Observation Summary
| OBSID: | 1342243855 |
| Instrument: | PACS |
| AOR label: | S11_R1_V5 |
| Proposal: | OT2_nbillot_2 |
| Target: | S11_HOPS88-1 |
| Actual RA: | 5h 35m 22.38s |
| Actual Dec.: | -5° 1' 17.4'' |
| Purpose: | offSelector |
| Concat.: | 1342243855,1342243856,1342243857,1342243858,1342243859,1342243860 |
| OD: | 1059 |
| Start: | 2012-04-07T10:25:39.000000 TAI (1712485539000000) |
| Duration: | 1541.0 seconds (incl. spacecraft on-target slew time) |
AOT and instrument configuration:
| AOT: | PacsRangeSpec |
| Mode: | Pointed, unchopped grating scan |
| Bands: | B3A R1 (prime diffraction orders selected) |
| Sampling: | Nyquist (with spectral dithering if range repetition > 1) |
| Nod cycles: | 1 |
Observation block summary
| Name(*) | Camera | ID | Band(*) | ReqWaveMin(*) | ReqWaveMax(*) | WaveMin | WaveMax | Repetitions(*) | ActualRep | Capacitance | OutOfBand | Channel |
| | | | micrometer | micrometer | micrometer | micrometer | | | pF | | |
Range 1 | blue | 2 | B2A,B3A | 57.000 | 71.000 | 50.562 | 71.164 | 2 | 2 | 0.14 | Yes, partly | prime |
- | red | 102 | R1 | - | - | 170.445 | 213.157 | 2 | 2 | 0.14 | No | parallel |
Range 2 | red | 103 | R1 | 102.000 | 142.000 | 101.293 | 142.319 | 2 | 2 | 0.14 | No | prime |
- | blue | 3 | B2A | - | - | 50.562 | 71.164 | 2 | 2 | 0.14 | Yes, partly | parallel |
(*) = requested in HSPOT
System configuration summary
| SPG pipeline version: | SPG v14.2.2 |
| SPG pipeline products creation date: | 2017-01-18T08:32:48.729000 TAI (1863419568729000) |
| Mission configuration: | MC_H98ASTR_P69ASTR_S66ASTR_RP |
| Processed to level: | RED: 2.5 BLUE: 2.5 |
| Quality Control: | PASSED |
| Action: | NONE |
Quality comments
On source observation in an unchopped range-scan pair; matched with the off-source observation 1342243856
The offset between the central spaxel and the requested sky coordinates is 1.65" 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.