Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...418..519p&link_type=abstract
Astrophysical Journal v.418, p.519
Astronomy and Astrophysics
Astronomy
85
Artificial Satellites, Space Probes, Instrumentation: Spectrographs, X-Rays: General
Scientific paper
In order to permit quantitative studies of the cosmic diffuse X-ray background (DXRB) and of extended X-ray sources, we present updated calibrations of the particle-induced background of the Position Sensitive Proportional Counters (PSPCs) on board the Röntgen Satellite (ROSAT). We present new parameterizations of the temporal, spectral, and spatial distributions of the particle-induced events following closely the analysis discussed in Snowden et al. (1992). The ROSAT Guest Observer (GO) may find a step-by-step method for applying these parameterizations to a GO observation in § 3.4. Except for a variable contamination which is present in channels ≤ 18 and a change in our understanding of the externally produced components, the current parameterizations are quite similar to the previous results. We have used the spectral information available on the variable contamination to formulate a method for determining the level of this contamination in a given observation. The PSPC rejection efficiency for particle background events in the pulse-height range 18 ≤ CH ≤ 249 is 99.90%, with a typical count rate of 4 × 10-6 counts s-1 arcmin-2 keV-1. During typical conditions, the count rate of residual events is well correlated with the Master Veto count rate. The spectrum in the pulse-height range 18 ≤ CH ≤ 249 is well described by a power law, a flat component, and an Al Kα line at 1.5 keV. The spatial distribution of counts with pulse heights ≥ 18 is uniform over the field of view except for a small radial gradient and shadowing of the Al Kα line and part of the flat continuum by the window support structure. During an astronomical observation in low-gain mode (after 1991 October 11), the particle background can also be monitored by the count rate in channels 260 ≤ CH ≤ 370, since in most cases all these events are produced by particles. We have used a 54 ks observation of the Ursa Major region to verify the accuracy of our model. We have also presented a summary of the particle background parameterizations valid for four different time epochs spanning the entire ROSAT mission, including a recalibration of the data presented previously.
Briel Ulrich G.
Hasinger Guenter
Pfeffermann Elmar
Plucinsky Paul P.
Snowden Steve L.
No associations
LandOfFree
An Updated Calibration of the ROSAT PSPC Particle Background for the Analysis of Diffuse and Extended Sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with An Updated Calibration of the ROSAT PSPC Particle Background for the Analysis of Diffuse and Extended Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An Updated Calibration of the ROSAT PSPC Particle Background for the Analysis of Diffuse and Extended Sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-809075