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Ricci, ClaudioTreister, Ezequiel.Bauer, Franz Erik.Trakhtenbrot, BennyKoss, M.Ueda, YoshihiroDel Vecchio, I.Schawinski, K.Paltani, S.Oh, K.Lamperti, I.[BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog.]BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog.

Civano, FrancescaBauer, Franz Erik.Luo, B.Saez, C.Treister, Ezequiel.Hickox, R. C.Puccetti, S.Comastri, A.Mullaney, J.Zappacosta, L.LaMassa, Stephanie M.[The Nustar Extragalactic Surveys: Overview and Catalog from the COSMOS Field]The Nustar Extragalactic Surveys: Overview and Catalog from the COSMOS Field

Mullaney, J.Bauer, Franz Erik.Treister, Ezequiel.Del Moro, A.Aird, J. A.Alexander, D. M.Civano, FrancescaHickox, R. C.Lansbury, George B.Ajello, MarcoAssef, R.[The NuSTAR Extragalactic Surveys: Initial Results and Catalog from the Extended Chandra Deep Field South]The NuSTAR Extragalactic Surveys: Initial Results and Catalog from the Extended Chandra Deep Field South

Lansbury, George B.Treister, Ezequiel.Bauer, Franz Erik.Stern, Daniel.Aird, J. A.Alexander, D. M.Fuentes, C.Harrison, F. A.Tomsick, J. A.Baloković, M.Del Moro, A.[The NuSTAR Serendipitous Survey: The 40-month Catalog and the Properties of the Distant High-energy X-Ray Source Population]The NuSTAR Serendipitous Survey: The 40-month Catalog and the Properties of the Distant High-energy X-Ray Source Population

Ricci, ClaudioBauer, Franz Erik.Treister, Ezequiel.Ho, L. C.Fabian, AC.Trakhtenbrot, B.Koss, M.Ueda, Y.Lohfink, A.Shimizu, T.Mushotzky, R.[BAT AGN Spectroscopic Survey - XII. The relation between coronal properties of active galactic nuclei and the Eddington ratio.]BAT AGN Spectroscopic Survey - XII. The relation between coronal properties of active galactic nuclei and the Eddington ratio.

Yang, G.Kim, Sam.Brandt, W N.Bauer, Franz Erik.Schulze, Steve.Luo, B.Xue, Y. Q.Sun, M. Y.Zheng, X. C.Paolillo, M.Shemmer, O.[Long-term x-ray variability of typical active galactic nuclei in the distant universe.]Long-term x-ray variability of typical active galactic nuclei in the distant universe.

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