A Simple Method to Find All Lensed Quasars
Author(s) -
C. S. Kochanek,
B. J. Mochejska,
N. D. Morgan,
K. Z. Stanek
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/500559
Subject(s) - quasar , astrophysics , physics , variable (mathematics) , population , variable star , astronomy , galaxy , stars , mathematics , mathematical analysis , demography , sociology
We demonstrate that gravitationally lensed quasars are easily recognizedusing image subtraction methods as time variable sources that are spatiallyextended. For Galactic latitudes |b|>20 deg, lensed quasars dominate thepopulation of spatially extended variable sources, although there is somecontamination from variable star pairs, variable star-quasar pairs and binaryquasars that can be easily controlled using other information in the surveysuch as the object light curves and colors. This will allow planned large-scalesynoptic surveys to find lensed quasars almost down to their detection limitswithout the need for extensive follow-up observations.Comment: 11 pages, 4 figures, submitted to ApJ
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom