Showing 781–800 of 1,782 results
/ Date/ Name
Mar 9, 2021Disk, Corona, Jet Connection in the Intermediate State of MAXI J1820+070 Revealed by NICER Spectral-Timing AnalysisMar 9, 2021Physics of Superluminous SupernovaeMar 3, 2021Thermal Emission and Radioactive Lines, but No Pulsar, in the Broadband X-Ray Spectrum of Supernova 1987AFeb 26, 2021Sub-MeV spectroscopy with AstroSat-CZT Imager for Gamma Ray BurstsFeb 26, 2021Exploring Sub-MeV Sensitivity of AstroSat-CZTI for ON-axis Bright SourcesFeb 21, 2021CRAFTS for Fast Radio Bursts Extending the dispersion-fluence relation with new FRBs detected by FASTFeb 11, 2021The KM3NeT potential for the next core-collapse supernova observation with neutrinosFeb 9, 2021Hard X-ray Emission Associated with White Dwarfs. IV. Signs of Accretion from Sub-stellar CompanionsFeb 3, 2021Infrared Spectropolarimetric Detection of Intrinsic Polarization from a Core-Collapse SupernovaJan 26, 2021The relentless variability of Mrk 421 from the TeV to the radioJan 25, 2021Middle aged $γ$-ray pulsar J1957+5033 in X-rays: pulsations, thermal emission and nebulaJan 21, 2021The X-ray emission of the Seyfert 2 galaxy MCG-01-24-12Jan 20, 2021The Observed Rate of Binary Black Hole Mergers can be Entirely Explained by Globular ClustersJan 19, 2021A Peculiar ICME Event in August 2018 Observed with the Global Muon Detector NetworkJan 15, 2021The simulation framework of the timing-based localization for future all-sky gamma-ray observations with a fleet of CubesatsJan 14, 2021SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovaeJan 13, 2021Gamma-ray Thermalization and Leakage from Millisecond Magnetar Nebulae: Towards a Self-Consistent Model for Superluminous SupernovaeJan 12, 2021Spectro-Timing Analysis of a highly variable narrow-line Seyfert 1 galaxy NGC 4748 with AstroSat and XMM-NewtonDec 23, 2020Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910Dec 22, 2020All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems