The Aao/Ukst Supercosmos H-alpha Survey (SHS)

Mon.Not.Roy.Astron.Soc.362:689-710,2005 The UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory completed a narrow-band H-alpha plus [NII] 6548, 6584A survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide-field photographic sur...

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Main Authors: Parker, Q. A, Phillipps, S, Pierce, M. J, Hartley, M, Hambly, N. C, Read, M. A, MacGillivray, H. T, Tritton, S. B, Cass, C. P, Cannon, R. D, Cohen, M, Drew, J. E, Frew, D. J, Hopewell, E, Mader, S, Malin, D. F, Masheder, M. R. W, Morgan, D. H, Morris, R. A. H, Russeil, D, Russell, K. S, Walker, R. N. F
Format: Journal Article
Language:English
Published: 24-06-2005
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Summary:Mon.Not.Roy.Astron.Soc.362:689-710,2005 The UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory completed a narrow-band H-alpha plus [NII] 6548, 6584A survey of the Southern Galactic Plane and Magellanic Clouds in late 2003. The survey, which was the last UKST wide-field photographic survey, and the only one undertaken in a narrow band, is now an on-line digital data product of the Wide-Field Astronomy Unit of the Royal Observatory Edinburgh (ROE). The survey utilised a high specification, monolithic H-alpha interference band-pass filter of exceptional quality. In conjunction with the fine grained Tech-Pan film as a detector it has produced a survey with a powerful combination of area coverage (4000 square degrees), resolution (~1 arcsecond) and sensitivity (<=5 Rayleighs), reaching a depth for continuum point sources of R~20.5. The main survey consists of 233 individual fields on a grid of centres separated by 4 degrees at declinations below +2 degrees and covers a swathe approximately 20 degrees wide about the Southern Galactic Plane. The original survey films were scanned by the SuperCOSMOS measuring machine at the Royal Observatory, Edinburgh to provide the on-line digital atlas called the SuperCOSMOS H-alpha Survey (SHS). We present the background to the survey, the key survey characteristics, details and examples of the data product, calibration process, comparison with other surveys and a brief description of its potential for scientific exploitation.
DOI:10.48550/arxiv.astro-ph/0506599