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Results 1 - 58 of 58
The Early Data Release of the Dark Energy Spectroscopic Instrument. (arXiv:2306.06308v1 [astro-ph.CO])
Volume 18, Issue 24 - article #7
DESI Collaboration: A. G. Adame
,
J. Aguilar
,
S. Ahlen
,
S. Alam
,
G. Aldering
,
D. M. Alexander
,
R. Alfarsy
,
C. Allende Prieto
,
M. Alvarez
,
O. Alves
,
A. Anand
,
F. Andrade-Oliveira
,
E. Armengaud
,
J. Asorey
,
S. Avila
,
A. Aviles
,
S. Bailey
,
A. Balaguera-Antolínez
,
O. Ballester
,
C. Baltay
,
A. Bault
,
J. Bautista
,
J. Behera
,
S. F. Beltran
,
S. BenZvi
,
L. Beraldo e Silva
,
J. R. Bermejo-Climent
,
A. Berti
,
R. Besuner
,
F. Beutler
,
D. Bianchi
,
C. Blake
,
R. Blum
,
A. S. Bolton
,
S. Brieden
,
A. Brodzeller
,
D. Brooks
,
Z. Brown
,
E. Buckley-Geer
,
E. Burtin
,
L. Cabayol-Garcia
,
Z. Cai
,
R. Canning
,
L. Cardiel-Sas
,
A. Carnero Rosell
,
F. J. Castander
,
J.L. Cervantes-Cota
,
S. Chabanier
,
E. Chaussidon
,
J. Chaves-Montero
,
S. Chen
,
C. Chuang
,
T. Claybaugh
,
S. Cole
,
A. P. Cooper
,
A. Cuceu
,
T. M. Davis
,
K. Dawson
,
R. de Belsunce
,
et al.
(205 additional authors not shown)
http://arxiv.org/abs/2306.06308
Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument. (arXiv:2306.06307v1 [astro-ph.CO])
Volume 18, Issue 24 - article #9
DESI Collaboration: A. G. Adame
,
J. Aguilar
,
S. Ahlen
,
S. Alam
,
G. Aldering
,
D. M. Alexander
,
R. Alfarsy
,
C. Allende Prieto
,
M. Alvarez
,
O. Alves
,
A. Anand
,
F. Andrade-Oliveira
,
E. Armengaud
,
J. Asorey
,
S. Avila
,
A. Aviles
,
S. Bailey
,
A. Balaguera-Antolínez
,
O. Ballester
,
C. Baltay
,
A. Bault
,
J. Bautista
,
J. Behera
,
S. F. Beltran
,
S. BenZvi
,
L. Beraldo e Silva
,
J. R. Bermejo-Climent
,
A. Berti
,
R. Besuner
,
F. Beutler
,
D. Bianchi
,
C. Blake
,
R. Blum
,
A. S. Bolton
,
S. Brieden
,
A. Brodzeller
,
D. Brooks
,
Z. Brown
,
E. Buckley-Geer
,
E. Burtin
,
L. Cabayol-Garcia
,
Z. Cai
,
R. Canning
,
L. Cardiel-Sas
,
A. Carnero Rosell
,
F. J. Castander
,
J.L. Cervantes-Cota
,
S. Chabanier
,
E. Chaussidon
,
J. Chaves-Montero
,
S. Chen
,
C. Chuang
,
T. Claybaugh
,
S. Cole
,
A. P. Cooper
,
A. Cuceu
,
T. M. Davis
,
K. Dawson
,
R. de Belsunce
,
et al.
