Observation Summary
| OBSID: | 1342210190 |
| Instrument: | PACS |
| AOR label: | PACS setting 2 - Vela IRS 19 |
| Proposal: | KPGT_evandish_1 |
| Target: | Vela IRS 19 |
| Actual RA: | 8h 48m 48.36s |
| Actual Dec.: | -43° 32' 27.63'' |
| Redshift: | 4.5 (rad. vel. km/s) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 552 |
| Start: | 2010-11-16T22:42:09.000000 TAI (1668638529000000) |
| Duration: | 1987.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsLineSpec |
| Mode: | Pointed, Chop/Nod |
| Bands: | B3A R1 (prime diffraction orders selected) |
| Is bright: | NO (default range mode) |
| Chopper: | large throw |
| Nod cycles: | 1 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | Wave(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | | | pF | | |
[O I] | blue | 2 | B3A | 63.185 | 62.939 | 63.445 | 1 | 1 | 0.14 | No | prime |
- | red | 102 | R1 | - | 188.787 | 190.321 | 1 | 1 | 0.14 | No | parallel |
[O I] | red | 104 | R1 | 145.528 | 144.393 | 146.795 | 1 | 1 | 0.14 | No | prime |
- | blue | 4 | B2A | - | 72.208 | 73.400 | 1 | - | - | Yes, fully | parallel |
CO 24-23 | red | 105, 106 | R1 | 108.765 | 106.789 | 110.227 | 1 | 1 | 0.14 | No | prime |
- | blue | 5 | B2A | - | 53.745 | 55.120 | 1 | 1 | 0.14 | No | parallel |
H2O 221-110 | red | 105 | R1 | 108.075 | 106.789 | 110.227 | 1 | 1 | 0.14 | No | prime |
- | blue | 5 | B2A | - | 53.745 | 55.120 | 1 | 1 | 0.14 | No | parallel |
CO 14-13 | red | 103 | R1 | 186.002 | 185.110 | 186.941 | 1 | 1 | 0.14 | No | prime |
- | blue | 3 | B3A | - | 61.715 | 62.319 | 1 | 1 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-24T09:03:57.131000 TAI (1848042237131000) |
| Mission configuration: | MC_H60ASTR_P58ASTR_S60ASTR_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 1.93" 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.