3 datasets were investigated: 
-124Xe with Scraper    (2. Xray calibration parameters needed) 
-124Xe without Scraper (2. Xray calibration parameters needed) 
-118Te with Scraper    (1. Xray calibration parameters needed) 
 
I looked all the 35°, 90° and 145° detector spectra: 
 -For both Xe measurements all 3 detector signal can be evaluated 
 -For Te beam one can see only in the 145° detector spectra the Kalpha and K-REC peaks (with high uncertainty). For the 35° probably the detector was simply not sensitive enough for such low beam intensities. For the 90° case, I am much surprised, the peaks supposed to be there the most prominent of all. In the spectra, I maybe can recognize a peak at ~27,8keV, but this is even in best case only the Kalpha peak. At the range of the expected K-REC (~40keV), there is a bit of increase in the background overlying the peak. This background increase is also in the background spectra. Also probably this twisted cables issue between 90° and 145° didn't help much. I think anyhow, that maybe this must have some noise related origin. I can remember that the cables (despite all of our and Uwe's tries) were not well grounded, the noise level was kind of floating.  
 
In general, I would also remark that we can see some peaks >60keV in the background, but these luckily don't disturb us. 
 
 
To evaluate the Xray spectra I used the following algorithm: 
1, for each type of beams I used the list of event numbers in the next entry (to exclude "bad" events) 
   To get the Kalpha and K-REC and other peaks I used the condition trigger==1 (jet ON) 
   To get the background spectra, I used trigger==2 (Jet OFF). The background spectra is only used to see that there is no underlying peak structure below K-REC. To subtract count, the background histo was NOT in use. 
2, While using a well-suiting number of bins, I plot the JetON and JetOFF histos. 
   By eye I choose the range of the K-REC peak and the range for the background fit on the JetON histo. Ofc range_bckgnd > range_peak. 
   Simultaneously, I check on the JetOFF histo that both, in the fit-range and in the peak-range, there should not be any peak structure visible. 
3, For the fit-range in JetON histo, excluding the peak-range, I fit a linear function, m*x+b. For each bin in the fit-range I subtract m*bin_center+b value from the bin content. After the subtraction I check if I got spectra looking like a single peak sitting on a zero 
   line.  
4, To get the K-REC counts, I sum together all the bin values for each bin of the subtracted histo within the peak-range. For the error calculation, I use Gaussian error prop. The uncertainty of the JetON histo counts = sqrt(counts). Also for the subtraction I make the  
   error like delta(m*bin_center+b)= sqrt(m*bin_center+b) instead using the uncertainty of the fit parameters. This second one wont make much sense, since the slope of the linear fit is usually close to 0 --> the errors grow unrealistically big. 
 
 
Based on the algorithm above I got the following counts: 
-124Xe with Scraper: 
 35°:    174 +/- 15 
 90°:  21299 +/- 150 
 145°:  2104 +/- 52 
 
-124Xe without Scraper: 
 35°:    65 +/- 9 
 90°:  7792 +/- 91 
 145°:  728 +/- 31 
 
-118Te_part1 with Scraper: 
 35°:   - 
 90°:   427 +/- 40 
 145°:  - 
 
-118Te_part2 with Scraper: 
 35°:   - 
 90°:   741 +/- 48 
 145°:  - 
 
-124Xe_lowRate with Scraper: 
 35°:   - 
 90°:   2121 +/- 52 
 145°:  - |