Variability-selected quasars behind the Small Magellanic Cloud
arXiv:astro-ph/0210601 · doi:10.1086/346144
Abstract
We present followup spectroscopic observations of quasar candidates in the Small Magellanic Cloud selected by Eyer from the OGLE database. Of twelve observed objects identified as "QSO Candidate", five are confirmed quasars, with the emission redshifts ranging from 0.28 to 2.16. Two of those quasars were also recently identified independently in the MACHO database by Geha et al. We discuss the prospects of using variability-based selection technique for quasar searches behind other dense stellar fields. An additional criterion utilizing the color-color diagram should reduce the number of stars in the candidate lists.
arXiv commentRevised version, AASTeX, 11 pages, 3 EPS figures, one table, accepted 14 Nov 2002 for publication in the Astronomical Journal, March 2003 issue
References in corpus (8)
- A method for optimal image subtraction
- Variability-Selected Quasars in MACHO Project Magellanic Cloud Fields
- Extinction Map of Baade's Window
- A ROSAT PSPC X-Ray Survey of the Small Magellanic Cloud
- Variability-selected quasars behind the Small Magellanic Cloud
- Discovery of four X-ray quasars behind the Large Magellanic Cloud
- Probes for Nearby Galaxies
- ROSAT X-ray sources in the field of the LMC I.Total LMC gas from the background AGN spectral fits
Cited by in corpus (28)
- Quantifying Quasar Variability As Part of a General Approach To Classifying Continuously Varying Sources
- The Proper Motion of the Large Magellanic Cloud using HST
- Is the SMC Bound to the LMC? The HST Proper Motion of the SMC
- Limitations on the recovery of the true AGN variability parameters using Damped Random Walk modeling
- Variability selected high-redshift quasars on SDSS Stripe 82
- How are AGN Found?
- The Optical Gravitational Lensing Experiment. Catalog of stellar proper motions in the OGLE-II Galactic bulge fields
- The Magellanic Quasars Survey. III. Spectroscopic Confirmation of 758 AGNs Behind the Magellanic Clouds
- A Simple Method To Find All Lensed Quasars
- XMM-Newton observations of High Mass X-ray Binaries in the SMC
- Variability-selected quasars behind the Small Magellanic Cloud
- The Magellanic Quasars Survey. II. Confirmation of 144 New Active Galactic Nuclei Behind the Southern Edge of the Large Magellanic Cloud
- The Chandra survey of the SMC "Bar": II. Optical counterparts of X-ray sources
- The Magellanic Quasars Survey. I. Doubling the Number of Known AGNs Behind the Small Magellanic Cloud
- Finding Quasars behind the Galactic Plane. I. Candidate Selections with Transfer Learning
- Variability of Luminous Stars in the Large Magellanic Cloud Using 10 Years of ASAS Data
- The VMC Survey - VI. Quasars behind the Magellanic system
- X-ray bright sources in the Chandra Small Magellanic Cloud Wing Survey - detection of two new pulsars
- Variability-selected QSO candidates in OGLE-II Galactic Bulge fields
- New Quasars Detected via Variability in the QUEST1 Survey
- Discovery of nine quasars behind the Large Magellanic Cloud
- Massive young stellar objects in the Local Group irregular galaxy NGC6822 identified using machine learning
- New quasars behind the Magellanic Clouds. Spectroscopic confirmation of near-infrared selected candidates
- New X-ray quasars behind the Small Magellanic Cloud
- The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- II. The Small Magellanic Cloud
- Identification of AGN in the XMM-Newton X-ray survey of the SMC
- The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- I. The bar and outskirts of the Small Magellanic Cloud
- AGN behind the SMC selected from radio and X-ray surveys