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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
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 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
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
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
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
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
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
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
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 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
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
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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
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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
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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
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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
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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
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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
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Chemical composition and constraints on mass loss for globular clusters in dwarf galaxies: WLM and IKN
Volume 9, Issue 15 - article #1
S. S. Larsen
(1),
J. P. Brodie
(2),
D. A. Forbes
(3),
J. Strader
(4)
((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen, The Netherlands,
(2) UCO/Lick Observatory, UC Santa Cruz, USA,
(3) Swinburne University of Technology, Australia,
(4) Department of Physics and Astronomy, Michigan State University, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 11 Apr
arXiv:1404.1916
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Detailed AGB evolutionary models and near infrared colours of intermediate-age stellar populations: Tests on star clusters
Volume 9, Issue 11 - article #8
M. Salaris
(1,2),
A. Weiss
(2),
L. Cassara'
,
(3,4),
L. Piovan
(3),
C. Chiosi
(3)
(1- Astrophysics Research Institute, Liverpool John Moores University, UK, 2- Max-Planck-Institut fur Astrophysik, D, 3- Department of Physics and Astronomy, University of Padova, I, 4- INAF-IASF Milano, I)
arXiv.org - Astrophysics - Volume: 2014, Issue: 14 Mar
arXiv:1403.2505
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On the metallicity distribution of classical Cepheids in the Galactic inner disk
Volume 8, Issue 20 - article #4
K. Genovali
(1),
B. Lemasle
(2),
G. Bono
(1 and 3),
M. Romaniello
(4),
F. Primas
(4),
M. Fabrizio
(5),
R. Buonanno
(1 and 5),
P. François
(6 and 7),
L. Inno
(1 and 4),
C.D. Laney
(8 and 9),
N. Matsunaga
(10),
S. Pedicelli
(1),
F. Thévenin
(11)
((1) Dipartimento di Fisica, Università di Roma Tor Vergata
(2) Astronomical Institute Anton Pannekoek
(3) INAF - Osservatorio Astronomico di Roma
(4) European Southern Observatory
(5) INAF - Osservatorio Astronomico di Collurania
(6) GEPI - Observatoire de Paris
(7) UPJV - Université de Picardie Jules Verne
(8) Department of Physics and Astronomy, Brigham Young University
(9) South African Astronomical Observatory
(10) Kiso Observatory, Institute of Astronomy, The University of Tokyo
(11) Laboratoire Lagrange, Université de Nice Sophia-Antipolis)
arXiv.org - Astrophysics - Volume: 2013, Issue: 17 May
arXiv:1305.2742
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A resolution of the cosmic Lithium problem
Volume 8, Issue 16 - article #3
Rachid Ouyed
(Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada)
arXiv.org - Astrophysics - Volume: 2013, Issue: 19 Apr
arXiv:1304.3715
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Fossil Evidence for the Two-phase Formation of Elliptical Galaxies
Volume 8, Issue 15 - article #5
Song Huang
(1,2,3),
Luis C. Ho
(2),
Chien Y. Peng
(4),
Zhao-Yu Li
(5),
Aaron J. Barth
(6)
((1) School of Astronomy and Space Science, Nanjing University,
(2) The Observatories of the Carnegie Institution for Science,
(3) Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University,
(4) Giant Magellan Telescope Organization,
(5) Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory,
(6) Department of Physics and Astronomy, University of California, Irvine)
arXiv.org - Astrophysics - Volume: 2013, Issue: 12 Apr
arXiv:1304.2299
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k-d Match: A Fast Matching Algorithm for Stellar Samples
Volume 8, Issue 14 - article #6
Jeremy S. Heyl
(Department of Physics and Astronomy, University of British Columbia, Canada)
arXiv.org - Astrophysics - Volume: 2013, Issue: 5 Apr
arXiv:1304.0838
