Very Low Frequency Continuum Survey of the Northern Sky

Details Very Low Frequency Continuum Survey of the Northern Sky Very Low Frequency Continuum Survey of the Northern Sky

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..12e..45v&link_type=abstract

Long Wavelength Astrophysics, 26th meeting of the IAU, Joint Discussion 12, 21 August 2006, Prague, Czech Republic, JD12, #45

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Ukrainian T-shape Radio telescope (UTR-2) has been used to make a multifrequency continuum survey of the large part of the Northern sky. Here are present maps of more 8000 square degree region of sky. The region covered is 0^ h < R.A. < 21^h, +29° < Dec. < + 55°. The measurements are fulfilled with the UTR-2 at five frequencies ranging from 12.6 to 25 MHz. The angular resolution of the survey is the better on these frequencies and varied from 65'′to 28'′ at the zenith direction correspondently. Fluctuation sensitivity at frequencies 25-12.6 MHz is within the range 1.36 - 7.27kK on the Galaxy plane and 0.94 - 5.58 kK away from the Galaxy plane. The maps include a portion of the Galactic plane, the high latitude region of the minimum radio sky brightness of the Galaxy emission, SNRs, H II regions and point sources.

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