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

^*此作品的通信作者

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

4 引文斯高帕斯（Scopus）

摘要

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.

原文	英語
頁（從 - 到）	710-714
頁數	5
期刊	Advances in Space Research
卷	36
發行號	4
DOIs	https://doi.org/10.1016/j.asr.2004.12.035
出版狀態	已發佈 - 2005
對外發佈	是

ASJC Scopus subject areas

航空工程
天文和天體物理學
地球物理
大氣科學
空間與行星科學
一般地球與行星科學

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10.1016/j.asr.2004.12.035

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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",

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pages = "710--714",

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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

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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

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ASJC Scopus subject areas

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