A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies-Reference-Cited by-同舟云学术

A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies

Published:2018-11-16 Issue:1 Volume:483 Page:223-234
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Tanimura Hideki¹²,Hinshaw Gary²³⁴,McCarthy Ian G⁵^ORCID,Van Waerbeke Ludovic²³,Aghanim Nabila¹,Ma Yin-Zhe⁶⁷,Mead Alexander²,Hojjati Alireza²,Tröster Tilman²^ORCID

Affiliation:

1. Institut d’Astrophysique Spatiale, CNRS (UMR 8617), Université Paris-Sud, Bâtiment 121, Orsay F-91405, France

2. Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada

3. Canadian Institute for Advanced Research, 180 Dundas St W, Toronto, ON M5G 1Z8, Canada

4. Canada Research Chair in Observational Cosmology

5. CAstrophysics Research Institute, Liverpool John Moores University, Liverpool, L3 5RF, UK

6. Astrophysics and Cosmology Research Unit, School of Chemistry and Physics, University of KwaZulu-Natal, Durban 4000, South Africa

7. NAOC-UKZN Computational Astrophysics Centre (NUCAC), University of KwaZulu-Natal, Durban 4000, South Africa

Funder

Ecological Society of Australia Incorporated

National Aeronautics and Space Administration

Alfred P. Sloan Foundation

National Science Foundation

U.S. Department of Energy Office of Science

Science and Technology Facilities Council

British Infection Society

Durham University

European Research Council

Horizon 2020

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/483/1/223/26996682/sty3118.pdf

Reference57 articles.

1. THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III

2. The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples

3. The Contribution of the Intergalactic Medium to Cosmic Microwave Background Anisotropies

4. Kinematic Sunyaev-Zel'dovich Cosmic Microwave Background Temperature Anisotropies Generated by Gas in Cosmic Structures

5. Gas and galaxies in filaments between clusters of galaxies

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