lsst.pipe.tasks.calibrateImage.CalibrateImageConnections Class Reference
Inheritance diagram for lsst.pipe.tasks.calibrateImage.CalibrateImageConnections:
Public Member Functions | |
| __init__ (self, *, config=None) | |
Detailed Description
Definition at line 108 of file calibrateImage.py.
Constructor & Destructor Documentation
◆ __init__()
| lsst.pipe.tasks.calibrateImage.CalibrateImageConnections.__init__ | ( | self, | |
| * | , | ||
| config = None ) |
Definition at line 248 of file calibrateImage.py.
Member Data Documentation
◆ applied_photo_calib
|
static |
Initial value:
= connectionTypes.Output(
doc=(
"Photometric calibration that was applied to exposure's pixels. "
"This connection is disabled when do_calibrate_pixels=False, or "
"when output_image_type='future'."
),
name="initial_photoCalib_detector",
storageClass="PhotoCalib",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 188 of file calibrateImage.py.
◆ astrometry_matches
|
static |
Initial value:
= connectionTypes.Output(
doc="Source to reference catalog matches from the astrometry solver.",
name="initial_astrometry_match_detector",
storageClass="Catalog",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 235 of file calibrateImage.py.
◆ astrometry_ref_cat
|
static |
Initial value:
= connectionTypes.PrerequisiteInput(
doc="Reference catalog to use for astrometric calibration.",
name="gaia_dr3_20230707",
storageClass="SimpleCatalog",
dimensions=("skypix",),
deferLoad=True,
multiple=True,
)
Definition at line 111 of file calibrateImage.py.
◆ background
|
static |
Initial value:
= connectionTypes.Output(
doc="Background models estimated during calibration task; calibrated to be in nJy units "
"if do_calibrate_pixels is True. This connection is disabled when output_image_type='future'.",
name="initial_pvi_background",
storageClass="Background",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 198 of file calibrateImage.py.
◆ background_flat
|
static |
Initial value:
= connectionTypes.PrerequisiteInput(
name="flat",
doc="Flat calibration frame used for background correction.",
storageClass="ExposureF",
dimensions=["instrument", "detector", "physical_filter"],
isCalibration=True,
)
Definition at line 143 of file calibrateImage.py.
◆ background_to_photometric_ratio
|
static |
Initial value:
= connectionTypes.Output(
doc="Ratio of a background-flattened image to a photometric-flattened image. Only persisted "
"if do_illumination_correction is True.",
name="background_to_photometric_ratio",
storageClass="Image",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 205 of file calibrateImage.py.
◆ camera_model
|
static |
Initial value:
= connectionTypes.PrerequisiteInput(
doc="Camera distortion model to use for astrometric calibration.",
name="astrometry_camera",
storageClass="Camera",
dimensions=("instrument", "physical_filter"),
isCalibration=True,
minimum=0, # Can fall back on WCS already attached to exposure.
)
Definition at line 127 of file calibrateImage.py.
◆ exposure
|
static |
Initial value:
= connectionTypes.Output(
doc="Photometrically calibrated, background-subtracted exposure with fitted calibrations and "
"summary statistics. To recover the original exposure, first add the background, and then, "
"if do_calibrate_pixels=True, divide by the applied photometric calibration.",
name="initial_pvi",
storageClass="ExposureF",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 167 of file calibrateImage.py.
◆ exposures
|
static |
Initial value:
= connectionTypes.Input(
doc="Exposure (or two snaps) to be calibrated, and detected and measured on.",
name="postISRCCD",
storageClass="Exposure",
multiple=True, # to handle 1 exposure or 2 snaps
dimensions=["instrument", "exposure", "detector"],
)
Definition at line 135 of file calibrateImage.py.
◆ illumination_correction
|
static |
Initial value:
= connectionTypes.PrerequisiteInput(
name="illuminationCorrection",
doc="Illumination correction frame.",
storageClass="Exposure",
dimensions=["instrument", "detector", "physical_filter"],
isCalibration=True,
)
Definition at line 150 of file calibrateImage.py.
◆ initial_stars_schema
|
static |
Initial value:
= connectionTypes.InitOutput(
doc="Schema of the output initial stars catalog.",
name="initial_stars_schema",
storageClass="SourceCatalog",
)
Definition at line 159 of file calibrateImage.py.
◆ mask
|
static |
Initial value:
= connectionTypes.Output(
doc="The mask plane of the calibrated exposure, written as a separate "
"output so that it can be passed to downstream tasks even if the "
"exposure is removed to save storage.",
name="preliminary_visit_mask",
storageClass="Mask",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 214 of file calibrateImage.py.
◆ photometry_matches
|
static |
Initial value:
= connectionTypes.Output(
doc="Source to reference catalog matches from the photometry solver.",
name="initial_photometry_match_detector",
storageClass="Catalog",
dimensions=("instrument", "visit", "detector"),
)
Definition at line 241 of file calibrateImage.py.
◆ photometry_ref_cat
|
static |
Initial value:
= connectionTypes.PrerequisiteInput(
doc="Reference catalog to use for photometric calibration.",
name="ps1_pv3_3pi_20170110",
storageClass="SimpleCatalog",
dimensions=("skypix",),
deferLoad=True,
multiple=True
)
Definition at line 119 of file calibrateImage.py.
◆ psf_stars
|
static |
Initial value:
= connectionTypes.Output(
doc="Catalog of bright unresolved sources detected on the exposure used for PSF determination.",
name="initial_psf_stars_detector",
storageClass="ArrowAstropy",
dimensions=["instrument", "visit", "detector"],
)
Definition at line 229 of file calibrateImage.py.
◆ psf_stars_footprints
|
static |
Initial value:
= connectionTypes.Output(
doc="Catalog of bright unresolved sources detected on the exposure used for PSF determination; "
"includes source footprints.",
name="initial_psf_stars_footprints_detector",
storageClass="SourceCatalog",
dimensions=["instrument", "visit", "detector"],
)
Definition at line 222 of file calibrateImage.py.
◆ stars
|
static |
Initial value:
= connectionTypes.Output(
doc="Catalog of unresolved sources detected on the calibrated exposure.",
name="initial_stars_detector",
storageClass="ArrowAstropy",
dimensions=["instrument", "visit", "detector"],
)
Definition at line 175 of file calibrateImage.py.
◆ stars_footprints
|
static |
Initial value:
= connectionTypes.Output(
doc="Catalog of unresolved sources detected on the calibrated exposure; "
"includes source footprints.",
name="initial_stars_footprints_detector",
storageClass="SourceCatalog",
dimensions=["instrument", "visit", "detector"],
)
Definition at line 181 of file calibrateImage.py.
The documentation for this class was generated from the following file:
- python/lsst/pipe/tasks/calibrateImage.py
Generated on for lsst.pipe.tasks by
1.18.0