APERO Documentation¶
Last Updated on 2024-03-21
APERO is a pipeline designed to reduce astrophysical observations (specifically from echelle spectrographs). It is the official pipeline for:
APERO Publications:
APERO is also be used by:
The Line-by-line code for precision radial velocity (Artigau et al. 2022) is also integrated into APERO.
Versions:¶
There are multiple branches and versions of APERO with different levels of stability and features.
The current versions are:
main (long term stable) V0.7.288 (2024-01-30)
This is the version currently recommended for all general use. It may not contain the most up-to-date features until long term support and stability can be verified.
developer (tested) V0.7.288 (2024-01-30)
Note the developer version should have been tested and semi-stable but not ready for full sets of processing and defintely not for release for non-developers or for data put on archives. Some changes may not be in this version that are in the working version.
stable-test (tested) V0.7.289 (2024-03-21)
Notrmally up-to-date with the live version has been or is currently being tested for stability
live (untested) V0.8.001 (2024-03-21)
Note the live version will be the most up-to-date version but has not been tested for stability - use at own risk.
Documentation written with version: 0.8.001