Showing 1–20 of 28 results
/ Date/ Name
Sep 19, 2019Calibration and monitoring of the ASTRI-Horn telescope by using the night-sky background measured by the photon-statistics ("variance") methodSep 26, 2007A tool for phase resolved spectroscopy with ISGRIFeb 28, 2013The merger fraction of active and inactive galaxies in the local Universe through an improved non-parametric classificationJul 22, 2019Compton-thick AGNs in the NuSTAR era. V: Joint NuSTAR and XMM-Newton spectral analysis of three "soft-Gamma" candidate CT-AGNs in the Swift-BAT 100-month catalogDec 21, 2018Compton-thick AGN in the NuSTAR era III: A systematic study of the torus covering factorSep 22, 2005A Compton reflection dominated spectrum in a peculiar accreting neutron starJul 19, 2013The Site of the ASTRI SST-2M Telescope PrototypeJul 18, 2014The puzzling source IGR J17361-4441 in NGC 6388: a possible planetary tidal disruption eventMay 9, 2017A broadband self-consistent modelling of the X-ray spectrum of 4U 1626--67Feb 21, 2022Chandra Follow-up Observations of Swift-BAT-selected AGNs IIAug 18, 2021Effective pointing of the ASTRI-Horn telescope using the Cherenkov camera with the Variance methodAug 18, 2015Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger ObservatorySep 27, 2004A puzzling event during the X-ray emission of the binary system GX 1+4Jul 18, 2013The Pierre Auger Observatory: Contributions to the 33rd International Cosmic Ray Conference (ICRC 2013)Feb 25, 2009Study of the accreting pulsar 4U 0115+634 with a bulk and thermal Comptonization modelSep 26, 2017Chandra and NuSTAR follow-up observations of Swift-BAT selected AGNJan 6, 2020Use of the Peak-Detector mode for gain calibration of SiPM sensors with ASIC CITIROC read-outFeb 15, 2022Disk precession to explain the super-orbital modulation of LMC X-4: results from the Swift monitoring campaignMay 9, 2016Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray EnergyMar 26, 2015Measurement of the cosmic ray spectrum above $4{\times}10^{18}$ eV using inclined events detected with the Pierre Auger Observatory