This paper includes data taken at the Mount John University Observatory of the University of Canterbury (New Zealand), the McDonald Observatory of the University of Texas at Austin (Texas, USA) and the European Southern Observatory at La Silla (Chile).
Spectroscopic pulsational frequency identification and mode determination of γ Doradus star HD 12901†
Article first published online: 20 NOV 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 427, Issue 3, pages 2512–2522, 11 December 2012
How to Cite
Brunsden, E., Pollard, K. R., Cottrell, P. L., Wright, D. J. and De Cat, P. (2012), Spectroscopic pulsational frequency identification and mode determination of γ Doradus star HD 12901. Monthly Notices of the Royal Astronomical Society, 427: 2512–2522. doi: 10.1111/j.1365-2966.2012.22125.x
- Issue published online: 20 NOV 2012
- Article first published online: 20 NOV 2012
- Manuscript Accepted: 13 SEP 2012
- Manuscript Received: 12 SEP 2012
- Royal Society of New Zealand
Disclaimer: Supplementary materials have been peer-reviewed but not copyedited.
|mnr_22125_sm_data.zip||249K||Data file. The line profile data including Modified Julian Date, velocity (on a relative scale) and the intensity at each of the 120 velocity sampling points for each profile. Line 1 is the axis scale, lines 2–478 are MJUO observations, lines 479–526 are La Silla observations and lines 527–586 are McDonald observations.|
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