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Results 1 - 32 of 32
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
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets. (arXiv:2111.01753v1 [astro-ph.EP])
Volume 16, Issue 45 - article #9
Robert F. Wilson
(1, 2),
Caleb I. Cañas
(3, 4),
Steven R. Majewski
(1),
Katia Cunha
(5, 6),
Verne V. Smith
(7),
Chad F. Bender
(6),
Suvrath Mahadevan
(3, 4),
Scott W. Fleming
(8),
Johanna Teske
(9),
Luan Ghezzi
(10),
Henrik Jönsson
(11),
Rachael L. Beaton
(12, 13),
Sten Hasselquist
(14),
Keivan Stassun
(15),
Christian Nitschelm
(16),
D. A. García-Hernández
(17, 18),
Christian R. Hayes
(19),
Jamie Tayar
(20, 21)
((1) University of Virginia Department of Astronomy,
(2) NASA Goddard Space Flight Center,
(3) The Pennsylvania State University Department of Astronomy & Astrophysics,
(4) The Pennsylvania State University Center for Exoplanets, Habitable Worlds,
(5) Observatório Nacional,
(6) Steward Observatory,
(7) NSF's NOIRLab,
(8) Space Telescope Science Institute,
(9) Carnegie Earth, Planets Laboratory,
(10) Universidade Federal do Rio de Janeiro,
(11) Malmö University Materials Science, Applied Mathematics,
(12) Princeton University Department of Astrophysical Sciences,
(13) The Observatories of the Carnegie Institution for Science,
(14) University of Utah Department of Physics & Astronomy,
(15) Vanderbilt University Department of Physics, Astronomy,
(16) Universidad de Antofagasta Centro de Astronomía,
(17) Instituto de Astrofísica de Canarias,
(18) Departamento de Astrofísica Universidad de La Laguna,
(19) University of Washington Department of Astronomy,
(20) University of Hawai'i at Manoa Institute for Astronomy,
(21) University of Florida Department of Astronomy)
http://arxiv.org/abs/2111.01753
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. (arXiv:2109.11600v1 [astro-ph.SR])
Volume 16, Issue 40 - article #2
Carlos Andrés Galarza
(1),
Simone Daflon
(1),
Vinicius M. Placco
(2),
Carlos Allende-Prieto
(3, 4),
Marcelo Borges Fernandes
(1),
Haibo Yuan
(5),
Carlos López-Sanjuan
(6),
Young Sun Lee
(7),
Enrique Solano
(8),
F. Jiménez-Esteban
(8),
David Sobral
(9),
Alvaro Alvarez Candal
(1, 17),
Claudio B. Pereira
(1),
Stavros Akras
(10),
Eduardo Martín
(3, 8),
Yolanda Jiménez Teja
(16),
Javier Cenarro
(6),
David Cristóbal-Hornillos
(6),
Carlos Hernández-Monteagudo
(6),
Antonio Marín-Franch
(6),
Mariano Moles
(6),
Jesús Varela
(6),
Héctor Vázquez Ramió
,
(6),
Jailson Alcaniz
(1),
Renato Dupke
(1, 13, 14, 15),
Alessandro Ederoclite
(11),
Laerte Sodré
,
Jr.
