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Results 1 - 3 of 3
The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees. (arXiv:1902.11265v1 [astro-ph.GA])
Volume 14, Issue 9 - article #7
K. Kuijken
(1),
C. Heymans
(2),
A. Dvornik
(1),
H. Hildebrandt
(3,4),
J.T.A. de Jong
(5),
A.H. Wright
(4),
T. Erben
(4),
M. Bilicki
(1,6),
B. Giblin
(2),
H.-Y. Shan
(4,7),
F. Getman
(8),
A. Grado
(8),
H. Hoekstra
(1),
L. Miller
(9),
N. Napolitano
(10,8),
M. Paolilo
(11),
M. Radovich
(12),
P. Schneider
(4),
W. Sutherland
(13),
M. Tewes
(4),
C. Tortora
(14),
E.A. Valentijn
(5),
G.A. Verdoes Kleijn
(5)
((1) Leiden Observatory,
(2) SUPA, Edinburgh,
(3) Astronomisches Inst., Bochum,
(4) Argelander Inst., Bonn,
(5) Kapteyn Astronomical Inst., Groningen,
(6) Ctr. For Theoretical Physics, Polish Academy of Sciences, Warsaw,
(7) Shanghai Astronomical Observatory,
(8) INAF Capodimonte,
(9) Dept. of Physics, Oxford,
(10) School of Physics, Astronomy, Sun Yat-sen University, Guangzhou,
(11) Dept. of Physics, Univ. Federico II, Naples,
(12) INAF Padua,
(13) School of Physics, Astronomy, Queen Mary University, London,
(14) INAF Arcetri)
http://arxiv.org/abs/1902.11265
The formation of a thick disk through the heating of a thin disk: Agreement with orbital eccentricities of stars in the solar neighborhood
Volume 5, Issue 47 - article #15
P. Di Matteo
,
M. D. Lehnert
,
Y. Qu
,
W. van Driel
arXiv.org - Astrophysics - Volume: 2010, Issue: 19 Nov
arXiv:1011.3825
[
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SN 2004A: Another Type II-P Supernova with a Red Supergiant Progenitor
Volume 1, Issue 10 - article #16
M. A. Hendry
(1),
S. J. Smartt
(2),
R. M. Crockett
(2),
J. R. Maund
(3),
A. Gal-Yam
(4 and 5),
D.-S. Moon
(6),
S. B. Cenko
(6),
D. W. Fox
(4),
R. P. Kudritzki
(7),
C. R. Benn
(8),
R. Ostensen
(8)
((1) Institute of Astronomy, University of Cambridge, Cambridge, UK,
(2) Department of Physics and Astronomy, Queen's University Belfast, Belfast, UK,
(3) Astronomy Department, University of Texas, Austin, TX, USA,
(4) Department of Astronomy, California Institute of Technology, Pasadena, CA, USA,
(5) Hubble Fellow,
(6) Department of Physics and Space Radiation Laboratory, California Institute of Technology, Pasadena, CA, USA,
(7) Institute for Astronomy, University of Hawaii, Honolulu, Hawaii, USA,
(8) Isaac Newton Group, Santa Cruz de La Palma, Espana)
ArXiv - Astrophysics
astro-ph/0603670 [
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