Observation Summary
| OBSID: | 1342245650 |
| Instrument: | PACS |
| AOR label: | SWloop OIII |
| Proposal: | OT2_abolatto_1 |
| Target: | SWdarkpk |
| Actual RA: | 0h 52m 56.28s |
| Actual Dec.: | -73° 12' 18.02'' |
| Redshift: | 160.0 (rad. vel. km/s) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 1094 |
| Start: | 2012-05-12T15:36:13.000000 TAI (1715528173000000) |
| Duration: | 454.0 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 | | |
O III 3P1-3P0 | blue | 2 | B2B | 88.404 | 87.822 | 89.033 | 1 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | 175.615 | 178.040 | 1 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-27T07:08:48.921000 TAI (1848294528921000) |
| Mission configuration: | MC_H100ASTR_P69ASTR_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 1.80" 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.