LARgE Survey – I. Dead monsters: the massive end of the passive galaxy stellar mass function at cosmic noon-Reference-Cited by-同舟云学术

LARgE Survey – I. Dead monsters: the massive end of the passive galaxy stellar mass function at cosmic noon

Published:2019-04-27 Issue:4 Volume:486 Page:4880-4893
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Arcila-Osejo Liz¹,Sawicki Marcin¹^ORCID,Arnouts Stéphane²,Golob Anneya¹,Moutard Thibaud¹,Sorba Robert¹³

Affiliation:

1. Saint Mary’s University, Department of Astronomy and Physics and the Institute for Computational Astrophysics, 923 Robie Street, Halifax, Nova Scotia B3H 3C3, Canada

2. Laboratoire d’Astrophysique de Marseille, Université Aix-Marseille, 38 rue Frederic Joliot Curie, Marseille F-13388, France

3. Physics Department, Mount Allison University, 62 York Street, Sackville, New Brunswick E4L 1E2, Canada

Funder

Natural Sciences and Engineering Research Council

National Research Council

Institut National des Sciences de l'Univers, Centre National de la Recherche Scientifique

University of Hawaii

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1169/28537827/stz1169.pdf

Reference93 articles.

1. The numbers of z ∼ 2 star-forming and passive galaxies in 2.5 square degrees of deep CFHT imaging

2. The most massive galaxies and black holes allowed by ΛCDM

3. VELOCITY DISPERSIONS AND DYNAMICAL MASSES FOR A LARGE SAMPLE OF QUIESCENT GALAXIES ATz> 1: IMPROVED MEASURES OF THE GROWTH IN MASS AND SIZE

4. MOSFIRE SPECTROSCOPY OF QUIESCENT GALAXIES AT 1.5

5. MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching

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