Observation Summary

OBSID:	1342216658
Instrument:	PACS
AOR label:	NGC7049 lines
Proposal:	OT1_nwerner_1
Target:	NGC7049
Actual RA:	21h 19m 0.1s
Actual Dec.:	-48° 33' 45.14''
Redshift:	0.007622 (z)
Purpose:	---
Concat.:	---
OD:	679
Start:	2011-03-23T23:49:54.000000 TAI (1679615394000000)
Duration:	5442.0 seconds (incl. spacecraft on-target slew time)

AOT and instrument configuration:

AOT:	PacsLineSpec
Mode:	Pointed, Chop/Nod
Bands:	B3A 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
OI	blue	2	B3A	63.682	63.444	63.943	2	2	0.14	No	prime
-	red	102	R1	-	190.303	191.813	2	2	0.14	No	parallel
CII	red	103	R1	158.902	157.842	160.085	2	2	0.14	No	prime
-	blue	3	B3A	-	52.621	53.404	2	2	0.14	Yes, partly	parallel
OIb	red	104	R1	146.609	145.490	147.880	3	3	0.14	No	prime
-	blue	4	B2A	-	72.755	73.942	3	-	-	Yes, fully	parallel

(*) = requested in HSPOT

System configuration summary

SPG pipeline version:	SPG v14.2.0
SPG pipeline products creation date:	2016-07-25T02:17:27.866000 TAI (1848104247866000)
Mission configuration:	MC_H66ASTR_P60ASTR_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  2.42" 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.