(202 additional authors not shown)
http://arxiv.org/abs/2306.06307
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 Galactic Chemical Evolution of phosphorus observed with IGRINS. (arXiv:2210.04940v1 [astro-ph.SR])
Volume 17, Issue 40 - article #10
G. Nandakumar
(1),
N. Ryde
(1),
M. Montelius
(2),
B. Thorsbro
(3),
H. Jönsson
(4),
G. Mace
(5)
(1)
Lund Observatory
,
Department of Astronomy
,
Theoretical Physics
,
Lund University
,
Box 43
,
SE-221 00 Lund
,
Sweden
,
(2)
Kapteyn Astronomical Institute
,
University of Groningen
,
Landleven 12
,
NL-9747 AD Groningen
,
the Netherlands
,
(3)
Department of Astronomy
,
School of Science
,
The University of Tokyo
,
7-3-1 Hongo
,
Bunkyo-ku
,
Tokyo 113-0033
,
Japan
,
(4)
Materials Science
,
Applied Mathematics
,
Malmö
,
University
,
SE-205 06 Malmö
,
Sweden
,
(5)
Department of Astronomy
,
McDonald Observatory
,
The University of Texas
,
Austin
,
TX 78712
,
USA
http://arxiv.org/abs/2210.04940
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
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
Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars. (arXiv:2010.13620v1 [astro-ph.SR])
Volume 15, Issue 44 - article #6
D. Karinkuzhi
(1,2,3),
S. Van Eck
(2),
S. Goriely
(2),
L. Siess
(2),
A. Jorissen
(2),
T. Merle
(2),
A. Escorza
(2,4),
T. Masseron
(5,6)
((1). Department of Physics, Indian Institute of Science, Bangalore, India.560012,
(2). Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium,
(3). Department of Physics, Jnana Bharathi Campus, Bangalore University, Bangalore, India. 560056,
(4). Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium,
(5). Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain,
(6). Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain)
http://arxiv.org/abs/2010.13620
Preliminary Target Selection for the DESI Milky Way Survey (MWS). (arXiv:2010.11284v1 [astro-ph.GA])
Volume 15, Issue 43 - article #4
Carlos Allende Prieto
(1, 2),
Andrew P. Cooper
(3),
Arjun Dey
(4),
Boris T. Gänsicke
(5),
Sergey E. Koposov
(6, 7, 8),
Ting Li
(9, 10),
Christopher Manser
(5),
David L. Nidever
(4, 11),
Constance Rockosi
(12, 13),
Mei-Yu Wang
(7, 14),
David S. Aguado
(8),
Robert Blum
(15),
David Brooks
(16),
Daniel J. Eisenstein
(17),
Yutong Duan
(18),
Sarah Eftekharzadeh
(19),
Enrique Gaztañaga
(20, 21),
Robert Kehoe
(22),
Martin Landriau
(23),
Chien-Hsiu Lee
(4),
Michael E. Levi
(23)
Aaron M. Meisner
(4),
Adam D. Myers
(24),
Joan Najita
(4),
Knut Olsen
(25),
Nathalie Palanque-Delabrouille
(26),
Claire Poppett
(23, 27),
Francisco Prada
(28),
David J. Schlegel
(23),
Michael Schubnell
(29),
Gregory Tarlé
,
(29),
Monica Valluri
(30),
Risa H. Wechsler
(31, 32),
Christophe Yèche
(26)
((1) Instituto de Astrofísica de Canarias,
(2) Universidad de La Laguna,
(3) National Tsing Hua University.
