Showing 1–20 of 53 results
/ Date/ Name
Jan 25, 2011Carbon Recombination Lines toward the Riegel-Crutcher Cloud and other Cold HI Regions in the inner GalaxyFeb 5, 2019A Model for Phased Array FeedFeb 5, 2019Phased Array Feed Model Equations corresponding to two definitions of embedded beam patternMar 3, 2005Multi-wavelength carbon recombination line observations with the VLA toward an UCHII region in W48: Physical properties and kinematics of neutral materialFeb 5, 2019Model for a Noise Matched Phased Array FeedFeb 5, 2012Advanced Multi-beam Spectrometer for the Green Bank TelescopeAug 10, 2023A Cryogenic Wideband (2.5-14 GHz) Receiver system for the Arecibo 12m TelescopeNov 6, 2017A Highly-Sensitive Cryogenic Phased Array Feed for the Green Bank TelescopeMay 12, 2023The Next Generation Arecibo Telescope: A preliminary studyMar 2, 2021The Future Of The Arecibo Observatory: The Next Generation Arecibo TelescopeJul 13, 2019Astro2020 Activities and Projects White Paper: Arecibo Observatory in the Next DecadeAug 1, 2014VLA and GBT Observations of Orion B (NGC 2024, W12) : Photo-dissociation Region Properties and Magnetic fieldJan 29, 2005A search for 53 MHz OH line near G48.4$-$1.4 using the National MST Radar FacilityJan 29, 2005An 8.5 GHz Arecibo survey of Carbon Recombination Lines toward Ultra-compact \HII regions: Physical properties of dense molecular materialSep 13, 2012A compact steep spectrum radio source in NGC1977Nov 3, 2021Arecibo-Green Bank-LOFAR Carbon Radio Recombination Line observations toward cold HI CloudsMar 9, 2017Helium Ionization in the Diffuse Ionized Gas surrounding UCHII regionsMar 12, 2018Performance of a highly sensitive, 19-element, dual-polarization, cryogenic L-band Phased Array Feed on the Green Bank TelescopeJun 17, 2002Carbon Recombination Lines near 327 MHz I: "Diffuse" CII regions in the Galactic DiskOct 4, 2001Low-frequency Carbon Recombination Lines towards HI self-absorption features in the Galactic Plane