| OBSID: | 1342244460 |
| Instrument: | PACS |
| AOR label: | PSpecR-SerSMM10-B2A |
| Proposal: | GT1_rvavrek_1 |
| Target: | SerSMM10 |
| Actual RA: | 18h 29m 52.12s |
| Actual Dec.: | 1° 15' 47.6'' |
| Purpose: | offSelector |
| Concat.: | 1342244458,1342244459,1342244460,1342244461,1342244462,1342244463,1342244464,1342244465,1342244466,1342244467,1342244468,1342244469 |
| OD: | 1068 |
| Start: | 2012-04-16T13:52:05.000000 TAI (1713275525000000) |
| Duration: | 1329.0 seconds (incl. spacecraft on-target slew time) |
| AOT: | PacsRangeSpec |
| Mode: | Pointed, unchopped grating scan |
| Bands: | B2A R1 (prime diffraction orders selected) |
| Sampling: | Nyquist (with spectral dithering if range repetition > 1) |
| Nod cycles: | 1 |
| Name(*) | Camera | ID | Band(*) | ReqWaveMin(*) | ReqWaveMax(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel | micrometer | micrometer | micrometer | micrometer | pF | SED B2A | red | 102 | R1 | 102.000 | 146.000 | 101.472 | 146.680 | 4 | 2 | 0.14 | No | prime | - | blue | 2 | B2A | - | - | 50.655 | 73.342 | 4 | 2 | 0.14 | Yes, partly | parallel |
|---|
| SPG pipeline version: | SPG v14.2.2 |
| SPG pipeline products creation date: | 2017-01-18T08:37:02.308000 TAI (1863419822308000) |
| Mission configuration: | MC_H100ASTR_P69ASTR_S66ASTR_RP |
| Processed to level: | RED: 2.5 BLUE: 2.5 |
| Quality Control: | PASSED |
| Action: | NONE |
Normally, for this observation the background spectrum is subtracted using its related off-source observation, and the results placed in Level 2.5. However, due to an oversight this was not done in SP 14.0. You can use a Useful script in HIPE to do this instead. The problem will be fixed in the 14.2 SPG products. On source observation in an unchopped range-scan pair; matched with the off-source observation 1342244458