(1) Object: "NGC6946_MI-2"
(2) TDT: 86100502
(3) Observing Mode: L02
(4) OLP Version: 7.0
(5) Observer_id: "GHELOU "
(6) Proposal_id: "SF_GLX_B"
Raster Positions; Epoch (J2000)
(1,1)
RA: 20h34m48.3s
Dec: +60d04m35s
(2,1)
RA: 20h34m58.5s
Dec: +60d05m40s
(3,1)
RA: 20h35m08.7s
Dec: +60d06m44s
(4,1)
RA: 20h35m18.9s
Dec: +60d07m49s
(5,1)
RA: 20h35m29.1s
Dec: +60d08m54s
75" LWS Pointing Overlays on DSS and Link to 1x1 degree IRAS Images
This observation has been reduced by the following steps:
- Estimate and remove dark current using LWS Interactive Analysis (LIA).
- Derive the Absolute Responsivity Correction (ARC) factors using LIA. The ARCs are derived from internal calibration flashes and scale the detector responsivities to the values measured during the LWS calibration.
- Remove outlying points by hand using ISAP. These points are typically caused by cosmic ray hits.
- Average the data across scans and scan directions using a 3-sigma "special clip" algorithm designed for LWS data found in ISAP.
- Write out to FITS and ASCII files.
Calibration Notes:
- The continuum flux may not be well determined, especially for weak sources. See the LWS Handbook and calibration notes for more information.
- For extended sources, NO EXTENDED SOURCE CORRECTION has been applied. See the LWS Handbook and calibration notes for more information.
Detectors Scanned during Line Observations:
Line: 0 Active Detector: 8
Reduced Spectra and Data:
Reduced data FITS file (Shift-click)
Reduced data ASCII file
