Stars
This is an unofficial backup of SigSpec (abbreviation of `SIGnificance SPECtrum'), which is a program that computes a significance spectrum for a time series, developed by Piet Reegen.
Python implementation of basic period detection and fitting routines for astronomical time series.
Lecture slides, Jupyter notebooks, and other material from the LSSTC Data Science Fellowship Program
ARES - Automatic Routine for line Equivalent widths in stellar Spectra
Python functions to find equivalent width of spectral lines
The Python ensemble sampling toolkit for affine-invariant MCMC
A tool for retrieving photometric data of stellar objects
Content in this repository is not maintained and is actively being migrated to other repos.
Pipeline to reduce echelle data (taken with a single or bifurcated fiber input)