| OBSID: | 1342206862 |
| Instrument: | PACS |
| AOR label: | KPGT_rguesten_1-CND_OI63_OI145_NII122_pacs_re6 |
| Proposal: | KPGT_rguesten_1 |
| Target: | PACS_reference |
| Actual RA: | 17h 44m 33.48s |
| Actual Dec.: | -28° 52' 8.94'' |
| Purpose: | Undefined |
| Concat.: | 1342206852,1342206853,1342206854,1342206855,1342206856,1342206857,1342206858,1342206859,1342206860,1342206861,1342206862,1342206863 |
| OD: | 523 |
| Start: | 2010-10-18T22:34:01.000000 TAI (1666132441000000) |
| Duration: | 257.0 seconds (incl. spacecraft on-target slew time) |
| AOT: | PacsRangeSpec |
| Mode: | Pointed, unchopped grating scan |
| Bands: | B3A R1 (prime diffraction orders selected) |
| Sampling: | High (default spectral mapping) |
| Nod cycles: | 1 |
| Name(*) | Camera | ID | Band(*) | ReqWaveMin(*) | ReqWaveMax(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel | micrometer | micrometer | micrometer | micrometer | pF | OI 63 | blue | 2 | B3A | 63.040 | 63.320 | 62.930 | 63.436 | 1 | 2 | 0.14 | No | prime | - | red | 102 | R1 | - | - | 188.760 | 190.294 | 1 | 2 | 0.14 | No | parallel | NII | red | 104 | R1 | 121.600 | 122.200 | 121.139 | 122.837 | 1 | 2 | 0.14 | No | prime | - | blue | 4 | B2A | - | - | 60.585 | 61.425 | 1 | 2 | 0.14 | No | parallel | OI 145 | red | 103 | R1 | 145.150 | 145.890 | 144.720 | 146.429 | 1 | 2 | 0.14 | No | prime | - | blue | 3 | B2A | - | - | 72.371 | 73.216 | 1 | - | - | Yes, fully | parallel |
|---|
| SPG pipeline version: | SPG v14.2.2 |
| SPG pipeline products creation date: | 2017-01-17T12:45:38.789000 TAI (1863348338789000) |
| Mission configuration: | MC_H58ASTR_P55ASTR_S59ASTR_RP |
| Processed to level: | RED: 2.0 BLUE: 2.0 |
| Quality Control: | PASSED |
| Action: | NONE |
Off source observation in unchopped range-scan pairs; matched with the on-source observations 1342206861, 1342206863 The offset between the central spaxel and the requested sky coordinates is 2.90" in the dispersion direction. 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.