Observation Summary
| OBSID: | 1342197812 |
| Instrument: | PACS |
| AOR label: | NearGalPACS-Sy1-01-red |
| Proposal: | KPGT_esturm_1 |
| Target: | NGC 4051 |
| Actual RA: | 12h 3m 9.87s |
| Actual Dec.: | 44° 31' 52.99'' |
| Redshift: | 0.002336 (z) |
| Purpose: | --- |
| Concat.: | --- |
| OD: | 388 |
| Start: | 2010-06-05T22:24:46.000000 TAI (1654467886000000) |
| Duration: | 6869.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsLineSpec |
| Mode: | Pointed, Chop/Nod |
| Bands: | B2B R1 (prime diffraction orders selected) |
| Is bright: | NO (default range mode) |
| Chopper: | large throw |
| Nod cycles: | 2 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | Wave(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | | | pF | | |
CII | red | 103 | R1 | 158.109 | 157.026 | 159.279 | 1 | 1 | 0.14 | No | prime |
- | blue | 3 | B2B | - | 78.530 | 79.653 | 1 | 1 | 0.14 | No | parallel |
O I 3P0-3P1 | red | 104 | R1 | 145.860 | 144.719 | 147.117 | 4 | 4 | 0.14 | No | prime |
- | blue | 4 | B2B | - | 72.378 | 73.573 | 4 | 4 | 0.14 | No | parallel |
N II 3P2-3P1 | red | 105 | R1 | 122.185 | 120.950 | 123.581 | 2 | 2 | 0.14 | No | prime |
- | blue | 5 | B2B | - | 60.478 | 61.810 | 2 | - | - | Yes, fully | parallel |
O III 3P1-3P0 | blue | 2 | B2B | 88.566 | 88.139 | 89.034 | 2 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | 176.249 | 178.042 | 2 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.0 |
| SPG pipeline products creation date: | 2016-07-23T16:25:27.573000 TAI (1847982327573000) |
| Mission configuration: | MC_H38ASTR_P48ASTR_S52ASTR_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 2.35" 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.