Observation Summary
OBSID: | 1342268746 |
Instrument: | PACS |
AOR label: | s051024-701406_pacs_2 |
Proposal: | OT1_joliveir_1 |
Target: | SAGE051024.1-701406.5 |
Actual RA: | 5h 10m 24.39s |
Actual Dec.: | -70° 14' 6.91'' |
Redshift: | 270.0 (rad. vel. km/s) |
Purpose: | --- |
Concat.: | 1342268746,1342268747 |
OD: | 1416 |
Start: | 2013-03-30T09:44:57.000000 TAI (1743327897000000) |
Duration: | 1843.0 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 | 63.242 | 62.916 | 63.576 | 2 | 4 | 0.14 | No | prime |
- | red | 102 | R1 | - | 188.717 | 190.715 | 2 | 4 | 0.14 | No | parallel |
CII C+ | red | 105 | R1 | 157.883 | 156.298 | 159.550 | 1 | 2 | 0.14 | No | prime |
- | blue | 5 | B3A | - | 52.105 | 53.228 | 1 | - | - | Yes, partly | parallel |
CO 14-13 | red | 103 | R1 | 186.167 | 184.855 | 187.501 | 1 | 2 | 0.14 | No | prime |
- | blue | 3 | B3A | - | 61.630 | 62.505 | 1 | 2 | 0.14 | No | parallel |
H20 212-101 | red | 104 | R1 | 179.689 | 178.302 | 181.109 | 1 | 2 | 0.14 | No | prime |
- | blue | 4 | B3A | - | 59.448 | 60.374 | 1 | 2 | 0.14 | No | parallel |
(*) = requested in HSPOT
System configuration summary
SPG pipeline version: | SPG v14.2.0 |
SPG pipeline products creation date: | 2016-07-28T17:59:14.241000 TAI (1848419954241000) |
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 1.54" 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.