XMM RPS 
Users' Manual
 
 
 
  
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Filling in RGS details
Similar to the EPIC exposures, a few details must be defined for each
RGS exposure. Fig. 14 provides an example for an 
RGS exposure formsheet.
  
Figure 14:
 Screen shot of an RGS exposure form sheet for a 45 ks
exposure of RGS-2 in the recommended mode for standrd spectroscopy.
  | 
 
For RGS the following inputs must be provided: exposure time, exposure 
offset (should normally be 0), RGS unit and RGS modes
.
- RGS modes
 - The descriptions of the RGS modes
 in the UHB and XRPS differ because
of the changes that the modes and their names have undergone with time
(see Tab. 4).
 
Table 4:
 Mapping of RGS mode names
|  UHB name | 
 XRPS name1 | 
| SPECTROSCOPY2 | 
SPECTROSCOPY3 | 
|  SPECTROSCOPY2 | 
 SPECTR+Q4 | 
| SPECTROSCOPY2 | 
HER5 | 
| SPECTROSCOPY2 | 
HER+SES6 | 
| SPECTROSCOPY2 | 
HER+SER7 | 
|  HIGH TIME RESOLUTION (HTR) | 
 HTR MULTIPLE8 | 
|  HIGH TIME RESOLUTION (HTR) | 
 HTR SINGLE CCD9 | 
 
Notes to Table 4:
1) During AO-1 only the highlighted modes are recommended for use. 
2) The SPECTROSCOPY mode comes in 5 different flavours (see text for
details). 
3) Not recommended for use, no Q calibration data transmitted 
   with the science data. 
4) Default and recommended SPECTROSCOPY mode. Q calibration
   data are telemetered interleaved with the science data to monitor
   the optical CCD loading. 
5) HIGH EVENT RATE spectroscopy mode. Reduction of data rate by
   onboard application of an event threshold. No Q data are 
   transmitted. Not recommended for use in AO-1. 
6) HER + Single Event Reconstruction; only single pixel events are
telemetered. Not recommended for use in AO-1. 
7) HER + Split Event Reconstruction. Split events are reconstructed
onboard before transmission to ground. Not recommended for use in 
   AO-1. 
8) Readout of all 9 CCDs. 
9) Readout of only a single CCD.
The users' choice for RGS is between ``SPECTR+Q'' and ``HTR SINGLE CCD'' 
or ``HTR MULTIPLE''. SPECTROSCOPY without Q data (i.e., Q memory 
calibration data based on which the optical loading of the RGS CCDs
is monitored) is not recommended, because then the optical loading of 
the CCD chips cannot be calibrated properly offline. Use of the other 
configurations of the spectroscopy mode (HER, HER+SER, HER+SES) reduces 
the instrument telemetry by reducing the level of detail to be transmitted 
per event. HER applies an onboard event threshold; onboard split event 
reconstruction (SER) further reduces the telemetry rate; the highest 
data reduction in a spectroscopy mode is reached with HER plus single 
event selection (SES). Use of these options is not suggested, unless 
there is concern that the instrument telemetry is likely to exceed the 
allocated limit. This should then be stated clearly in the scientific 
justification. When the telemetry rate is exceeded in the SPECTR+Q mode, 
the first alternate choice should be HER observations. The recommended 
modes are highlighted in Tab. 4. Note that there is 
an additional page which must be filled out in case special observation 
details are required (§ 5.3.3.4).
 - Exposure offset
 - Should be 0 again in order to avoid times during which the instrument
is idle.
 - RGS unit
 - As in the case of EPIC MOS, there are also two RGS units. When first 
entering the RGS exposure form sheet the RGS unit is a selectable 
parameter. When re-entering the page again later (after successful 
committal of the input to memory), this parameter is fixed. Exposures 
must be defined for both RGS units independently.  It is not possible
to copy an RGS-1 exposure for use with RGS-2.
 
 
 
 
  
 Next: Filling in RGS exposure
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European Space Agency - XMM Science Operations Centre