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Results 1 - 35 of 35
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
Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program. (arXiv:2108.13045v1 [astro-ph.IM])
Volume 16, Issue 36 - article #5
Hiroaki Aihara
,
Yusra AlSayyad
,
Makoto Ando
,
Robert Armstrong
,
James Bosch
,
Eiichi Egami
,
Hisanori Furusawa
,
Junko Furusawa
,
Sumiko Harasawa
,
Yuichi Harikane
,
Bau-Ching Hsieh
,
Hiroyuki Ikeda
,
Kei Ito
,
Ikuru Iwata
,
Tadayuki Kodama
,
Michitaro Koike
,
Mitsuru Kokubo
,
Yutaka Komiyama
,
Xiangchong Li
,
Yongming Liang
,
Yen-Ting Lin
,
Robert H. Lupton
,
Nate B Lust
,
Lauren A. MacArthur
,
Ken Mawatari
,
Sogo Mineo
,
Hironao Miyatake
,
Satoshi Miyazaki
,
Surhud More
,
Takahiro Morishima
,
Hitoshi Murayama
,
Kimihiko Nakajima
,
Fumiaki Nakata
,
Atsushi J. Nishizawa
,
Masamune Oguri
,
Nobuhiro Okabe
,
Yuki Okura
,
Yoshiaki Ono
,
Ken Osato
,
Masami Ouchi
,
Yen-Chen Pan
,
Andrés A. Plazas Malagón
,
Paul A. Price
,
Sophie L Reed
,
Eli S. Rykoff
,
Takatoshi Shibuya
,
Mirko Simunovic
,
Michael A. Strauss
,
Kanako Sugimori
,
et al.
(18 additional authors not shown)
http://arxiv.org/abs/2108.13045
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
EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with ?1.0 (Fe/O)? and 0.02 (O/H)? : Possible Traces of Super Massive (>300M?) Stars in Early Galaxies
Volume 15, Issue 24 - article #7
Takashi Kojima
(1,2),
Masami Ouchi
(3,1,4),
Michael Rauch
(5),
Yoshiaki Ono
(1),
Kimihiko Nakajima
(3),
Yuki Isobe
(1,2),
Seiji Fujimoto
(6,7),
Yuichi Harikane
(3,8,1),
Takuya Hashimoto
(9),
Masao Hayashi
(3),
Yutaka Komiyama
(3),
Haruka Kusakabe
(10),
Ji Hoon Kim
(11,12),
Chien-Hsiu Lee
(13),
Shiro Mukae
(1,2),
Tohru Nagao
(14),
Masato Onodera
(11,15),
Takatoshi Shibuya
(16),
Yuma Sugahara
(17),
Masayuki Umemura
(18),
Kiyoto Yabe
(4)
((1) ICRR,
(2) Univ. of Tokyo,
(3) NAOJ,
(4) Kavli IPMU,
(5) Carnegie Observatory,
(6) DAWN fellow,
(7) Univ. of Copenhagen,
(8) UCL,
(9) TCHoU,
(10) Observatoire de Geneve,
(11) Subaru Telescope,
(12) Metaspace,
(13) NOAO,
(14) Ehime Univ.,
(15) SOKENDAI,
(16) Kitami Institute of Tech.,
(17) Waseda Univ.,
(18) Univ. of Tsukuba)
http://arxiv.org/abs/2006.03831
Hunting for open clusters in textit{Gaia} DR2: $582$ new OCs in the Galactic disc. (arXiv:2001.07122v1 [astro-ph.GA])
Volume 15, Issue 4 - article #5
A. Castro-Ginard
(1),
C. Jordi
(1),
X. Luri
(1),
J. Álvarez Cid-Fuentes
(2),
L. Casamiquela
(3),
F. Anders
(1),
T. Cantat-Gaudin
(1),
M. Monguió
,
(1),
L. Balaguer-Núñez
(1),
S. Solà
,
(2),
R.M. Badia
(2)
((1) Dept. Física Quàntica i Astrofísica, Institut de Ciències del Cosmos
(ICCUB), Universitat de Barcelona
(IEEC-UB), Martí i Franquès 1, E08028 Barcelona, Spain,
(2) Barcelona Supercomputing Center
(BSC),
(3) Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France)
http://arxiv.org/abs/2001.07122
Identification of strontium in the merger of two neutron stars. (arXiv:1910.10510v1 [astro-ph.HE])
Volume 14, Issue 43 - article #4
Darach Watson
(1, 2),
Camilla J. Hansen
(3),
