11. Class reference¶
This is a list of modules, classes, and functions available in astroML
.
For more details, please refer to the user guide or
the text book. Examples of the use of astroML
can also be found in the code examples, the
text book figures and the
paper figures.
11.1. Plotting Functions: astroML.plotting
¶
11.1.1. Functions¶
|
Deprecated since version 0.4. |
|
Scatter plot with contour over dense regions |
11.1.2. Classes¶
|
Visualize Multiple-dimensional data |
11.2. Density Estimation & Histograms: astroML.density_estimation
¶
11.2.1. Histogram Tools¶
|
Deprecated since version 0.4. |
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Deprecated since version 0.4. |
|
Deprecated since version 0.4. |
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Deprecated since version 0.4. |
Deprecated since version 0.4. |
11.2.2. Density Estimation¶
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Extreme Deconvolution |
K-neighbors density estimation |
|
Empirically learn a distribution from one-dimensional data |
|
Generate random variables distributed according to an arbitrary function |
11.3. Linear Regression & Fitting: astroML.linear_model
¶
11.3.1. Linear Regression¶
Simple Linear Regression with errors in y |
|
|
Polynomial Regression with errors in y |
Basis Function with errors in y |
|
|
Nadaraya-Watson Kernel Regression |
11.3.2. Functions¶
|
Compute the total least squares log-likelihood |
11.4. Loading of Datasets: astroML.datasets
¶
11.4.1. Astronomy Datasets¶
|
Fetch an SDSS spectrum from the Data Archive Server |
Loader for Iterative PCA pre-processed galaxy spectra |
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Loader for SDSS stripe82 standard star catalog |
|
|
Loader for SDSS DR7 quasar catalog |
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Loader for SDSS moving objects datasets |
Loader for SDSS galaxy colors. |
|
|
Loader for NASA galaxy atlas data |
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Loader for SDSS SEGUE Stellar Parameter Pipeline data |
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Loader for SDSS Galaxies with spectral information |
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Get the 2D SDSS “Great Wall” distribution, following Cowan et al 2008 |
|
Loader for SDSS Imaging sample data |
|
Loader for WMAP temperature map data |
|
Loader for RR-Lyrae data |
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Loader for RR-Lyrae combined data |
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Loader for LINEAR data sample |
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Loader for LINEAR geneva data. |
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Loader for LIGO bigdog event |
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Loader for LIGO large dataset |
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Fetch the Hogg et al 2010 test data |
Loader for RR-Lyrae template data |
|
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Loader for SDSS Filter profiles |
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Loader for Vega reference spectrum |
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Generate a dataset of distance modulus vs redshift. |
11.5. Time Series Analysis: astroML.time_series
¶
11.5.1. Periodic Time Series¶
|
Deprecated since version 0.4. |
|
Deprecated since version 0.4. |
|
Deprecated since version 0.4. |
|
Utility Routine to find the best frequencies |
|
Multi-term Fourier fit to a light curve |
11.5.2. Aperiodic Time Series¶
|
Compute the Auto-correlation function via Scargle’s method |
|
Auto-correlation function via the Edelson-Krolik method |
|
Generate a power-law light curve |
|
Generate a damped random walk light curve |
11.6. Statistical Functions: astroML.stats
¶
|
Compute a binned statistic for a set of data. |
|
Compute a bidimensional binned statistic for a set of data. |
|
Compute a multidimensional binned statistic for a set of data. |
|
Compute the rank-based estimate of the standard deviation |
|
Compute median and rank-based estimate of the standard deviation |
|
Compute mean and standard deviation for an array |
|
Fit bivariate normal parameters to a 2D distribution of points |
|
Sample points from a 2D normal distribution |
A truncated positive exponential continuous random variable. |
|
A truncated positive exponential continuous random variable. |
11.7. Dimensionality Reduction: astroML.dimensionality
¶
|
|
11.8. Correlation Functions: astroML.correlation
¶
Tools for computing two-point correlation functions.
|
Two-point correlation function |
|
Angular two-point correlation function |
|
Bootstrapped two-point correlation function |
Angular two-point correlation function |
11.9. Filters: astroML.filters
¶
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Deprecated since version 1.0. |
|
Compute a Wiener-filtered time-series |
|
Minimum component filtering |
11.10. Fourier and Wavelet Transforms: astroML.fourier
¶
|
Approximate a continuous 1D Fourier Transform with sampled data. |
|
Approximate a continuous 1D Inverse Fourier Transform with sampled data. |
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Approximate a continuous 1D Power Spectral Density of sampled data. |
|
Compute the wavelet PSD as a function of f0 and t |
|
Sine-gaussian wavelet |
|
Fourier transform of the sine-gaussian wavelet. |
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Compute the PSD of the sine-gaussian function at frequency f |
11.11. Luminosity Functions: astroML.lumfunc
¶
|
Lynden-Bell’s C-minus method |
|
Compute the binned distributions using the Cminus method |
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Compute the binned distributions using the Cminus method, with bootstrapped estimates of the errors |
11.12. Classification: astroML.classification
¶
|
GaussianMixture Bayes Classifier |
11.13. Resampling: astroML.resample
¶
|
Compute bootstraped statistics of a dataset. |
|
Compute first-order jackknife statistics of the data. |