PMN J1838-3427: A new gravitationally lensed quasar
Abstract
We report the discovery of a new double-image quasar that was found during a search for gravitational lenses in the southern sky. Radio source PMN J1838-3427 is composed of two flat-spectrum components with separation 1", flux density ratio 14:1 and matching spectral indices, in VLA and VLBA images. Ground-based BRI images show the optical counterpart (total I=18.6) is also double with the same separation and position angle as the radio components. An HST/WFPC2 image reveals the lens galaxy. The optical flux ratio (27:1) is higher than the radio value probably due to differential extinction of the components by the lens galaxy. An optical spectrum of the bright component contains quasar emission lines at z=2.78 and several absorption features, including prominent Ly-alpha absorption. The lens galaxy redshift could not be measured but is estimated to be z=0.36 +/- 0.08. The image configuration is consistent with the simplest plausible models for the lens potential. The flat radio spectrum and observed variability of PMN J1838-3427 suggest the time delay between flux variations of the components is measurable, and could thus provide an independent measurement of H_0.
Keywords
Cite
@article{arxiv.astro-ph/0008036,
title = {PMN J1838-3427: A new gravitationally lensed quasar},
author = {Joshua N. Winn and Jacqueline N. Hewitt and Paul L. Schechter and Alan Dressler and E. E. Falco and C. D. Impey and C. S. Kochanek and J. Lehar and J. E. J. Lovell and B. A. McLeod and Nicholas D. Morgan and J. A. Munoz and H. -W. Rix and Maria Teresa Ruiz},
journal= {arXiv preprint arXiv:astro-ph/0008036},
year = {2009}
}
Comments
23 pages, incl. 6 figures, to appear in A.J.; replaced with accepted version; minor changes to text, improved figures