Volume 368, Number 3, March IV 2001
|Page(s)||1123 - 1132|
|Section||Numerical methods and codes|
|Published online||15 March 2001|
A radio continuum survey of the southern sky at 1420 MHz
Observations and data reduction
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
Corresponding author: P. Reich, firstname.lastname@example.org
Accepted: 8 January 2001
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 for declinations less than . The sensitivity is about 50 mK TB (full beam brightness) and the angular resolution (HPBW) is , which matches the existing northern sky survey at the same frequency.
Key words: methods: observational / surveys / Galaxy: general / radio continuum: general
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.