... PSPC

Based on observations made with the ROSAT satellite.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... RX J1856-37

A two-blackbody model for RXJ 1856-27 and TMAP spectra for HZ43 and Sirius B. For the latter see http://astro.uni-tuebingen.de/~rauch/TMAP/UserGuide/UserGuide.html

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... matrix

The nominal detector response matrices, DRMPSPC-AO1 and DRMPSPC, the effective areas of both PSPCs, and the correction vectors drived here, $c_{\rm AO1}(x)$ and c(x), are available via http://www.mpe.mpg.de/xray/wave/rosat/doc/calibration/index.php
We use the nominal effective areas of PSPC C and PSPC B as given by effarea-pspcc and effarea-pspcb except for a minor correction that more accurately represents the structure of the carbon K-edge at 43.6 Å (Freyberg, private communication).

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.