RAVE across the Galaxy
- Volume 9, Issue 16 - article #9
- T. Antoja, A. Helmi, W. Dehnen, O. BienaymÃ©, J. Bland-Hawthorn, B. Famaey, K. Freeman, B. K. Gibson, G. Gilmore, E. K. Grebel, et al. (13 more) G. Kordopatis, A. Kunder, I. Minchev, U. Munari, J. Navarro, Q. Parker, W. A. Reid, G. Seabroke, A. Siebert, M. Steinmetz, F. Watson, R. F. G. Wyse and T. Zwitter
- Astronomy and Astrophysics - Volume: 563, Issue: March 2014
- http://dx.doi.org/10.1051/0004-6361/201322623
  Abstract Full HTML PDF (4.601 MB) References Online Material NASA ADS Abstract Service
A single low-energy, iron-poor supernova as the source of metals in the star SMSS J031300.36−670839.3
- Volume 9, Issue 9 - article #15
- The optical spectrum of the star SMSS J031300.36−670839.3 shows no evidence of iron, this, together with comparisons of the star’s observed element abundance pattern with those of models, means that SMSS J031300.36−670839.3 must have been seeded with material from a single supernova with an original mass about 60 times that of the Sun.
- Nature - Volume: 506, Issue: 7489
- 410-522
Chemical gradients in the Milky Way from the RAVE data - I. Dwarf stars
- Volume 8, Issue 50 - article #15
- C. Boeche, A. Siebert, T. Piffl, A. Just, M. Steinmetz, S. Sharma, G. Kordopatis, G. Gilmore, C. Chiappini, M. Williams, et al. (13 more) E. K. Grebel, J. Bland-Hawthorn, B. K. Gibson, U. Munari, A. Siviero, O. BienaymÃ©, J. F. Navarro, Q. A. Parker, W. Reid, G. M. Seabroke, F. G. Watson, R. F. G. Wyse and T. Zwitter
- Astronomy and Astrophysics - Volume: 559, Issue: November 2013
- http://dx.doi.org/10.1051/0004-6361/201322085
  Abstract Full HTML PDF (1.749 MB) References NASA ADS Abstract Service
The M4 Core Project with HST --- I. Overview and First-Epoch
- Volume 8, Issue 49 - article #11
- L. R. Bedin (1) J. Anderson (2), D. C. Heggie (3), G. Piotto (4,1), A. P. Milone (5,6,7), M. Giersz (8), V. Nascimbeni (4,1), A. Bellini (2), R. M. Rich (9), M. van den Berg (10,11), D. Pooley (12,13), K. Brogaard (14,15), S. Ortolani (4,1), L. Malavolta (4,1), L. Ubeda (2), A. F. Marino (7). ((1) INAF-OAPD, (2) STScI, (3) Univ. of Edinburg, (4) Univ. of Padova, (5) IAC, (6) Univ. of La Laguna, (7) RSAA-ANU, (8) N. Copernicus AC Warsaw, (9) UCLA, (10) Univ. of Amsterdam, (11) Harvard-Smithsonian CfA, (12) Sam Houston State Univ., (13) Eureka Scientific, Inc., (14) Aarhus Univ., (15) Univ. of Victoria)
- arXiv.org - Astrophysics - Volume: 2013, Issue: 6 Dec
- arXiv:1312.1096 [pdf, ps, other]
The AGORA High-Resolution Galaxy Simulations Comparison Project
- Volume 8, Issue 33 - article #11
- Ji-hoon Kim (1), Tom Abel (2), Oscar Agertz (3, 4), Greg L. Bryan (5), Daniel Ceverino (6), Charlotte Christensen (7), Charlie Conroy (1), Avishai Dekel (8), Nickolay Y. Gnedin (3, 9, 10), Nathan J. Goldbaum (1), Javiera Guedes (11), Oliver Hahn (11), Alexander Hobbs (11), Philip F. Hopkins (12, 13), Cameron B. Hummels (7), Francesca Iannuzzi (14), Dusan Keres (15), Anatoly Klypin (16), Andrey V. Kravtsov (3, 10), Mark R. Krumholz (1), Michael Kuhlen (1, 13), Samuel N. Leitner (17), Piero Madau (1), Lucio Mayer (18), Christopher E. Moody (1), Kentaro Nagamine (19, 20), Michael L. Norman (15), Jose Oñorbe (21), Brian W. O'Shea (22), Annalisa Pillepich (1), Joel R. Primack (1), Thomas Quinn (23), Justin I. Read (4), Brant E. Robertson (7), Miguel Rocha (21), Douglas H. Rudd (10, 24), et al. (11 additional authors not shown)
