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GBNCC — Green Bank North Celestial Cap Survey
The Green Bank North Celestial Cap (GBNCC) survey is a 350MHz all-sky pulsar survey using the Robert C. Byrd Green Bank Telescope in West Virginia. When complete, the survey will cover the entire sky north of Declination -40° (85% of the celestial sphere). Data taking began in 2009 and processing of GBNCC data, in 2011.…
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NANOGrav — North American Nanohertz Observatory for Gravitational Waves
Overview The North American Nanohertz Observatory for Gravitational Waves Physics Frontiers Center (NANOGrav PFC) is an international collaboration using ultra-stable millisecond pulsars to detect gravitational waves. NANOGrav observes a pulsar timing array (PTA) of dozens of millisecond pulsars with approximately monthly cadence using the Robert C. Byrd Green Bank Telescope and the William E. Gordon…
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GOTHAM — GBT Observations of TMC-1: Hunting Aromatic Molecules
GOTHAM is an extremely high-sensitivity (2 mK), high-resolution (0.02 km/s) spectral line survey of the cold core TMC-1 in X, K, and Ka bands. Pilot, targeted observations of the source over only <2 GHz of total bandwidth resulted in the detection of three new astronomical molecules, including the first radio detection of a benzene-ring aromatic…
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GDIGS — The GBT Diffuse Ionized Gas Survey
The GBT Diffuse Ionized Gas Survey (GDIGS) is a large ongoing survey to map radio recombination line emission from diffuse ionized gas in the Galactic plane. Diffuse ionized gas known as the “Warm Ionized Medium (WIM)” is a major component of the interstellar medium, making up ∼20% of the total Milky Way gas mass and…
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Drift Scan Survey for Pulsars, FRBs, Radio Transients, and Gas in Galaxies
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AstroBIO 2019
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MUSTANG Penetrates the Central Molecular Zone
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Holiday Asteroid Imaged with NASA Radar