NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z ∼ 5
External Source
chorus
Document Type
Version of Record
Authors
L Legrand
(Institut d’Astrophysique Spatiale, CNRS (UMR 8617), Université Paris-Sud, Bâtiment 121, 91405 Orsay Cedex, France)
H J McCracken
(Institut d’Astrophysique de Paris, Sorbonne Universités, UPMC Univ Paris 6 et CNRS, UMR 7095, 98 bis bd Arago, F-75014 Paris, France)
I Davidzon
(IPAC, Mail Code 314-6, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA)
O Ilbert
(Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France)
J Coupon
(Department of Astronomy, University of Geneva, Ch. d’Ecogia 16, CH-1290 Versoix, Switzerland)
N Aghanim
(Institut d’Astrophysique Spatiale, CNRS (UMR 8617), Université Paris-Sud, Bâtiment 121, 91405 Orsay Cedex, France)
M Douspis
(Institut d’Astrophysique Spatiale, CNRS (UMR 8617), Université Paris-Sud, Bâtiment 121, 91405 Orsay Cedex, France)
P L Capak
(IPAC, Mail Code 314-6, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA)
O Le Fèvre
(Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France)
B Milvang-Jensen
(Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark)
Date Acquired
February 10, 2024
Publication Date
May 2, 2019
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 486
Issue: 4
Issue Publication Date: July 11, 2019
ISSN: 0035-8711
e-ISSN: 1365-2966
Distribution Limits
Public
Keywords
space and planetary science
astronomy and astrophysics

Available Downloads

There are no available downloads for this record.
Document Not Available for PreviewClick to Access Document