Jonatan Selsing
(1, 2),
Andreas Koch
(4),
Daniele B. Malesani
(1, 2, 5),
Anja C. Andersen
(1),
Johan P. U. Fynbo
(1, 2),
Almudena Arcones
(6, 7),
Andreas Bauswein
(7, 8),
Stefano Covino
(9),
Aniello Grado
(10),
Kasper E. Heintz
(1, 2, 11),
Leslie Hunt
(12),
Chryssa Kouveliotou
(13, 14),
Giorgos Leloudas
(1, 5),
Andrew Levan
(15, 16),
Paolo Mazzali
(17, 18),
Elena Pian
(19)
((1) Niels Bohr Institute, University of Copenhagen,
(2) Cosmic Dawn Center
(DAWN),
(3) Max-Planck-Institut für Astronomie, Heidelberg,
(4) Zentrum für Astronomie der Universität Heidelberg,
(5) DTU Space, Technical University of Denmark,
(6) Institut für Kernphysik, Technische Universität Darmstadt,
(7) GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt,
(8) Heidelberger Institut für Theoretische Studien, Heidelberg,
(9) INAF / Brera Astronomical Observatory, Merate,
(10) INAF-OACN, Naples,
(11) Centre for Astrophysics, Cosmology, University of Iceland,
(12) INAF - Osservatorio Astrofisico di Arcetri, Firenze,
(13) Physics Department, the George Washington University,
(14) Astronomy, Physics, Statistics Institute of Sciences
(APSIS), Washington, DC,
(15) Department of Astrophysics/IMAPP, Radboud University Nijmegen,
(16) Department of Physics, University of Warwick,
(17) Astrophysics Research Institute, Liverpool John Moores University,
(18) Max-Planck Institute for Astrophysics, Garching,
(19) INAF, Astrophysics, Space Science Observatory, Bologna)
http://arxiv.org/abs/1910.10510
Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri. (arXiv:1906.08550v1 [astro-ph.SR])
Volume 14, Issue 25 - article #2
D. Magurno
(1, 2, 3),
C. Sneden
(4),
G. Bono
(1, 2),
V. F. Braga
(5, 6),
M. Mateo
(7),
S. E. Persson
(8),
G. Preston
(8),
F. Thevenin
(9),
R. da Silva
(10),
M. Dall'Ora
(11),
M. Fabrizio
(2, 10),
I. Ferraro
(2),
G. Fiorentino
(12),
G. Iannicola
(2),
L. Inno
(13),
M. Marengo
(14),
S. Marinoni
(10),
P. M. Marrese
(10),
C. E. Martinez-Vazquez
(15),
N. Matsunaga
(16),
M. Monelli
(17),
J. R. Neeley
(18),
M. Nonino
(19),
A. R. Walker
(15)
((1) University of Roma Tor Vergata - Department of Physics - Roma - Italy,
(2) INAF Osservatorio Astronomico di Roma - Monte Porzio Catone RM - Italy,
(3) University of Bologna - Department of Physics, Astronomy - Bologna - Italy,
(4) Department of Astronomy, McDonald Observatory - The University of Texas - Austin - TX - USA,
(5) Instituto Milenio de Astrofisica - Santiago - Chile,
(6) Departamento de Fisica - Facultad de Ciencias Exactas - Universidad Andres Bello - Las Condes - Santiago - Chile,
(7) Department of Astronomy - University of Michigan - Ann Arbor - MI - USA,
(8) Observatories of the Carnegie Institution for Science - Pasadena - CA 91101 - USA,
(9) Universite de La Cote d'Azur - OCA - Laboratoire Lagrange CNRS - Nice Cedex - France,
(10) SSDC - via del Politecnico snc - I-00133 Roma - Italy,
(11) INAF Osservatorio Astronomico di Capodimonte - Salita Moiariello 16 - Napoli - Italy,
(12) INAF Osservatorio Astronomico di Bologna - Via Ranzani 1 - Bologna - Italy,
(13) Max Planck Institute fur Astronomie - Konigstuhl - Heidelberg - Germany,
(14) Department of Physics, Astronomy - Iowa State University - Zaffarano - Ames - IA - USA,
(15) Cerro Tololo Inter-American Observatory - National Optical Astronomy Observatory - Casilla - La Serena - Chile,
(16) Department of Astronomy - The University of Tokyo - Hongo - Bunkyo-ku - Tokyo - Japan,
(17) IAC - Instituto de Astrofsica de Canarias - Calle Via Lactea - La Laguna - Tenerife - Espana,
(18) Department of Physics - Florida Atlantic University - Boca Raton - FL - USA,
(19) INAF Osservatorio Astronomico di Trieste - Trieste - Italy)
http://arxiv.org/abs/1906.08550
The Fornax 3D project: Thick disks in a cluster environment. (arXiv:1904.01260v1 [astro-ph.GA])
Volume 14, Issue 14 - article #11
F. Pinna
(1, 2),
J. Falcón-Barroso
(1, 2),
M. Martig
(3),
L. Coccato
(4),
E. M. Corsini
(5, 6),
P.T. de Zeeuw
(7, 8),
D.A. Gadotti
(4),
E. Iodice
(9),
R. Leaman
(10),
M. Lyubenova
(4),
I. Martín-Navarro
(11, 10),
L. Morelli
(12, 6),
M. Sarzi
(13),
G. van de Ven
(14, 4),
S. Viaene
(15, 16),
R.M. McDermid
(17, 18)
((1) Instituto de Astrofísica de Canarias,
(2) Depto. Astrofísica, Universidad de La Laguna,
(3) Astrophysics Research Institute, Liverpool John Moores University,
(4) European Southern Observatory,
(5) Dipartimento di Fisica e Astronomia 'G. Galilei', Università di Padova,
(6) INAF-Osservatorio Astronomico di Padova,
(7) Sterrewacht Leiden, Leiden University,
(8) Max-Planck-Institut fuer extraterrestrische Physik,
(9) INAF-Osservatorio Astronomico di Capodimonte,
(10) Max-Planck Institut fuer Astronomie,
(11) University of California Observatories,
(12) Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama,
(13) Armagh Observatory, Planetarium,
(14) Department of Astrophysics, University of Vienna,
(15) Sterrenkundig Observatorium, Universiteit Gent,
(16) Centre for Astrophysics Research, University of Hertfordshire,
(17) Department of Physics, Astronomy, Macquarie University,
(18) Australian Astronomical Observatory)
http://arxiv.org/abs/1904.01260
The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library. (arXiv:1812.02759v1 [astro-ph.IM])
Volume 13, Issue 50 - article #4
D. S. Aguado
,
Romina Ahumada
,
Andres Almeida
,
Scott F. Anderson
,
Brett H. Andrews
,
Borja Anguiano
,
Erik Aquino Ortiz
,
Alfonso Aragon-Salamanca
,
Maria Argudo-Fernandez
,
Marie Aubert
,
Vladimir Avila-Reese
,
Carles Badenes
,
Sandro Barboza Rembold
,
Kat Barger
,
Jorge Barrera-Ballesteros
,
Dominic Bates
,
Julian Bautista
,
Rachael L. Beaton
,
Timothy C. Beers
,
Francesco Belfiore
,
Mariangela Bernardi
,
Matthew Bershady
,
Florian Beutler
,
Jonathan Bird
,
Dmitry Bizyaev
,
Guillermo A. Blanc
,
Michael R. Blanton
,
Michael Blomqvist
,
Adam S. Bolton
,
Mederic Boquien
,
Jura Borissova
,
Jo Bovy
,
William Nielsen Brandt
,
Jonathan Brinkmann
,
Joel R. Brownstein
,
Kevin Bundy
,
Adam Burgasser
,
Nell Byler
,
Mariana Cano Diaz
,
Michele Cappellari
,
Ricardo Carrera
,
Bernardo Cervantes Sodi
,
Yanping Chen
,
Brian Cherinka
,
Peter Doohyun Choi
,
et al.