- arXiv.org - Astrophysics - Volume: 2013, Issue: 16 Aug
- arXiv:1308.2669 [pdf, ps, other]
Reviews in Modern Astronomy 25
- Volume 8, Issue 28 - article #17
- Article first published online: 1 JUL 2013 | DOI: 10.1002/asna.201390009
- Astronomische Nachrichten - Volume: 334, Issue: 6
- Abstract PDF(4217K)References Request Permissions
The relation between chemical abundances and kinematics of the Galactic disc with RAVE
- Volume 8, Issue 23 - article #15
- C. Boeche, C. Chiappini, I. Minchev, M. Williams, M. Steinmetz, S. Sharma, G. Kordopatis, J. Bland-Hawthorn, O. BienaymÃ©, B. K. Gibson, et al. (13 more)G. Gilmore, E. K. Grebel, A. Helmi, U. Munari, J. F. Navarro, Q. A. Parker, W. Reid, G. M. Seabroke, A. Siebert, A. Siviero, F. G. Watson, R. F. G. Wyse and T. Zwitter
- Astronomy and Astrophysics - Volume: 553, Issue: May 2013
- http://dx.doi.org/10.1051/0004-6361/201219607
  Abstract Full HTML PDF (2.630 MB) References NASA ADS Abstract Service
Main Sequence Star Populations in the Virgo Overdensity Region
- Volume 8, Issue 13 - article #11
- H. Jerjen (1), G.S. Da Costa (1), B. Willman (2), P. Tisserand (1), N. Arimoto (3,4), S. Okamoto (5), M. Mateo (6), I. Saviane (7), S. Walsh (8), M. Geha (9), A. Jordán (10,11), E. Olszewski (12), M. Walker (13), M. Zoccali (10,11), P. Kroupa (14) ((1) Research School of Astronomy and Astrophysics (2) Haverford College (3) National Astronomical Observatory of Japan (4) The Graduate University for Advanced Studies (5) Kavli Institute for Astronomy and Astrophysics (6) University of Michigan (7) European Southern Observatory (8) Australian Astronomical Observatory (9) Yale University (10) Pontificia Universidad Catolica de Chile (11) The Milky Way Millennium Nucleus (12) The University of Arizona (13) Harvard-Smithsonian Center for Astrophysics (14) Argelander Institute for Astronomy)
- arXiv.org - Astrophysics - Volume: 2013, Issue: 29 Mar
- arXiv:1303.5489 [pdf, other]
The Panchromatic Hubble Andromeda Treasury I: Bright UV Stars in the Bulge of M31
- Volume 7, Issue 25 - article #22
- Philip Rosenfield (1), L. Clifton Johnson (1), Léo Girardi (2), Julianne J. Dalcanton (1), Alessandro Bressan (16), Dustin Lang (3), Benjamin F. Williams (1), Puragra Guhathakurta (5), Kirsten M. Howley (15), Tod R. Lauer (9), Eric F. Bell (14), Luciana Bianchi (12) Nelson Caldwell (7), Andrew Dolphin (6), Claire E. Dorman (5), Karoline M. Gilbert (1,13), Jason Kalirai (11), Søren S. Larsen (17), Knut A.G. Olsen (9), Hans-Walter Rix (10), Anil C. Seth (4), Evan D. Skillman (8), Daniel R. Weisz (1) ((1) Department of Astronomy, University of Washington, (2) Osservatorio Astronomico di Padova -- INAF, Italy, (3) Department of Astrophysical Sciences, Princeton University, (4) Department of Physics and Astronomy, University of Utah, (5) University of California Observatories/Lick Observatory, (6) Raytheon Company, (7) Harvard-Smithsonian