Showing 1–20 of 82 results
/ Date/ Name
Jul 6, 2023Long-term follow-up observations of extreme coronal line emitting galaxiesDec 21, 2023Supernova environments in J-PLUS. Normalized Cumulative Rank distributions and stellar population synthesis, combining narrow- and broad-band filtersMay 30, 2013Spectroscopy of Type Ia Supernovae by the Carnegie Supernova ProjectFeb 21, 2020The AMUSING++ Nearby Galaxy Compilation: I. Full Sample Characterization and Galactic--Scale Outflows SelectionNov 5, 2020SN 2019muj -- a well-observed Type Iax supernova that bridges the luminosity gap of the classSep 7, 2017Type II supernova spectral diversity I: Observations, sample characterization and spectral line evolutionAug 3, 2023Carnegie Supernova Project-I and -II: Measurements of $H_0$ using Cepheid, TRGB, and SBF Distance Calibration to Type Ia SupernovaeJan 7, 2026A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13Feb 9, 2026A Faint Progenitor System for the Faint Supernova 2024vjmFeb 26, 2026The extremely low-luminosity Type Iax SNe 2022ywf and 2023zgxOct 28, 2024Unveiling the nature of SN 2022jli: The first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late timesJul 5, 2023A Precursor Plateau and Pre-Maximum [O II] Emission in the Superluminous SN2019szu: A Pulsational Pair-Instability CandidateSep 26, 2023Recovering lost light: discovery of supernova remnants with integral field spectroscopyJan 28, 2024HII regions and diffuse ionized gas in the AMUSING++ Compilation: I. Catalogue presentationDec 2, 2010The old environment of the faint calcium-rich supernova SN 2005czAug 27, 2020Direct evidence of two-component ejecta in supernova 2016gkg from nebular spectroscopyJun 26, 2020The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratioOct 29, 2020Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red SupergiantsJul 19, 2021Probing the Progenitors of Type Ia Supernovae using Circumstellar Material Interaction SignaturesAug 18, 2021A puzzle solved after two decades: SN 2002gh among the brightest of superluminous supernovae