Observation Summary
| OBSID: | 1342268742 |
| Instrument: | PACS |
| AOR label: | iras05328-6827_pacs_1 |
| Proposal: | OT1_joliveir_1 |
| Target: | IRAS05328-6827 |
| Actual RA: | 5h 32m 38.99s |
| Actual Dec.: | -68° 25' 23.15'' |
| Redshift: | 270.0 (rad. vel. km/s) |
| Purpose: | --- |
| Concat.: | 1342268742,1342268743 |
| OD: | 1416 |
| Start: | 2013-03-30T07:14:36.000000 TAI (1743318876000000) |
| Duration: | 2039.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsLineSpec |
| Mode: | Pointed, unchopped grating scan |
| Bands: | B2B R1 (prime diffraction orders selected) |
| Is bright: | NO (default range mode) |
| Nod cycles: | 1 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | Wave(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | | | pF | | |
OH 11101-22-102 | blue | 4 | B2B | 79.251 | 78.593 | 79.958 | 2 | 4 | 0.14 | No | prime |
- | red | 104 | R1 | - | 157.153 | 159.889 | 2 | 4 | 0.14 | No | parallel |
OH | blue | 3 | B2B | 84.676 | 84.057 | 85.336 | 2 | 4 | 0.14 | No | prime |
- | red | 103 | R1 | - | 168.085 | 170.646 | 2 | 4 | 0.14 | No | parallel |
O III 3P1-3P0 | blue | 2 | B2B | 88.436 | 87.849 | 89.060 | 1 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | 175.670 | 178.093 | 1 | 2 | 0.14 | No | parallel |
H2O 221-110 | red | 105 | R1 | 108.167 | 106.276 | 110.222 | 1 | 2 | 0.14 | No | prime |
- | blue | 5 | B2B | - | 53.126 | 55.133 | 1 | - | - | Yes, fully | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-28T17:59:14.134000 TAI (1848419954134000) |
| Mission configuration: | MC_H102ASTR_P70ASTR_S66ASTR_RP |
| Processed to level: | RED: 2.0 BLUE: 2.0 |
| Quality Control: | PASSED |
| Action: | NONE |
Quality comments
The offset between the central spaxel and the requested sky coordinates is 2.10" 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.