Center for Astrophysics, (8) Minnesota Institute for Astrophysics, University of Minnesota, (9) National Optical Astronomy Observatory, (10) Max Planck Institute for Astronomy, Heidelberg, (11) Space Telescope Science Institute, (12) Department of Physics and Astronomy, Johns Hopkins University, (13) Hubble Fellow, (14) Department of Astronomy, University of Michigan, (15) Lawrence Livermore National Laboratory, (16) SISSA, Italy, (17) Department of Astrophysics, Radboud University, The Netherlands)
- arXiv.org - Astrophysics - Volume: 2012, Issue: 22 Jun
- arXiv:1206.4045 [pdf, other]
A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old
- Volume 7, Issue 15 - article #3
- Wei Zheng, Marc Postman, Adi Zitrin, John Moustakas, Xinwen Shu, Stephanie Jouvel, Ole Host, Alberto Molino, Larry Bradley, Dan Coe, Leonidas A. Moustakas, Mauricio Carrasco, Holland Ford, Narciso Benıtez, Tod R. Lauer, Stella Seitz, Rychard Bouwens, Anton Koekemoer, Elinor Medezinski, Matthias Bartelmann, Tom Broadhurst, Megan Donahue, Claudio Grillo, Leopoldo Infante, Saurabh Jha, Daniel D. Kelson, Ofer Lahav, Doron Lemze, Peter Melchior, Massimo Meneghetti, Julian Merten, Mario Nonino, Sara Ogaz, Piero Rosati, Keiichi Umetsu, Arjen van der Wel
- arXiv.org - Astrophysics - Volume: 2012, Issue: 13 Apr
- arXiv:1204.2305 [pdf, ps, other]
Chemical abundances of distant extremely metal-poor unevolved stars
- Volume 7, Issue 15 - article #5
- P. Bonifacio (1), L. Sbordone (2,1,3), E. Caffau (2,1), H.-G. Ludwig (2,1), M. Spite (1), J. I. González Hernández (4,5), N. T. Behara (6) ((1) GEPI, Observatoire de Paris, CNRS, Univ. Paris Diderot, (2) Zentrum für Astronomie der Universität Heidelberg, Landessternwarte, (3) Max-Planck Institut für Astrophysik, (4) Instituto de Astrofısica de Canarias, (5) Depto. Astrofısica, Universidad de La Laguna, (6) Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles)
- arXiv.org - Astrophysics - Volume: 2012, Issue: 13 Apr
- arXiv:1204.1641 [pdf, ps, other]
One or more bound planets per Milky Way star from microlensing observations
- Volume 7, Issue 11 - article #15
- A statistical analysis of microlensing data from 2002–07 reveals that stars in the Milky Way are orbited by planets as a rule, rather than an exception.
- Nature - Volume: 481, Issue: 7380
- 113-230
Non-Blazhko RR Lyrae Stars Observed with the KEPLER Space Telescope
- Volume 6, Issue 35 - article #9
- J.M. Nemec (1,2), R. Smolec (3), J.M. Benko (4), P. Moskalik (5), K. Kolenberg (3,6), R. Szabo (4), D.W. Kurtz (7), S. Bryson (8), E. Guggenberger (3), M. Chadid (9), Y.-B. Jeon (10), A. Kunder (12), A.C. Layden (13), K. Kinemuchi (8), L.L. Kiss (4), E. Poretti (14), J. Christensen-Dalsgaard (11), H. Kjeldsen (11), D. Caldwell (15), V. Ripepi (16), A. Derekas (4), J. Nuspl (4), F.Mullally (15), S.E. Thompson (15), W.J. Borucki (8) ((1) Department of Physics and Astronomy, Camosun College, Victoria, Canada (2) International Statistics and Research Corporation, Brentwood Bay, Canada (3) Institut fur Astronomie, University of Vienna, Vienna, Austria (4) Konkoly Obs.Hung.Acad.Sciences, Budapest, Hungary (5) Copernicus Astronomical Center, Warsaw, Poland (6) Harvard College Observatory, Cambridge, USA (7) Jeremiah Horrocks Institute of Astrophysics, Univ. Central Lancashire, UK (8) NASA Ames Research Center, Moffett Field, CA, USA (9) Obs. Cote d'Azur, Univ.Nice Sophia-Antipolis, Parc Valrose, France (10) Korea Astronomy and Space Science Institute, Daejeon, Korea (11) Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark (12) Cerro Tololo Inter-American Observatory, La Serena, Chile (13) Physics and Astronomy Dept., Bowling Green State University, OH, USA (14) Osservatorio Astronomico di Brera, Merate, Italy (15) SETI Institute/NASA Ames Research Center, Moffett Field, CA, USA (16) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy)
- arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Sep
- arXiv:1108.5683 [pdf, other]
Searches for Dark Matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
- Volume 6, Issue 9 - article #4
- The MAGIC Collaboration (and others): J. Aleksić, (1), E. A. Alvarez (2), L. A. Antonelli (3), P. Antoranz (4), M. Asensio (2), M. Backes (5), J. A. Barrio (2), D. Bastieri (6), J. Becerra González (7,8), W. Bednarek (9), A. Berdyugin (10), K. Berger (7,8), E. Bernardini (11), A. Biland (12), O. Blanch (1), R. K. Bock (13), A. Boller (12), G. Bonnoli (3), D. Borla Tridon (13), I. Braun (12), T. Bretz (14,26), A. Cañellas (15), E. Carmona (13), A. Carosi (3), P. Colin (13), E. Colombo (7), J. L. Contreras (2), J. Cortina (1), L. Cossio (16), S. Covino (3), F. Dazzi (16,27), A. De Angelis (16), E. De Cea del Pozo (17), B. De Lotto (16), C. Delgado Mendez (7,28), A. Diago Ortega (7,8), M. Doert (5), A. Domínguez (18), D. Dominis Prester (19), D. Dorner (12), M. Doro (20), et al. (113 additional authors not shown)
- arXiv.org - Astrophysics - Volume: 2011, Issue: 4 Mar
- arXiv:1103.0477 [pdf, ps, other]
WASP-37b: a 1.7 MJ exoplanet transiting a metal-poor star
- Volume 5, Issue 34 - article #20
- E. K. Simpson (1), F. Faedi (1), S. C. C. Barros (1), D. J. A. Brown (2), A. Collier Cameron (2), L. Hebb (3), D. Pollacco (1), B. Smalley (4), I. Todd (1), O. W. Butters (5), G. Hebrard (6), J. McCormac (1), G. R. M. Miller (2), A. Santerne (7), R. A. Street (8), I. Skillen (9), A. H. M. J. Triaud (10), D. R. Anderson (4), J. Bento (11), I. Boisse (6), F. Bouchy (6 12), B. Enoch (2), C. A. Haswell (13), C. Hellier (4), S. Holmes (13), K. Horne (2), F. P. Keenan (1), T. A. Lister (8), P. F. L. Maxted (4), V. Moulds (1), C. Moutou (7), A. J. Norton (13), N. Parley (2), F. Pepe (10), D. Queloz (10), D. Segransan (10), A. M. S. Smith (4), H. C. Stempels (14), S. Udry (10), C. A. Watson (1), R. G. West (5), P. J. Wheatley (11) ((1) Queen's University Belfast, (2) University of St Andrews, (3) Vanderbilt University, (4) Keele University, (5) University of Leicester, (6) Institut d'Astrophysique de Paris, (7) Laboratoire d'Astrophysique de Marseille, (8) Las Cumbres Observatory Global Telescope Network, (9) Isaac Newton Group of Telescopes, (10) Observatoire de Geneve, (11) University of Warwick, (12) Observatoire de Haute-Provence, (13) The Open University, (14) Uppsala University)
- arXiv.org - Astrophysics - Volume: 2010, Issue: 20 Aug
