Showing 1–20 of 23 results
/ Date/ Name
Jun 13, 2022The impostor revealed: SN 2016jbu was a terminal explosionDec 20, 2023SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environmentSep 25, 2024Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgcMay 29, 2025The ambiguous AT2022rze: Changing-look AGN mimicking a supernova in a merging galaxy systemOct 10, 2023SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon linesJan 26, 2024Spectroscopic observations of progenitor activity 100 days before a Type Ibn supernovaJan 7, 2022The Automated Photometry Of Transients (AutoPhOT) pipelineOct 25, 2022A long life of excess: The interacting transient SN 2017hccApr 21, 2022Probing for the host galaxies of the fast X-ray transients XRT 000519 and XRT 110103Sep 27, 2021How low can you go? SN 2018zd as a low-mass Fe core-collapse supernovaAug 27, 2024Sample of hydrogen-rich superluminous supernovae from the Zwicky Transient FacilityAug 18, 2022Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observationsMar 16, 2023Photometric study of the late-time near-infrared plateau in Type Ia supernovaeJun 1, 2022SN 2021foa, a transitional event between a Type IIn (SN 2009ip-like) and a Type Ibn supernovaFeb 18, 2021Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)Sep 2, 2025Long-term evolution of the SN 2009ip-like transient SN 2016cvkDec 15, 2006Experimental Results from an Antineutrino Detector for Cooperative Monitoring of Nuclear ReactorsSep 16, 2021SN 2018bsz: significant dust formation in a nearby superluminous supernovaFeb 18, 2021Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)Mar 11, 2025Precursor Activity Preceding Interacting Supernovae I: Bridging the Gap with SN 2022mop