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...
Main Authors: | , , , , , , , , |
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Format: | Journal article |
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2003
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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. |
first_indexed | 2024-03-06T18:21:46Z |
format | Journal article |
id | oxford-uuid:06883393-735c-4550-93e7-d9177deeeb9c |
institution | University of Oxford |
last_indexed | 2024-03-06T18:21:46Z |
publishDate | 2003 |
record_format | dspace |
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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