(4) NSF's NOIRLab,
(5) Department of Physics, University of Warwick,
(6) Institute for Astronomy, University of Edinburgh,
(7) McWilliams Center for Cosmology, Carnegie Mellon University,
(8) Institute of Astronomy, University of Cambridge,
(9) Observatories of the Carnegie Institution for Science,
(10) Department of Astrophysical Sciences, Princeton University,
(11) Department of Physics, Montana State University,
(12) Department of Astronomy, Astrophysics, University of California Santa Cruz,
(13) University of California Observatories,
(14) Department of Physics, Carnegie Mellon University,
(15) Vera C. Rubin Observatory/NSF's NOIRLab,
(16) Department of Physics, Astronomy, University College London,
(17) Harvard-Smithsonian Center for Astrophysics,
(18) Physics Department, Boston University,
(19) Department of Physics, Astronomy, The University of Utah,
(20) Institute of Space Sciences
(ICE, CSIC),
(21) Institut d' Estudis Espacials de Catalunya
(IEEC),
(22) Department of Physics, Southern Methodist University,
(23) Lawrence Berkeley National Laboratory,
(24) University of Wyoming,
(25) Community Science, Data Center/NSF's NOIRLab,
(26) IRFU, CEA, Université Paris-Saclay,
(28) Instituto de Astrofisica de Andalucía,
(29) Department of Physics, University of Michigan,
(30) Department of Astronomy, University of Michigan,
(31) Kavli Institute for Particle Astrophysics, Cosmology, Department of Physics,
(32) SLAC National Accelerator Laboratory)
http://arxiv.org/abs/2010.11284
The Dark Energy Spectroscopic Instrument (DESI). (arXiv:1907.10688v1 [astro-ph.IM])
Volume 14, Issue 30 - article #5
Michael E. Levi
(LBNL),
Lori E. Allen
(NOAO),
Anand Raichoor
(EPFL, Switzerland),
Charles Baltay
(Yale University),
Segev BenZvi
(University of Rochester),
Florian Beutler
(University of Portsmouth, UK),
Adam Bolton
(NOAO),
Francisco J. Castander
(IEEC, Spain),
Chia-Hsun Chuang
(KIPAC),
Andrew Cooper
(National Tsing Hua University, Taiwan),
Jean-Gabriel Cuby
(Aix-Marseille University, France),
Arjun Dey
(NOAO),
Daniel Eisenstein
(Harvard University),
Xiaohui Fan
(University of Arizona),
Brenna Flaugher
(FNAL),
Carlos Frenk
(Durham University, UK),
Alma X. Gonzalez-Morales
(Universidad de Guanajuato, Mexico),
Or Graur
(CfA),
Julien Guy
(LBNL),
Salman Habib
(ANL),
Klaus Honscheid
(Ohio State University),
Stephanie Juneau
(NOAO),
Jean-Paul Kneib
(EPFL, Switzerland),
Ofer Lahav
(UCL, UK),
Dustin Lang
(Perimter Institute, Canada),
et al.
(20 additional authors not shown)
http://arxiv.org/abs/1907.10688
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
Planck 2018 results. VI. Cosmological parameters. (arXiv:1807.06209v1 [astro-ph.CO])
Volume 13, Issue 29 - article #8
Planck Collaboration: N. Aghanim
,
Y. Akrami
,
M. Ashdown
,
J. Aumont
,
C. Baccigalupi
,
M. Ballardini
,
A. J. Banday
,
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http://arxiv.org/abs/1807.06209
When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic. (arXiv:1807.06332v1 [astro-ph.SR])
Volume 13, Issue 29 - article #16
D. Karinkuzhi
(1),
S. Van Eck
(1),
A. Jorissen
(1),
S. Goriely
(1),
L. Siess
(1),
T. Merle
(1),
A. Escorza
(1, 2),
M. Van der Swaelmen
(1),
H.M.J. Boffin
(3),
T. Masseron
(4,5),
S. Shetye
(1,2),
B. Plez
(6)
((1). Institute of Astronomy, Astrophysics, University of Brussels, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium.
(2) Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium.
(3) ESO, Karl Schwarzschild Strasse 2, D-85748 Garching bei Munchen, Germany.
(4) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain.
(5) Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain.
(6) Laboratoire Univers et Particules de Montpellier, Universite Montpellier, CNRS, 34095, Montpellier Cedex 05, France.)
