Observation Summary
OBSID: | 1342210830 |
Instrument: | PACS |
AOR label: | NearGalPACS-Elusive-01-red - corrected |
Proposal: | KPGT_esturm_1 |
Target: | NGC4418 |
Actual RA: | 12h 26m 54.56s |
Actual Dec.: | -0° 52' 37.45'' |
Redshift: | 0.007268 (z) |
Purpose: | --- |
Concat.: | --- |
OD: | 570 |
Start: | 2010-12-05T06:45:21.000000 TAI (1670222721000000) |
Duration: | 2704.0 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: | 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 | 158.887 | 157.831 | 160.075 | 1 | 1 | 0.14 | No | prime |
- | blue | 3 | B2B | - | 78.933 | 80.051 | 1 | 1 | 0.14 | No | parallel |
O I 3P0-3P1 | red | 104 | R1 | 146.578 | 145.462 | 147.853 | 2 | 2 | 0.14 | No | prime |
- | blue | 4 | B2B | - | 72.750 | 73.940 | 2 | 2 | 0.14 | No | parallel |
N II 3P2-3P1 | red | 105 | R1 | 122.786 | 121.571 | 124.197 | 2 | 2 | 0.14 | No | prime |
- | blue | 5 | B2B | - | 60.789 | 62.118 | 2 | - | - | Yes, fully | parallel |
O III 3P1-3P0 | blue | 2 | B2B | 89.002 | 88.591 | 89.480 | 2 | 2 | 0.14 | No | prime |
- | red | 102 | R1 | - | 177.153 | 178.933 | 2 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
SPG pipeline version: | SPG v14.2.0 |
SPG pipeline products creation date: | 2016-07-24T10:41:30.635000 TAI (1848048090635000) |
Mission configuration: | MC_H62ASTR_P58ASTR_S61ASTR_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 1.59" 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.