Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification
We have compiled a catalog of 903 quasar candidates (including known quasars) at 3 < z < 5.5 selected among X-ray sources from the XMM-Newton serendipitous survey (3XMM-DR4 catalog). We used photometric SDSS, 2MASS, and WISE data to select the objects. The surface number density of obj...
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doaj-c2131787eac840f4894cf638690c88562020-11-24T23:46:03ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2017-11-01410.3389/fspas.2017.00037307689Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic VerificationGeorgii Khorunzhev0Sergey Sazonov1Rodion Burenin2Maxim Eselevich3High Energy Astrophysics, Space Research Institute, Russian Academy of Sciences, Moscow, RussiaHigh Energy Astrophysics, Space Research Institute, Russian Academy of Sciences, Moscow, RussiaHigh Energy Astrophysics, Space Research Institute, Russian Academy of Sciences, Moscow, RussiaLaboratory of Infrared Methods in Astrophysics, Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Irkutsk, RussiaWe have compiled a catalog of 903 quasar candidates (including known quasars) at 3 < z < 5.5 selected among X-ray sources from the XMM-Newton serendipitous survey (3XMM-DR4 catalog). We used photometric SDSS, 2MASS, and WISE data to select the objects. The surface number density of objects in our sample exceeds that in the SDSS spectroscopic quasar sample at the same redshifts by a factor of 1.5. We have performed spectroscopic observations of a subsample of new quasar candidates using a new low- and medium-resolution spectrograph at the 1.6-m AZT-33IK telescope (Mondy, Russia) and demonstrated that the purity of these candidates is about 65%. We have discovered one of the most distant (z = 5.08) X-ray selected quasars.http://journal.frontiersin.org/article/10.3389/fspas.2017.00037/fullactive galactic nucleiquasarsX-ray surveysphotometric redshiftsspectroscopyXMM-Newton |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Georgii Khorunzhev Sergey Sazonov Rodion Burenin Maxim Eselevich |
spellingShingle |
Georgii Khorunzhev Sergey Sazonov Rodion Burenin Maxim Eselevich Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification Frontiers in Astronomy and Space Sciences active galactic nuclei quasars X-ray surveys photometric redshifts spectroscopy XMM-Newton |
author_facet |
Georgii Khorunzhev Sergey Sazonov Rodion Burenin Maxim Eselevich |
author_sort |
Georgii Khorunzhev |
title |
Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification |
title_short |
Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification |
title_full |
Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification |
title_fullStr |
Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification |
title_full_unstemmed |
Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification |
title_sort |
catalog of 3 < z < 5.5 quasar candidates selected among xmm-newton sources and its spectroscopic verification |
publisher |
Frontiers Media S.A. |
series |
Frontiers in Astronomy and Space Sciences |
issn |
2296-987X |
publishDate |
2017-11-01 |
description |
We have compiled a catalog of 903 quasar candidates (including known quasars) at 3 < z < 5.5 selected among X-ray sources from the XMM-Newton serendipitous survey (3XMM-DR4 catalog). We used photometric SDSS, 2MASS, and WISE data to select the objects. The surface number density of objects in our sample exceeds that in the SDSS spectroscopic quasar sample at the same redshifts by a factor of 1.5. We have performed spectroscopic observations of a subsample of new quasar candidates using a new low- and medium-resolution spectrograph at the 1.6-m AZT-33IK telescope (Mondy, Russia) and demonstrated that the purity of these candidates is about 65%. We have discovered one of the most distant (z = 5.08) X-ray selected quasars. |
topic |
active galactic nuclei quasars X-ray surveys photometric redshifts spectroscopy XMM-Newton |
url |
http://journal.frontiersin.org/article/10.3389/fspas.2017.00037/full |
work_keys_str_mv |
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