WSRT survey of Cygnus OB2 (Setia Gunawan+, 2003)

Details WSRT survey of Cygnus OB2 (Setia Gunawan+, 2003) WSRT survey of Cygnus OB2 (Setia Gunawan+, 2003)

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..21490123s&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/149/123. Originally published in: 2003ApJS..149..123S

Physics

Associations: Stellar, Radio Sources

Scientific paper

The Cygnus region is too large to be imaged with a single pointing of the 25m dishes of the WSRT. The half-power beamwidths (HPBW) of the WSRT at 350 and 1400MHz are about 2.4{deg} and 0.6{deg}, respectively. Therefore, we used a mosaicking technique at both frequencies. The 350MHz observations were taken in 1994 as part of a larger survey of the Galactic plane in the Cygnus area (Vashist & de Bruyn, unpublished); only a small part of it is used in this study.
(2 data files).

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