Observation Summary
| OBSID: | 1342245975 |
| Instrument: | PACS |
| AOR label: | PSpecL-CWLeo_Unchopped |
| Proposal: | GT2_mgroen01_7 |
| Target: | CW Leo Arc-1 |
| Actual RA: | 9h 48m 30.11s |
| Actual Dec.: | 13° 15' 51.49'' |
| Redshift: | 0.0 (z) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 1104 |
| Start: | 2012-05-22T08:33:14.000000 TAI (1716366794000000) |
| Duration: | 2325.0 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: | 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 I 3P1-3P2 | blue | 2 | B3A | 63.180 | 62.848 | 63.510 | 5 | 10 | 0.14 | No | prime |
- | red | 102 | R1 | - | 188.514 | 190.515 | 5 | 10 | 0.14 | No | parallel |
CII C+ | red | 103 | R1 | 157.741 | 156.143 | 159.396 | 5 | 10 | 0.14 | No | prime |
- | blue | 3 | B3A | - | 52.053 | 53.177 | 5 | - | - | Yes, partly | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-27T08:37:31.868000 TAI (1848299851868000) |
| 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 1.64" 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.