Bibcode
Prieto, M. A.; Hasinger, G.; Snowden, S. L.
Referencia bibliográfica
Astronomy and Astrophysics Supplement, v.120, p.187-193
Fecha de publicación:
11
1996
Número de citas
20
Número de citas referidas
19
Descripción
The existence of systematic spectral-fit residuals in ROSAT PSPC
spectra, and their dependence on time, is by now a well established
fact. This paper describes how those residuals may be related to second
order variations of the gain of the PSPC as a function of energy and
time. As a result, the energy scale used for the interpretation of PSPC
spectra can be incorrect producing significant systematic effects, in
particular at energies where the effective area of the instrument
changes rapidly. A monotonic gain decay of ~1% per year is measured at 1
keV. A quantitative description of the PSPC gain-time variation as a
function of energy is provided. The functional dependence of this
variation is found to be well represented by a second order polynomial.