On Apr 25, 2011, at 11:18 PM, Fabien Grisé wrote: > But, what I would like to get now is the unabsorbed data fluxes with > their errors. And I have not been able to figure out how to export > those ... I guess I have missed something obvious. Unabsorbed data fluxes is not something we normally do in X-ray astronomy. (Yeah, I know, optical guys do it all the time... Crazy!) Best I can suggest is get the model values with and without absorption, take the ratio, and multiply the data flux values (and their errors) by that ratio. Not perfect (it ignores the error in the N_h), but it should work. -Mike ---- 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 Apr 25 2011 - 23:25:41 EDT
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