Free Access
Issue
A&A
Volume 368, Number 3, March IV 2001
Page(s) 1123 - 1132
Section Instruments, observational techniques and data processing
DOI https://doi.org/10.1051/0004-6361:20010088
Published online 15 March 2001


A&A 368, 1123-1132 (2001)
DOI: 10.1051/0004-6361:20010088

A radio continuum survey of the southern sky at 1420 MHz

Observations and data reduction
J. C. Testori1, P. Reich2, J. A. Bava1, F. R. Colomb1, E. E. Hurrel1, J. J. Larrarte1, W. Reich2 and A. J. Sanz1

1  Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa (Prov. de Bs.As.), Argentina
2  Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany

(Received 7 November 2000 / Accepted 8 January 2001 )

Abstract
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 $\rm0^h \leq RA \leq 24^h$ for declinations less than $-10\degr$. The sensitivity is about 50 mK $T_{\rm B}$ (full beam brightness) and the angular resolution (HPBW) is $35\farcm4$, which matches the existing northern sky survey at the same frequency.


Key words: methods: observational -- surveys -- Galaxy: general -- radio continuum: general

Offprint request: P. Reich, preich@mpifr-bonn.mpg.de

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© ESO 2001

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