(189 additional authors not shown)
http://arxiv.org/abs/1812.02759
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
(11),
K. J. Schlesinger
(5),
S. Sharma
(7,6),
J. D. Simpson
(9),
D. B. Zucker
(12,9),
T. Zwitter
(13),
K. Cotar
(13),
A. Dotter
(14),
M. R. Hayden
(7,6),
E. A. Hyde
(15),
P. R. Kafle
(16),
D. M. Nataf
(17),
T. Nordlander
(5,6),
W. Reid
(15,12),
H.-W. Rix
(1),
A. Skuladottir
(1),
D. Stello
(11,18,7,6),
Y.-S. Ting
(19,20,21),
G. Traven
(13),
R. F. G. Wyse
(17)
((1) MPIA Heidelberg,
(2) Uppsala University,
(3) Columbia University New York,
(4) CCA New York,
(5) RSAA/MSO Canberra,
(6) ASTRO-3D Australia,
(7) SIfA Sydney,
(8) Monash University,
(9) AAO North Ryde,
(10) INAF Padova,
(11) UNSW Sydney,
(12) Macquarie University Sydney,
(13) University of Ljubljana,
(14) Harvard/CfA Cambridge,
(15) Western Sydney University,
(16) University of Western Australia,
(17) Johns Hopkins University Baltimore,
(18) Aarhus University,
(19) IAS Princeton,
(20) Princeton University,
(21) Carnegie Observatories Pasadena)
http://arxiv.org/abs/1804.05869
The GALAH Survey: Second Data Release. (arXiv:1804.06041v1 [astro-ph.SR])
Volume 13, Issue 16 - article #12
S. Buder
(1,2),
M. Asplund
(3,4),
L. Duong
(3),
J. Kos
(5),
K. Lind
(1,6),
M. K. Ness
(7,8),
S. Sharma
(5,4),
J. Bland-Hawthorn
(5,4),
A. R. Casey
(9),
G. M. De Silva
(10,5),
V. D'Orazi
(11),
K. C. Freeman
(3),
G. F. Lewis
(5),
J. Lin
(3,4),
S. L. Martell
(12),
K. J. Schlesinger
(3),
J. D. Simpson
(10),
D. B. Zucker
(13,10),
T. Zwitter
(14),
A. M. Amarsi
(1),
B. Anguiano
(15),
D. Carollo
(16),
K. Cotar
(14),
P. L. Cottrell
(9,17),
G. Da Costa
(3),
X. D. Gao
(1),
M. R. Hayden
(5,4),
J. Horner
(18),
M. J. Ireland
(3),
P. R. Kafle
(19),
U. Munari
(20),
D. M. Nataf
(21),
T. Nordlander
(3,4),
Dennis Stello
(12,22,4),
Y.-S. Ting
(23,24,25),
G. Traven
(14),
F. Watson
(10,26),
R. A. Wittenmyer
(18),
R. F. G. Wyse
(21),
D. Yong
(3),
J. C. Zinn
(27),
M. Zerjal
(3)
((1) MPIA Heidelberg,
(2) IMPRS HD,
(3) RSAA/MSO Canberra,
(4) ASTRO-3D Australia,
(5) SIfA Sydney,
(6) Uppsala University,
(7) Columbia University New York,
(8) CCA New York
(9) Monash University,
(10) AAO North Ryde,
(11) INAF Padova,
(12) UNSW Sydney,
(13) Macquarie University Sydney,
(14) University of Ljubljana,
(15) University of Virginia,
(16) INAF Turin,
(17) University of Canterbury,
(18) University of Southern Queensland,
(19) University of Western Australia,
(20) INAF Padova,
(21) Johns Hopkins University Baltimore,
(22) Aarhus University,
(23) IAS Princeton,
(24) Princeton University,
(25) Carnegie Observatories Pasadena,
(26) Western Sydney University,
(27) The Ohio State University)
http://arxiv.org/abs/1804.06041
The local rotation curve of the Milky Way based on SEGUE and RAVE data. (arXiv:1802.07658v1 [astro-ph.GA])
Volume 13, Issue 8 - article #12
K. Sysoliatina
(1),
A. Just
(1),
O. Golubov
(2,3,4),
Q.A. Parker
(5,6),
E.K. Grebel
(1),
G. Kordopatis
(17),
T. Zwitter
(15),
J. Bland-Hawthorn
(14),
B.K. Gibson
(8),
A. Kunder
(16),
U. Munari
(7),
J. Navarro
(12),
W. Reid
(10,11),
G. Seabroke
(9),
M.Steinmetz
(18),
F. Watson
(13)
((1) Astronomisches Rechen-Institut, Heidelberg, Germany,
(2) Schools of Physics, Technology, Karazin Kharkiv National University, Kharkiv, Ukraine,
(3) Institute of Astronomy, Karazin Kharkiv National University, Kharkiv, Ukraine,
(4) Department of Aerospace Engineering Sciences, University of Colorado at Boulder, USA,
(5) Department of Physics, the University of Hong Kong, China,
(6) The Laboratory for Space Research, the university of Hong Kong, China,
(7) INAF Astronomical Observatory of Padova, Italy,
(8) E.A. Milne Centre for Astrophysics, University of Hull, UK,
(9) Mullard Space Science Laboratory, University College London, UK,
