The INTEGRAL/IBIS AGN catalogue: an update
Abstract
In the most recent IBIS survey based on observations performed during the first 1000 orbits of INTEGRAL, are listed 363 high-energy emitters firmly associated with AGN, 107 of which are reported here for the first time. We have used X-ray data to image the IBIS 90 per cent error circle of all the AGN in the sample of 107, in order to obtain the correct X-ray counterparts, locate them with arcsec accuracy and therefore pinpoint the correct optical counterparts. This procedure has led to the optical and spectral characterization of the entire sample. This new set consists of 34 broad line or type 1 AGN, 47 narrow line or type 2 AGN, 18 blazars and 8 sources of unknown class. These eight sources have been associated with AGN from their positional coincidence with 2MASX/Radio/X-ray sources. Seven high-energy emitters have been included since they are considered to be good AGN candidates. Spectral analysis has been already performed on 55 objects and the results from the most recent and/or best statistical measurements have been collected. For the remaining 52 sources, we report the spectral analysis for the first time in this work. We have been able to obtain the full X-ray coverage of the sample making use of data from Swift/XRT, XMM–Newton and NuSTAR. In addition to the spectral characterization of the entire sample, this analysis has enabled us to identify peculiar sources and by comparing different data sets, highlight flux variability in the 2–10 keV and 20–40 keV bands.
Additional Information
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2016 April 21. Received 2016 April 19; in original form 2016 February 2. Published: 23 April 2016. This research has made use of data obtained from the SIMBAD data base operated at CDS, Strasbourg, France; the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA's Goddard Space Flight Center NASA/IPAC Extragalactic Database (NED). The authors acknowledge the ASI financial support via ASI–INAF grant 2013-025-R.0.Attached Files
Accepted Version - nustar_4_22.pdf
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Additional details
- Eprint ID
- 66411
- DOI
- 10.1093/mnras/stw972
- Resolver ID
- CaltechAUTHORS:20160422-122726356
- Agenzia Spaziale Italiana (ASI)
- 2013-025-R.0
- Istituto Nazionale di Astrofisica (INAF)
- Created
-
2016-04-22Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- NuSTAR, Infrared Processing and Analysis Center (IPAC)