FgcmCalibrateTractTask¶
FgcmCalibrateTractTask
will run the full fgcmcal
processing cycle on a single tract with multi-band coverage.
Note that the results will not be as robust as a full global calibration because of the limited ability to tract instrumental changes from observations in a single tract.
Running FgcmCalibrateTractTask
requires a look-up table generated by FgcmMakeLutTask.
FgcmCalibrateTractTask
uses FgcmBuildStarsTask to extract stars from individual calexp source catalog files.
If sourceTable_visit
parquet tables are available, use of FgcmCalibrateTractTableTask is recommended in place of this task.
FgcmCalibrateTractTask
is available as a command-line task, fgcmCalibrateTract.py.
Processing summary¶
FgcmCalibrateTractTask
runs the full fgcmcal
processing, from building star lists to fitting to the output of final products.
Specifically, it will:
- Build the star lists: FgcmBuildStarsTask
- Run the fitter until convergence: FgcmFitCycleTask
- Output the final data products: FgcmOutputProductsTask
fgcmCalibrateTract.py command-line interface¶
fgcmCalibrateTract.py REPOPATH [@file [@file2 ...]] [--output OUTPUTREPO | --rerun RERUN] [--id] [other options]
Key arguments:
REPOPATH
- The input Butler repository’s URI or file path.
Key options:
--id
:- The data IDs to process. The
tract
must be specified.
See also
See Command-line task argument reference for details and additional options.
Python API summary¶
from lsst.fgcmcal.fgcmCalibrateTract import FgcmCalibrateTractTask
-
class
(butler=None, **kwargs)FgcmCalibrateTractTask
Calibrate a single tract using fgcmcal
...
-
attribute
config
Access configuration fields and retargetable subtasks.
-
method
(dataRefDict, tract, buildStarsRefObjLoader=None, returnCatalogs=True, butler=None)run
Run the calibrations for a single tract with fgcm
...
-
method
(butler, dataRefs)runDataRef
Run full FGCM calibration on a single tract, including building star list, fitting multiple cycles, and making outputs
...
See also
See the FgcmCalibrateTractTask
API reference for complete details.
Butler datasets¶
When run as the fgcmCalibrateTract.py
command-line task, or directly through the runDataRef
method, FgcmCalibrateTractTask
obtains datasets from the input Butler data repository and persists outputs to the output Butler data repository.
Note that configurations for FgcmCalibrateTractTask
, and its subtasks, affect what datasets are persisted and what their content is.
Input datasets¶
camera
- Camera geometry and detector object
fgcmLookupTable
- FGCM look-up table produced by FgcmMakeLutTask
Output datasets¶
fgcm_stars
- Reference catalog of standard stars. See FgcmOutputProductsTask
fgcm_photoCalib_tract
- One
fgcm_photoCalib_tract
photometric calibration file is output for each visit / ccd / tract. transmission_atmosphere_fgcm_tract
- One atmospheric transmission curve is output for each visit.
Retargetable subtasks¶
fgcmBuildStars¶
- Default
lsst.fgcmcal.fgcmBuildStars.FgcmBuildStarsTask
- Field type
ConfigurableField
fgcmOutputProducts¶
- Default
lsst.fgcmcal.fgcmOutputProducts.FgcmOutputProductsTask
- Field type
ConfigurableField
Configuration fields¶
convergenceTolerance¶
fgcmFitCycle¶
- Data type
lsst.fgcmcal.fgcmFitCycle.FgcmFitCycleConfig
- Field type
ConfigField
Examples¶
fgcmCalibrateTract.py /datasets/hsc/repo --rerun <rerun name> --id visit=26024^26028^26032^26036^26044^26046^26048^26050^26058^26060^26062^26070^26072^26074^26080^26084^26094^23864^23868^23872^23876^23884^23886^23888^23890^23898^23900^23902^23910^23912^23914^23920^23924^28976^1258^1262^1270^1274^1278^1280^1282^1286^1288^1290^1294^1300^1302^1306^1308^1310^1314^1316^1324^1326^1330^24494^24504^24522^24536^24538^23212^23216^23224^23226^23228^23232^23234^23242^23250^23256^23258^27090^27094^27106^27108^27116^27118^27120^27126^27128^27130^27134^27136^27146^27148^27156^380^384^388^404^408^424^426^436^440^442^446^452^456^458^462^464^468^470^472^474^478^27032^27034^27042^27066^27068 ccd=0..8^10..103 tract=9615