Showing 1–20 of 39 results
/ Date/ Name
Aug 20, 2025The radio flare and multi-wavelength afterglow of the short GRB 231117A: energy injection from a violent shell collisionMay 19, 2025The evolution of CME sheath turbulence from L1 to Earth: Wind and MMS observations of the 2023-04-23 CMENov 9, 2022SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environmentJun 30, 2021Simulating Reflected Light Exoplanet Spectra of the Promising Direct Imaging Target, $\upsilon$ Andromedae d, with a New, Fast Sampling Method Using the Planetary Spectrum GeneratorApr 7, 2021Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppmApr 7, 2021Beam dynamics corrections to the Run-1 measurement of the muon anomalous magnetic moment at FermilabNov 20, 2020The luminous red nova variety: AT 2020hat and AT 2020kogFeb 5, 2020Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bvMar 28, 2019The Sporadic Activity of (6478) Gault: A YORP-driven event?Nov 10, 2017The early detection and follow-up of the highly obscured Type II supernova 2016ija/DLT16amAug 4, 2017Hydrogen-Poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep SurveyMay 1, 2017Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae starsMar 3, 2017Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospectsNov 1, 2016The progenitor and early evolution of the Type IIb SN 2016gkgSep 6, 2016A Search for Very High-Energy Gamma Rays from the Missing Link Binary Pulsar J1023+0038 with VERITASAug 9, 2016Discovery of Very High Energy Gamma Rays from 1ES 1440+122Aug 5, 2016Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum LightAug 4, 2016Very High Energy outburst of Markarian 501 in May 2009May 17, 2016PS1-14bj: A Hydrogen-Poor Superluminous Supernova With a Long Rise and Slow DecayApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914