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New quasars behind the Magellanic Clouds. Spectroscopic confirmation of near-infrared selected candidates

Piatti, Andres E.; Ivanov, Valentin D.; Cioni, Maria-Rosa L.; Bekki, Kenji; Cioni, Maria Rosa L.; de Grijs, Richard; Emerson, Jim; Gibson, Brad K.; For, Bi Qing; Kamath, Devika; van Loon, Jacco Th.; Piatti, Andrés E.; For, Bi-Qing


Andres E. Piatti

Valentin D. Ivanov

Maria-Rosa L. Cioni

Kenji Bekki

Maria Rosa L. Cioni

Richard de Grijs

Jim Emerson

Bi Qing For

Devika Kamath

Jacco Th. van Loon

Andrés E. Piatti

Bi-Qing For


Context. Quasi-stellar objects (quasars) located behind nearby galaxies provide an excellent absolute reference system for astrometric studies, but they are difficult to identify because of fore- and background contamination. Deep wide-field, high angular resolution surveys spanning the entire area of nearby galaxies are needed to obtain a complete census of such quasars. Aims. We embarked on a program to expand the quasar reference system behind the Large and the Small Magellanic Clouds, the Magellanic Bridge, and the Magellanic Stream that connects the Clouds with the Milky Way. Methods. Hundreds of quasar candidates were selected based on their near-infrared colors and variability properties from the ongoing public ESO VISTA Magellanic Clouds survey. A subset of 49 objects was followed up with optical spectroscopy. Results. We confirmed the quasar nature of 37 objects (34 new identifications): four are low redshift objects, three are probably stars, and the remaining three lack prominent spectral features for a secure classification. The bona fide quasars, identified from their broad emisison lines, are located as follows: 10 behind the LMC, 13 behind the SMC, and 14 behind the Bridge. The quasars span a redshift range from z ~ 0.5 to z ~ 4.1. Conclusions. Upon completion the VMC survey is expected to yield a total of ~1500 quasars with Y< 19.32 mag, J< 19.09 mag, and Ks< 18.04 mag.

Publication Date Apr 1, 2016
Journal Astronomy & astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 588
Article Number A93
APA6 Citation Ivanov, V. D., Cioni, M. L., Bekki, K., de Grijs, R., Emerson, J., Gibson, B. K., …For, B. (2016). New quasars behind the Magellanic Clouds. Spectroscopic confirmation of near-infrared selected candidates. Astronomy and Astrophysics, 588,
Keywords Surveys -- infrared; Galaxies -- quasars; General -- Magellanic Clouds
Publisher URL
Copyright Statement ©ESO 2016
Additional Information Copy of article first published in: Astronomy & astrophysics, 2016, v.588


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