C H A N D R A
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Abstract: In a sample of 15,900 SDSS quasars, Eracleous et al. (2012) found 88 objects exhibiting broad emission lines with >1000 km/s velocity offsets with respect to the host galaxy rest frame. One leading hypothesis for the origin of these velocity-offset broad lines is the dynamics of a binary supermassive black hole (SMBH), with competing hypotheses of recoiling SMBH and a broad line region (BLR) gas outflow due to entrainment by a relativistic jet. We propose Chandra ACIS S observations of 10 quasars from this parent sample, with a combined total exposure request of 257 ks. These Chandra observations will serve as an Iron K-alpha line finder survey, necessary to test the BLR-outflow hypothesis. We will also measure black hole masses in order to constrain binary SMBH models. |
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