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
- 
classFgcmMakeLutTask
- Make Look-Up Table for FGCM - ...
- 
attributeconfig
- 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