LSST Applications g02d81e74bb+86cf3d8bc9,g180d380827+7a4e862ed4,g2079a07aa2+86d27d4dc4,g2305ad1205+e1ca1c66fa,g29320951ab+012e1474a1,g295015adf3+341ea1ce94,g2bbee38e9b+0e5473021a,g337abbeb29+0e5473021a,g33d1c0ed96+0e5473021a,g3a166c0a6a+0e5473021a,g3ddfee87b4+c429d67c83,g48712c4677+f88676dd22,g487adcacf7+27e1e21933,g50ff169b8f+96c6868917,g52b1c1532d+585e252eca,g591dd9f2cf+b41db86c35,g5a732f18d5+53520f316c,g64a986408d+86cf3d8bc9,g858d7b2824+86cf3d8bc9,g8a8a8dda67+585e252eca,g99cad8db69+84912a7fdc,g9ddcbc5298+9a081db1e4,ga1e77700b3+15fc3df1f7,ga8c6da7877+a2b54eae19,gb0e22166c9+60f28cb32d,gba4ed39666+c2a2e4ac27,gbb8dafda3b+6681f309db,gc120e1dc64+f0fcc2f6d8,gc28159a63d+0e5473021a,gcf0d15dbbd+c429d67c83,gdaeeff99f8+f9a426f77a,ge6526c86ff+0433e6603d,ge79ae78c31+0e5473021a,gee10cc3b42+585e252eca,gff1a9f87cc+86cf3d8bc9,w.2024.17
LSST Data Management Base Package
|
Public Member Functions | |
getExecutionOrder (cls) | |
calculate (self, diaObjects, diaSources, filterDiaSources, band, **kwargs) | |
Static Public Attributes | |
ConfigClass = LinearFitDiaPsfFluxConfig | |
list | inputCols = ["psfFluxMean"] |
list | outputCols = ["psfFluxStetsonJ"] |
str | plugType = "multi" |
bool | needsFilter = True |
Protected Member Functions | |
_stetson_J (self, fluxes, errors, mean=None) | |
_stetson_mean (self, values, errors, mean=None, alpha=2., beta=2., n_iter=20, tol=1e-6) | |
Compute the StetsonJ statistic on the DIA point source fluxes.
Definition at line 851 of file diaCalculationPlugins.py.
|
protected |
Compute the single band stetsonJ statistic. Parameters ---------- fluxes : `numpy.ndarray` (N,) Calibrated lightcurve flux values. errors : `numpy.ndarray` (N,) Errors on the calibrated lightcurve fluxes. mean : `float` Starting mean from previous plugin. Returns ------- stetsonJ : `float` stetsonJ statistic for the input fluxes and errors. References ---------- .. [1] Stetson, P. B., "On the Automatic Determination of Light-Curve Parameters for Cepheid Variables", PASP, 108, 851S, 1996
Definition at line 909 of file diaCalculationPlugins.py.
|
protected |
Compute the stetson mean of the fluxes which down-weights outliers. Weighted biased on an error weighted difference scaled by a constant (1/``a``) and raised to the power beta. Higher betas more harshly penalize outliers and ``a`` sets the number of sigma where a weighted difference of 1 occurs. Parameters ---------- values : `numpy.dnarray`, (N,) Input values to compute the mean of. errors : `numpy.ndarray`, (N,) Errors on the input values. mean : `float` Starting mean value or None. alpha : `float` Scalar down-weighting of the fractional difference. lower->more clipping. (Default value is 2.) beta : `float` Power law slope of the used to down-weight outliers. higher->more clipping. (Default value is 2.) n_iter : `int` Number of iterations of clipping. tol : `float` Fractional and absolute tolerance goal on the change in the mean before exiting early. (Default value is 1e-6) Returns ------- mean : `float` Weighted stetson mean result. References ---------- .. [1] Stetson, P. B., "On the Automatic Determination of Light-Curve Parameters for Cepheid Variables", PASP, 108, 851S, 1996
Definition at line 939 of file diaCalculationPlugins.py.
lsst.meas.base.diaCalculationPlugins.StetsonJDiaPsfFlux.calculate | ( | self, | |
diaObjects, | |||
diaSources, | |||
filterDiaSources, | |||
band, | |||
** | kwargs ) |
Compute the StetsonJ statistic on the DIA point source fluxes. Parameters ---------- diaObject : `dict` Summary object to store values in. diaSources : `pandas.DataFrame` DataFrame representing all diaSources associated with this diaObject. filterDiaSources : `pandas.DataFrame` DataFrame representing diaSources associated with this diaObject that are observed in the band pass ``band``. band : `str` Simple, string name of the filter for the flux being calculated. **kwargs Any additional keyword arguments that may be passed to the plugin.
Reimplemented from lsst.meas.base.diaCalculation.DiaObjectCalculationPlugin.
Definition at line 868 of file diaCalculationPlugins.py.
lsst.meas.base.diaCalculationPlugins.StetsonJDiaPsfFlux.getExecutionOrder | ( | cls | ) |
Used to set the relative order of plugin execution. The values returned by `getExecutionOrder` are compared across all plugins, and smaller numbers run first. Notes ----- `CatalogCalculationPlugin`\s must run with `BasePlugin.DEFAULT_CATALOGCALCULATION` or higher. All plugins must implement this method with an appropriate run level
Reimplemented from lsst.meas.base.catalogCalculation.CatalogCalculationPlugin.
Definition at line 865 of file diaCalculationPlugins.py.
|
static |
Definition at line 855 of file diaCalculationPlugins.py.
|
static |
Definition at line 858 of file diaCalculationPlugins.py.
|
static |
Definition at line 862 of file diaCalculationPlugins.py.
|
static |
Definition at line 860 of file diaCalculationPlugins.py.
|
static |
Definition at line 861 of file diaCalculationPlugins.py.