Members Eric Miller (chair, Suzaku, Astro-H) Andy Beardmore (Swift) Larry David (Chandra) Tadayasu Dotani (Astro-H) Megan Eckart (Astro-H SXS) Michael Freyberg (eROSITA) Terry Gaetz (Chandra) Catherine Grant (Chandra) Kenji Hamaguchi (Suzaku) Maurice Leutenegger (Astro-H SXS) Herman Marshall (Chandra) Steve O'Dell (Chandra) Paul Plucinsky (Chandra) Steve Sembay (XMM-Newton EPIC) Doug Swartz (Chandra) Masahiro Tsujimoto (Suzaku, Astro-H) Cor de Vries (XMM-Newton RGS) Qazuya Wada (Suzaku)
Topics (with thanks to Herman M., Michael F., and Doug S.)
comparison among instruments and missions
chemical composition
time dependence
spatial dependence (micron to cm scales)
temperature dependence (where is the coldest surface?)
XSPEC contamination model hcnofcol: hcnofcol.tar.gz allows composition to be specified in column densities rather than with respect to H (a la varabs) see the included README file for parameters and installation instructions
This is markup without migration.
h1. Bobobasdf
*This is bold*
Contamination WG Telecon #1 (2014-03-31)