(10) Department of Physics, Astronomy, Macquarie University, Sydney, Australia,
(11) Western Sydney University, Australia,
(12) Senior CIfAR Fellow, University of Victoria, Canada,
(13) Australian Astronomical Observatory
(14) Sydney Institute for Astronomy, School of Physics, University of Sydney, Australia,
(15) Faculty of Mathematics, Physics, University of Ljubljana, Slovenia,
(16) Saint Martin's University, Lacey, USA,
(17) Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, France,
(18) Leibniz Institut für Astrophysik Potsdam, Germany)
http://arxiv.org/abs/1802.07658
On the RR Lyrae stars in globulars: V. the complete Near-Infrared (JHKs) census of omega Centauri RR Lyrae variables. (arXiv:1802.03578v1 [astro-ph.SR])
Volume 13, Issue 7 - article #7
V. F. Braga
(1, 2, 3, 4),
P. B. Stetson
(5),
G. Bono
(3, 6),
M. Dall'Ora
(7),
I. Ferraro
(6),
G. Fiorentino
(8),
G. Iannicola
(6),
M. Marconi
(7),
M. Marengo
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A. J. Monson
(10),
J. Neeley
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S. E. Persson
(10),
R. L. Beaton
(10),
R. Buonanno
(3, 11),
A. Calamida
(12),
M. Castellani
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E. Di Carlo
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M. Fabrizio
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W. L. Freedman
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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
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L. M. Freyhammer
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G. Iannicola
(4),
M. Marengo
(8),
J. Neeley
(8),
E. Valenti
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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
Subaru/HDS study of CH stars: elemental abundances for stellar neutron-capture process studies
Volume 10, Issue 40 - article #15
Aruna Goswami
(1),
Wako Aoki
(2),
Drisya Karinkuzhi
(1)
((1) Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India
(2) National Astronomical Observatory, Mitaka, Tokyo, 181-8588 Japan)
arXiv.org - Astrophysics - Volume: 2015, Issue: 30 Oct
arXiv:1510.07814
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TOPoS: II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies
Volume 10, Issue 16 - article #19
P. Bonifacio
(1),
E. Caffau
(1,2),
M. Spite
(2),
M. Limongi
(3,4),
A. Chieffi
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R.S. Klessen
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P. François
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P. Molaro
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H. G. Ludwig
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S. Zaggia
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F. Spite
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B. Plez
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R. Cayrel
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N. Christlieb
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P.C. Clark
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S.C.O. Glover
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F. Hammer
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A. Koch
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L. Monaco
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L. Sbordone
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M. Steffen
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((1) GEPI, Observatoire de Paris,
(2) ZAH-LSW,
(3) INAF - OA Roma,
(4) Kavli IPMU, Univ. Tokyo
(5) INAF - IASFC,
(6) ZAH-ARI,
(7) Kavli, IPAC, Stanford Univ.,
(8) Dep A&A Univ, Calfornia,
(9) UPJV, Univ. Picardie,
(10) INAF - OA Trieste,
(11) INAF- OA Padova,
(12) LUPM, Univ. Montpellier,
(13) School of Physics and Astronomy, Cardiff Univ.
