Showing 101–120 of 193 results
/ Date/ Name
Sep 2, 2020The boulder population of asteroid 4 Vesta: Size-frequency distribution and survival timeJun 24, 2020TRAPPIST-1: Global Results of the Spitzer Exploration Science Program {\it Red Worlds}Mar 13, 2020Evaluation and mitigation of trace $^{210}$Pb contamination on copper surfacesJan 27, 2020Prospects for Fundamental Physics with LISAJan 6, 2020GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$Jan 3, 2020The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 SystemJan 3, 2020A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing RunsDec 25, 2019Open data from the first and second observing runs of Advanced LIGO and Advanced VirgoSep 14, 2019Robust block magnetism in the spin ladder compound BaFe$_2$Se$_3$ under hydrostatic pressureAug 29, 2019A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signalsJun 19, 2019Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo networkMar 11, 2019Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1Feb 22, 2019Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015-2017 LIGO DataFeb 22, 2019Narrow-band search for gravitational waves from known pulsars using the second LIGO observing runFeb 5, 2019Search for transient gravitational wave signals associated with magnetar bursts during Advanced LIGO's second observing runJan 28, 2019Probing nucleon's spin structures with polarized Drell-Yan in the Fermilab SpinQuest experimentDec 20, 2018Spectrophotometric Modeling and Mapping of CeresDec 18, 2018Towards Deep Conversational RecommendationsDec 18, 2018The early instability scenario: terrestrial planet formation during the giant planet instability, and the effect of collisional fragmentationNov 30, 2018Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo