Observation Summary
| OBSID: | 1342257692 |
| Instrument: | PACS |
| AOR label: | cygxn38-PACSredON |
| Proposal: | OT2_tcsenger_1 |
| Target: | cygxn38_sw-1 |
| Actual RA: | 20h 38m 58.88s |
| Actual Dec.: | 42° 22' 20.59'' |
| Purpose: | offSelector |
| Concat.: | 1342257691,1342257692,1342257693,1342257694 |
| OD: | 1319 |
| Start: | 2012-12-23T06:58:42.000000 TAI (1734937122000000) |
| Duration: | 2875.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsRangeSpec |
| Mode: | Mapping, unchopped grating scan |
| Bands: | B2B R1 (prime diffraction orders selected) |
| Sampling: | Nyquist (with spectral dithering if range repetition > 1) |
| Raster lines: | 2 |
| Raster columns: | 2 |
| Raster line step: | 4.5 (arcseconds) |
| Raster point step: | 4.5 (arcseconds) |
| Nod cycles: | 1 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | ReqWaveMin(*) | ReqWaveMax(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | micrometer | | | pF | | |
Range 1 | blue | 2 | B2B | 70.000 | 91.000 | 69.707 | 91.268 | 2 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | - | 139.379 | 182.508 | 2 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.2 |
| SPG pipeline products creation date: | 2017-01-18T08:41:54.049000 TAI (1863420114049000) |
| Mission configuration: | MC_H102ASTR_P70ASTR_S66ASTR_RP |
| Processed to level: | RED: 2.5 BLUE: 2.5 |
| Quality Control: | PASSED |
| Action: | NONE |
Quality comments
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 1342257691