LSST Applications 27.0.0,g0265f82a02+469cd937ee,g02d81e74bb+21ad69e7e1,g1470d8bcf6+cbe83ee85a,g2079a07aa2+e67c6346a6,g212a7c68fe+04a9158687,g2305ad1205+94392ce272,g295015adf3+81dd352a9d,g2bbee38e9b+469cd937ee,g337abbeb29+469cd937ee,g3939d97d7f+72a9f7b576,g487adcacf7+71499e7cba,g50ff169b8f+5929b3527e,g52b1c1532d+a6fc98d2e7,g591dd9f2cf+df404f777f,g5a732f18d5+be83d3ecdb,g64a986408d+21ad69e7e1,g858d7b2824+21ad69e7e1,g8a8a8dda67+a6fc98d2e7,g99cad8db69+f62e5b0af5,g9ddcbc5298+d4bad12328,ga1e77700b3+9c366c4306,ga8c6da7877+71e4819109,gb0e22166c9+25ba2f69a1,gb6a65358fc+469cd937ee,gbb8dafda3b+69d3c0e320,gc07e1c2157+a98bf949bb,gc120e1dc64+615ec43309,gc28159a63d+469cd937ee,gcf0d15dbbd+72a9f7b576,gdaeeff99f8+a38ce5ea23,ge6526c86ff+3a7c1ac5f1,ge79ae78c31+469cd937ee,gee10cc3b42+a6fc98d2e7,gf1cff7945b+21ad69e7e1,gfbcc870c63+9a11dc8c8f
LSST Data Management Base Package
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Public Member Functions | |
__init__ (self, table=None, **kwargs) | |
updateMetadata (self, setDate=False, **kwargs) | |
fromDict (cls, dictionary) | |
toDict (self) | |
fromTable (cls, tableList) | |
toTable (self) | |
validate (self) | |
Public Attributes | |
abscissaCorrections | |
tableData | |
Static Protected Attributes | |
str | _OBSTYPE = "PHOTODIODE_CORRECTION" |
str | _SCHEMA = 'PhotodiodeCorrection' |
float | _VERSION = 1.1 |
Parameter set for photodiode correction. These parameters are included in cameraGeom.Amplifier, but should be accessible externally to allow for testing. Parameters ---------- table : `numpy.array`, optional Lookup table; a 2-dimensional array of floats: - one row for each row index (value of coef[0] in the amplifier) - one column for each image value. To avoid copying the table the last index should vary fastest (numpy default "C" order) log : `logging.Logger`, optional Logger to handle messages. kwargs : `dict`, optional Other keyword arguments to pass to the parent init. Raises ------ RuntimeError Raised if the supplied table is not 2D, or if the table has fewer columns than rows (indicating that the indices are swapped). Notes ----- The photodiode correction attributes stored are: abscissaCorrections : `dict` : [`str`, `float`] Correction value indexed by exposure pair
Definition at line 32 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.__init__ | ( | self, | |
table = None, | |||
** | kwargs ) |
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 69 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.fromDict | ( | cls, | |
dictionary ) |
Construct a PhotodiodeCorrection from a dictionary of properties. Parameters ---------- dictionary : `dict` Dictionary of properties. Returns ------- calib : `lsst.ip.isr.PhotodiodeCorrection` Constructed photodiode data. Raises ------ RuntimeError Raised if the supplied dictionary is for a different calibration type.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 100 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.fromTable | ( | cls, | |
tableList ) |
Construct calibration from a list of tables. This method uses the `fromDict` method to create the calibration after constructing an appropriate dictionary from the input tables. Parameters ---------- tableList : `list` [`astropy.table.Table`] List of tables to use to construct the crosstalk calibration. Returns ------- calib : `lsst.ip.isr.PhotodiodeCorrection` The calibration defined in the tables.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 161 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.toDict | ( | self | ) |
Return a dictionary containing the photodiode correction properties. The dictionary should be able to be round-tripped through. `fromDict`. Returns ------- dictionary : `dict` Dictionary of properties.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 136 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.toTable | ( | self | ) |
Construct a list of tables containing the information in this calibration. The list of tables should create an identical calibration after being passed to this class's fromTable method. Returns ------- tableList : `list` [`astropy.table.Table`] List of tables containing the photodiode correction information.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 196 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.updateMetadata | ( | self, | |
setDate = False, | |||
** | kwargs ) |
Update metadata keywords with new values. This calls the base class's method after ensuring the required calibration keywords will be saved. Parameters ---------- setDate : `bool`, optional Update the CALIBDATE fields in the metadata to the current time. Defaults to False. kwargs : Other keyword parameters to set in the metadata.
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 82 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.validate | ( | self | ) |
Validate photodiode correction
Reimplemented from lsst.ip.isr.calibType.IsrCalib.
Definition at line 223 of file photodiodeCorrection.py.
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staticprotected |
Definition at line 65 of file photodiodeCorrection.py.
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staticprotected |
Definition at line 66 of file photodiodeCorrection.py.
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staticprotected |
Definition at line 67 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.abscissaCorrections |
Definition at line 70 of file photodiodeCorrection.py.
lsst.ip.isr.photodiodeCorrection.PhotodiodeCorrection.tableData |
Definition at line 71 of file photodiodeCorrection.py.