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Photometric properties of stellar populations in Galactic globular clusters: the role of the Mg-Al anticorrelation
Volume 8, Issue 12 - article #5
Santi Cassisi
(INAF - Astronomical Observatory Teramo, Italy),
Alessio Mucciarelli
(Dipartimento di Fisica e Astronomia, Universita' degli Studi di Bologna, Italy),
Adriano Pietrinferni
(INAF - Astronomical Observatory of Teramo),
Maurizio Salaris
(ARI, Liverpool John Moores University, UK),
Jason Ferguson
(Department of Physics, Wichita State University Wichita, USA)
arXiv.org - Astrophysics - Volume: 2013, Issue: 22 Mar
arXiv:1303.5222
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Does the Oosterhoff Dichotomy Exist in The Andromeda Galaxy? I. The case of G11
Volume 8, Issue 3 - article #5
Rodrigo Contreras Ramos
(1,2,3),
Gisella Clementini
(1),
Luciana Federici
(1),
Giuliana Fiorentino
(1),
Carla Cacciari
(1),
Marcio Catelan
(3,8),
Horace A. Smith
(4),
Flavio Fusi Pecci
(1),
Marcella Marconi
(5),
Barton J. Pritzl
(6),
Karen Kinemuchi
(7)
((1) INAF-Osservatorio Astronomico di Bologna, Italy,
(2) Dipartimento di Astronomia, Universita' di Bologna, Italy,
(3) Pontificia Universidad Catolica de Chile, Departamento de Astronomia y Astrofisica, Santiago, Chile,
(4) Department of Physics and Astronomy, Michigan State University, USA,
(5) INAF-Osservatorio Astronomico di Capodimonte, Italy,
(6) Department of Physics and Astronomy, University of Wisconsin Oshkosh, USA,
(7) Apache Point Observatory/New Mexico State University, USA,
(8) The Milky Way Millennium Nucleus, Santiago, Chile)
arXiv.org - Astrophysics - Volume: 2013, Issue: 18 Jan
arXiv:1301.4100
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Detailed abundance analysis from integrated high-dispersion spectroscopy: Globular clusters in the Fornax Dwarf Spheroidal
Volume 7, Issue 36 - article #7
S. S. Larsen
(1),
J. P. Brodie
(2),
J. Strader
(3 and 4)
((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen, The Netherlands
(2) UCO/Lick Observatory, USA
(3) Harvard-Smithsonian Center for Astrophysics, USA
(4) Department of Physics and Astronomy, Michigan State University, USA)
arXiv.org - Astrophysics - Volume: 2012, Issue: 7 Sep
arXiv:1209.1092
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Evidence for Substructure in Ursa Minor Dwarf Spheroidal Galaxy using a Bayesian Object Detection Method
Volume 7, Issue 34 - article #4
Andrew B. Pace
(1),
Gregory D. Martinez
(1,2),
Manoj Kaplinghat
(1),
Ricardo R. Muñoz
(3, 4),
((1) Center for Cosmology, Department of Physics and Astronomy, University of California, Irvine,
(2) The Oskar Klein Center, Department of Physics, Stockholm University,
(3) Departamento de Astronomía, Universidad de Chile,
(4) Department of Astronomy, Yale University)
arXiv.org - Astrophysics - Volume: 2012, Issue: 24 Aug
arXiv:1208.4146
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An upper limit on the sulphur abundance in HE 1327-2326
Volume 7, Issue 28 - article #1
P. Bonifacio
(1),
E. Caffau
(2,1),
K. A. Venn
(3),
D. L. Lambert
(4)
((1) GEPI-Observatoire de Paris, CNRS, Univ. Paris Diderot,
(2) Zentrum für Astronomie der Universität Heidelberg, Landessternwarte,
(3) Department of Physics & Astronomy, University of Victoria,
(4) The W. J. McDonald Observatory, The University of Texas at Austin)
arXiv.org - Astrophysics - Volume: 2012, Issue: 13 Jul
arXiv:1207.1806
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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
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A universal, post Big-Bang Nucleo-synthesis, pre-Galactic, origin of the Lithium (Spite) Plateau
Volume 7, Issue 11 - article #4
Rachid Ouyed
(Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada)
arXiv.org - Astrophysics - Volume: 2012, Issue: 16 Mar
arXiv:1203.2703
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The past, present and future of Galactic planetary nebula surveys
Volume 7, Issue 10 - article #14
Quentin A. Parker
(1,2,3),
D.J. Frew
(1,2),
A. Acker
(4),
B. Miszalski
(5),
((1) Department of Physics and Astronomy, Macquarie University,
(2) Macquarie University Research Centre in Astronomy, Astrophysics and Astrophotonics,
(3) Australian Astronomical Observatory,
(4) Observatoire Astronomique de Strasbourg,
(5) South African Astronomical Observatory)
arXiv.org - Astrophysics - Volume: 2012, Issue: 9 Mar
arXiv:1203.1694
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Allan Sandage and the Cosmic Expansion
Volume 6, Issue 48 - article #2
G. A. Tammann
,
B. Reindl
(Department of Physics and Astronomy, Univ. of Basel)
arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Dec
arXiv:1112.0170
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What is a Spectrum?
