CTQ 327: A new gravitational lens

Morgan, ND; Gregg, MD; Wisotzki L.; Becker, R; Maza, J; Schechter, PL; White, RL

Abstract

We present the second gravitationally lensed quasar discovered during the course of a Hubble Space Telescope Space Telescope Imaging Spectrograph snapshot survey for small-separation gravitational lenses. CTQ 327 is a double quasar with an image separation of 1?.22 and a g-band flux ratio of roughly 5 to 1. Spectra reveal both components to be z = 1.37 quasars, and the lensing galaxy is clearly visible after point-spread function subtraction of the two quasar components. The light profile of the lensing galaxy is well modeled by an r1/4 law, indicative of an early-type elliptical galaxy. An estimate of the lens galaxy redshift is z ? 0.4-0.6, based on the Faber-Jackson relationship and photometric considerations, although values outside this range are still consistent with the present data. Resolved spectra of the two quasars show similar, but not identical, continuum and emission-line features: component A exhibits weaker emission lines with respect to the continuum than does component B, and there is evidence of intrinsic differences in the emission-line profiles between the two components. Optical monitoring of the quasar pair also shows a change in the g-band flux ratio of 0.14 mag over a 3 month period. These spectral and photometric differences may be due to microlensing fluctuations from stars in the lensing galaxy, intrinsic quasar variability coupled with the system's differential time delay, or some combination of the two. The observed variability makes CTQ 327 an attractive target for future flux monitoring, aimed at time-delay or microlensing studies.

Más información

Título según WOS: CTQ 327: A new gravitational lens
Título según SCOPUS: CTQ 327: A new gravitational lens
Título de la Revista: ASTRONOMICAL JOURNAL
Volumen: 126
Número: 2
Editorial: IOP PUBLISHING LTD
Fecha de publicación: 2003
Página de inicio: 696
Página final: 705
Idioma: English
URL: http://stacks.iop.org/1538-3881/126/i=2/a=696
DOI:

10.1086/376470

Notas: ISI, SCOPUS