Showing 1–20 of 77 results
/ Date/ Name
Sep 13, 2021Detection of the Crab Nebula by the prototype Schwarzschild-Couder TelescopeApr 30, 2025Absence of TeV halos around millisecond pulsarsJul 3, 2024Analysis of the Emission and Morphology of the Pulsar Wind Nebula Candidate HAWC J2031+415Nov 15, 2019New hard-TeV extreme blazars detected with the MAGIC telescopesSep 24, 2021Observation of the gamma-ray binary HESS J0632+057 with the H.E.S.S., MAGIC, and VERITAS telescopesOct 3, 2020Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagationOct 5, 2023Multi-year characterisation of the broad-band emission from the intermittent extreme BL Lac 1ES~2344+514Sep 20, 2022Gamma-ray observations of MAXI J1820+070 during the 2018 outburstDec 21, 2020VHE gamma-ray detection of FSRQ QSO B1420+326 and modeling of its enhanced broadband state in 2020Jun 11, 2020An intermittent extreme BL Lac: MWL study of 1ES 2344+514 in an enhanced stateMar 27, 2023Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova RemnantsJun 19, 2025Longtime Monitoring of TeV Radio Galaxies with HAWCSep 8, 2023HAWC Study of Very-High-Energy $γ$-ray Spectrum of HAWC J1844-034Apr 9, 2026Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing StrategiesFeb 5, 2022Investigating the blazar TXS 0506+056 through sharp multi-wavelength eyes during 2017-2019Jul 17, 2019Monte Carlo Studies of Combined MAGIC and LST1 ObservationsOct 7, 2022A lower bound on intergalactic magnetic fields from time variability of 1ES 0229+200 from MAGIC and Fermi/LAT observationsSep 7, 2023Search for Decaying Dark Matter in the Virgo Cluster of Galaxies with HAWCJul 11, 2023Development of a SiPM Pixel Prototype for the Large-Sized Telescope of the Cherenkov Telescope ArrayJul 15, 2024Testing the Molecular Cloud Paradigm for Ultra-High-Energy Gamma Ray Emission from the Direction of SNR G106.3+2.7