Showing 1–20 of 173 results
/ Date/ Name
Dec 2, 2022A Survey for C II Emission-Line Stars in the Large Magellanic Cloud. II. Final Results and the Origin of C II Emission in [WC] SpectraNov 11, 2022Carnegie Supernova Project-II: Near-infrared spectral diversity and template of Type Ia SupernovaeApr 23, 2025The Search for Stable Nickel: Investigating the Origins of Type Ia Supernovae with Late-time NIR Spectroscopy from the Carnegie Supernova Project-IIOct 11, 2022Near-infrared and Optical Nebular-phase Spectra of Type Ia Supernovae SN 2013aa and SN 2017cbv in NGC 5643Oct 27, 2021The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of EvolutionOct 13, 2025Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfsSep 8, 2025Carnegie Supernova Project: Fast-Declining Type Ia Supernovae as Cosmological Distance IndicatorsMay 23, 20241991T-like SupernovaeAug 3, 2023Carnegie Supernova Project-I and -II: Measurements of $H_0$ using Cepheid, TRGB, and SBF Distance Calibration to Type Ia SupernovaeSep 13, 2021The winking eye of a very massive star: WR 21a revealed as an eclipsing binary by TESSJun 16, 2025A New Determination of the Mass of NGC 3603-A1: the Most Massive Binary Known?Mar 14, 2019Binary Red Supergiants II: Discovering and Characterizing B-type CompanionsFeb 22, 2023The Carnegie Supernova Project-I. Spectroscopic analysis of stripped-envelope supernovaeJul 3, 2023Swift/UVOT discovery of Swift J221951-484240: a UV luminous ambiguous nuclear transientFeb 22, 2023The Carnegie Supernova Project-I. Optical spectroscopy of stripped-envelope supernovaeJul 17, 2021ASASSN-15hy: an under-luminous, red 03fg-like type Ia supernovaNov 27, 2018A remarkable change of the spectrum of the magnetic Of?p star HD 148937 reveals evidence of an eccentric, high-mass binaryApr 8, 2025Analyzing type Ia supernovae near-infrared light curves with Principal Component AnalysisSep 29, 2021A Tale of Two Type Ia Supernovae: The fast-declining siblings SNe 2015bo and 1997cnJul 26, 2025JWST Observations of SN 2023ixf II: The Panchromatic Evolution Between 250 and 720 Days After the Explosion