Showing 1–20 of 41 results
/ Date/ Name
Mar 29, 2023The broad-lined Type-Ic supernova SN 2022xxf with extraordinary two-humped light curvesOct 28, 2020From core collapse to superluminous: The rates of massive stellar explosions from the Palomar Transient FactoryNov 18, 2021SN 2020kyg and the rates of faint Iax Supernovae from ATLASDec 11, 2017Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at redshift twoNov 14, 2022The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 SupernovaeSep 2, 2024SN 2021foa: The "Flip-Flop" Type IIn / Ibn supernovaDec 9, 2025University of Hawaii 88-inch Telescope Observations of the Interstellar Comet 3I/ATLAS: Spectrophotometric Blue-Sensitive Spectral Time Series Spanning Two Months from DiscoveryAug 31, 2022A fast rising tidal disruption event from a candidate intermediate mass black holeJun 16, 2023SN 2023emq: a flash-ionised Ibn supernova with possible CIII emissioFeb 8, 2022Systematic errors on optical-SED stellar mass estimates for galaxies across cosmic time and their impact on cosmologyApr 13, 2020The broad-line type Ic SN 2020bvc: signatures of an off-axis gamma-ray burst afterglowSep 3, 2024Double "acct": a distinct double-peaked supernova matching pulsational pair-instability modelsMar 4, 2024Final Moments II: Observational Properties and Physical Modeling of CSM-Interacting Type II SupernovaeJan 30, 2020DES16C3cje: A low-luminosity, long-lived supernovaJan 8, 2020Supernova Host Galaxies in the Dark Energy Survey: I. Deep Coadds, Photometry, and Stellar MassesApr 25, 2020The first Hubble diagram and cosmological constraints using superluminous supernovaFeb 3, 2022SN 2018bsz: a Type I superluminous supernova with aspherical circumstellar materialJan 11, 2019Discovery and Follow-up of the Unusual Nuclear Transient OGLE17aajNov 9, 2022SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environmentMar 31, 2022Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves