Showing 1–20 of 79 results
/ Date/ Name
Sep 20, 2022BASS XXXIII: Swift-BAT blazars and their jets through cosmic timeFeb 28, 2014Simultaneous NuSTAR and XMM-Newton 0.5-80 keV spectroscopy of the Narrow Line Seyfert 1 galaxy SWIFT J2127.4+5654May 13, 2015Broadband Observations of the Compton-thick Nucleus of NGC 3393Jun 16, 2015NuSTAR Reveals Extreme Absorption in z < 0.5 Type 2 QuasarsMay 14, 2014Observations of MCG-5-23-16 with Suzaku, XMM-Newton and NuSTAR: Disk tomography and Compton hump reverberationSep 7, 2016First NuSTAR observations of the BL Lac - type blazar PKS~2155-304: constraints on the jet content and distribution of radiating particlesOct 24, 2017RoboPol: Connection between optical polarization plane rotations and gamma-ray flares in blazarsJun 29, 2016A growth-rate indicator for Compton-thick active galactic nucleiJan 13, 2016RoboPol: optical polarization-plane rotations and flaring activity in blazarsJul 20, 2017The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keVSep 8, 2014Early-time polarized optical light curve of GRB 131030ANov 13, 2015The NuSTAR Extragalactic Surveys: The Number Counts of Active Galactic Nuclei and the Resolved Fraction of the Cosmic X-ray BackgroundNov 13, 2015The NuSTAR Extragalactic Surveys: Initial Results and Catalog from the Extended Chandra Deep Field SouthJun 24, 2020$NuSTAR$ Observations of Four Nearby X-ray Faint AGN: Low Luminosity or Heavy Obscuration?Mar 28, 2024Joint ALMA/X-ray monitoring of the radio-quiet type 1 AGN IC 4329ADec 18, 2014Coronal Properties of the Seyfert 1.9 Galaxy MCG -05-23-016 Determined from Hard X-ray Spectroscopy with NuSTARNov 13, 2013The RoboPol optical polarization survey of gamma-ray - loud blazarsMar 11, 2014NuSTAR J033202-2746.8: direct constraints on the Compton reflection in a heavily obscured quasar at z~2Mar 12, 2014NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-Selected Quasars at z ~ 2Dec 19, 2016The NuSTAR Serendipitous Survey: The 40 month Catalog and the Properties of the Distant High Energy X-ray Source Population