An XSPEC for all wavelengths

Details An XSPEC for all wavelengths An XSPEC for all wavelengths

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.0905a&link_type=abstract

American Astronomical Society, HEAD meeting #11, #9.05; Bulletin of the American Astronomical Society, Vol. 41, p.668

Astronomy and Astrophysics

Astronomy

Scientific paper

This is primarily an appeal for help. The most important part of XSPEC is the model library which has provided a way for theorists to make their models available to observers and observers to be sure they are all using the same model when they do comparisons. I would like to extend these benefits beyond the high-energy regime. This will require a few internal changes to XSPEC but the major effort is in extending the model library. I hereby solicit suggestions for useful models, especially those for which public-domain code is available.

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