Published November 13, 2017 | Version v1
Journal article

Catalog of 3 < z < 5.5 Quasar Candidates Selected among XMM-Newton Sources and Its Spectroscopic Verification

  • 1. High Energy Astrophysics, Space Research Institute, Russian Academy of Sciences, Moscow (Russian Federation)
  • 2. Laboratory of Infrared Methods in Astrophysics, Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Irkutsk (Russian Federation)

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.

Availability note (English)

Available from http://dx.doi.org/10.3389/fspas.2017.00037

Additional details

Identifiers

Publishing Information

Journal Title
Frontiers in Astronomy and Space Sciences
Journal Volume
4
Journal Page Range
[5 p.]
ISSN
2296-987X

INIS

Country of Publication
Switzerland
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
49023432
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CATALOGS; GALAXY NUCLEI; QUASARS; RED SHIFT; SPECTROSCOPY; TELESCOPES; X-RAY SOURCES
Descriptors DEC
COSMIC RADIO SOURCES; DOCUMENT TYPES; RADIATION SOURCES

Optional Information

Copyright
Copyright (c) 2017 Khorunzhev, Sazonov, Burenin and Eselevich.