(11),
Raul E. Angulo
(12)
((1) Observatório Nacional - MCTI ON, Rio de Janeiro, Brazil,
(2) NSF's NOIRLab, Tucson, AZ 85719, USA,
(3) Instituto de Astrofísica de Canarias, Tenerife, Spain,
(4) Universidad de La Laguna, Departamento de Astrofísica, Tenerife, Spain,
(5) Department of Astronomy, Beijing Normal University, Beijing, People's Republic of China,
(6) Centro de Estudios de Física del Cosmos de Aragón CEFCA, Unidad Asociada al CSIC, Teruel, Spain,
(7) Department of Astronomy, Space Science, Chungnam National University, South Korea,
(8) Departamento de Astrofísica, Centro de Astrobiología CSIC-INTA, ESAC Campus, Villanueva de la Cañada, Madrid, Spain,
(9) Department of Physics, Lancaster University, Lancaster, UK,
(10) Institute for Astronomy, Astrophysics, Space Applications, Remote Sensing, National Observatory of Athens, GR Penteli, Greece,
(11) Universidade de São Paulo, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, São Paulo, Brazil,
(12) Ikerbasque, Basque Foundation for Science, Bilbao, Spain,
(13) Department of Astronomy, University of Michigan, Ann Arbor, MI USA,
(14) Eureka Scientific Inc., Oakland, CA, USA,
(15) Department of Physics, Astronomy, University of Alabama, Tuscaloosa, AL, USA,
(16) Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía, Granada, Spain,
(17) Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain)
http://arxiv.org/abs/2109.11600
On the Use of Field RR Lyrae as Galactic Probes. III. The $alpha$-element abundances. (arXiv:2104.08113v1 [astro-ph.GA])
Volume 16, Issue 17 - article #2
J. Crestani
(1,2,3),
V.F. Braga
(3,4),
M. Fabrizio
(3,4),
G. Bono
(2,3),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
M. Nonino
(7),
G. Fiorentino
(3),
F. Thévenin
(8),
B. Lemasle
(9),
Z. Prudil
(8),
A. Alves-Brito
(1),
G. Altavilla
(3,4),
B. Chaboyer
(10),
M. Dall'Ora
(11),
V. D'Orazi
(12,13),
C.K. Gilligan
(10),
E. Grebel
(8),
A.J. Koch-Hansen
(9),
H. Lala
(9),
M. Marengo
(14),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J.P. Mullen
(14),
J. Neeley
(18),
R. da Silva
(3,4),
P.B. Stetson
(19),
M. Salaris
(20),
J. Storm
(21),
E. Valenti
(22),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(9) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(10) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(11) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(12) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(13) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(16) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(19) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(20) Astrophysics Research Institute, Liverpool John Moores University, Liverpool, UK,
(21) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2104.08113
On the Use of Field RR Lyrae as Galactic Probes. II. A new $Delta$S calibration to estimate their metallicity. (arXiv:2012.02284v1 [astro-ph.SR])
Volume 15, Issue 50 - article #6
J. Crestani
(1,2,3),
M. Fabrizio
(3,4),
V.F. Braga
(3,4),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
G. Bono
(2,3),
A. Alves-Brito
(1),
M. Nonino
(7),
V. D'Orazi
(8,9),
L. Inno
(10),
M. Monelli
(11),
J. Storm
(12),
G. Altavilla
(3,4),
B. Chaboyer
(13),
M. Dall'Ora
(14),
G. Fiorentino
(3),
C.K. Gilligan
(13),
E. Grebel
(15),
H. Lala
(16),
B. Lemasle
(16),
M. Marengo
(17),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(18),
N. Matsunaga
(19),
J.P. Mullen
(17),
J. Neeley
(20),
Z. Prudil
(15),
R. da Silva
(3,4),
P.B. Stetson
(21),
F. Thévenin
(15),
E. Valenti
(22),
A.R. Walker
(18),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(9) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(10) Università degli Studi di Napoli "Parthenope'', Napoli, Italy,
(11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(12) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(13) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(14) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(15) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(16) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(17) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(18) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(19) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(20) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(21) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2012.02284
Preliminary Target Selection for the DESI Milky Way Survey (MWS). (arXiv:2010.11284v1 [astro-ph.GA])
Volume 15, Issue 43 - article #4
Carlos Allende Prieto
(1, 2),
Andrew P. Cooper
(3),
Arjun Dey
(4),
Boris T. Gänsicke
(5),
Sergey E. Koposov
(6, 7, 8),
Ting Li
(9, 10),
Christopher Manser
(5),
David L. Nidever
(4, 11),
Constance Rockosi
(12, 13),
Mei-Yu Wang
(7, 14),
David S. Aguado
(8),
Robert Blum
(15),
David Brooks
(16),
Daniel J. Eisenstein
(17),
Yutong Duan
(18),
Sarah Eftekharzadeh
(19),
Enrique Gaztañaga
(20, 21),
Robert Kehoe
(22),
Martin Landriau
(23),
Chien-Hsiu Lee
(4),
Michael E. Levi
(23)
Aaron M. Meisner
(4),
Adam D. Myers
(24),
Joan Najita
(4),
Knut Olsen
(25),
Nathalie Palanque-Delabrouille
(26),
Claire Poppett
(23, 27),
Francisco Prada
(28),
David J. Schlegel
(23),
Michael Schubnell
(29),
Gregory Tarlé
,
(29),
Monica Valluri
(30),
Risa H. Wechsler
(31, 32),
Christophe Yèche
(26)
((1) Instituto de Astrofísica de Canarias,
(2) Universidad de La Laguna,
(3) National Tsing Hua University.
