Observation Summary
| OBSID: | 1342214638 |
| Instrument: | PACS |
| AOR label: | PSpecL-lmc-n11A-CEA-CIIOIII |
| Proposal: | KPGT_esturm_1 |
| Target: | lmc n11 A-1-1 |
| Actual RA: | 4h 57m 16.4s |
| Actual Dec.: | -66° 23' 25.61'' |
| Redshift: | 0.0 (z) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 649 |
| Start: | 2011-02-22T09:59:07.000000 TAI (1677059947000000) |
| Duration: | 844.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsLineSpec |
| Mode: | Pointed, unchopped grating scan |
| Bands: | B3A R1 (prime diffraction orders selected) |
| Is bright: | YES (shortened range mode) |
| Nod cycles: | 1 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | Wave(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | | | pF | | |
CII C+ | red | 103 | R1 | 157.741 | 156.153 | 159.406 | 1 | 2 | 0.14 | No | prime |
- | blue | 3 | B3A | - | 52.056 | 53.181 | 1 | - | - | Yes, partly | parallel |
O I 3P1-3P2 | blue | 2 | B3A | 63.185 | 62.858 | 63.519 | 1 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | 188.542 | 190.543 | 1 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-24T21:06:19.803000 TAI (1848085579803000) |
| Mission configuration: | MC_H64ASTR_P60ASTR_S61ASTR_RP |
| Processed to level: | RED: 2.0 BLUE: 2.0 |
| Quality Control: | PASSED |
| Action: | NONE |
Quality comments
This observation was performed at 'warm' attitude conditions (Star Tracker 2 temperature > -15 C), leading to astrometry shifts induced by thermoelastic drifts which in the case of this observation are estimated to result in an offset of -5.6" in Right Ascension and -0.5" in Declination.
The offset between the central spaxel and the requested sky coordinates is 2.00" 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.