Skip to main content

Research Repository

Advanced Search

Identification of AGN in the XMM-Newton X-ray survey of the SMC

Maitra, Chandreyee; Haberl, Frank; Ivanov, Valentin D.; Cioni, Maria-Rosa L.; Van Loon, Jacco Th.

Identification of AGN in the XMM-Newton X-ray survey of the SMC Thumbnail


Authors

Chandreyee Maitra

Frank Haberl

Valentin D. Ivanov

Maria-Rosa L. Cioni



Abstract

Context
Finding Active Galactic Nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult because of the high stellar density in these fields. Although the first AGN behind the Small Magellanic Cloud (SMC) were reported in the 1980s, it is only recently thatthe number of AGN known behind the SMC has increased by several orders of magnitude.

Aims. The mid-infrared colour selection technique has been proven to be an efficient means of identifying AGN, especially obscured sources. The X-ray regime is complementary in this regard and we use XMM-Newton observations to support the identification of AGN behind the SMC.

Methods. We present a catalogue of AGN behind the SMC by correlating an updated X-ray point source catalogue from our XMMNewton survey of the SMC with already known AGN from the literature as well as a list of candidates obtained from the ALLWISE mid-infrared colour selection criterion. We studied the properties of the sample with respect to their redshifts, luminosities and X-ray spectral characteristics. We also identified the near-infrared counterpart of the sources from the VISTA observations.

Results. The redshift and luminosity distributions of the sample (where known) indicate that we detect sources from nearby Seyfert galaxies to distant and obscured quasars. The X-ray hardness ratios are compatible with those typically expected for AGN. The VISTA colours and variability are also consistent in this regard. A positive correlation was observed between the integrated X-ray flux (0.2–12 keV) and the ALLWISE and VISTA magnitudes. We further present a sample of new candidate AGN and candidates for obscured AGN. All of these make an interesting subset for further follow-up studies. An initial spectroscopic follow-up of 6 out of the 81 new candidates showed all six sources are active galaxies, albeit two with narrow emission lines.

Citation

Maitra, C., Haberl, F., Ivanov, V. D., Cioni, M. L., & Van Loon, J. T. (2019). Identification of AGN in the XMM-Newton X-ray survey of the SMC. Astronomy & Astrophysics, 622, Article A29. https://doi.org/10.1051/0004-6361/201833663

Journal Article Type Article
Acceptance Date Oct 29, 2018
Online Publication Date Jan 24, 2019
Publication Date 2019-02
Publicly Available Date May 26, 2023
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 622
Article Number A29
DOI https://doi.org/10.1051/0004-6361/201833663
Keywords magellanic clouds, quasars, general, X-rays, galaxies, infrared, galaxies, catalogues
Public URL https://keele-repository.worktribe.com/output/412107
Publisher URL https://doi.org/10.1051/0004-6361/201833663

Files






You might also like



Downloadable Citations