(4) NSF's NOIRLab,
(5) Department of Physics, University of Warwick,
(6) Institute for Astronomy, University of Edinburgh,
(7) McWilliams Center for Cosmology, Carnegie Mellon University,
(8) Institute of Astronomy, University of Cambridge,
(9) Observatories of the Carnegie Institution for Science,
(10) Department of Astrophysical Sciences, Princeton University,
(11) Department of Physics, Montana State University,
(12) Department of Astronomy, Astrophysics, University of California Santa Cruz,
(13) University of California Observatories,
(14) Department of Physics, Carnegie Mellon University,
(15) Vera C. Rubin Observatory/NSF's NOIRLab,
(16) Department of Physics, Astronomy, University College London,
(17) Harvard-Smithsonian Center for Astrophysics,
(18) Physics Department, Boston University,
(19) Department of Physics, Astronomy, The University of Utah,
(20) Institute of Space Sciences
(ICE, CSIC),
(21) Institut d' Estudis Espacials de Catalunya
(IEEC),
(22) Department of Physics, Southern Methodist University,
(23) Lawrence Berkeley National Laboratory,
(24) University of Wyoming,
(25) Community Science, Data Center/NSF's NOIRLab,
(26) IRFU, CEA, Université Paris-Saclay,
(28) Instituto de Astrofisica de Andalucía,
(29) Department of Physics, University of Michigan,
(30) Department of Astronomy, University of Michigan,
(31) Kavli Institute for Particle Astrophysics, Cosmology, Department of Physics,
(32) SLAC National Accelerator Laboratory)
http://arxiv.org/abs/2010.11284
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
On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $omega$ Centauri as a first test case. (arXiv:1811.07069v1 [astro-ph.SR])
Volume 13, Issue 47 - article #2
G. Bono
(1, 2),
G. Iannicola
(2),
V.F. Braga
(3, 4),
I. Ferraro
(2),
P.B. Stetson
(5),
D. Magurno
(1),
N. Matsunaga
(6),
R.L. Beaton
(7),
R. Buonanno
(8),
B. Chaboyer
(9),
M. Dall'Ora
(10),
M. Fabrizio
(2, 11),
G. Fiorentino
(12),
W.L. Freedman
(13,7),
C.K. Gilligan
(9),
B.F. Madore
(7),
M. Marconi
(10),
M. Marengo
(14),
S. Marinoni
(2, 11),
P. Marrese
(2, 11),
C.E. Martinez-Vazquez
(15),
M. Mateo
(16),
M. Monelli
(17, 18),
J.R. Neeley
(19),
M. Nonino
(20),
C. Sneden
(21),
F. Thevenin
(22),
E. Valenti
(23),
A.R. Walker
(15)
((1) Department of Physics, Università di Roma Tor Vergata, Roma, Italy,
(2) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(3) Instituto Milenio de Astrofisica, Santiago, Chile,
(4) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile,
(5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria BC, Canada,
(6) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Nagano Japan,
(7) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(8) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy,
(9) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA,
(10) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(11) SSDC, Roma, Italy,
(12) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy,
(13) Department of Astronomy, Astrophysics, University of Chicago, Chicago, IL, USA,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile,
(16) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain,
(19) Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA,
(20) INAF-Osservatorio Astronomico di Trieste, Trieste, Italy,
(21) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(22) Universite de Nice Sophia-antipolis, CNRS, Observatoire de la Cote d'Azur, Laboratoire Lagrange, Nice, France,
(23) European Southern Observatory, Garching bei Munchen, Germany)
http://arxiv.org/abs/1811.07069
The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS. (arXiv:1804.05869v1 [astro-ph.SR])
Volume 13, Issue 16 - article #10
S. Buder
(1),
K. Lind
(1,2),
M. K. Ness
(3,4),
M. Asplund
(5,6),
L. Duong
(5),
J. Lin
(5),
J. Kos
(7),
L. Casagrande
(5,6),
J. Bland-Hawthorn
(7,6),
A. R. Casey
(8),
G. M. De Silva
(9, 7),
V. D'Orazi
(10),
K. C. Freeman
(5),
G. F. Lewis
(7),
S. L. Martell
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K. J. Schlesinger
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J. D. Simpson
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D. B. Zucker
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K. Cotar
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T. Nordlander
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W. Reid
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A. Skuladottir
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D. Stello
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Y.-S. Ting
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G. Traven
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R. F. G. Wyse
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((1) MPIA Heidelberg,
(2) Uppsala University,
(3) Columbia University New York,
(4) CCA New York,
(5) RSAA/MSO Canberra,
(6) ASTRO-3D Australia,
(7) SIfA Sydney,
(8) Monash University,
(9) AAO North Ryde,
(10) INAF Padova,
(11) UNSW Sydney,
(12) Macquarie University Sydney,
(13) University of Ljubljana,
(14) Harvard/CfA Cambridge,
(15) Western Sydney University,
(16) University of Western Australia,
(17) Johns Hopkins University Baltimore,
(18) Aarhus University,
(19) IAS Princeton,
(20) Princeton University,
(21) Carnegie Observatories Pasadena)
http://arxiv.org/abs/1804.05869
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
Volume 13, Issue 16 - article #12
S. Buder
(1,2),
M. Asplund
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L. Duong
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J. Kos
(5),
K. Lind
(1,6),
M. K. Ness
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S. Sharma
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J. Bland-Hawthorn
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A. R. Casey
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G. M. De Silva
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V. D'Orazi
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K. C. Freeman
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G. F. Lewis
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K. J. Schlesinger
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J. D. Simpson
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D. B. Zucker
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T. Zwitter
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A. M. Amarsi
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D. Carollo
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K. Cotar
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P. L. Cottrell
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G. Da Costa
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X. D. Gao
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M. R. Hayden
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J. Horner
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M. J. Ireland
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P. R. Kafle
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U. Munari
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D. M. Nataf
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T. Nordlander
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Dennis Stello
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Y.-S. Ting
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G. Traven
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F. Watson
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R. A. Wittenmyer
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R. F. G. Wyse
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D. Yong
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J. C. Zinn
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M. Zerjal
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((1) MPIA Heidelberg,
(2) IMPRS HD,
(3) RSAA/MSO Canberra,
(4) ASTRO-3D Australia,
(5) SIfA Sydney,
(6) Uppsala University,
(7) Columbia University New York,
(8) CCA New York
(9) Monash University,
(10) AAO North Ryde,
(11) INAF Padova,
(12) UNSW Sydney,
(13) Macquarie University Sydney,
(14) University of Ljubljana,
(15) University of Virginia,
(16) INAF Turin,
(17) University of Canterbury,
(18) University of Southern Queensland,
(19) University of Western Australia,
(20) INAF Padova,
(21) Johns Hopkins University Baltimore,
(22) Aarhus University,
(23) IAS Princeton,
(24) Princeton University,
(25) Carnegie Observatories Pasadena,
(26) Western Sydney University,
(27) The Ohio State University)
http://arxiv.org/abs/1804.06041
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
On the RR Lyrae stars in globulars: IV. $omega$ Centauri Optical UBVRI Photometry. (arXiv:1609.04916v1 [astro-ph.SR])
