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PROGRAM |
INSTRUMENTS |
THE MSC |
DATA |
WEB TOOLS |
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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.
Last updated: 14 Feb 2008
KI Nulling Data
Products
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