Observation Summary
| OBSID: | 1342270680 |
| Instrument: | PACS |
| AOR label: | G48.930-0.286_p2_line |
| Proposal: | OT2_yokada_2 |
| Target: | G48.930-0.286_p2 |
| Actual RA: | 19h 22m 14.47s |
| Actual Dec.: | 14° 4' 20.4'' |
| Redshift: | 0.0 (z) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 1438 |
| Start: | 2013-04-21T13:28:51.000000 TAI (1745242131000000) |
| Duration: | 1421.0 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 | | |
O I 3P1-3P2 | blue | 3 | B3A | 63.185 | 62.943 | 63.460 | 1 | 2 | 0.14 | No | prime |
- | red | 103 | R1 | - | 188.797 | 190.366 | 1 | 2 | 0.14 | No | parallel |
N II 3P2-3P1 | red | 106 | R1 | 121.800 | 120.460 | 123.347 | 1 | 2 | 0.14 | No | prime |
- | blue | 6 | B2A | - | 60.246 | 61.680 | 1 | 2 | 0.14 | No | parallel |
O I 3P0-3P1 | red | 105 | R1 | 145.535 | 144.305 | 146.937 | 1 | 2 | 0.14 | No | prime |
- | blue | 5 | B2A | - | 72.164 | 73.471 | 1 | - | - | Yes, fully | parallel |
CII C+ | red | 104 | R1 | 157.741 | 156.576 | 159.052 | 1 | 2 | 0.14 | No | prime |
- | blue | | ??? | - | - | - | 1 | - | - | ??? | parallel |
N II 3P1-3P0 | red | 102 | R1 | 205.300 | 204.542 | 206.141 | 1 | 2 | 0.14 | No | prime |
- | blue | 2 | B3A | - | 68.189 | 68.732 | 1 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-28T23:08:53.893000 TAI (1848438533893000) |
| 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 1.77" 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.