(14) ESO,
(15) DCF - Univ. A. Bello,
(16) MAS,
(17) PUC - Chile,
(18) Leibniz-Institut AIP)
arXiv.org - Astrophysics - Volume: 2015, Issue: 24 Apr
arXiv:1504.05963
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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
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Eric Armengaud
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Éric Aubourg
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Stephen Bailey
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Julian E. Bautista
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Rachael L. Beaton
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Timothy C. Beers
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Chad F. Bender
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Andreas A. Berlind
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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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Decoding the stellar fossils of the dusty Milky Way progenitors
Volume 9, Issue 22 - article #31
Matteo de Bennassuti
(1 and 2),
Raffaella Schneider
(2),
Rosa Valiante
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Stefania Salvadori
(3)
((1) Dipartimento di Fisica, Sapienza, Universita` di Roma, Piazzale Aldo Moro 5, 00185, Roma, Italy,
(2) INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040 Monte Porzio Catone, Italy,
(3) Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands)
arXiv.org - Astrophysics - Volume: 2014, Issue: 26 Sep
arXiv:1409.5798
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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 RAVE investigation on Galactic open clusters - I. Radial velocities and metallicities
Volume 9, Issue 9 - article #8
C. Conrad
,
R.-D. Scholz
,
N. V. Kharchenko
,
A. E. Piskunov
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E. Schilbach
,
S. Röser
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C. Boeche
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G. Kordopatis
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A. Siebert
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M. Williams
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et al.
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U. Munari
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G. MatijeviÄ
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E. K. Grebel
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T. Zwitter
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R. S. de Jong
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M. Steinmetz
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G. Gilmore
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G. Seabroke
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K. Freeman
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J. F. Navarro
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Q. Parker
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W. Reid
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F. Watson
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B. K. Gibson
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O. Bienaymé
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R. Wyse
,
J. Bland-Hawthorn
and
A. Siviero
Astronomy and Astrophysics - Volume: 562, Issue: February 2014
http://dx.doi.org/10.1051/0004-6361/201322070
Abstract
Full HTML
PDF (3.852 MB)
References
Tables at CDS
NASA ADS Abstract Service
The AGORA High-Resolution Galaxy Simulations Comparison Project
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Ji-hoon Kim
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Tom Abel
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Oscar Agertz
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Greg L. Bryan
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Daniel Ceverino
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Charlotte Christensen
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Charlie Conroy
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Avishai Dekel
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Nickolay Y. Gnedin
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Nathan J. Goldbaum
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Javiera Guedes
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Oliver Hahn
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Alexander Hobbs
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Philip F. Hopkins
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Cameron B. Hummels
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Francesca Iannuzzi
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Mark R. Krumholz
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Michael Kuhlen
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Samuel N. Leitner
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Piero Madau
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Lucio Mayer
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Christopher E. Moody
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Kentaro Nagamine
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Michael L. Norman
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Jose Oñorbe
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Brian W. O'Shea
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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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arXiv.org - Astrophysics - Volume: 2013, Issue: 16 Aug
arXiv:1308.2669
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The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment
Volume 8, Issue 31 - article #14
Christopher P. Ahn
,
Rachael Alexandroff
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Carlos Allende Prieto
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Friedrich Anders
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Scott F. Anderson
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Timothy Anderton
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Brett H. Andrews
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Éric Aubourg
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Stephen Bailey
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Fabienne A. Bastien
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Julian E. Bautista
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Timothy C. Beers
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Alessandra Beifiori
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Vaishali Bhardwaj
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Michael R. Blanton
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Michael Blomqvist
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The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey
Volume 7, Issue 31 - article #15
SDSS-III Collaboration: Christopher P. Ahn
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Rachael Alexandroff
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Scott F. Anderson
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Brett H. Andrews
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The signature of the first stars in atomic hydrogen at redshift 20
Volume 7, Issue 27 - article #35
A simulation of the distribution of the first stars at a cosmic age of about 180 million years reveals that the 21-cm atomic hydrogen signature of these stars is an enhanced
(ten millikelvin)
fluctuation signal on scales of a few hundred million light-years.
