arXiv · 1212.2957
X-ray properties of the Northern Galactic Cap AGNs in the 58-month Swift-BAT catalog
Abstract
We present a detailed X-ray spectral analysis of a complete sample of hard X-ray selected AGN in the Northern Galactic Cap of the 58-month Swift Burst Alert Telescope (Swift/BAT) catalog, consisting of 100 AGN with b>50deg. This region has excellent potential for further study due to the availability of a wide range of archival multi-wavelength data, and we propose it as a low-redshift analog to the `deep fields' work on AGN at higher redshifts. We present distributions of luminosity, absorption, and other key quantities, from fitting new and archival X-ray data gathered from XMM-Newton, Swift/XRT, ASCA and Swift/BAT. We probe to deeper redshifts than the 9-month BAT catalog ( =0.043), and uncover a broader absorbing column density distribution. The fraction of obscured (log N_H >= 22) objects in the sample is ~60%, and 43--56% of the sample exhibits `complex' 0.4--10keV spectra. The soft excess is either well-detected in AGN or undetected, suggesting that the process responsible for producing the soft excess is not ubiquitous. The fraction of Compton-thick sources in our sample is ~9%, and `hidden/buried AGN' constitute ~14% of our sample. Compton reflection is found to be important in a large fraction of our sample using joint XMM-Newton+BAT fits (reflection amplitude = 2.7 +/- 0.75), indicating light bending or extremely complex absorption. The average 1--10keV spectrum for the sample reproduces the 1--10keV X-ray background slope as found for the 9-month BAT AGN sample. The completeness limit for the sample is ~4 times fainter than that for the 9-month catalog (abridged).
Explore related subjects
Keep this discovery
Ranjan V. Vasudevan, William N. Brandt, Richard F. Mushotzky, Lisa M. Winter, Wayne H. Baumgartner, Thomas T. Shimizu, Donald P. Schneider, John A. Nousek. 2012-12-12. X-ray properties of the Northern Galactic Cap AGNs in the 58-month Swift-BAT catalog. https://doi.org/10.1088/0004-637x%2F763%2F2%2F111
Cite the original work for its findings. Save a collection to share your selection of sources.