Volume 6, Issue 48 - article #21
Adam S. Bolton
(1),
Stephen Bailey
(2),
Joel Brownstein
(1),
Parul Pandey
(1),
David Schlegel
(2),
Yiping Shu
(1)
((1) Department of Physics and Astronomy, The University of Utah,
(2) Physics Division, Lawrence Berkeley National Lab)
arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Dec
arXiv:1111.6525
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Two distinct halo populations in the solar neighborhood. III. Evidence from stellar ages and orbital parameters
Volume 6, Issue 46 - article #13
William J. Schuster
(1),
Edmundo Moreno
(2),
Poul E. Nissen
(3),
Barbara Pichardo
(2)
((1) Observatorio Astronomico Nacional, Universidad Nacional Autonoma de Mexico, Ensenada, Mexico,
(2) Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico,
(3) Department of Physics and Astronomy, University of Aarhus, Aarhus, Denmark)
arXiv.org - Astrophysics - Volume: 2011, Issue: 18 Nov
arXiv:1111.4026
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Infall Times for Milky Way Satellites From Their Present-Day Kinematics
Volume 6, Issue 40 - article #3
Miguel Rocha
,
Annika H.G. Peter
,
James S. Bullock
(Center for Cosmology, Department of Physics and Astronomy, University of California, Irvine)
arXiv.org - Astrophysics - Volume: 2011, Issue: 7 Oct
arXiv:1110.0464
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Galactic distributions of carbon- and oxygen-rich AGB stars revealed by the AKARI mid-infrared all-sky survey
Volume 6, Issue 35 - article #7
Daisuke Ishihara
(1),
Hidehiro Kaneda
(1),
Takashi Onaka
(2),
Yoshifusa Ita
(3),
Mikako Matsuura
(4,5),
Noriyuki Matsunaga
(6)
((1) Nagoya University,
(2) University of Tokyo,
(3) Tohoku University,
(4) Institute of Origins, Department of Physics and Astronomy, University College London,
(5) Institute of Origins, Mullard Space Science Laboratory, University College London,
(6) Kiso Observatory, Univ. of Tokyo)
arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Sep
arXiv:1108.6161
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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
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The Bulge Radial Velocity/Abundance Assay
Volume 6, Issue 35 - article #16
R. Michael Rich
(1)
((1) Department of Physics and Astronomy, University of California, Los Angeles)
arXiv.org - Astrophysics - Volume: 2011, Issue: 2 Sep
arXiv:1108.6044
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The Information Of The Milky Way From 2MASS Whole Sky Star Count: The Structure Parameters
Volume 6, Issue 29 - article #16
Chan-Kao Chang
(1),
Chung-Ming Ko
(1 and 2),
Ting-Hung Peng
(1)
((1) Institute of Astronomy, National Central University, Jhongli, Taiwan
(2) Department of Physics and Center of Complex Systems, National Central University, Jhongli, Taiwan)
arXiv.org - Astrophysics - Volume: 2011, Issue: 22 Jul
arXiv:1107.3884
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Enhanced Management of Personal Astronomical Data with FITSManager
Volume 6, Issue 26 - article #9
Chenzhou Cui
(1),
Dongwei Fan
(1),
Yongheng Zhao
(1),
Ajit Kembhavi
(2),
Boliang He
(1),
Zihuang Cao
(1),
Jian Li
(1),
Deoyani Nandrekar
(2,3)
((1) National Astronomical Observatories, Chinese Academy of Sciences,
(2) Inter University Centre for Astronomy and Astrophysics, India,
(3) Department of Physics and Astronomy, The Johns Hopkins University)
arXiv.org - Astrophysics - Volume: 2011, Issue: 1 Jul
arXiv:1106.4847
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The most metal-poor damped Lyman-alpha systems: Insights into chemical evolution in the very metal-poor regime
Volume 6, Issue 24 - article #8
Ryan Cooke
(Institute of Astronomy, University of Cambridge),
Max Pettini
(Institute of Astronomy, University of Cambridge),
Charles C. Steidel
(California Institute of Technology),
Gwen C. Rudie
(California Institute of Technology),
Poul E. Nissen
(Department of Physics and Astronomy, University of Aarhus)
arXiv.org - Astrophysics - Volume: 2011, Issue: 17 Jun
arXiv:1106.2805
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r-Java : An r-process Code and Graphical User Interface for Heavy-Element Nucleosynthesis
Volume 6, Issue 14 - article #5
Camille Charignon
(1,2),
Mathew Kostka
(1),
Nico Koning
(1),
Prashanth Jaikumar
(3,4),
Rachid Ouyed
(1)
((1) Department of Physics&Astronomy, University of Calgary, Alberta, Canada,
(2) Department de Physique, Ecole Normale Superieure de Cachan, France,
(3) Department of Physics&Astronomy, California State University Long Beach, California, USA,
(4) Institute of Mathematical Sciences, CIT Campus, Chennai, India)
arXiv.org - Astrophysics - Volume: 2011, Issue: 8 Apr
arXiv:1104.0340
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Fluorine and Sodium in C-rich low-metallicity stars
Volume 5, Issue 51 - article #6
Sara Lucatello
(1),
Thomas Masseron
(2),
Jennifer A. Johnson
(2),
Marco Pignatari
(3),
Falk Herwig
(4)
((1) INAF - Osservatorio Astronomico di Padova, Italy,
(2) Astronomy department, Ohio State University, USA,
(3) Basel University, Switzerland,
(4) Department of Physics & Astronomy, University of Victoria, Victoria, Canada)
arXiv.org - Astrophysics - Volume: 2010, Issue: 17 Dec
arXiv:1012.2800
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UV-Bright Stellar Populations and Their Evolutionary Implications in the Collapsed-Core Cluster M15
Volume 5, Issue 40 - article #11
Nathalie C. Haurberg
(1),
Gabriel M. G. Lubell
(1),
Haldan N. Cohn
(1),
Phyllis M. Lugger
(1),
Jay Anderson
(2),
Adrienne M. Cool
(3),
Aldo Serenelli
(4)
((1) Indiana University Department of Astronomy Bloomington,
(2) Space Telescope Science Institute,
(3) Department of Physics and Astronomy, San Francisco State University,
(4) Max Planck Institute for Astrophysics - Instituto de Ciencias del Espacio
(IEEC - CSIC))
arXiv.org - Astrophysics - Volume: 2010, Issue: 1 Oct
arXiv:1009.5694
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Dwarf galaxies beyond our doorstep: the Centaurus A group
Volume 5, Issue 39 - article #4
D. Crnojević
,
(1),
E. K. Grebel
(1),
A. A. Cole
(2),
A. Koch
(3),
M. Rejkuba
(4),
G. Da Costa
(5),
H. Jerjen
(5)
((1) Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Germany,
(2) School of Mathematics & Physics, University of Tasmania, Australia,
(3) Department of Physics and Astronomy, University of Leicester, UK,
(4) European Southern Observatory, Garching, Germany,
(5) Research School of Astronomy & Astrophysics, Institute of Advanced Studies, Australian National University, Australia)
arXiv.org - Astrophysics - Volume: 2010, Issue: 24 Sep
arXiv:1009.4198
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Evidence of V-band polarimetric separation of carbon stars at high Galactic latitude
Volume 5, Issue 39 - article #5
Aruna Goswami
(1),
Sreeja S. Kartha
(1),
Asoke K. Sen
(2)
((1) Indian Institute of Astrophysics, Bangalore 560034, India,
(2) Department of Physics, Assam University, Silchar, Assam, India)
arXiv.org - Astrophysics - Volume: 2010, Issue: 24 Sep
arXiv:1009.3912
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On the metallicity of open clusters I. Photometry
Volume 5, Issue 35 - article #20
E. Paunzen
(1),
U. Heiter
(2),
M. Netopil
(1 and 3),
C. Soubiran
(4)
((1) Institute for Astronomy, Vienna University,
(2) Department of Physics and Astronomy, Uppsala University,
(3) Hvar Observatory, Faculty of Geodesy, University of Zagreb,
(4) Universite Bordeaux 1, CNRS, Laboratoire d'Astrophysique de Bordeaux)
arXiv.org - Astrophysics - Volume: 2010, Issue: 27 Aug
arXiv:1008.3476
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The case of the disappearing CN-strong AGB stars in Galactic globular clusters -- Preliminary Results
Volume 5, Issue 16 - article #9
S. W. Campbell
(1 and 2),
D. Yong
(3),
E. C. Wylie-de Boer
(3),
R. J. Stancliffe
(2),
J. C. Lattanzio
(2),
G. C. Angelou
(2),
F. Grundahl
(4),
C. Sneden
(5)
