Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-12T08:53:23.807Z Has data issue: false hasContentIssue false

Colour Equations for Techpan Films

Published online by Cambridge University Press:  25 May 2016

D.H. Morgan
Affiliation:
Royal Observatory Edinburgh
Q.A. Parker
Affiliation:
Anglo-Australian Observatory

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The UK 1.2m Schmidt Telescope (UKST) at Siding Spring Observatory in Australia has been routinely using panchromatic Tech-Pan emulsion on film as a detector since 1992. Details of how the telescope was adapted to take film and how hypersensitization techniques have been modified for film have been described by Parker (1992). The film has a much finer grain than its equivalent spectroscopic emulsion on glass (IIIa-F) and consequently records images typically one magnitude fainter than IIIa-F when properly hypersensitized. The improved depth, resolution and low noise also permit better differentiation between stars and galaxies (see Parker et al. 1994). Consequently Tech-Pan film has become one of the most useful and commonly used emulsions at the UKST for a variety of passbands and may in time be used for a full or partial sky survey.

Type
Part 7. Data Processing Techniques
Copyright
Copyright © Kluwer 1998 

References

Blair, M. and Gilmore, G. (1982) Publ. Astron. soc. Pacific, 94, 742.Google Scholar
Miller, L., Cormack, W., Paterson, M., Beard, S. and Lawrence, L., (1995) In Digitised optical Sky Surveys, Astr Sp Sci Lib, 174, p. 133, eds MacGillivray, H.T. & Thomson, E.B., Kluwer.Google Scholar
Menzies, J.W., Cousins, A.W.J., Banfield, R.M. and Laing, J.D. (1989) SAAO Circ, No 13, p1.Google Scholar
Parker, Q.A. (1992) Kodak Tech Pan Estar-based emulsion, AAO Internal Report.Google Scholar
Parker, Q.A., Morgan, D.H. and Phillipps, S. (1993) In IAU Commission 9 Working Group on Wide-Field Imaging Newsletter, No 3, p60.Google Scholar
Parker, Q.A., Phillipps, S., Morgan, D.H., Malin, D.F., Russell, K.S., Hartley, M. and Savage, A. (1994) In Astronomy from Wide-Field Imaging, Proc. IAU Symp. No 161, p. 129, eds MacGillivray, H.T. et al., Kluwer.CrossRefGoogle Scholar