New cluster candidates in the extended XMM Lockman Hole field

A. Finoguenov; A. Streblyanska; G. Hasinger; Y. Hashimoto; G. Szokoly

doi:10.1016/j.asr.2004.12.035

New cluster candidates in the extended XMM Lockman Hole field

A. Finoguenov
, A. Streblyanska^*
, G. Hasinger
, Y. Hashimoto
, G. Szokoly

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

4 Citations (Scopus)

Abstract

We describe the results of a search for diffuse sources in the 0.4 deg ² area of the XMM-Newton 770 ks survey of the Lockman Hole. An abundant population of sources is revealed, which is likely to stem from low-mass galaxy clusters at redshift near 1. We present the optical images in the K′ and R-bands for our candidates, suggesting a concentration of red galaxies at the position of the X-ray sources. Together with our improved understanding of the baryon physics in low-mass clusters these results reveal the important role that deep X-ray surveys will play in cosmological studies.

Original language	English
Pages (from-to)	710-714
Number of pages	5
Journal	Advances in Space Research
Volume	36
Issue number	4
DOIs	https://doi.org/10.1016/j.asr.2004.12.035
Publication status	Published - 2005
Externally published	Yes

Keywords

Clusters
Galaxy clusters
Galaxy groups
Large scale structure of the Universe
Observational cosmology
X-ray sources

ASJC Scopus subject areas

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
General Earth and Planetary Sciences

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10.1016/j.asr.2004.12.035

Cite this

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title = "New cluster candidates in the extended XMM Lockman Hole field",

abstract = " We describe the results of a search for diffuse sources in the 0.4 deg 2 area of the XMM-Newton 770 ks survey of the Lockman Hole. An abundant population of sources is revealed, which is likely to stem from low-mass galaxy clusters at redshift near 1. We present the optical images in the K′ and R-bands for our candidates, suggesting a concentration of red galaxies at the position of the X-ray sources. Together with our improved understanding of the baryon physics in low-mass clusters these results reveal the important role that deep X-ray surveys will play in cosmological studies.",

keywords = "Clusters, Galaxy clusters, Galaxy groups, Large scale structure of the Universe, Observational cosmology, X-ray sources",

author = "A. Finoguenov and A. Streblyanska and G. Hasinger and Y. Hashimoto and G. Szokoly",

note = "Funding Information: Based on observations obtained with XMM-Newton, an ESA Science Mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). COSPAR conference attendance was partially supported by an grant from the ESA Education Office. ",

year = "2005",

doi = "10.1016/j.asr.2004.12.035",

language = "English",

volume = "36",

pages = "710--714",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Limited",

number = "4",

}

TY - JOUR

T1 - New cluster candidates in the extended XMM Lockman Hole field

AU - Finoguenov, A.

AU - Streblyanska, A.

AU - Hasinger, G.

AU - Hashimoto, Y.

AU - Szokoly, G.

N1 - Funding Information: Based on observations obtained with XMM-Newton, an ESA Science Mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). COSPAR conference attendance was partially supported by an grant from the ESA Education Office.

PY - 2005

Y1 - 2005

N2 - We describe the results of a search for diffuse sources in the 0.4 deg 2 area of the XMM-Newton 770 ks survey of the Lockman Hole. An abundant population of sources is revealed, which is likely to stem from low-mass galaxy clusters at redshift near 1. We present the optical images in the K′ and R-bands for our candidates, suggesting a concentration of red galaxies at the position of the X-ray sources. Together with our improved understanding of the baryon physics in low-mass clusters these results reveal the important role that deep X-ray surveys will play in cosmological studies.

AB - We describe the results of a search for diffuse sources in the 0.4 deg 2 area of the XMM-Newton 770 ks survey of the Lockman Hole. An abundant population of sources is revealed, which is likely to stem from low-mass galaxy clusters at redshift near 1. We present the optical images in the K′ and R-bands for our candidates, suggesting a concentration of red galaxies at the position of the X-ray sources. Together with our improved understanding of the baryon physics in low-mass clusters these results reveal the important role that deep X-ray surveys will play in cosmological studies.

KW - Clusters

KW - Galaxy clusters

KW - Galaxy groups

KW - Large scale structure of the Universe

KW - Observational cosmology

KW - X-ray sources

UR - https://www.scopus.com/pages/publications/27744452198

UR - https://www.scopus.com/pages/publications/27744452198#tab=citedBy

U2 - 10.1016/j.asr.2004.12.035

DO - 10.1016/j.asr.2004.12.035

M3 - Article

AN - SCOPUS:27744452198

SN - 0273-1177

VL - 36

SP - 710

EP - 714

JO - Advances in Space Research

JF - Advances in Space Research

IS - 4

ER -

New cluster candidates in the extended XMM Lockman Hole field

Abstract

Keywords

ASJC Scopus subject areas

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