((1) Departament de Fisica i Enginyeria Nuclear, Universitat Politecnica de Catalunya, Barcelona, Spain,
(2) Centre for Stellar and Planetary Astrophysics, Monash University, Australia,
(3) Research School of Astronomy and Astrophysics, Australian National University, Australia,
(4) Department of Physics and Astronomy, Aarhus University, Denmark,
(5) Department of Astronomy and McDonald Observatory, University of Texas, Austin, USA)
arXiv.org - Astrophysics - Volume: 2010, Issue: 16 Apr
arXiv:1004.2249
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Two distinct sequences of blue straggler stars in the globular cluster M30
Volume 5, Issue 2 - article #15
F. R. Ferraro
(1),
G. Beccari
(2),
E. Dalessandro
(1),
B. Lanzoni
(1),
A. Sills
(3),
R. T. Rood
(4),
F. Fusi Pecci
(5),
A. I. Karakas
(6),
P. Miocchi
(1),
S. Bovinelli
(1)
((1) Department of Astronomy, University of Bologna, Italy,
(2) ESA, Space Science Department, The Netherlands,
(3) McMaster University, Department of Physics and Astronomy, Canada,
(4) Astronomy Department, University of Virginia, USA,
(5) INAF, Osservatorio Astronomico di Bologna, Italy,
(6) Research School of Astronomy and Astrophysics, Mt Stromlo Observatory, Australia)
arXiv.org - Astrophysics - Volume: 2010, Issue: 8 Jan
arXiv:1001.1096
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The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge
Volume 4, Issue 49 - article #22
F. R. Ferraro
(1),
E. Dalessandro
(1),
A. Mucciarelli
(1),
G. Beccari
(2),
R. M. Rich
(3),
L. Origlia
(4),
B. Lanzoni
(1),
R. T. Rood
(5),
E. Valenti
(6,7),
M. Bellazzini
(4),
S. M. Ransom
(8),
G. Cocozza
(4)
((1) Department of Astronomy, University of Bologna,
(2) ESA, Space Science Department, The Netherlands,
(3) Department of Physics and Astronomy, UCLA,
(4) INAF-Osservatorio Astronomico di Bologna,
(5) Astronomy Department, University of Virginia, Charlottesville,
(6) ESO, Santiago, Chile,
(7) Pontificia Universidad Catolica de Chile, Departamento de Astronomia)
arXiv.org - Astrophysics - Volume: 2009, Issue: 4 Dec
arXiv:0912.0192
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Star clusters as laboratories for stellar and dynamical evolution
Volume 4, Issue 45 - article #13
Jason S. Kalirai
(1),
Harvey B. Richer
(2)
((1) Space Telescope Science Institute, USA;
(2) Department of Physics and Astronomy, University of British Columbia, Canada)
arXiv.org - Astrophysics - Volume: 2009, Issue: 6 Nov
arXiv:0911.0789
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Population Synthesis of Binary Carbon-enhanced Metal-poor Stars
Volume 4, Issue 42 - article #14
Robert G. Izzard
(1,2),
Evert Glebbeek
(1,3),
Richard J. Stancliffe
(4,5),
Onno Pols
(1)
((1) Sterrenkundig Instituut, Universiteit Utrecht
(2) Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles
(3) Department of Physics and Astronomy, McMaster University
(4) Institute of Astronomy, University of Cambridge
(5) School of Mathematical Sciences, Monash University)
arXiv.org - Astrophysics - Volume: 2009, Issue: 16 Oct
arXiv:0910.2158
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Binary Populations of Carbon-Enhanced Metal-Poor Stars
Volume 4, Issue 40 - article #5
Robert G. Izzard
(1,2),
Evert Glebbeek
(2,3),
Richard J. Stancliffe
(4,5),
Onno Pols
(2)
((1) Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles,
(2) Sterrenkundig Instituut, Universiteit Utrecht,
(3) Department of Physics and Astronomy, McMaster University,
(4) School of Mathematical Sciences, Monash University,
(5) Institute of Astronomy, University of Cambridge)
arXiv.org - Astrophysics - Volume: 2009, Issue: 2 Oct
arXiv:0909.4891
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Star clusters as building blocks for dSph galaxies formation
Volume 4, Issue 40 - article #13
P. Assmann
(1),
M. Fellhauer
(1),
M.I. Wilkinson
(2)
((1) Departamento de Astronomia, Universidad de Concepcion, Chile,
(2) Department of Physics and Astronomy, University of Leicester, UK)
