Hi, > This is because the voigt() model has changed, apparently. > This is a backward compatibility problem. Is the old voigt model still around? > Also, when did voigt() change? Consider the file Changes.txt from the ISIS sources: # Changes since 1.4.5 (released Mar 2007) # 9. Voigt profile norm now includes factor 1/(sqrt(PI)*Doppler_width) # (set Isis_Voigt_Is_Normalized=0 to restore the previous behavior > What are the formulae to convert between old and new voigt parameters? Before, ISIS's voigt() implemented the Voigt-function H(a,v) rather than the normalized (\int \Phi(\nu) d\nu = 1) Voigt-profile Phi(\nu) = \frac{1}{sqrt{\pi}\Delta\nu_D} \times H(\frac{\nu-\nu_0}{\Delta\nu_D}, \frac{\Gamma}{4\pi\Delta\nu_D}) The parameter voigt().norm was thus somehow normalized to the Doppler-broadening \Delta\nu_D = (thermal velocity)/c \times \nu_0 and thus dependent on the position \nu_0 of the line. > Also, is there a way to tell what version of ISIS I'm running at run-time This is contained in the variable _isis_version . Cheers, Manfred -- Manfred Hanke Manfred.Hanke(at)sternwarte.uni-erlangen.de Dr. Karl Remeis-Sternwarte, Universität Erlangen-Nürnberg Sternwartstraße 7, 96049 Bamberg Tel. (0951) 95222-34 Fax (0951) 95222-22 www: http://pulsar.sternwarte.uni-erlangen.de/hanke -- ---- You received this message because you are subscribed to the isis-users list. To unsubscribe, send a message to isis-users-request_at_email.domain.hiddenwith the first line of the message as: unsubscribeReceived on Mon Oct 29 2007 - 12:46:43 EDT
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