Statistics – Computation
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.4406n&link_type=abstract
American Astronomical Society, 200th AAS Meeting, #44.06; Bulletin of the American Astronomical Society, Vol. 34, p.713
Statistics
Computation
Scientific paper
Recent advances in observational and computational techniques have brought about a renaissance in low frequency radio astronomy. The NRL-NRAO 74 and 330 MHz VLA systems have enabled the first high-resolution (25 and 6 arcseconds, respectively), high-dynamic range imaging at these frequencies. Similar images at complimentary frequencies are also now starting to emerge from the GMRT. We present multi-configuration VLA images of the Galactic center. These images are being used to: Identify new radio transients toward the Galactic center (Hyman et al. 2002, AJ, 123, 1497); Probe the radial distribution of Galactic cosmic rays toward the Galactic center; Search for new non-thermal filaments; Search for Galactic center pulsars; and Constrain HII region physical parameters Basic research in radio astronomy at the Naval Research Laboratory is supported by the Office of Naval Research.
Brogan Crystal
Denn G.
Duric Neb
Hyman Scott
Kassim Namir E.
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