- arXiv:1008.3096 [pdf, ps, other]
Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
- Volume 5, Issue 31 - article #6
- T. Zwitter (1 and 2), G. Matijeviv{c) (1), M. A. Breddels (3), M. C. Smith (3, 4), A. Helmi (3), U. Munari (5), O. Bienaym'{e) (6), J. Binney (7), J. Bland-Hawthorn (8), C. Boeche (9), A. G. A. Brown (10), R. Campbell (11), K. C. Freeman (12), J. Fulbright (13), B. Gibson (14), G. Gilmore (15), E. K. Grebel (16), J. F. Navarro (17), Q. A. Parker (18), G. M. Seabroke (19), A. Siebert (6), A. Siviero (5, 9), M. Steinmetz (9), F. G. Watson (20), M. Williams (9), R. F. G. Wyse (13) ((1) University of Ljubljana, Faculty of Mathematics, Physics, Ljubljana, Slovenia} (2) Center of excellence SPACE-SI, Ljubljana, Slovenia, (3) Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands, (4) Kavli Institute for Astronomy, Astrophysics, Peking University, Beijing, China, (5) INAF Astronomical Observatory of Padova, et al. (36 additional authors not shown)
- arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
- arXiv:1007.4411 [pdf, ps, other]
The metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundances
- Volume 5, Issue 13 - article #19
- L. Sbordone (1 and 2 and 3), P. Bonifacio (1 and 2 and 4), E. Caffau (2), H.-G. Ludwig (1 and 2 and 5), N. T. Behara (1 and 2 and 6), J. I. Gonzalez Hernandez (1 and 2 and 7), M. Steffen (8), R. Cayrel (9), B. Freytag (9), C. Van't Veer (2), P. Molaro (4), B. Plez (10), T. Sivarani (11), M. Spite (2), F. Spite (2), T. C. Beers (12), N. Christlieb (5), P. Francois (2), V. Hill (2 and 13) ((1) CIFIST Marie Curie Excellence Team, (2) GEPI - Observatoire de Paris France, (3) Max Planck Institute for Astrophysics Garching Germany, (4) INAF - Oss. Trieste Italy, (5) Landessternwarte Heidelberg Germany, (6) Universite' Libre de Bruxelles Belgium, (7) Universidad Complutense de Madrid Spain, (8) Astrophysikalische Institut Pottsdam Germany, (9) Ecole Normale Superieure de Lyon France, (10) Universite' Montpellier France, (11) Indian Institute for Astrophysiscs Bangalore India, (12) Michigan State University USA, (13) Observatoire de la Cote d'Azur Nice France)
- arXiv.org - Astrophysics - Volume: 2010, Issue: 26 Mar
- arXiv:1003.4510 [pdf, ps, other]
On a new Near-Infrared method to estimate the absolute ages of star clusters: NGC3201 as a first test case
- Volume 4, Issue 50 - article #9
- G. Bono (2,3), P.B. Stetson (4), D.A. VandenBerg (5), A. Calamida (6), M. Dall'Ora (7), G. Iannicola (3), P. Amico (6), A. Di Cecco (2), E. Marchetti (6), M. Monelli (7), N. Sanna (2), A.R. Walker (9), M. Zoccali (10), R. Buonanno (2), F. Caputo (3), S. Degl'Innocenti (11,12), S. D'Odorico (6), I. Ferraro (3), R. Gilmozzi (6), J. Melnick (6), M. Nonino (13), S. Ortolani (14), A.M. Piersimoni (15), P.G. Prada Moroni (11,12), L. Pulone (3), M. Romaniello (6), J. Storm (16) ((2) UniToV (3) INAF/OAR (4) HIA-NRC (5) UVIC (6) ESO (7) INAF/OACN (8) IAC (9) CTIO (10) PUC (11) Univ. Pisa (12) INFN Pisa (13) INAF/OAT (14) Univ. of Padova (15) INAF-OACTe (16) AIP (8) Aarhus Univ. (9) IAC (10) Univ. Concepcion (11) Astrophys. In. Potsdam (12) CTIO)
- arXiv.org - Astrophysics - Volume: 2009, Issue: 11 Dec
