FgcmMakeLutTask¶
FgcmMakeLutTask computes a look-up table tracking atmosphere and instrumental variations for use in the fgcmcal fits.  The intention is that this is run once for a given observatory/instrument and should only be updated when instrumental parameters change (e.g., updated filter and ccd throughput curves), or in the extremely rare case if an observatory is relocated to a different elevation or latitude.
This is the first task in a typical fgcmcal processing chain.  The second is FgcmBuildStarsTableTask or lsst.fgcmcal.fgcmBuildStars.FgcmBuildStarsTask, the third is FgcmFitCycleTask, and the fourth is FgcmOutputProductsTask.
Processing summary¶
FgcmMakeLutTask uses an input atmosphere table (preferable) or a list of atmosphere parameters, combined with the instrumental throughput as a function of position, to compute a look-up table used in the fgcmcal fits.
Python API summary¶
from lsst.fgcmcal.fgcmMakeLut import FgcmMakeLutTask
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class
(butler=None, initInputs=None, **kwargs)FgcmMakeLutTask Make Look-Up Table for FGCM
...
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attribute
config Access configuration fields and retargetable subtasks.
See also
See the FgcmMakeLutTask API reference for complete details.
Retargetable subtasks¶
No subtasks.
Configuration fields¶
atmosphereTableName¶
connections¶
- Data type
 lsst.pipe.base.config.Connections- Field type
 ConfigField
parameters¶
- Data type
 lsst.fgcmcal.fgcmMakeLut.FgcmMakeLutParametersConfig- Field type
 ConfigField