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Parameters:
- Ratio SLW central detector flux before background subtraction [%]:

- Ratio SSW central detector flux before background subtraction [%]:

- Gap in overlap region (944-1080 GHz) [Jy] after background subtraction:

- Relative Gap in overlap region (944-1080 GHz) [%] after background subtraction:

- raDecOffset: The offset between the commanded position and the actual reconstructed pointing, which includes any systematic BSM offset (bsmOffset), but not the APE. Included in the observation's Meta Data.
Selection parameters:
- Skip: Observations that do not need processing with Background Subtraction, SECT or Pointing Offset Corrector.
- Good: Observations that do not need more processing than Background Subtraction.
- Extended: Uniformly extended emission over a region that is much larger that the spectrometer beam.
- Semi-Extended: Extended source with spatially dependent distribution. Spectra needs application of SECT.
- Pointing Offset: Observation needs pointing offset correction.
- Problem: Observations with a very high value of raDecOffset, strange shaped spectra or with SLW under SSW in overlap region.
Note: The Background Subtraction applied in these observations includes the emission from all off-axis detectors except for the habitual outliers SSWE2 and SSWF2. The subtracted emission was the
median of the smoothed spectra from all other off-axis detectors.
Background Subtraction Page 5
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Laura Susana Alvarez Mera - 2015-11-09
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