Showing 21–40 of 74 results
/ Date/ Name
Oct 3, 2022Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWSTJun 29, 2023Roman CCS White Paper: Options to Increase the Coverage Area of Prism Time Series in the High-Latitude Time Domain Core Community SurveySep 10, 2023Approaches to lowering the cost of large space telescopesMay 26, 2020SN2019dge: a Helium-rich Ultra-Stripped Envelope SupernovaApr 15, 2019Discovery of an intermediate-luminosity red transient in M51 and its likely dust-obscured, infrared-variable progenitorJun 26, 2013The International Linear Collider Technical Design Report - Volume 3.II: Accelerator Baseline DesignJan 27, 2026Union3.1: Self-consistent Measurements of Host Galaxy Properties for 2000 Type Ia SupernovaeJul 5, 2023Roman CCS White Paper: Measuring Type Ia Supernovae Discovered in the Roman High Latitude Time Domain SurveyJan 27, 2023The DEHVILS Survey Overview and Initial Data Release: High-Quality Near-Infrared Type Ia Supernova Light Curves at Low RedshiftJul 22, 2019Accelerating Experimental Design by Incorporating Experimenter HunchesAug 14, 2017Science-Driven Optimization of the LSST Observing StrategyApr 20, 2026Testing $Λ$CDM versus dynamical dark energy in one year: A DESI spectroscopic follow-up program for Rubin supernovaeMar 12, 2019The Next Generation of Cosmological Measurements with Type Ia SupernovaeApr 22, 2019The Hyper Suprime-Cam SSP Transient Survey in COSMOS: OverviewMay 29, 2024DESI Constraints on Exponential QuintessenceFeb 23, 2023Estimating the Instantaneous Reproduction Number With Imperfect Data: A Method to Account for Case-Reporting Variation and Serial Interval UncertaintyJun 29, 2023Roman CCS White Paper: Considerations for Selecting Fields for the Roman High-latitude Time Domain Core Community SurveyMar 8, 2024Hawai'i Supernova Flows: A Peculiar Velocity Survey Using Over a Thousand Supernovae in the Near-InfraredJun 17, 2021A Spitzer Survey for Dust-Obscured SupernovaeAug 6, 2018Characterization of Unstable Pixels Using a Mixture Model: Application to HST WFC3 IR