http://arxiv.org/abs/1807.06332
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
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L. Casagrande
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J. Bland-Hawthorn
(7,6),
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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S. L. Martell
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K. J. Schlesinger
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S. Sharma
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J. D. Simpson
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D. B. Zucker
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T. Zwitter
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K. Cotar
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A. Dotter
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M. R. Hayden
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E. A. Hyde
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P. R. Kafle
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D. M. Nataf
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T. Nordlander
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W. Reid
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H.-W. Rix
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A. Skuladottir
(1),
D. Stello
(11,18,7,6),
Y.-S. Ting
(19,20,21),
G. Traven
(13),
R. F. G. Wyse
(17)
((1) MPIA Heidelberg,
(2) Uppsala University,
(3) Columbia University New York,
(4) CCA New York,
(5) RSAA/MSO Canberra,
(6) ASTRO-3D Australia,
(7) SIfA Sydney,
(8) Monash University,
(9) AAO North Ryde,
(10) INAF Padova,
(11) UNSW Sydney,
(12) Macquarie University Sydney,
(13) University of Ljubljana,
(14) Harvard/CfA Cambridge,
(15) Western Sydney University,
(16) University of Western Australia,
(17) Johns Hopkins University Baltimore,
(18) Aarhus University,
(19) IAS Princeton,
(20) Princeton University,
(21) Carnegie Observatories Pasadena)
http://arxiv.org/abs/1804.05869
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
Volume 13, Issue 16 - article #12
S. Buder
(1,2),
M. Asplund
(3,4),
L. Duong
(3),
J. Kos
(5),
K. Lind
(1,6),
M. K. Ness
(7,8),
S. Sharma
(5,4),
J. Bland-Hawthorn
(5,4),
A. R. Casey
(9),
G. M. De Silva
(10,5),
V. D'Orazi
(11),
K. C. Freeman
(3),
G. F. Lewis
(5),
J. Lin
(3,4),
S. L. Martell
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K. J. Schlesinger
(3),
J. D. Simpson
(10),
D. B. Zucker
(13,10),
T. Zwitter
(14),
A. M. Amarsi
(1),
B. Anguiano
(15),
D. Carollo
(16),
K. Cotar
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P. L. Cottrell
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G. Da Costa
(3),
X. D. Gao
(1),
M. R. Hayden
(5,4),
J. Horner
(18),
M. J. Ireland
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P. R. Kafle
(19),
U. Munari
(20),
D. M. Nataf
(21),
T. Nordlander
(3,4),
Dennis Stello
(12,22,4),
Y.-S. Ting
(23,24,25),
G. Traven
(14),
F. Watson
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R. A. Wittenmyer
(18),
R. F. G. Wyse
(21),
D. Yong
(3),
J. C. Zinn
(27),
M. Zerjal
(3)
((1) MPIA Heidelberg,
(2) IMPRS HD,
(3) RSAA/MSO Canberra,
(4) ASTRO-3D Australia,
(5) SIfA Sydney,
(6) Uppsala University,
(7) Columbia University New York,
(8) CCA New York
(9) Monash University,
(10) AAO North Ryde,
(11) INAF Padova,
(12) UNSW Sydney,
(13) Macquarie University Sydney,
(14) University of Ljubljana,
(15) University of Virginia,
(16) INAF Turin,
(17) University of Canterbury,
(18) University of Southern Queensland,
(19) University of Western Australia,
(20) INAF Padova,
(21) Johns Hopkins University Baltimore,
(22) Aarhus University,
(23) IAS Princeton,
(24) Princeton University,
(25) Carnegie Observatories Pasadena,
(26) Western Sydney University,
(27) The Ohio State University)
http://arxiv.org/abs/1804.06041
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
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
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
Population III Stars in I Zw 18
Volume 10, Issue 15 - article #6
Sally Heap
(NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA),
Jean-Claude Bouret
(Aix Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, UMR 7326, 13388, Marseille, France),
Ivan Hubeny
(University of Arizona, USA)
arXiv.org - Astrophysics - Volume: 2015, Issue: 17 Apr
arXiv:1504.02742
[
pdf
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Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)
Volume 10, Issue 7 - article #13
The origin of lithium is key to understanding the enrichment history of the Universe
,
now the classical nova V339 Del
(Nova Delphini 2013)
reveals that nova explosions could have been contributing to the recent rapid increase of the amount of lithium in the Universe.
