lsst.analysis.tools¶
analysis_tools
is the plotting and metric framework that is used to perform QA on the pipeline products.
It is a very powerful way to explore and interact with the pipeline outputs.
Using lsst.analysis.tools¶
For a tutorial on working with
analysis_tools
please see the getting started guide.
Need Help?¶
If you get stuck with analysis_tools
then feel free to reach out to the #rubinobs-analysis-tools
channel on slack and hopefully someone will help you!
Contributing¶
lsst.analysis.tools
is developed at https://github.com/lsst/analysis_tools.
You can find Jira issues for this module under the analysis_tools component.
Python API reference¶
lsst.analysis.tools Package¶
Variables¶
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Compute the median absolute deviation of the data along the given axis. |
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Compute the median absolute deviation of the data along the given axis. |
lsst.analysis.tools.actions.plot Package¶
Classes¶
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A configurable class describing a panel in a bar plot. |
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A plotting tool which can take multiple keyed data inputs and can create one or more bar graphs. |
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Makes a color-color plot and overplots a prefited line to the specified area of the plot. |
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Configuration options for DiaSkyPlot panels. |
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Generic pseudo base class for plotting DiaSources (or DiaObjects) on the sky. |
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A Config class that holds parameters to configure a single panel of a histogram plot. |
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Make an N-panel plot with a configurable number of histograms displayed in each panel. |
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A Config class that holds parameters to configure a the stats panel shown for histPlot. |
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Plot the coverage for a set of visits. |
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Make multiple plots of rho statistics. |
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Calculates the statistics needed for the scatter plot with two hists. |
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Makes a scatter plot of the data with a marginal histogram for each axis. |
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Plots the on sky distribution of a parameter. |
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Make a plot (with errorbars) of one quantity (X) vs another (Y). |
lsst.analysis.tools.actions.vector Package¶
Classes¶
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Calculate the difference between two columns, assuming their units are degrees, and convert the difference to arcseconds. |
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Makes a mask for sources observed in a specified set of bands. |
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A Config class that holds some of the parameters supported by treecorr. |
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Calculate a complex value representation of the ellipticity. |
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Calculate \(e_1\) (distortion-type) or \(g_1\) (shear-type). |
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Calculate \(e_2\) (distortion-type) or \(g_2\) (shear-type). |
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Calculate the difference of two ellipticities as a complex quantity. |
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Calculate rho statistics. |
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Calculate a size: \((I_{xx}I_{yy}-I_{xy}^2)^{\frac{1}{4}}\) (determinant radius) or \(\sqrt{(I_{xx}+I_{yy})/2}\) (trace radius). |
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This default setting makes it take the band from the kwargs. |
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Return a constant scalar value. |
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Calculate (A/B) |
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Get a vector from KeyedData, apply specified selector, return the shorter Vector. |
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A selector that picks between extended and point sources. |
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Compute the difference between two magnitudes and correct for extinction By default bands are derived from the <band>_ prefix on flux columns, per the naming convention in the Object Table: e.g. |
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The base flag selector to use to select valid sources for QA. |
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Calculate (A-B)/B. |
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A selector that picks out galaxies based off of their extendedness values. |
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Selects good DIA sources from diaSourceTables. |
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Load and return a Vector from KeyedData. |
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Turn nano janskies into magnitudes. |
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Calculate the difference between two magnitudes; each magnitude is derived from a flux column. |
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Get a vector from KeyedData, apply specified set of selectors with AND logic, and return the shorter Vector. |
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Compute per-group statistic values and return result as a vector with one element per group. |
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Selects rows within a range, inclusive of min/exclusive of max. |
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Calculate the signal-to-noise. |
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Selects sky objects in the given band(s). |
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Selects sky sources from sourceTables. |
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Compute signal-to-noise in the given flux type. |
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Selects points that have S/N > threshold in the given flux type. |
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A selector that picks out stars based off of their extendedness values. |
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Calculate (A-B). |
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Return a mask corresponding to an applied threshold. |
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A selector that picks out unclassified objects based off of their extendedness values. |
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Load a boolean vector from KeyedData and return it for use as a selector. |
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Select on a set of flags appropriate for making visit-level plots (i.e., using sourceTable_visit catalogs). |
lsst.analysis.tools.actions.scalar Package¶
Classes¶
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Returns the median of the lowest ten values of the sorted input. |
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Returns the number of non-NaN entries in the given column. |
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Counts the number of unique rows in a given column. |
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Compute the fraction of a distribution that is between specified minimum and maximum values, and is not NaN. |
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Compute the fraction of vector entries that are NaN. |
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Compute the fraction of a distribution that is above or below a specified threshold. |
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Returns the maximum of the given data. |
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Calculates the mean of the given data. |
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Calculates the median of the given data. |
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Returns the minimum of the given data. |
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Calculates the sigma mad of the given data. |
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Calculates the standard deviation of the given data. |