- arXiv:0912.0824 [ps, pdf, other]
Stromgren photometry of Galactic Globular Clusters. II Metallicity distribution of red giants in Omega Centauri
- Volume 4, Issue 40 - article #14
- A. Calamida (1), G. Bono (2), P.B. Stetson (3), L.M. Freyhammer (4), A.M. Piersimoni (5), R. Buonanno (2), F. Caputo (6), S. Cassisi (5), M. Castellani (6), C.E. Corsi (6), M. Dall'Ora (7), S. Degl'Innocenti (8), I. Ferraro (6), F. Grundahl (9), M. Hilker (1), M. Monelli (10), M. Nonino (11), N. Patat (1), A. Pietrinferni (5), P.G. Prada Moroni (8), F. Primas (1), L. Pulone (6), T. Richtler (12), M. Romaniello (1), J. Storm (13), A.R. Walker (14) ((1) ESO (2) Univ. Roma Tor Vergata (3) HIA-NRC (4) Univ. Lancashire (5) INAF/OATe (6) INAF/OAR (7) INAF/OAC (8) Univ. Pisa (9) Aarhus Univ. (10) IAC (11) OAT (12) Univ. Concepcion (13) Astrophys. In. Potsdam (14) CTIO)
- arXiv.org - Astrophysics - Volume: 2009, Issue: 2 Oct
- arXiv:0909.4661 [ps, pdf, other]
Nobel Lecture: From the Big Bang to the Nobel Prize and beyond
- Volume 3, Issue 41 - article #27
- John C. Mather<BR&gt, Published 2 November 2007 (18 pages) pp. 1331-1348 Abstract Full Text: [ PDF (1445 kB) GZipped PS ] Free to Read Free to Read Nobel Lecture: Cosmic microwave background radiation anisotropies: Their discovery and utilization<br&gt, George F. Smoot
- Reviews of Modern Physics - Volume: 79, Issue: 4
- Abstract Full Text: [ PDF (4379 kB) GZipped PS ] Free to Read
Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey
- Volume 3, Issue 23 - article #11
- D. J. Pinfield (1), B. Burningham (1), M. Tamura (2), S. K. Leggett (3), N. Lodieu (4), P. W. Lucas (1), D. J. Mortlock (5), S. J. Warren (5), D. Homeier (6), M. Ishi (7), N. R. Deacon (8), R. G. McMahon (9), P. C. Hewett (9), M. R. Zapatero Osorio (4), E. L. Martin (4), H. R. A. Jones (1), B.P. Venemans (9), A. Day-Jones (1), P. D. Dobbie (10), S. L. Folkes (1), S. Dye (11), F. Allard (12), I. Baraffe (13), D. Barrado y Navascues (14), S. L. Casewell (15), K. Chiu (16), G. Chabrier (13), F. Clarke (17), S. T. Hodgkin (9), A. Magazzu (18), M. J. McCaughrean (16), E. Moraux (19), T. Nakajima (2), Y. Pavlenko (20), C. G. Tinney (21) ((1) University of Hertfordshire, UK, (2) National Astronomical Observatory, Japan, (3) Gemini Observatory, USA, (4) Instituto de Astrofisica de Canarias, Spain, (5) Imperial College London, UK, (6) Georg-August-Universitat, Germany, (7) Subaru Telescope, USA, (8) Radboud University, The Netherlands, (9) Cambridge University, UK, (10) Anglo-Australian Observatory, Australia, (11) Cardif University, UK, (12) Universite de Lyon, France, (13) C.R.A.L., France, (14) Laboratorio de Astrofisica Espacial y Fisica Fundamental, Spain, (15) University of Leicester, UK, (16) University of Exeter, UK, (17) European Southern Observatory, Chile, (18) Fundacion Galileo Galilei-INAF, Spain, (19) Laboratoire d'Astrophysique de Grenoble, France, (20) Main Astronomical Observatory, Ukraine, (21) University of New South Wales, Australia)
- arXiv.org - Astrophysics - Volume: 2008, Issue: 5 Jun
- arXiv:0806.0294 [ps, pdf, other]
A Curious New Milky Way Satellite in Ursa Major
- Volume 1, Issue 22 - article #3
