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Oh, KyuseokRicci, ClaudioTreister, Ezequiel.Schawinski, KevinKoss, M.Trakhtenbrot, BennyLamperti, IsabellaMushotzky, RichardVeilleux, SylvainBerney, SimonCrenshaw, D. Michael[BAT AGN Spectroscopic Survey - III : an observed link between AGN Eddington ratio and narrow-emission-line ratios.]BAT AGN Spectroscopic Survey - III : an observed link between AGN Eddington ratio and narrow-emission-line ratios.

Lamperti, IsabellaRicci, ClaudioTreister, Ezequiel.Koss, M.Trakhtenbrot, BennySchawinski, KevinOh, KyuseokLandt, HermineRiffel, RogérioRodrìguez-Ardila, AlbertoGehrels, Neil[BAT AGN Spectroscopic Survey - IV : near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray emission.]BAT AGN Spectroscopic Survey - IV : near-Infrared Coronal Lines, Hidden Broad Lines, and Correlation with Hard X-ray emission.

Ricci, ClaudioBauer, Franz ErikTreister, EzequielPrivon, G. C.Schawinski, K.Blecha, L.Arevalo, P.Armus, LeeHarrison, F.Ho, L. C.Iwasawa, K.Sanders, David B.Stern, Daniel[Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured.]Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured.

Lansbury, George B.Bauer, Franz Erik.Treister, Ezequiel.Ricci, ClaudioAlexander, D. M.Aird, J. A.Gandhi, P.Stern, Daniel.Koss, M.Lamperti, IsabellaAjello, Marco[The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV]The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV

Trakhtenbrot, BennyRicci, ClaudioTreister, Ezequiel.Koss, M.Schawinski, KevinMushotzky, RichardUeda, YoshihiroVeilleux, SylvainLamperti, IsabellaOh, KyuseokStern, DanielHarrison, F.Baloković, MislavGehrels, Neil[BAT AGN Spectroscopic Survey (BASS) – VI. The ΓX–L/LEdd relation.]BAT AGN Spectroscopic Survey (BASS) – VI. The ΓX–L/LEdd relation.

Baronchelli, LindaRicci, ClaudioTreister, Ezequiel.Koss, M.Schawinski, K.Cardamone, C.Civano, F.Comastri, A.Elvis, M.Lanzuisi, G.Marchesi, S.[Inferring Compton-thick AGN candidates at z > 2 with Chandra using the > 8 keV rest-frame spectral curvature.]Inferring Compton-thick AGN candidates at z > 2 with Chandra using the > 8 keV rest-frame spectral curvature.

Zappacosta, L.Ricci, ClaudioTreister, Ezequiel.Comastri, A.Civano, FrancescaPuccetti, S.Fiore, F.Aird, J. A.Del Moro, A.Lansbury, George B.Lanzuisi, G.[The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample]The NuSTAR Extragalactic Surveys: X-Ray Spectroscopic Analysis of the Bright Hard-band Selected Sample

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.

Sartori, Lia F.Ricci, ClaudioTreister, Ezequiel.Schawinski, KevinKoss, M.Stern, DanielLansbury, GeorgeMaksym, W. PeterBaloković, MislavGandhi, PoshakKeel, William C.[Joint NuSTAR and Chandra analysis of the obscured quasar in IC 2497 - Hanny's Voorwerp system.]Joint NuSTAR and Chandra analysis of the obscured quasar in IC 2497 - Hanny's Voorwerp system.

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