arXiv.org - Astrophysics - Volume: 2009, Issue: 2 Oct
arXiv:0910.0226
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Effects of Galactic fountains and delayed mixing in the chemical evolution of the Milky Way
Volume 4, Issue 25 - article #5
E. Spitoni
(1),
F. Matteucci
(1,2),
S. Recchi
(3,2),
G. Cescutti
(1),
A. Pipino
(4)
((1) Dipartimento di Astronomia, Universita' di Trieste, Italy,
(2) I.N.A.F. Osservatorio Astronomico di Trieste, Italy,
(3) Institute of Astronomy, Vienna University, Austria
(4) Department of Physics and Astronomy, University of Southern California, U.S.A)
arXiv.org - Astrophysics - Volume: 2009, Issue: 19 Jun
arXiv:0906.3400
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OGLE-2009-BLG-076S - The most metal-poor dwarf star in the Galactic bulge
Volume 4, Issue 25 - article #9
T. Bensby
(1),
S. Feltzing
(2),
J.A. Johnson
(3),
A. Gal-Yam
(4),
A. Udalski
(5)
A. Gould
(3),
C. Han
(6),
D. Adén
(2),
J. Simmerer
(2)
((1) European Southern Observatory, Chile,
(2) Lund Observatory, Sweden,
(3) Dept. of Astronomy, Ohio State Univ., USA,
(4) Benoziyo Center for Astrophyics, Weizmann Institute of Science, Israel,
(5) Warsaw University Observatory, Poland,
(6) Department of Physics, Chungbuk National University, Republic of Korea)
arXiv.org - Astrophysics - Volume: 2009, Issue: 19 Jun
arXiv:0906.2235
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Interferometric properties of pulsating C-rich AGB stars I. Intensity profiles and uniform disc diameters of dynamic model atmospheres
Volume 4, Issue 16 - article #2
C. Paladini
(1),
B. Aringer
(1 and 2),
J. Hron
(1),
W. Nowotny
(1),
S. Sacuto
(1),
S. Hoefner
(3)
((1) Department of Astronomy, Vienna, Austria,
(2) INAF-OAPD, Padova, Italy,
(3) Department of Physics and Astronomy, Uppsala, Sweden)
arXiv.org - Astrophysics - Volume: 2009, Issue: 17 Apr
arXiv:0904.2166
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First stars XII. Abundances in extremely metal-poor turnoff stars,and comparison with the giants
Volume 4, Issue 13 - article #12
P. Bonifacio
(1,2,3),
M. Spite
(2),
R. Cayrel
(2),
V. Hill
(2,4),
F. Spite
(2),
P. Francois
(2),
B. Plez
(5,6),
H.-G Ludwig
(1,2),
E. Caffau
(2),
P. Molaro
(3),
E. Depagne
(7),
J. Andersen
(8,9),
B. Barbuy
(10),
T.C. Beers
(11),
B. Nordstrom
(8),
F. Primas
(12)
((1) CIFIST
(2) GEPI, Observatoire de Paris
(3) INAF- OA Trieste
(4) Cassiopee, Observatoire de la Cote d'Azur
(5) GRAAL, Universite de Montpellier
(6) Department of Physics & Astronomy, Uppsala Astronomical Observatory
(7) Las Cumbres Observatory
(8) The Niels Bohr Institute
(9) Nordic Optical Telescope
(10) IAG, Universidade de Sao Paulo
(11) Department of Physics & Astronomy, CSCE, JINA, Michigan State University
(12) European Southern Observatory)
arXiv.org - Astrophysics - Volume: 2009, Issue: 27 Mar
arXiv:0903.4174
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A holistic approach to carbon-enhanced metal-poor stars
Volume 4, Issue 5 - article #2
T. Masseron
(1,2),
J. A. Johnson
(1),
B. Plez
(2,3),
S. Van Eck
(4),
F. Primas
(5),
S. Goriely
(4),
A. Jorissen
(4)
((1) The Ohio State University, USA,
(2) GRAAL, Université Montpellier II, France
(3) Department of Physics and Astronomy, Uppsala Astronomical Observatory, Sweden
(4) Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Belgium
(5) European Southern Observatory, Germany)
arXiv.org - Astrophysics - Volume: 2009, Issue: 29 Jan
arXiv:0901.4737
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Primordial black holes are again on the limelight
Volume 4, Issue 2 - article #7
Marco Roncadelli
(INFN, Sezione di Pavia, Italy),
Aldo Treves
(Physics Department, Universita' dell'Insubria, Italy),
Roberto Turolla
(Department of Physics, Universita' di Padova, Italy)
arXiv.org - Astrophysics - Volume: 2009, Issue: 8 Jan
arXiv:0901.1093
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Galactic Parameters from Whole Sky 2MASS Star Count
