X-RAY MONITORING OF GRAVITATIONAL LENSES WITH CHANDRA

摘要

We present Chandra monitoring data for six gravitationally lensed quasars: QJ?0158–4325, HE?0435–1223, SDSS?0924+0219, SDSS?1004+4112, HE?1104–1805, and Q?2237+0305. X-ray microlensing variability is detected in all six lenses with high confidence. We furthermore detect energy-dependent microlensing in HE?0435–1223, SDSS?0924+0219, SDSS?1004+4112, and Q?2237+0305. Through a detailed spectral analysis for each lens we find that simple power-law models plus Gaussian emission lines give good fits to the spectra. We detect intrinsic spectral variability in two epochs of Q?2237+0305, and differential absorption between images in QJ?0158–4325 and Q2237+0305. We also detect the Fe?Kα emission line in all six lenses, and the Ni XXVII Kα line in two images of Q?2237+0305. The rest-frame equivalent widths of the Fe?Kα lines are measured to be 0.4-1.2?keV, significantly higher than those measured in typical active galactic nuclei of similar X-ray luminosities. This suggests that the Fe?Kα emission region is more compact or centrally concentrated than the continuum emission region.