Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?

Results of optical identification of the ASCA Lynx deep survey are presented. Six X-ray sources are detected in the 2-7 keV band using the SIS in a 20'x20' field of view with fluxes larger than ~4x10^{-14} erg s-1 cm-2 in the band. Follow-up optical spectroscopic observations were made, an...

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Main Authors: Ohta, K, Akiyama, M, Ueda, Y, Yamada, T, Nakanishi, K, Dalton, G, Ogasaka, Y, Kii, T, Hayashida, K
Format: Journal article
Published: 2003
_version_ 1797051596099551232
author Ohta, K
Akiyama, M
Ueda, Y
Yamada, T
Nakanishi, K
Dalton, G
Ogasaka, Y
Kii, T
Hayashida, K
author_facet Ohta, K
Akiyama, M
Ueda, Y
Yamada, T
Nakanishi, K
Dalton, G
Ogasaka, Y
Kii, T
Hayashida, K
author_sort Ohta, K
collection OXFORD
description Results of optical identification of the ASCA Lynx deep survey are presented. Six X-ray sources are detected in the 2-7 keV band using the SIS in a 20'x20' field of view with fluxes larger than ~4x10^{-14} erg s-1 cm-2 in the band. Follow-up optical spectroscopic observations were made, and five out of six sources are identified with AGNs/QSOs at redshifts of 0.5-1.3. We also identify two more additional X-ray sources detected in a soft X-ray band with AGNs/QSOs. It is found that three QSOs identified are located at z~1.3. Two rich clusters and several groups of galaxies are also placed at the same redshift in the surveyed field, and projected separations between the QSOs and the clusters are 3-8 Mpc at the redshift.
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spelling oxford-uuid:06883393-735c-4550-93e7-d9177deeeb9c2022-03-26T09:03:02ZOptical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:06883393-735c-4550-93e7-d9177deeeb9cSymplectic Elements at Oxford2003Ohta, KAkiyama, MUeda, YYamada, TNakanishi, KDalton, GOgasaka, YKii, THayashida, KResults of optical identification of the ASCA Lynx deep survey are presented. Six X-ray sources are detected in the 2-7 keV band using the SIS in a 20'x20' field of view with fluxes larger than ~4x10^{-14} erg s-1 cm-2 in the band. Follow-up optical spectroscopic observations were made, and five out of six sources are identified with AGNs/QSOs at redshifts of 0.5-1.3. We also identify two more additional X-ray sources detected in a soft X-ray band with AGNs/QSOs. It is found that three QSOs identified are located at z~1.3. Two rich clusters and several groups of galaxies are also placed at the same redshift in the surveyed field, and projected separations between the QSOs and the clusters are 3-8 Mpc at the redshift.
spellingShingle Ohta, K
Akiyama, M
Ueda, Y
Yamada, T
Nakanishi, K
Dalton, G
Ogasaka, Y
Kii, T
Hayashida, K
Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title_full Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title_fullStr Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title_full_unstemmed Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title_short Optical Identification of the ASCA Lynx Deep Survey: An Association of QSOs and a Supercluster at z=1.3?
title_sort optical identification of the asca lynx deep survey an association of qsos and a supercluster at z 1 3
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