Showing 1–20 of 33 results
/ Date/ Name
Nov 18, 2024DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering MeasurementsNov 18, 2024DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and QuasarsNov 18, 2024DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering StatisticsApr 30, 2024Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and IIApr 3, 2024DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic OscillationsApr 3, 2024DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha ForestApr 3, 2024DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and QuasarsFeb 2, 2024La Silla-QUEST RR Lyrae Star Survey II: The Crater II Tidal StreamsJun 9, 2023The Early Data Release of the Dark Energy Spectroscopic InstrumentJun 9, 2023Validation of the Scientific Program for the Dark Energy Spectroscopic InstrumentMay 22, 2022Overview of the Instrumentation for the Dark Energy Spectroscopic InstrumentSep 25, 2019SUGAR: An improved empirical model of Type Ia Supernovae based on spectral featuresOct 22, 2018SNEMO: Improved Empirical Models for Type Ia SupernovaeApr 10, 2018Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxiesJan 5, 2017The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cuApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914Feb 26, 2016Localization and broadband follow-up of the gravitational-wave transient GW150914Mar 11, 2015On the diversity of super-luminous supernovae: ejected mass as the dominant factorDec 19, 2014Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble ConstantFeb 27, 2014Type Ia supernova bolometric light curves and ejected mass estimates from the Nearby Supernova Factory