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A radio continuum survey of the southern sky at 1420 MHz. Observations and data reduction

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arxiv astro-ph/0101322 v1 pith:LTTI5WTQ submitted 2001-01-18 astro-ph

J.C. Testori (1) , P. Reich (2) , J.A. Bava (1) , F. R. Colomb (1) , E.E. Hurrel (1) , J.J. Larrarte (1) , W. Reich (2) , A.J. Sanz (1) ((1) Instituto Argentino de Radioastronomia
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Argentina (2) MPI fuer Radioastronomie Bonn Germany)
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keywords surveycontinuumfrequencyobservationsradioreductionabsolutelyangular
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We describe the equipment, observational method and reduction procedure of an absolutely calibrated radio continuum survey of the South Celestial Hemisphere at a frequency of 1420 MHz. These observations cover the area 0h < R.A. < 24h for declinations less than -10 degree. The sensitivity is about 50 mK T_B (full beam brightness) and the angular resolution (HPBW) is 35.4', which matches the existing northern sky survey at the same frequency.

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Cited by 2 Pith papers

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  2. Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions

    hep-ph 2026-01 conditional novelty 5.0 of 10

    Galactic synchrotron emissions above 20 MHz can set tighter upper limits on the abundance of primordial black holes with masses above 10^16 grams than previous cosmic-ray electron data.

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