Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..135w&link_type=abstract
Communications in Astroseismology, Vol. 150, p.135
Astronomy and Astrophysics
Astronomy
2
Scientific paper
At the University of Canterbury we have been developing a set of tools for the analysis of spectra of varying types of non-radially pulsating objects. This set currently includes: calculation of the moments, calculations of the phase across the profile as well as basic binary profile fitting for determination of orbital characteristics and projected rotational velocity (v sin i) measurement. Recently the ability to calculate cross-correlation profiles using either specified or synthesized line lists has been added, all implemented in MATLAB. A number of observations of γ Doradus candidates is currently being used to test these tools. For information on our observing facilities see Pollard et al. (2007).
Cottrell Peter L.
Pollard Karen R.
Wright Douglas J.
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