Volume 11, Issue 39 - article #12
V. F. Braga
(1, 2),
P. B. Stetson
(3),
G. Bono
(1, 4),
M. Dall'Ora
(5),
I. Ferraro
(4),
G. Fiorentino
(6),
L. M. Freyhammer
(7),
G. Iannicola
(4),
M. Marengo
(8),
J. Neeley
(8),
E. Valenti
(9),
R. Buonanno
(1, 10),
A. Calamida
(11),
M. Castellani
(4),
R. da Silva
(4, 2),
S. Degl'Innocenti
(12, 13),
A. Di Cecco
(10),
M. Fabrizio
(10, 2),
W. L. Freedman
(14),
G. Giuffrida
(4, 2),
J. Lub
(15),
B. F. Madore
(16),
M. Marconi
(5),
S. Marinoni
(4, 2),
N. Matsunaga
(17),
M. Monelli
(18),
S. E. Persson
(16),
A. M. Piersimoni
(10),
A. Pietrinferni
(10),
P. Prada-Moroni
(12, 13),
L. Pulone
(4),
R. Stellingwerf
(19),
E. Tognelli
(12, 13),
A. R. Walker
(20)
((1) Department of Physics, Università di Roma Tor Vergata
(2) ASDC
(3) NRC-Herzberg, Dominion Astrophysical Observatory
(4) INAF-Osservatorio Astronomico di Roma
(5) INAF-Osservatorio Astronomico di Capodimonte
(6) INAF-Osservatorio Astronomico di Bologna
(7) Jeremiah Horrocks Institute of Astrophysics, University of Central Lancashire
(8) Department of Physics, Astronomy, Iowa State University
(9) European Southern Observatory
(10) INAF-Osservatorio Astronomico di Teramo
(11) National Optical Astronomy Observatory
(12) INFN, Sezione di Pisa
(13) Dipartimento di Fisica Enrico Fermi, Università di Pisa
(14) Department of Astronomy & Astrophysics, University of Chicago
(15) Sterrewacht Leiden, Leiden University
(16) The Observatories of the Carnegie Institution for Science
(17) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo
(18) Instituto de Astrofísica de Canarias
(19) Stellingwerf Consulting
(20) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory)
http://arxiv.org/abs/1609.04916
The LSST Data Management System
Volume 11, Issue 1 - article #3
Mario Jurić
,
Jeffrey Kantor
,
K-T Lim
,
Robert H. Lupton
,
Gregory Dubois-Felsmann
,
Tim Jenness
,
Tim S. Axelrod
,
Jovan Aleksić
,
Roberta A. Allsman
,
Yusra AlSayyad
,
Jason Alt
,
Robert Armstrong
,
Jim Basney
,
Andrew C. Becker
,
Jacek Becla
,
Steven J. Bickerton
,
Rahul Biswas
,
James Bosch
,
Dominique Boutigny
,
Matias Carrasco Kind
,
David R. Ciardi
,
Andrew J. Connolly
,
Scott F. Daniel
,
Gregory E. Daues
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Frossie Economou
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Hsin-Fang Chiang
,
Angelo Fausti
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Merlin Fisher-Levine
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D. Michael Freemon
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Perry Gee
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Philippe Gris
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Fabio Hernandez
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Joshua Hoblitt
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Željko Ivezić
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Fabrice Jammes
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Darko Jevremović
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R. Lynne Jones
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J. Bryce Kalmbach
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Vishal P. Kasliwal
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K. Simon Krughoff
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Dustin Lang
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Nate B. Lust
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Peter Melchior
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arXiv.org - Astrophysics - Volume: 2016, Issue: 1 Jan
arXiv:1512.07914
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A disintegrating minor planet transiting a white dwarf
Volume 10, Issue 39 - article #27
The atmospheres of white dwarfs often contain elements heavier than helium
,
even though these elements would be expected to settle into the stars’
,
interiors
,
observations of the white dwarf WD 1145+017 suggest that disintegrating rocky bodies are orbiting the star
,
perhaps contributing heavy elements to its atmosphere.
Nature - Volume: 526, Issue: 7574
478-602
Cosmology: The oldest cosmic light
Volume 10, Issue 6 - article #27
A review of the phases of copper oxides
(especially the ‘strange metal’),
discussing their high-temperature superconductivity
and
their various forms of quantum matter
,
and
the implications for fundamental theory.
Nature - Volume: 518, Issue: 7538
140-268
The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
Volume 10, Issue 1 - article #8
Shadab Alam
(1),
Franco D. Albareti
(2),
Carlos Allende Prieto
(3,4),
F. Anders
(5),
Scott F. Anderson
(6),
Brett H. Andrews
(7,8),
Eric Armengaud
(9),
Éric Aubourg
(10),
Stephen Bailey
(11),
Julian E. Bautista
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Rachael L. Beaton
(12,13),
Timothy C. Beers
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Chad F. Bender
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Andreas A. Berlind
(17),
Florian Beutler
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Vaishali Bhardwaj
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Jonathan C. Bird
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Dmitry Bizyaev
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Cullen H. Blake
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Michael R. Blanton
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Michael Blomqvist
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John J. Bochanski
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Adam S. Bolton
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Jo Bovy
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A. Shelden Bradley
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W. N. Brandt
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D. E. Brauer
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J. Brinkmann
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Peter J. Brown
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Joel R. Brownstein
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Angela Burden
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Etienne Burtin
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Nicolás G. Busca
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Zheng Cai
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Diego Capozzi
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Aurelio Carnero Rosell
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arXiv.org - Astrophysics - Volume: 2015, Issue: 9 Jan
arXiv:1501.00963
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Synthetic biology: Engineering explored
Volume 9, Issue 19 - article #17
A simulation that starts 12 million years after the Big Bang
and
traces 13 billion years of cosmic evolution yields a reasonable population of elliptical
and
spiral galaxies
,
reproduces the observed distribution of galaxies in clusters
and
the characteristics of hydrogen on large scales
,
and
at the same time matches the ‘metal’
,
and
hydrogen content of galaxies on small scales.
Nature - Volume: 509, Issue: 7499
136-254
A single low-energy, iron-poor supernova as the source of metals in the star SMSS J031300.36−670839.3
Volume 9, Issue 9 - article #15
The optical spectrum of the star SMSS J031300.36−670839.3 shows no evidence of iron
,
this
,
together with comparisons of the star’s observed element abundance pattern with those of models
,
means that SMSS J031300.36−670839.3 must have been seeded with material from a single supernova with an original mass about 60 times that of the Sun.
Nature - Volume: 506, Issue: 7489
410-522
The AGORA High-Resolution Galaxy Simulations Comparison Project
Volume 8, Issue 33 - article #11
Ji-hoon Kim
(1),
Tom Abel
(2),
Oscar Agertz
(3, 4),
Greg L. Bryan
(5),
Daniel Ceverino
(6),
Charlotte Christensen
(7),
Charlie Conroy
(1),
Avishai Dekel
(8),
Nickolay Y. Gnedin
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Nathan J. Goldbaum
(1),
Javiera Guedes
(11),
Oliver Hahn
(11),
Alexander Hobbs
(11),
Philip F. Hopkins
(12, 13),
Cameron B. Hummels
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Francesca Iannuzzi
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Dusan Keres
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Anatoly Klypin
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Andrey V. Kravtsov
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Mark R. Krumholz
(1),
Michael Kuhlen
(1, 13),
Samuel N. Leitner
(17),
Piero Madau
(1),
Lucio Mayer
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Christopher E. Moody
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Kentaro Nagamine
(19, 20),
Michael L. Norman
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Jose Oñorbe
(21),
Brian W. O'Shea
(22),
Annalisa Pillepich
(1),
Joel R. Primack
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Thomas Quinn
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Justin I. Read
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Brant E. Robertson
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Miguel Rocha
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arXiv.org - Astrophysics - Volume: 2013, Issue: 16 Aug
arXiv:1308.2669
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Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
Volume 7, Issue 36 - article #20
The abundance of interstellar Li in the low-metallicity gas of the Small Magellanic Cloud
,
a nearby galaxy with a quarter the Sun’s metallicity
,
is nearly equal to the Big Bang nucleosynthesis predictions.