Volume 3, Issue 47 - article #10
C.K. Chang
(1),
C.M. Ko
(1 and 2),
T.H. Peng
(1)
((1) Institute of Astronomy, National Central University, Taiwan,
(2) Department of Physics and Center of Complex System, National Central University, Taiwan)
arXiv.org - Astrophysics - Volume: 2008, Issue: 20 Nov
arXiv:0811.3269
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The s process in massive stars at low metallicity. Effect of primary N14 from fast rotating stars
Volume 3, Issue 40 - article #11
M. Pignatari
(1,2),
R. Gallino
(3,4),
G. Meynet
(5),
R. Hirschi
(1,6),
F. Herwig
(1,7),
M. Wiescher
(2)
((1) Keele University, Keele, UK,
(2) JINA, University of Notre Dame, Notre Dame, IN, USA,
(3) Dipartimento di Fisica Generale, Universita' di Torino, Via Pietro Giuria 1, Torino, Italy,
(4) Center for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria, Australia,
(5) Geneva Observatory, Sauverny, Switzerland,
(6) IPMU, University of Tokyo, Kashiwa, Japan,
(7) Department of Physics & Astronomy, University of Victoria, Victoria, BC, Canada)
arXiv.org - Astrophysics - Volume: 2008, Issue: 2 Oct
arXiv:0810.0182
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L dwarfs in the Hyades
Volume 3, Issue 19 - article #12
E. Hogan
(1),
R. F. Jameson
(1),
S. L. Casewell
(1),
S. L. Osbourne
(1),
N. C. Hambly
(2)
((1) Department of Physics and Astronomy, University of Leicester,
(2) Scottish Universities' Physics Alliance
(SUPA), Institute for Astronomy, School of Physics, University of Edinburgh)
arXiv.org - Astrophysics - Volume: 2008, Issue: 8 May
arXiv:0805.1189
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Robust Machine Learning Applied to Astronomical Datasets III: Probabilistic Photometric Redshifts for Galaxies and Quasars in the SDSS and GALEX
Volume 3, Issue 17 - article #11
Nicholas M. Ball
(1),
Robert J. Brunner
(1 and 2),
Adam D. Myers
(1),
Natalie E. Strand
(3),
Stacey L. Alberts
(1),
David Tcheng
(2)
((1) Department of Astronomy, University of Illinois at Urbana-Champaign,
(2) National Center for Supercomputing Applications,
(3) Department of Physics, University of Illinois at Urbana-Champaign)
arXiv.org - Astrophysics - Volume: 2008, Issue: 24 Apr
arXiv:0804.3413
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The Dichotomy of the Halo of the Milky Way
Volume 3, Issue 16 - article #10
Daniela Carollo
(1),
Timothy C. Beers
(2)
((1) Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, The Australian National University, Australia, and INAF, Osservatorio Astronomico di Torino, Italy,
(2) Department of Physics and Astronomy, and JINA: Joint Institute for Nuclear Astrophysics, Michigan State University)
arXiv.org - Astrophysics - Volume: 2008, Issue: 17 Apr
arXiv:0804.2183
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A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae
Volume 3, Issue 10 - article #2
C.S. Kochanek
(1,3),
J.F. Beacom
(1,2,3),
M.D. Kistler
(2,3),
J.L. Prieto
(1,3)
K.Z. Stanek
(1,3),
T.A. Thompson
(1,3),
H. Yuksel
(2,3)
((1) Department of Astronomy, The Ohio State University,
(2) Department of Physics, The Ohio State University,
(3) Center for Cosmology and Astroparticle Physics, The Ohio State University)
arXiv.org - Astrophysics - Volume: 2008, Issue: 7 Feb
arXiv:0802.0456
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Disentangling the Galaxy at low Galactic latitudes
Volume 3, Issue 10 - article #12
M. Cignoni
(1 and 2),
M. Tosi
(2),
A. Bragaglia
(2),
J.S. Kalirai
(3),
D.S. Davis
(4)
((1) Dipartimento di Astronomia, Universita' degli Studi di Bologna, Italy,
(2) INAF-Osservatorio Astronomico di Bologna, Italy,
(3) UCO/Lick Observatory, Department of Astronomy and Astrophysics, University of California at Santa Cruz, CA,
(4) Department of Physics and Astronomy, University of British Columbia, Canada)
arXiv.org - Astrophysics - Volume: 2008, Issue: 6 Mar
arXiv:0803.0674
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The ESO Large Programme First Stars