Nature - Volume: 518, Issue: 7539
276-450
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
(10),
Rachael L. Beaton
(12,13),
Timothy C. Beers
(14),
Chad F. Bender
(15,16)
Andreas A. Berlind
(17),
Florian Beutler
(11),
Vaishali Bhardwaj
(6,11),
Jonathan C. Bird
(17),
Dmitry Bizyaev
(18,19),
Cullen H. Blake
(20),
Michael R. Blanton
(21),
Michael Blomqvist
(22),
John J. Bochanski
(6,23),
Adam S. Bolton
(24),
Jo Bovy
(25,26),
A. Shelden Bradley
(18),
W. N. Brandt
(15,27),
D. E. Brauer
(5),
J. Brinkmann
(18),
Peter J. Brown
(28),
Joel R. Brownstein
(24),
Angela Burden
(29),
Etienne Burtin
(9),
Nicolás G. Busca
(30,31,10),
Zheng Cai
(32),
Diego Capozzi
(29),
Aurelio Carnero Rosell
(30,31),
et al.
(238 additional authors not shown)
arXiv.org - Astrophysics - Volume: 2015, Issue: 9 Jan
arXiv:1501.00963
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The exclusion of a significant range of ages in a massive star cluster
Volume 9, Issue 25 - article #53
Hubble Space Telescope observations of the stellar cluster NGC 1651
,
which is approximately two billion years old
,
show that the colour–brightness distribution of stars old enough to have left the main sequence can be explained only by a single-age population
,
despite having a feature usually interpreted to indicate an age spread of more than 300 million years.
Nature - Volume: 516, Issue: 7531
290-444
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
The Gaia-ESO Survey: Kinematic structure in the Gamma Velorum cluster
Volume 9, Issue 16 - article #22
R. D. Jeffries
,
R. J. Jackson
,
M. Cottaar
,
S. E. Koposov
,
A. C. Lanzafame
,
M. R. Meyer
,
L. Prisinzano
,
S. Randich
,
G. G. Sacco
,
E. Brugaletta
,
et al.
(20 more)
M. Caramazza
,
F. Damiani
,
E. Franciosini
,
A. Frasca
,
G. Gilmore
,
S. Feltzing
,
G. Micela
,
E. Alfaro
,
T. Bensby
,
E. Pancino
,
A. Recio-Blanco
,
P. de Laverny
,
J. Lewis
,
L. Magrini
,
L. Morbidelli
,
M. T. Costado
,
P. Jofré
,
A. Klutsch
,
K. Lind
and
E. Maiorca
Astronomy and Astrophysics - Volume: 563, Issue: March 2014
http://dx.doi.org/10.1051/0004-6361/201323288
Abstract
Full HTML
PDF (3.213 MB)
References
Tables at CDS
NASA ADS Abstract Service
The remnant of a merger between two dwarf galaxies in Andromeda II
Volume 9, Issue 12 - article #18
At the lowest galactic mass scales
,
evidence of a merger between two galaxies is provided by the kinematic detection of a stellar stream —
,
indicative of an accretion event —
,
in the dwarf spheroidal galaxy Andromeda II
,
one of the satellite galaxies of Andromeda.
Nature - Volume: 507, Issue: 7492
276-394
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
Popular science: Get the word out
Volume 8, Issue 49 - article #17
Writing science books for the public is rewarding
,
but can take a lot of time —
,
and
financial gain is uncertain.
