About
ROSAT
ROSAT Home Page ROSAT
Images

next up previous contents index
Next: MPE Notes on the Up: Notes on the Spectral Previous: Notes on the Spectral

For PROS users:

The correspondence between the PROS 34-channel spectra and PI bins is listed in Tab. 3.3.   The PI bins,  256 channels, are 10eV wide, with the low energy given by tex2html_wrap_inline16937 eV (by the inherent nature of proportional counters, this is not an exact relation and should only be considered in a statistical sense). The lower level discriminator is set in ADC channel 7, for the observations before 1991 October, and ADC channel 10-11 for those thereafter. To be conservative, in the 256 channel scheme, for data taken before 1991 October 14 channels 1-8 and channels above tex2html_wrap_inline16939 200 should be ignored. For data taken since 1991 October 14 channels 1-10 and channels above tex2html_wrap_inline16941 should be ignored. The upper limit is a loose one, as the effective area calibration gets gradually worse between 2 - 2.5keV. We do not recommend using data above tex2html_wrap_inline16943 keV at this time. The counts detected in channels 260-370 are due almost entirely to the particle background. PROS will display these events, by specifying the desired range in PI channels.  

 

SASS channel Low energy High energy PI channels Channels recommended
(keV) (keV) (inclusive) For spectral fitting
1 0.07 0.09 7+8 not to be used in any fit
2 0.09 0.11 9+10
3 0.11 0.14 11-13 start here after
4 0.14 0.17 14-16 1991 October 11
5 0.17 0.20 17-19
6 0.20 0.24 20-23
7 0.24 0.28 24-27
8 0.28 0.32 28-31
9 0.32 0.37 32-36
10 0.37 0.42 37-41
11 0.42 0.47 42-46
12 0.47 0.52 47-51
13 0.52 0.58 52-57
14 0.58 0.64 58-63
15 0.64 0.70 64-69
16 0.70 0.77 70-76
17 0.77 0.84 77-83
18 0.84 0.91 84-90
19 0.91 0.99 91-98
20 0.99 1.07 99-106
21 1.07 1.15 107-114
22 1.15 1.23 115-122
23 1.23 1.32 123-131
24 1.32 1.41 132-140
25 1.41 1.50 141-149
26 1.50 1.60 150-159
27 1.60 1.70 160-169
28 1.70 1.80 170-179
29 1.80 1.91 180-190
30 1.91 2.02 191-201
31 2.02 2.13 202-212 Insufficient calibration of
32 2.13 2.24 213-223 eff. area and energy
33 2.24 2.36 224-235 response at energies
34 2.36 2.48 236-247 above 2 keV
Table 3.3:   Relationship between the 34 SASS and PI spectral channels

   


next up previous contents index
Next: MPE Notes on the Up: Notes on the Spectral Previous: Notes on the Spectral

If you have problems/suggestions please send mail to rosat_svc@mpe-garching.mpg.de