[vsnet-alert 10925] Re: re FWD ATEL 1892

qso at Safe-mail.net qso at Safe-mail.net
Wed Jan 7 05:25:33 JST 2009


> Ok, Well thanks a lot for clarifying all the conditions and assumptions under which this transformation should be good. I should add that when doing calibrations, it is important to include a sufficient range of different stars and observers/equipment to make sure you are acounting for many of the important variables, such as: Filter charcteristics, detector responses, optical system characteristics(especially coatings for such a wide range in wavelengths) Source emission characteristics, interstellar and atmospheric absorption differences between 0.5, 1.2 and 2.5u... etc.<

I said it was unpublished and unpeer reviewed, no one needs to do anything with it.

Cheers

John


More information about the vsnet-alert mailing list