Volume 3, Issue 2 - article #19
P. Bonifacio
(1,2,3),
J. Andersen
(4,5),
S. Andrievsky
(6),
B. Barbuy
(7),
T. C. Beers
(8),
E. Caffau
(2),
R. Cayrel
(2),
E. Depagne
(9),
P. Francois
(2),
J. I. Gonzalez Hernandez
(1,2),
C. J. Hansen
(10),
F. Herwig
(11),
V. Hill
(2),
S. A. Korotin
(6),
H.-G. Ludwig
(1,2),
P. Molaro
(3),
B. Nordstrom
(4),
B. Plez
(12),
F. Primas
(10),
T. Sivarani
(8),
F. Spite
(2),
M. Spite
(2)
((1) CIFIST Marie Curie Excellence Team,
(2) GEPI, Observatoire de Paris, CNRS, Universite' Paris Diderot,
(3) Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Trieste,
(4) The Niels Bohr Institute, Astronomy,
(5) Nordic Optical Telescope,
(6) Department of Astronomy and Astronomical Observatory, Odessa National University,
(7) Universidade de Sao Paulo, Departamento de Astronomia,
(8) Department of Physics & Astronomy and JINA: Joint Institute for Nuclear Astrophysics, Michigan State University,
(9) Las Cumbres Observatory, Santa Barbara,
(10) European Southern Observatory
(ESO),
(11) Keele Astrophysics Group, School of Physical and Geographical Sciences, Keele University,
(12) GRAAL, Université de Montpellier II)
arXiv.org - Astrophysics - Volume: 2008, Issue: 10 Jan
arXiv:0801.1293
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Metal Abundance Properties of M81 Globular Cluster System
Volume 2, Issue 35 - article #13
Jun Ma
(1),
David Burstein
(2),
Zhou Fan
,
Xu Zhou
,
Jiansheng Chen
,
Zhaoji Jiang
,
Zhenyu Wu
,
Jianghua Wu
((1)National Astronomical Observatories, Chinese Academy of Sciences,
(2)Department of Physics and Astronomy, Arizona State University, Tempe, AZ)
ArXiv - Astrophysics
arXiv:0708.4083
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A Wide-Field View of Leo II -- A Structural Analysis Using the SDSS
Volume 2, Issue 33 - article #13
Matthew G. Coleman
(1),
Katrin Jordi
(2),
Hans-Walter Rix
(1),
Eva K. Grebel
(2),
Andreas Koch
(3)
((1) Max-Planck-Institut fur Astronomie, Heidelberg, Germany,
(2) Astronomisches Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Heidelberg, Germany,
(3) Department of Physics and Astronomy, UCLA, Los Angeles, CA, USA)
ArXiv - Astrophysics
arXiv:0708.1853
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Variable stars in the Fornax dSph Galaxy. I. The Globular Cluster Fornax 4
Volume 2, Issue 32 - article #13
C. Greco
(1,2,3),
G. Clementini
(1),
M. Catelan
(4),
E. V. Held
(5),
E. Poretti
(6),
M. Gullieuszik
(7),
M. Maio
(1),
A. Rest
(8),
N. De Lee
(9),
H. A. Smith
(9),
B. J. Pritzl
(10)
((1) INAF - Osservatorio Astronomico di Bologna,
(2) Dipartimento di Astronomia, Universita' di Bologna,
(3) Marco Polo Fellow at the Pontificia Universidad de Chile,
(4) Pontificia Universidad de Chile,
(5) INAF - Osservatorio Astronomico di Padova,
(6) INAF - Osservatorio Astronomico di Brera,
(7) Dipartimento di Astronomia, Universita' di Padova,
(8) Cerro Tololo Inter American Observatory,
(9) Department of Physics and Astronomy, Michigan State University,
(10) Macalester College)
ArXiv - Astrophysics
arXiv:0708.0405
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Low-mass lithium-rich AGB stars in the Galactic bulge: evidence for Cool Bottom Processing?
Volume 2, Issue 28 - article #10
Stefan Uttenthaler
(1),
Thomas Lebzelter
(1),
Sara Palmerini
(2),
Maurizio Busso
(2),
Bernhard Aringer
(1),
Michael T. Lederer
(1)
((1) Institute for Astronomy, University of Vienna, Austria
(2) Department of Physics, University of Perugia, Italy)
ArXiv - Astrophysics
arXiv:0707.1380
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Investigation of the single neutron exposure model for the s-process: the primary nature of the neutron source
Volume 2, Issue 9 - article #10
Kun Ma
(1),
W. Y. Cui
(1 and 2),
B. Zhang
(1)
((1) Department of Physics, Hebei Normal University, China,
(2) National Astronomical observatories, Chinese Academy of Sciences, China)
ArXiv - Astrophysics
astro-ph/0702677 [
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