Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy-Reference-Cited by-同舟云学术

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Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy

Published:2018-04-27 Issue:3 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Ota Naomi¹,Nagai Daisuke²³,Lau Erwin T²³

Affiliation:

1. Department of Physics, Nara Women’s University, Kitauoyanishi-machi, Nara, Nara 630-8506, Japan

2. Department of Physics, Yale University, New Haven, CT 06520, USA

3. Yale Center for Astronomy and Astrophysics, Yale University, New Haven, CT 06520, USA

Funder

JSPS KAKENHI

National Science Foundation

NASA ATP

NASA Chandra Theory

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/3/51/25055060/psy040.pdf

Reference60 articles.

1. Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters

2. Abundances of the elements: Meteoritic and solar

3. ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ONY-MSCALING RELATIONS

4. Investigating the velocity structure and X-ray observable properties of simulated galaxy clusters with PHOX

5. AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence

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3. Halo scaling relations and hydrostatic mass bias in the simba simulation from realistic mock X-ray catalogues;Monthly Notices of the Royal Astronomical Society;2023-09-07

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5. Galaxy cluster hydrostatic bias in Kottler spacetime;Physics of the Dark Universe;2022-03

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