Nature - Volume: 504, Issue: 7478
10-182
The AGORA High-Resolution Galaxy Simulations Comparison Project
Volume 8, Issue 33 - article #11
Ji-hoon Kim
(1),
Tom Abel
(2),
Oscar Agertz
(3, 4),
Greg L. Bryan
(5),
Daniel Ceverino
(6),
Charlotte Christensen
(7),
Charlie Conroy
(1),
Avishai Dekel
(8),
Nickolay Y. Gnedin
(3, 9, 10),
Nathan J. Goldbaum
(1),
Javiera Guedes
(11),
Oliver Hahn
(11),
Alexander Hobbs
(11),
Philip F. Hopkins
(12, 13),
Cameron B. Hummels
(7),
Francesca Iannuzzi
(14),
Dusan Keres
(15),
Anatoly Klypin
(16),
Andrey V. Kravtsov
(3, 10),
Mark R. Krumholz
(1),
Michael Kuhlen
(1, 13),
Samuel N. Leitner
(17),
Piero Madau
(1),
Lucio Mayer
(18),
Christopher E. Moody
(1),
Kentaro Nagamine
(19, 20),
Michael L. Norman
(15),
Jose Oñorbe
(21),
Brian W. O'Shea
(22),
Annalisa Pillepich
(1),
Joel R. Primack
(1),
Thomas Quinn
(23),
Justin I. Read
(4),
Brant E. Robertson
(7),
Miguel Rocha
(21),
Douglas H. Rudd
(10, 24),
et al.
(11 additional authors not shown)
arXiv.org - Astrophysics - Volume: 2013, Issue: 16 Aug
arXiv:1308.2669
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other
]
Reviews in Modern Astronomy 25
Volume 8, Issue 28 - article #17
Article first published online: 1 JUL 2013 | DOI: 10.1002/asna.201390009
Astronomische Nachrichten - Volume: 334, Issue: 6
Abstract
PDF(4217K)
References
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Lab life: Don't bristle at blunders
Volume 8, Issue 20 - article #18
Embrace mistakes
,
urges Mario Livio —
,
they are portals to scientific progress.
Nature - Volume: 497, Issue: 7449
290-402
The secrets of my prizewinning research
Volume 7, Issue 42 - article #13
Serge Haroche
,
co-winner of the 2012 Nobel Prize in Physics
,
warns against the growing trend towards short-termism in science funding.
Nature - Volume: 490, Issue: 7420
309-440
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
Transit of Venus: Last chance to see
Volume 7, Issue 20 - article #24
The June 2012 transit of Venus across the Sun offers an opportunity to check our methods for spotting distant planets crossing far-away stars
,
says Jay M. Pasachoff.
Nature - Volume: 485, Issue: 7398
279-410
One or more bound planets per Milky Way star from microlensing observations
Volume 7, Issue 11 - article #15
A statistical analysis of microlensing data from 2002–07 reveals that stars in the Milky Way are orbited by planets as a rule
,
rather than an exception.
Nature - Volume: 481, Issue: 7380
113-230
Tough choices
Volume 7, Issue 7 - article #27
Scientists must find ways to make more efficient use of funds —
,
or politicians may do it for them.
Nature - Volume: 482, Issue: 7385
Searches for Dark Matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
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arXiv.org - Astrophysics - Volume: 2011, Issue: 4 Mar
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Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory
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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
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G. Matijeviv{c)
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((1) University of Ljubljana
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(2) Center of excellence SPACE-SI
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Ljubljana
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Slovenia
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University of Groningen
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Groningen
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The Netherlands
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Peking University
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arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
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LSST Science Book, Version 2.0
Volume 4, Issue 49 - article #13
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J. Roger P. Angel
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arXiv.org - Astrophysics - Volume: 2009, Issue: 4 Dec
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A double stellar generation in the globular cluster NGC 6656 (M 22) - Two stellar groups with different iron and
s
-process element abundances
Volume 4, Issue 42 - article #27
A. F. Marino
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L. R. Bedin
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Astronomy and Astrophysics - Volume: 505, Issue: 3
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|
PDF file (1.034 MB)
|
PS file (373.1 KB)
The radial distribution of the two stellar populations in NGC 1851
Volume 4, Issue 36 - article #25
A. P. Milone
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Astronomy and Astrophysics - Volume: 503, Issue: 3
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Multiple stellar populations in Magellanic Cloud clusters - I. An ordinary feature for intermediate age globulars in the LMC?
