Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects 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 Solid-State Imaging Spectrometer in a ∼20′ × 20′ field of view with fluxes larger than ∼4 × 10-14 ergs s -1 cm-2 in the band. Follow-up optical spectroscopic obs...
Glavni autori: | , , , , , , , , |
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Format: | Journal article |
Jezik: | English |
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Institute of Physics Publishing
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 Solid-State Imaging Spectrometer in a ∼20′ × 20′ field of view with fluxes larger than ∼4 × 10-14 ergs s -1 cm-2 in the band. Follow-up optical spectroscopic observations were made, and five out of six sources are identified with active galactic nuclei/quasi-stellar objects (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. We find 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 | 2024-03-07T06:25:50Z |
format | Journal article |
id | oxford-uuid:f44255fe-15e0-4b9a-948b-e7c2af8cffc1 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T06:25:50Z |
publishDate | 2003 |
publisher | Institute of Physics Publishing |
record_format | dspace |
spelling | oxford-uuid:f44255fe-15e0-4b9a-948b-e7c2af8cffc12022-03-27T12:18:25ZOptical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3?Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:f44255fe-15e0-4b9a-948b-e7c2af8cffc1EnglishSymplectic Elements at OxfordInstitute of Physics Publishing2003Ohta, 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 Solid-State Imaging Spectrometer in a ∼20′ × 20′ field of view with fluxes larger than ∼4 × 10-14 ergs s -1 cm-2 in the band. Follow-up optical spectroscopic observations were made, and five out of six sources are identified with active galactic nuclei/quasi-stellar objects (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. We find 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 quasi-stellar objects and a supercluster at z = 1.3? |
title | Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3? |
title_full | Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3? |
title_fullStr | Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3? |
title_full_unstemmed | Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3? |
title_short | Optical identification of the ASCA Lynx Deep Survey: An association of quasi-stellar objects and a supercluster at z = 1.3? |
title_sort | optical identification of the asca lynx deep survey an association of quasi stellar objects and a supercluster at z 1 3 |
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