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KI Nulling Data Products

In the Nuller mode the main science data measurment is the coherent null leakage, nominally equal to one minus 1/2 of the visibility amplitude squared for a given source. Integrations on the target source and calibrators are interleaved in time. Each integration includes all local (detector, background) calibrations.

As with the V2 mode, the MSC will reduce the raw data and provide average null values (Level 1 data) in a set of files available through the KI database as either ASCII or FITS files. The MSC will also provide the programs necessary to calibrate the Level 1 data for the system response. After this calibration, the data are ready for astrophysical modeling and interpretation.

Level 1 Nulling files

filename contents
YYYYDDD.nullsum Wide-band nulling data
YYYYDDD.nullspec Spectrometer nulling data
YYYYDDD.nullbaseline A priori baseline model
YYYYDDD.nullinfo Reduction configuration info, etc.
YYYYDDD.nullanc Ancillary data
YYYYDDD.nulllog Observer log
YYYYDDD.rpt Nightly report

Last updated: 14 Feb 2008