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A. P. Milone
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Astronomy and Astrophysics - Volume: 497, Issue: 3
Abstract
|
PDF file (13.69 MB)
|
PS file (5.911 MB)
Nobel Lecture: From the Big Bang to the Nobel Prize and beyond
Volume 3, Issue 41 - article #27
John C. Mather<BR>
,
Published 2 November 2007
(<i>18 pages</i>)<BR>
pp. 1331-1348 Abstract Full Text: [ PDF
(1445 kB)
GZipped PS ] Free to Read Free to Read <strong>Nobel Lecture: Cosmic microwave background radiation anisotropies: Their discovery
and
utilization</strong><br>
,
George F. Smoot
Reviews of Modern Physics - Volume: 79, Issue: 4
Abstract
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GZipped PS
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Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey
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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
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The Sixth Data Release of the Sloan Digital Sky Survey
Volume 3, Issue 13 - article #44
Jennifer K. Adelman‐McCarthy
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The Astrophysical Journal Supplement - Volume: 175, Issue: 2
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Low Metallicity Indicates That the Hypervelocity Star HE 0437−5439 was Ejected from the Large Magellanic Cloud
Volume 3, Issue 9 - article #6
Alceste Z. Bonanos
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Mercedes López‐Morales
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Ian Hunter
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The Astrophysical Journal Letters - Volume: 675, Issue: 2
Abstract
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The Elongated Structure of the Hercules Dwarf Spheroidal Galaxy from Deep Large Binocular Telescope Imaging
Volume 3, Issue 5 - article #32
Matthew G. Coleman
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Jelte T. A. de Jong
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Hans‐Walter Rix
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The Astrophysical Journal Letters - Volume: 668, Issue: 1
Abstract
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r
‐Process Nucleosynthesis in Shocked Surface Layers of O‐Ne‐Mg Cores
Volume 3, Issue 4 - article #1
H. Ning
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Y.‐Z. Qian
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The Astrophysical Journal Letters - Volume: 667, Issue: 2
Abstract
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The ACS Survey of Galactic Globular Clusters: M54 and Young Populations in the Sagittarius Dwarf Spheroidal Galaxy
Volume 3, Issue 4 - article #14
Michael H. Siegel
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Giampaolo Piotto
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The Astrophysical Journal Letters - Volume: 667, Issue: 1
Abstract
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The ACS Survey of Galactic Globular Clusters. III. The Double Subgiant Branch of NGC 1851
Volume 3, Issue 3 - article #30
A. P. Milone
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The Astrophysical Journal - Volume: 673, Issue: 1
Abstract
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Lithium Production on a Low‐Mass Secondary in a Black Hole Soft X‐Ray Transient
Volume 3, Issue 2 - article #7
Shin‐ichiro Fujimoto
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Ryuichi Matsuba
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The Astrophysical Journal Letters - Volume: 673, Issue: 1
Abstract
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Evidence of a Merger of Binary White Dwarfs: The Case of GD 362
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E. García‐Berro
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The Astrophysical Journal Letters - Volume: 661, Issue: 2
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Andromeda X, a New Dwarf Spheroidal Satellite of M31: Photometry
Volume 2, Issue 52 - article #7
Daniel B. Zucker
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The Astrophysical Journal Letters - Volume: 659, Issue: 1
Abstract
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A Deep Large Binocular Telescope View of the Canes Venatici I Dwarf Galaxy
Volume 2, Issue 51 - article #3
Nicolas F. Martin
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Jelte T. A. De Jong
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Abstract
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Statistical Properties of the
GALEX
‐SDSS Matched Source Catalogs, and Classification of the UV Sources
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Luciana Bianchi
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The Astrophysical Journal Supplement - Volume: 173, Issue: 2
Abstract
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UV Star Formation Rates in the Local Universe
Volume 2, Issue 51 - article #43
Samir Salim
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R. Michael Rich
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Stéphane Charlot
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,
Alex S. Szalay
,
Barry Y. Welsh
,
and
Sukyoung K. Yi
The Astrophysical Journal Supplement - Volume: 173, Issue: 2
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