Serendipitous discovery of a projected pair of QSOs separated by 4.5 arcsec on the sky
arXiv:1604.01361 · doi:10.3847/0004-6256/152/1/13
Abstract
We present the serendipitous discovery of a projected pair of quasi-stellar objects (QSOs) with an angular separation of arcsec. The redshifts of the two QSOs are widely different: one, our programme target, is a QSO with a spectrum consistent with being a narrow line Seyfert 1 AGN at . For this target we detect Lyman-, \ion{C}{4}, and \ion{C}{3]}. The other QSO, which by chance was included on the spectroscopic slit, is a Type 1 QSO at a redshift of , for which we detect \ion{C}{4}, \ion{C}{3]} and \ion{Mg}{2}. We compare this system to previously detected projected QSO pairs and find that only about a dozen previously known pairs have smaller angular separation.
arXiv comment4 pages, 3 figures. Accepted for publication in AJ
References in corpus (17)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The Sloan Digital Sky Survey: Technical Summary
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
- Cosmic-Ray Rejection by Laplacian Edge Detection
- Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
- The 2dF QSO Redshift Survey - XII. The spectroscopic catalogue and luminosity function
- An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1
- Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales
- The 2dF-SDSS LRG and QSO Survey: The z<2.1 Quasar Luminosity Function from 5645 Quasars to g=21.85
- Quasars Probing Quasars I: Optically Thick Absorbers Near Luminous Quasars
- The Sloan Digital Sky Survey Quasar Lens Search. V. Final Catalog from the Seventh Data Release
- Binary quasars
- Optical/near-infrared selection of red QSOs: Evidence for steep extinction curves towards galactic centers?
- The High A(V) Quasar Survey: Reddened quasi-stellar objects selected from optical/near-infrared photometry - II
- Correcting second-order contamination in low-resolution spectra