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
-
class
(butler=None, initInputs=None, **kwargs)FgcmMakeLutTask
Make Look-Up Table for FGCM
...
-
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