Showing 21–40 of 56 results
/ Date/ Name
Oct 10, 2025JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the ExplosionJul 26, 2025JWST Observations of SN 2023ixf II: The Panchromatic Evolution Between 250 and 720 Days After the ExplosionJul 24, 2025JWST Observations of SN 2024ggi I: Interpretation and Model Comparison of the Type II Supernova 2024ggi at 55 days Past ExplosionDec 3, 2025The broad-lined type Ic supernova 2020lao experienced an energetic explosion with no central-engine signaturesNov 13, 2021Close, bright and boxy: the superluminous SN 2018htiJan 16, 2021A Bright Ultraviolet Excess in the Transitional 02es-like Type Ia Supernova 2019yvqFeb 18, 2021Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)Feb 26, 2019Carnegie Supernova Project-II: Using Near-Infrared Spectroscopy to determine the location of the outer $^{56}$Ni in Type Ia SupernovaeApr 2, 2019A Physical Basis for the H-band Blue-edge Velocity and Light-Curve Shape Correlation in Context of Type Ia Supernova Explosion PhysicsApr 9, 2019Gas phase SiO in the circumstellar environment of the recurrent nova T Coronae BorealisOct 8, 2019Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II SupernovaeSep 14, 2023SN 2021gno: a Calcium-rich transient with double-peaked light curvesJul 1, 2019SN 2017gmr: An energetic Type II-P supernova with asymmetriesNov 5, 2022Photometric and spectroscopic analysis of the Type II SN 2020jfo with a short plateauJan 9, 2023JWST Low-Resolution MIRI Spectral Observations of SN~2021aefx: High-density Burning in a Type Ia SupernovaOct 23, 2023Newly Formed Dust within the Circumstellar Environment of SNIa-CSM 2018evtDec 12, 2024Using nebular near-IR spectroscopy to measure asymmetric chemical distributions in 2003fg-like thermonuclear supernovaeNov 18, 2024Testing for Intrinsic Type Ia Supernova Luminosity Evolution at z>2 with JWSTJul 17, 2021ASASSN-15hy: an under-luminous, red 03fg-like type Ia supernovaApr 20, 2026Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO