Showing 1–20 of 366 results
/ Date/ Name
Oct 28, 2019The Zwicky Transient Facility Bright Transient Survey I: Spectroscopic Classification and the Redshift Completeness of Local Galaxy CatalogsJan 7, 2002MERLIN radio detection of an interaction zone within a binary Orion proplyd systemJul 29, 2002Two jets from the Orion (M42) `proplyds' - kinematics, morphologies and originsAug 29, 2019Infrastructure and Strategies for Time Domain and MMA and Follow-UpMay 11, 2012Fundamental Physics at the Intensity FrontierFeb 27, 2012Evolution of the Red Sequence Giant to Dwarf Ratio in Galaxy Clusters out to z ~ 0.5Nov 8, 2023Photometric prioritization of neutron star merger candidatesMay 10, 2013Las Cumbres Observatory Global Telescope NetworkApr 11, 2019Achieving Transformative Understanding of Extreme Stellar Explosions with ELT-enabled Late-time SpectroscopyOct 14, 2019The luminous and rapidly evolving SN 2018bcc: Clues toward the origin of Type Ibn SNe from the Zwicky Transient FacilityMar 15, 2019Astro2020 Science White Paper: The Next Decade of Astroinformatics and AstrostatisticsSep 22, 2021AT2018lqh and the nature of the emerging population of day-scale duration optical transientsMar 25, 2021Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design ReportFeb 7, 2020Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume III: DUNE Far Detector Technical CoordinationJan 12, 2016Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNFSep 4, 2013On the Challenge of Plasma Heating with the JET Metallic WallJun 26, 2020Long-baseline neutrino oscillation physics potential of the DUNE experimentDec 8, 2025ZTF-SEDm Type Ia supernova sample for Twins Embedding spectrophotometric standardisationSep 4, 2025ZTF SNe Ia DR2: Towards cosmology-grade ZTF supernova light curves using scene modeling photometryDec 18, 2024ZTF SN Ia DR2: Properties of the low-mass host galaxies of Type Ia supernovae in a volume-limited sample