HI obs. of low surface brightness dwarf gal. (Roberts+, 2004)

Details HI obs. of low surface brightness dwarf gal. (Roberts+, 2004) HI obs. of low surface brightness dwarf gal. (Roberts+, 2004)

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..73520478r&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/352/478. Originally published in: 2004MNRAS.352..478R

Physics

Clusters: Galaxy, H I Data, Redshifts

Scientific paper

The optical data for this paper were obtained using the Wide Field Camera (WFC) on the Isaac Newton Telescope, La Palma, Canary Islands as part of the Wide Field Survey, a multicolour data survey covering over 200deg2 of sky. The Millennium Galaxy strip (MGS) data were obtained during four observing runs in 1999 and 2000 and consist of 144 fields running along the celestial equator (full details can be found in Liske et al., 2003, Cat. ). The 305-m Arecibo telescope was initially used to observe a pilot sample of 12 objects from our catalogue of candidate LSB dwarf galaxies in 2003 May and a further 56 objects were observed in 2004 January.
(3 data files).

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