Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T20:18:32.187Z Has data issue: false hasContentIssue false
  • English
  • Français

The Monash Spectrograph Simulation Program

Published online by Cambridge University Press:  05 March 2013

S. C. Marsden  and
D. W. Coates
S. C. Marsden
Affiliation:
Department of Physics, Monash University, Clayton, Vic. 3168, Australia
D. W. Coates*
Affiliation:
Department of Physics, Monash University, Clayton, Vic. 3168, Australia
*
[email protected]
Rights & Permissions [Opens in a new window]

Abstract

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 Monash University Physics Department is constructing a spectrograph, to be attached to a 0·46-m Cassegrainian telescope. To help future users of the spectrograph determine the operational capabilities of the spectrograph a PC-based software package was created. This program allows the user to simulate the response of the spectrograph to various stellar types under differing observational constraints. We have estimated the precision of measurements of stellar radial velocities with the spectrograph. The estimates are reasonable but are yet to be compared with real data.

Keywords

instrumentation: spectrographs
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 14 , Issue 3 , 1997 , pp. 274 - 277
Copyright
Copyright © Astronomical Society of Australia 1997

References

Allen, C. W. 1973, Astrophysical Quantities, 3rd edn (London: Athlone Press)Google Scholar
Couch, W. 1989, FORS Users Manual (Epping: Anglo-Australian Observatory)Google Scholar
Coutures, J. L., & Boucharlat, C. 1987, A 2 × 2048 Pixel Bi-linear CCD Array for Spectroscopy (Boulogue: Thomson-CSF)Google Scholar
Dworetsky, M. M., & Jacobs, J. M. 1985, Astronomers Guide to Spectrum Synthesis and Curve of Growth Analysis with UCLA Spectrum Synthesis program (London: University College London)Google Scholar
Etzel, P. B. 1982, The J. E. Ross Stellar Spectrum Synthesis Code: Kludge Documentation (Los Angeles: Astronomy Department UCLA)Google Scholar
Hardie, R. H. 1962, in Astronomical Techniques. Stars and Stellar Systems, Vol. 2, ed. W. A. Hiltner (Univ. Chicago Press), 178 Google Scholar
Innis, J. L. 1986, A study of several late-type very active-chromosphere stars, PhD Thesis, Monash University Google Scholar
Marsden, S. C. 1996, Simulation of the Monash Spectrograph: A study of the radial velocities of cool stars, MSc Thesis, Monash University Google Scholar
Robinson, R. D. 1985, The RGO Spectrograph, 2nd edn (Epping: Anglo-Australian Observatory)Google Scholar
Sadler, E., Harrison, S., & Lee, S. 1991, Anglo-Australian Observatory: Observers Guide, 4th edn (Epping: Anglo-Australian Observatory)Google Scholar
Shortridge, K. 1991, Figaro Release Notes–Version 3.0 (Epping: Anglo-Australian Observatory)Google Scholar
Thévenin, F. 1989, A&A Suppl. Series, 77, 137 Google Scholar
Thévenin, F. 1990, A&A Suppl. Series, 82, 179 Google Scholar
Walker, A. R. 1984, MNRAS, 209, 83 CrossRefGoogle Scholar