pwkit¶
This documentation has a lot of stubs.
- About the Software
- Foundations
- Scientific Algorithms
- Basic astronomical calculations (
pwkit.astutil) - File-format-agnostic loading of astronomical images (
pwkit.astimage) - The Bayesian Blocks algorithm (
pwkit.bblocks) - Constants in CGS units (
pwkit.cgs) - Simple synchrotron radiation emission coefficients (
pwkit.dulk_models) - Representations of and computations with ellipses (
pwkit.ellipses) - Run the Fleischman & Kuznetsov (2010) synchrotron code (
pwkit.fk10) - Modeling sources in images (
pwkit.immodel) - Bayesian confidence intervals for count rates (
pwkit.kbn_conf) - Nonlinear least-squares minimization with Levenberg-Marquardt (
pwkit.lmmin) - Fitting generic models with least-squares minimization (
pwkit.lsqmdl) - Math with uncertain and censored measurements (
pwkit.msmt) - Period-finding with Phase Dispersion Minimization (
pwkit.pdm) - Loading the outputs of PHOENIX atmospheric models (
pwkit.phoenix) - Flux density models of radio calibrators (
pwkit.radio_cal_models) - Helpers for X-ray spectral modeling with the Sherpa packge (
pwkit.sherpa) - Synthetic photometry (
pwkit.synphot) - Scaling relations for physical properties of ultra-cool dwarfs (
pwkit.ucd_physics)
- Basic astronomical calculations (
- Command-line tools
- Data Visualization
- Data input and output
- Streaming output from other programs (
pwkit.slurp) - A simple “ini” file format (
pwkit.inifile) - Outputting data in LaTeX format (
pwkit.latex) - Reading and writing data tables with types and uncertainties (
pwkit.tabfile) - An “ini” file format with typed, uncertain data (
pwkit.tinifile) - Converting Unicode to LaTeX notation (
pwkit.unicode_to_latex)
- Streaming output from other programs (
- External Software Environments
- Tools for writing command-line programs
- Behind-the-scenes infrastructure