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.2017.00037Additional 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.