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The research utilized X-ray data from NASA's Neil Gehrels Swift Observatory and radio data from the Karl G. Jansky Very Large Array.
Significant U.S. scientific infrastructures supporting this study include ALMA, the Very Large Array, and NASA's Hubble Space Telescope.
Radio measurements for the 1ES 1927+654 study were acquired from the Very Long Baseline Array, the Very Large Array in New Mexico, and the European VLBI Network.
The decadal called on the NSF to begin studies for the Next Generation Very Large Array, a radio observatory with an estimated construction cost of $3,200,000,000 planned to begin late in the decade.
The decadal survey estimated the Next Generation Very Large Array would cost $3,200,000,000 and supported construction beginning late in the decade.
Radio wave images from the Karl G. Jansky Very Large Array observatory revealed a pair of large-scale plasma jets emerging from either side of VV 340a.
The National Science Foundation's Very Large Array radio telescope in New Mexico monitored faint radio emission from SN 2023fyq for about 18 months after the explosion.