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Contamination
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working
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group
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- Members
Eric Miller (chair,
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- Suzaku,
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- Astro-H)
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Andy
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- Beardmore
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- (Swift)
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Larry
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- David
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- (Chandra)
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Tadayasu
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- Dotani (Astro-H)
Megan Eckart (Astro-H SXS)
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Michael
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- Freyberg
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- (eROSITA)
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Terry
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- Gaetz
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- (Chandra)
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Catherine
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- Grant
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- (Chandra)
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Kenji
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- Hamaguchi
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- (Suzaku)
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Maurice Leutenegger (Astro-H SXS)
Herman Marshall (Chandra)
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Steve
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- O'Dell
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- (Chandra)
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Paul
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- Plucinsky (Chandra)
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Steve
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- Sembay
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- (XMM-Newton
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- EPIC)
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Doug
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- Swartz
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- (Chandra)
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Masahiro
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- Tsujimoto
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- (Suzaku,
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- Astro-H)
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Cor
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- de
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- Vries
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- (XMM-Newton
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- RGS)
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Qazuya
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- Wada
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- (Suzaku)
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- Topics
(with
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- thanks
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- to
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- Herman
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- M.,
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- Michael
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- F.,
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- and
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- Doug
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- S.)
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- comparison
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- among
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- instruments
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- and
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- missions
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- chemical
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- composition
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- time
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- dependence
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- spatial
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- dependence
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- (micron
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- to
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- cm
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- scales)
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- temperature
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- dependence
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- (where
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- is
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- the
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- coldest
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- surface?)
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- environmental
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- dependence
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- (orbit)
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- mitigation
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- for
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- current
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- instruments
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- celestial
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- monitoring
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- targets
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- effects
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- on
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- calibration
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- and
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- science
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- results
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- "bake-out"
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- procedures
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- mitigation
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- for
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- future
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- instruments
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- design
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- (cold
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- traps,
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- contamination
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- blocking
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- filters)
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- procurement
- ground procedures
- ground testing and calibration
- on-orbit
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- monitoring
- Meetings
- Reference Materials
- 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
- XSPEC contamination model hcnofcol: hcnofcol.tar.gz