Showing 21–40 of 82 results
/ Date/ Name
Mar 2, 2021Real-time Discovery of AT2020xnd: A Fast, Luminous Ultraviolet Transient with Minimal Radioactive EjectaSep 12, 2016The High Cadence Transient Survey (HiTS) - I. Survey design and supernova shock breakout constraintsApr 16, 2012The Local Environments of Core-Collapse SNe within Host GalaxiesOct 14, 2015A correlation between SN II metal line strength and host HII region oxygen abundanceMar 26, 2014H-alpha Spectral diversity of type II supernovaeMar 27, 2014Characterizing the V-band light-curves of hydrogen-rich type II supernovaeNov 30, 2017SN 2017dio: a type-Ic supernova exploding in a hydrogen-rich circumstellar mediumDec 6, 2023Light-Curve Structure and Halpha Line Formation in the Tidal Disruption Event AT 2019azhJun 16, 2023Environmental dependence of Type IIn supernova propertiesMay 4, 2020SN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral FeaturesAug 15, 2025SN 2021aaev: a Hydrogen-Rich Superluminous Supernova with Early Flash and Long-Lived Circumstellar Interaction in an Unusual Host EnvironmentFeb 10, 2026Narrow absorption lines from intervening material in supernovae. IV. Type Ia supernovae: Na I D line strength relating to external material and intrinsic propertiesSep 23, 2020Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbvJun 21, 2023A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE: I. Sample selection, analysis of local environments, and correlations with light curve propertiesApr 5, 2022Two years of optical and NIR observations of the superluminous supernova UID 30901 discovered by the UltraVISTA SN surveyJan 28, 2016Supernova 2010ev: A reddened high velocity gradient type Ia supernovaApr 15, 2015Statistical studies of supernova environmentsMar 7, 2025Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor SystemsMar 15, 2022Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yjaNov 7, 2022Revealing the progenitor of SN 2021zby through analysis of the $TESS$ shock-cooling light curve