2006ApJ...640..569B

Optical and X-ray observations of the quadruply imaged quasar 1RXS J1131-1231 show flux ratio anomalies among the images of factors of ∼2 in the optical and ∼3-9 in X-rays. Temporal variability of the quasar seems an unlikely explanation for the discrepancies between the X-ray and optical flux ratio anomalies. The negative parity of the most affected image and the decreasing trend of the anomalies with wavelength suggest microlensing as a possible explanation; this would imply that the source of optical radiation in RXS J1131 is ∼10⁴R_g_in size for a black hole mass of ∼10⁸ M_☉. We also present evidence for different X-ray spectral hardness ratios among the four images.