Nature - Volume: 489, Issue: 7414
5-170
Lithium-rich giants in the Galactic thick disk
Volume 6, Issue 10 - article #16
L. Monaco
(1),
S. Villanova
(2),
C. Moni Bidin
(2),
G. Carraro
(1),
D. Geisler
(2),
P. Bonifacio
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O. A. Gonzalez
(4),
M. Zoccali
(5),
L. Jilkova
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((1) ESO, Casilla 19001, Santiago, Chile,
(2) Universidad de Concepción, Casilla 160-C, Concepción, Chile,
(3) GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, Place Jules Janssen, 92190 Meudon, France,
(4) ESO, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany,
(5) Departamento Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860 Stgo., Chile,
(6) Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University,
(Kotlářská 2, CZ-611 37) Brno, Czech Republic)
arXiv.org - Astrophysics - Volume: 2011, Issue: 11 Mar
arXiv:1103.1658
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Searches for Dark Matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
Volume 6, Issue 9 - article #4
The MAGIC Collaboration
(and others):
J. Aleksić
,
(1),
E. A. Alvarez
(2),
L. A. Antonelli
(3),
P. Antoranz
(4),
M. Asensio
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M. Backes
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J. A. Barrio
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D. Bastieri
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J. Becerra González
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W. Bednarek
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A. Berdyugin
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K. Berger
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E. Bernardini
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A. Biland
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O. Blanch
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R. K. Bock
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A. Boller
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G. Bonnoli
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D. Borla Tridon
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I. Braun
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T. Bretz
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A. Cañellas
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E. Carmona
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A. Carosi
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P. Colin
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J. L. Contreras
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J. Cortina
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L. Cossio
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S. Covino
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F. Dazzi
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A. De Angelis
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E. De Cea del Pozo
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C. Delgado Mendez
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A. Diago Ortega
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M. Doert
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A. Domínguez
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D. Dominis Prester
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D. Dorner
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M. Doro
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arXiv.org - Astrophysics - Volume: 2011, Issue: 4 Mar
arXiv:1103.0477
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Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
Volume 5, Issue 31 - article #6
T. Zwitter
(1 and 2),
G. Matijeviv{c)
(1)
,
M. A. Breddels
(3)
,
M. C. Smith
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,
4)
,
A. Helmi
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U. Munari
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O. Bienaym'{e)
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J. Binney
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J. Bland-Hawthorn
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C. Boeche
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A. G. A. Brown
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R. Campbell
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K. C. Freeman
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B. Gibson
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G. Gilmore
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J. F. Navarro
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Q. A. Parker
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G. M. Seabroke
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A. Siebert
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A. Siviero
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M. Steinmetz
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F. G. Watson
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M. Williams
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R. F. G. Wyse
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((1) University of Ljubljana
,
Faculty of Mathematics
,
Physics
,
Ljubljana
,
Slovenia}
(2) Center of excellence SPACE-SI
,
Ljubljana
,
Slovenia
,
(3) Kapteyn Astronomical Institute
,
University of Groningen
,
Groningen
,
The Netherlands
,
(4) Kavli Institute for Astronomy
,
Astrophysics
,
Peking University
,
Beijing
,
China
,
(5) INAF Astronomical Observatory of Padova
,
et al.
(36 additional authors not shown)
arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
arXiv:1007.4411
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Orbital periods of cataclysmic variables identified by the SDSS - VI. The 4.5-h period eclipsing system SDSS J100658.40+233724.4
Volume 4, Issue 47 - article #22
J. Southworth
,
R. D. G. Hickman
,
T. R. Marsh
,
A. Rebassa-Mansergas
,
B. T. Gänsicke
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C. M. Copperwheat
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and
P. Rodríguez-Gil
Astronomy and Astrophysics - Volume: 507, Issue: 2
Abstract
|
PDF file (861.8 KB)
|
PS file (2.836 MB)
On the metallicity gradient of the Galactic disk
Volume 4, Issue 37 - article #20
S. Pedicelli
,
G. Bono
,
B. Lemasle
,
P. François
,
M. Groenewegen
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J. Lub
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J. W. Pel
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A. Piersimoni
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M. Romaniello
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R. Buonanno
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S. Cassisi
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F. Castelli
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S. Leurini
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A. Pietrinferni
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F. Primas
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J. Pritchard
Astronomy and Astrophysics - Volume: 504, Issue: 1
Abstract
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Full HTML
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PDF file (371.4 KB)
|
PS file (425.1 KB)
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References
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Departures from LTE for neutral Li in late-type stars
Volume 4, Issue 35 - article #10
K. Lind
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Astronomy and Astrophysics - Volume: 503, Issue: 2
Abstract
|
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Properties of RR Lyrae stars in the inner regions of the Large Magellanic Cloud - III. Near-infrared study
Volume 4, Issue 32 - article #11
J. Borissova
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Astronomy and Astrophysics - Volume: 502, Issue: 2
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Multiple stellar populations in Magellanic Cloud clusters - I. An ordinary feature for intermediate age globulars in the LMC?
Volume 4, Issue 16 - article #8
A. P. Milone
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L. R. Bedin
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Astronomy and Astrophysics - Volume: 497, Issue: 3
Abstract
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Spectroscopic and photometric evidence of two stellar populations in the Galactic globular cluster NGC 6121 (M 4)
Volume 3, Issue 42 - article #27
A. F. Marino
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,
and
A. M. Medling
Astronomy and Astrophysics - Volume: 490, Issue: 2
Abstract
|
PDF file (1.254 MB)
|
PS file (403.1 KB)
Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey
Volume 3, Issue 23 - article #11
D. J. Pinfield
(1),
B. Burningham
(1),
M. Tamura
(2),
S. K. Leggett
(3),
N. Lodieu
(4),
P. W. Lucas
(1),
D. J. Mortlock
(5),
S. J. Warren
(5),
D. Homeier
(6),
M. Ishi
(7),
N. R. Deacon
(8),
R. G. McMahon
(9),
P. C. Hewett
(9),
M. R. Zapatero Osorio
(4),
E. L. Martin
(4),
H. R. A. Jones
(1),
B.P. Venemans
(9),
A. Day-Jones
(1),
P. D. Dobbie
(10),
S. L. Folkes
(1),
S. Dye
(11),
F. Allard
(12),
I. Baraffe
(13),
D. Barrado y Navascues
(14),
S. L. Casewell
(15),
K. Chiu
(16),
G. Chabrier
(13),
F. Clarke
(17),
S. T. Hodgkin
(9),
A. Magazzu
(18),
M. J. McCaughrean
(16),
E. Moraux
(19),
T. Nakajima
(2),
Y. Pavlenko
(20),
C. G. Tinney
(21)
((1) University of Hertfordshire, UK,
(2) National Astronomical Observatory, Japan,
(3) Gemini Observatory, USA,
(4) Instituto de Astrofisica de Canarias, Spain,
(5) Imperial College London, UK,
(6) Georg-August-Universitat, Germany,
(7) Subaru Telescope, USA,
(8) Radboud University, The Netherlands,
(9) Cambridge University, UK,
(10) Anglo-Australian Observatory, Australia,
(11) Cardif University, UK,
(12) Universite de Lyon, France,
(13) C.R.A.L., France,
(14) Laboratorio de Astrofisica Espacial y Fisica Fundamental, Spain,
(15) University of Leicester, UK,
(16) University of Exeter, UK,
(17) European Southern Observatory, Chile,
(18) Fundacion Galileo Galilei-INAF, Spain,
(19) Laboratoire d'Astrophysique de Grenoble, France,
(20) Main Astronomical Observatory, Ukraine,
(21) University of New South Wales, Australia)
arXiv.org - Astrophysics - Volume: 2008, Issue: 5 Jun
arXiv:0806.0294
[
ps
,
pdf
,
other
]
A Wide‐Field Kinematic Survey for Tidal Tails around Five Globular Clusters
Volume 2, Issue 52 - article #5
L. L. Kiss
,
P. Székely
,
T. R. Bedding
,
G. Á. Bakos
,
and
G. F. Lewis
The Astrophysical Journal Letters - Volume: 659, Issue: 2
Abstract
-
Full Text
-
PDF Version (333 kB)
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