(Chair: Paul Plucinsky):
Aims to use the time-invariant, line-rich spectra of the SNRs 1E 0102.2-7219 and N132D to improve the response models of the various instruments (gain, CTI correction, QE, spectral redistribution function, etc) Â and to compare the absolute effective areas of the instruments at the energies of the bright line complexes.
Current members: Andy Beardmore, Sunil Chandra, Konrad Dennerl, Jelle de Plaa, Gulab Dewangan, Adam Foster, Michael Freyberg, Terrance Gaetz, Brian Grefenstette, Frank Haberl, Jelle Kaastra, Xi Long, Kristin Madsen, Eric Miller, Paul Plucinsky, Andy Pollock, Manami Sasaki, Steve Sembay, KP Singh, Martin Stuhlinger, Firoza Sutaria, Hiroya Yamaguchi