- D.B. Zucker (1), V. Belokurov (1), N.W. Evans (1), M.J. Irwin (1), J.T. Kleyna (2), M.I. Wilkinson (1), M. Fellhauer (1), D.M. Bramich (1), G. Gilmore (1), H.J. Newberg (3), B. Yanny (4), J.A. Smith (5,6), P.C. Hewett (1), E.F. Bell (7), H.-W. Rix (7), O.Y. Gnedin (8), S. Vidrih (1), R.F.G. Wyse (9), B. Willman (10), E.K. Grebel (11), D.P. Schneider (12), T.C. Beers (13), A.Y. Kniazev (7,14), J.C. Barentine (15), H. Brewington (15), J. Brinkmann (15), M. Harvanek (15), S.J. Kleinman (16), J. Krzesinski (15,17) D. Long (15), A. Nitta (18), S.A. Snedden (15) ((1) Cambridge, (2) Hawaii, (3) RPI, (4) FNAL, (5) LANL, (6) Austin Peay State University, (7) MPIA, (8) OSU, (9) JHU, (10) NYU, (11) Basel, (12) Penn State University, (13) Michigan State University, (14) SAAO, (15) Apache Point, (16) Subaru Telescope, (17) Cracow, (18) Gemini Observatory)
- ArXiv - Astrophysics
- astro-ph/0606633 [abs, ps, pdf, other]
A Faint New Milky Way Satellite in Bootes
- Volume 1, Issue 13 - article #17
- V. Belokurov (1), D. B. Zucker (1), N. W. Evans (1), M. I. Wilkinson (1), M. J. Irwin (1), S. Hodgkin (1), D. M. Bramich (1), J. M. Irwin (1), G. Gilmore (1), B. Willman (2), S. Vidrih (1), H. J. Newberg (3), R. F. G. Wyse (4), M. Fellhauer (1), P. C. Hewett (1), N. Cole (3), E. F. Bell (5), T. C. Beers (6), C. M. Rockosi (7), B. Yanny (8), E. K. Grebel (9), D. P. Schneider (10), R. Lupton (11), J. C. Barentine (12), H. Brewington (12), J. Brinkmann (12), M. Harvanek (12), S. J.Kleinman (12), J. Krzesinski (12,13), D. Long (12), A. Nitta (12), J. A. Smith (14), S. A. Snedden (12) ((1) Cambridge University, (2) New York University, (3) Rensselaer Polytechnical Institute, (4) JHU, (5) MPIA, Heidelberg, (6) Michigan State University, (7) Lick Observatory, UCSC, (8) FNAL, (9) University of Basel, (10) Pennsylvania State University, (11) Princeton University, (12) Apache Point Observatory, (13) Cracow Pedagogical University, (14) LANL)
- ArXiv - Astrophysics
- astro-ph/0604355 [abs, ps, pdf, other]
A New Milky Way Dwarf Satellite in Canes Venatici
- Volume 1, Issue 13 - article #18
- D. B. Zucker (1), V. Belokurov (1), N. W. Evans (1), M. I. Wilkinson (1), M. J. Irwin (1), T. Sivarani (2), S. Hodgkin (1), D. M. Bramich (1), J. M. Irwin (1), G. Gilmore (1), B. Willman (3), S. Vidrih (1), M. Fellhauer (1), P. C. Hewett (1), T. C. Beers (2), E. F. Bell (4), E. K. Grebel (5), D. P. Schneider (6), H. J. Newberg (7), R. F. G. Wyse (8), C. M. Rockosi (9), B. Yanny (10), R. Lupton (11), J. A. Smith (12), J. C. Barentine (13), H. Brewington (13), J. Brinkmann (13), M. Harvanek (13), S. J.Kleinman (13), J. Krzesinski (13,14), D. Long (13), A. Nitta (13), S. A. Snedden (13) ((1) Cambridge University, (2) Michigan State University, (3) New York University, (4) MPIA, Heidelberg, (5) University of Basel, (6) Pennsylvania State University, (7) Rensselaer Polytechnic Institute, (8) JHU, (9) Lick Observatory/UCSC, (10) FNAL, (11) Princeton University, (12) LANL, (13) Apache Point Observatory, (14) Cracow Pedagogical University)
- ArXiv - Astrophysics
- astro-ph/0604354 [abs, ps, pdf, other]

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