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 &lt; z &lt; 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...

Full description

Bibliographic Details
Main Authors: Georgii Khorunzhev, Sergey Sazonov, Rodion Burenin, Maxim Eselevich
Format: Article
Language:English
Published: Frontiers Media S.A. 2017-11-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:http://journal.frontiersin.org/article/10.3389/fspas.2017.00037/full
id doaj-c2131787eac840f4894cf638690c8856
record_format Article
spelling 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 &lt; z &lt; 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 &lt; z &lt; 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 AT georgiikhorunzhev catalogof3z55quasarcandidatesselectedamongxmmnewtonsourcesanditsspectroscopicverification
AT sergeysazonov catalogof3z55quasarcandidatesselectedamongxmmnewtonsourcesanditsspectroscopicverification
AT rodionburenin catalogof3z55quasarcandidatesselectedamongxmmnewtonsourcesanditsspectroscopicverification
AT maximeselevich catalogof3z55quasarcandidatesselectedamongxmmnewtonsourcesanditsspectroscopicverification
_version_ 1725494903512760320