Showing 621–640 of 1,571 results
/ Date/ Name
Sep 29, 2021Apertif, Phased Array Feeds for the Westerbork Synthesis Radio TelescopeSep 28, 2021ArtPop: A Stellar Population and Image Simulation Python PackageSep 28, 2021Detectability of southern gamma-ray sources beyond 100 TeV with ALPAQUITA, the prototype experiment of ALPACASep 28, 2021Developing the Future of Gamma-ray Astrophysics with Monolithic Silicon PixelsSep 27, 2021SCExAO, a testbed for developing high-contrast imaging technologies for ELTsSep 21, 2021Rapid stellar and binary population synthesis with COMPASSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and HighlightsSep 13, 2021Reconstruction of stereoscopic CTA events using deep learning with CTLearnSep 10, 2021Design and performance of the prototype Schwarzschild-Couder Telescope cameraSep 10, 2021Fast map-based simulations of systematics in CMB surveys including effects of the scanning strategySep 10, 2021Unsupervised classification of simulated magnetospheric regionsSep 7, 2021The Planetary Systems Imager Adaptive Optics System: An Initial Optical Design and Performance Analysis Tools for the PSI-Red AO SystemSep 6, 2021The TESS Mission Target Selection ProcedureAug 27, 2021First Experimental Results of the Fast Atmospheric Self-coherent Camera Technique on the Santa cruz Extreme Adaptive optics Laboratory Testbed: Demonstration of High Speed Focal Plane Wavefront Control of Residual Atmospheric SpecklesAug 27, 2021Analytical simulations of the effect of satellite constellations on optical and near-infrared observationsAug 25, 2021First Results from the REAL-time Transient Acquisition backend (REALTA) at the Irish LOFAR stationAug 24, 2021Using Gaia DR2 to make a systematic comparison between two geometric distortion solutionsAug 19, 2021High-contrast integral field spectropolarimetry of planet-forming disks with SCExAO/CHARISAug 18, 2021Dark zone maintenance results for segmented aperture wavefront error drift in a high contrast space coronagraphAug 17, 2021Characterization of the background for a neutrino search with the HAWC observatory