Nature - Volume: 487, Issue: 7405
5-134
Searches for Dark Matter annihilation signatures in the Segue 1 satellite galaxy with the MAGIC-I telescope
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E. A. Alvarez
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L. A. Antonelli
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P. Antoranz
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M. Asensio
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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. Biland
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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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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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E. De Cea del Pozo
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B. De Lotto
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C. Delgado Mendez
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A. Diago Ortega
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M. Doert
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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
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G. Matijeviv{c)
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M. A. Breddels
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M. C. Smith
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A. Helmi
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U. Munari
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O. Bienaym'{e)
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A. G. A. Brown
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((1) University of Ljubljana
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Faculty of Mathematics
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Physics
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Ljubljana
,
Slovenia}
(2) Center of excellence SPACE-SI
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Ljubljana
,
Slovenia
,
(3) Kapteyn Astronomical Institute
,
University of Groningen
,
Groningen
,
The Netherlands
,
(4) Kavli Institute for Astronomy
,
Astrophysics
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Peking University
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Beijing
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China
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(5) INAF Astronomical Observatory of Padova
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arXiv.org - Astrophysics - Volume: 2010, Issue: 30 Jul
arXiv:1007.4411
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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
Full Text: [
PDF
(4379 kB)
GZipped PS
] Free to Read
Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey
Volume 3, Issue 23 - article #11
D. J. Pinfield
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B. Burningham
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M. Tamura
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S. K. Leggett
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N. Lodieu
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P. W. Lucas
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S. J. Warren
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N. R. Deacon
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M. J. McCaughrean
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E. Moraux
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T. Nakajima
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Y. Pavlenko
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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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Spectropolarimetric Survey of Hydrogen-rich White Dwarf Stars
Volume 2, Issue 1 - article #2
ao5,b18
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A. Kawka
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S. Vennes
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G. D. Schmidt
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D. T. Wickramasinghe
,
and
R. Koch
The Astrophysical Journal - Volume654, Issue 1
ABSTRACT
,
FULL TEXT
,
PDF
(1295 kB),
PS
A Curious New Milky Way Satellite in Ursa Major
Volume 1, Issue 22 - article #3
D.B. Zucker
(1),
V. Belokurov
(1),
N.W. Evans
(1),
M.J. Irwin
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J.T. Kleyna
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M.I. Wilkinson
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M. Fellhauer
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D.M. Bramich
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G. Gilmore
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H.J. Newberg
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B. Yanny
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J.A. Smith
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P.C. Hewett
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H.-W. Rix
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O.Y. Gnedin
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S. Vidrih
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R.F.G. Wyse
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B. Willman
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E.K. Grebel
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D.P. Schneider
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T.C. Beers
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A.Y. Kniazev
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H. Brewington
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J. Brinkmann
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M. Harvanek
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J. Krzesinski
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D. Long
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A. Nitta
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S.A. Snedden
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((1) Cambridge,
(2) Hawaii,
(3) RPI,
(4) FNAL,
(5) LANL,
(6) Austin Peay State University,
(7) MPIA,
(8) OSU,
(9) JHU,
(10) NYU,
(11) Basel,
(12) Penn State University,
(13) Michigan State University,
(14) SAAO,
(15) Apache Point,
(16) Subaru Telescope,
(17) Cracow,
(18) Gemini Observatory)
ArXiv - Astrophysics
astro-ph/0606633 [
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