If we knew all the answers to this question, we would all be
unemployed!
Tahir
On Wed, 13 Jun 2001, Belinda Wilkes wrote:
>
> From: Ryan Foley <rfoley@draco.astro.lsa.umich.edu>
> To: chandra-users@head-cfa.harvard.edu
> Subject: Models for fitting spectral data
> Message-ID: <Pine.SOL.4.10.10106102219100.23672-100000@draco.astro.lsa.umich.ed
> u>
> MIME-Version: 1.0
> Content-Type: TEXT/PLAIN; charset=US-ASCII
>
> I was wondering what models people were using to fit different spectrums.
> The threads seem to use POW and XSWABS which seem to work well for
> quasars, but for clusters of stars these don't work well. Can anyone
> suggest which model to use in a particular situation (ie for quasars, use
> POW and XSWABS, for X use Y and Z, ...)?
>
> Thanks,
> Ryan Foley
>
>
> ------------------------------------------------------------------------
> Dr. Belinda Wilkes Tel : (617) - 495 - 7268
> Harvard/Smithsonian email: belinda@cfa.harvard.edu
> Center for Astrophysics fax : (617) - 495 - 7356
> 60 Garden Street Assistant Director
> Cambridge MA 02138 Chandra X-ray Center (CXC)
> ------------------------------------------------------------------------
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