Showing 1–20 of 31 results
/ Date/ Name
Mar 14, 2026Nebular Phase Evolution of SN 2023ixf (I): From Circumstellar Infrared Echo to the onset of in-situ Dust Formation in a Type II SupernovaJan 16, 2026Study of the anisotropy of cosmic expansion on ZTF type Iasupernovae simulationsSep 9, 2025SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernovaJul 24, 2025SVOM GRB 250314A at z $\simeq$ 7.3: an exploding star in the era of reionizationJul 24, 2025JWST Observations of SN 2024ggi I: Interpretation and Model Comparison of the Type II Supernova 2024ggi at 55 days Past ExplosionMar 18, 2025Data Release 1 of the Dark Energy Spectroscopic InstrumentJan 7, 2025Expanding the parameter space of 2002es-like type Ia supernovae: on the underluminous ASASSN-20jq / SN 2020qxpSep 6, 2024ZTF SN Ia DR2: Simulations and volume limited sampleSep 6, 2024ZTF SN Ia DR2: The diversity and relative rates of the thermonuclear SN populationJul 31, 2024A study in scarlet -- II. Spectroscopic properties of a sample of Intermediate Luminosity Red TransientsApr 30, 2024Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and IIAug 11, 2023SN 2022joj: A Potential Double Detonation with a Thin Helium shellNov 29, 2022Sociology and hierarchy of voids: A study of seven nearby CAVITY galaxy voids and their dynamical CosmicFlows-3 environmentNov 9, 2022SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environmentJan 14, 2021SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovaeAug 10, 2020The Exotic Type Ic Broad-Lined Supernova SN 2018gep: Blurring the Line Between Supernovae and Fast Optical TransientsFeb 5, 2020Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bvOct 14, 2019The CALIFA view on stellar angular momentum across the Hubble sequenceNov 28, 2018The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051Nov 6, 2018Cosmological Constraints from Multiple Probes in the Dark Energy Survey