Observation Summary

OBSID:1342218571
Instrument:PACS
AOR label:HEXOS-orikl-pacsmap-red_reference
Proposal:KPGT_ebergin_1
Target:Orion KL-MAP-OFF
Actual RA:5h 36m 41.27s
Actual Dec.:-5° 22' 32.87''
Purpose:Undefined
Concat.:1342218571,1342218572
OD:697
Start:2011-04-11T17:10:58.000000 TAI (1681233058000000)
Duration:1220.0 seconds (incl. spacecraft on-target slew time)

AOT and instrument configuration:

AOT:PacsRangeSpec
Mode:Pointed, unchopped grating scan
Bands:B2B R1 (prime diffraction orders selected)
Sampling:Nyquist (with spectral dithering if range repetition > 1)
Nod cycles:1

Observation block summary

Name(*)CameraIDBand(*)ReqWaveMin(*)ReqWaveMax(*)WaveMinWaveMaxRepetitions(*)ActualRepCapacitanceOutOfBandChannel
micrometermicrometermicrometermicrometerpF
Range 1red102R1109.000188.000108.312188.377220.14Noprime
-blue2B2B--54.14694.206220.14Yes, partlyparallel
(*) = requested in HSPOT

System configuration summary

SPG pipeline version:SPG v14.2.2
SPG pipeline products creation date:2017-01-17T12:44:46.784000 TAI (1863348286784000)
Mission configuration:MC_H72ASTR_P60ASTR_S61ASTR_AO
Processed to level:RED: 2.0 BLUE: 2.0
Quality Control:PASSED
Action:NONE

Quality comments

Off source observation in an unchopped range-scan pair; matched with the on-source observation 1342218572
The offset between the central spaxel and the requested sky coordinates is  4.32" and the offset is  3.91" in the dispersion direction.
These have two consequences:
  1) For point sources offset from the central spaxel by >~4", the point-source correction applied to the spectra in the
point-source table (products which have "hpsspec" in their filenames) will become less and less applicable.
Alternative corrections tasks are provided in HIPE. See the advice in the "Product Decision Trees", which can be found on 
https://www.cosmos.esa.int/web/herschel/legacy-documentation-pacs
  2) If the target is point-like and is offset from the centre of a spaxel in the dispersion direction, the spectral line 
profiles will develop a skew. This skewed Gaussian profile becomes more extreme as the offset increases. 
Be aware that this can be confused with real velocity structure.
This will affect spectra from a single spaxel of a rebinned cube (products with filenames "..hps3dr[r|b].."), 
and combined spaxel-spectra, i.e. added rebinned cube spaxels, or single spaxels from an interpolated or projected cube 
(products with filenames "..hps3di[r|b].." or "..hps3dp[r|b].."). See the "PACS Handbook" for more information.