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Investigations of CP and Normal Stars with Coadded Dominion Astrophysical Observatory Spectrograms
Published online by Cambridge University Press: 12 April 2016
Abstract
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We describe the procedures developed at the Dominion Astrophysical Observatory to coadd high dispersion coude spectrograms and thus increase the signal-to-noise ratio in photographic data. These techniques can yield low noise spectra over a considerable wavelength range. Preliminary results of the analyses of such coadditions are shown to demonstrate the power of these procedures.
- Type
- Section II - Systematics, Photometry
- Information
- Copyright
- Copyright © Reidel 1986
References
Bevington, P.R.
1969, Data Reduction and Error Analysis for the Physical Sciences (McGraw-Hill: New York)Google Scholar
Brenner, N.M.
1970, “FOURT” available COSMIC/SHARE, Univ. of Georgia, Barrow Hall, Athens, Georgia
Google Scholar
Fletcher, J.M., Harmer, C.F.W., and Harmer, D.L.
1980, Pub. Dom. Astrophys. Obs.
15, 405
Google Scholar
Hill, G., Ramsden, D., Fisher, W.A., and Morris, S.C.
1982, Pub. Dom. Astrophys. Obs.
16, 11
Google Scholar
Slettebak, A., Collins, G.W., Boyce, P.B., White, N.M., and Parkinson, T.C.
1975, Astrophys. J. Suppl. 29, 137
Google Scholar