Weak Hard X-Ray Emission from Broad Absorption Line Quasars: Evidence for Intrinsic X-Ray Weakness

B. Luo, W. N. Brandt, D. M. Alexander, D. Stern, S. H. Teng, P. Arevalo, F. E. Bauer, S. E. Boggs, Finn Erland Christensen, A. Comastri, W. W. Craig, D. Farrah, P. Gandhi, C. J. Hailey, F. A. Harrison, M. Koss, P. Ogle, S. Puccetti, C. Saez, A. E. ScottD. J. Walton, W. W. Zhang

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Abstract

We report NuSTAR observations of a sample of six X-ray weak broad absorption line (BAL) quasars. These targets, at z = 0.148-1.223, are among the optically brightest and most luminous BAL quasars known at z <1.3. However, their rest-frame ≈2 keV luminosities are 14 to >330 times weaker than expected for typical quasars. Our results from a pilot NuSTAR study of two low-redshift BAL quasars, a Chandra stacking analysis of a sample of high-redshift BAL quasars, and a NuSTAR spectral analysis of the local BAL quasar Mrk 231 have already suggested the existence of intrinsically X-ray weak BAL quasars, i.e., quasars not emitting X-rays at the level expected from their optical/UV emission. The aim of the current program is to extend the search for such extraordinary objects. Three of the six new targets are weakly detected by NuSTAR with ≲ 45 counts in the 3-24 keV band, and the other three are not detected. The hard X-ray (8-24 keV) weakness observed by NuSTAR requires Compton-thick absorption if these objects have nominal underlying X-ray emission. However, a soft stacked effective photon index (Γeff ≈ 1.8) for this sample disfavors Compton-thick absorption in general. The uniform hard X-ray weakness observed by NuSTAR for this and the pilot samples selected with
Original languageEnglish
Article number70
JournalAstrophysical Journal
Volume794
Issue number1
Number of pages11
ISSN0004-637X
DOIs
Publication statusPublished - 2014

Cite this

Luo, B., Brandt, W. N., Alexander, D. M., Stern, D., Teng, S. H., Arevalo, P., Bauer, F. E., Boggs, S. E., Christensen, F. E., Comastri, A., Craig, W. W., Farrah, D., Gandhi, P., Hailey, C. J., Harrison, F. A., Koss, M., Ogle, P., Puccetti, S., Saez, C., ... Zhang, W. W. (2014). Weak Hard X-Ray Emission from Broad Absorption Line Quasars: Evidence for Intrinsic X-Ray Weakness. Astrophysical Journal, 794(1), [70]. https://doi.org/10.1088/0004-637X/794/1/70