C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: Chandra observations of quadruply gravitationally lensed quasars have a unique power to address several fundamental astrophysical issues. These observations have been used to (1) determine the cause of flux ratio anomalies, (2) measure the sizes of quasar accretion disks, (3) determine the dark matter content of the lensing galaxies, and (4) measure the stellar mass-to-light ratio (in fact, this is the only way to measure the stellar mass-to-light ratio beyond the solar neighborhood). In all cases, the main source of uncertainty in the results is the small size of the sample of known quads; until recently, only about a dozen systems were available for study with Chandra. We propose Chandra observations of four newly discovered quads. |
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