ARC Echelle Spectroscopic Observation Pipeline (aesop)
The ARC Echelle Spectroscopic Observation Pipeline, or aesop, is a high resolution spectroscopy software toolkit tailored for observations from the ARC Echelle Spectrograph (ARCES) mounted on the ARC 3.5 m Telescope at Apache Point Observatory. aesop picks up where the traditional IRAF reduction scripts leave off, offering an open development, object-oriented Pythonic analysis framework for echelle spectra.
Basic functionality of aesop includes: (1) blaze function normalization by polynomial fits to observations of early-type stars, (2) an additional/alternative robust least-squares normalization method, (3) radial velocity measurements (or offset removals) via cross-correlation with model spectra, including barycentric radial velocity calculations, (4) concatenation of multiple echelle orders into a simple 1D spectrum, and (5) approximate flux calibration.
Installation
You can install aesop from the source code by doing the following:
git clone https://github.com/bmorris3/aesop.git cd aesop pip install .
For more information, read the docs.
License
This project is Copyright (c) Brett Morris & Trevor Dorn-Wallenstein and licensed under the terms of the MIT license. This package is based upon the Astropy package template which is licensed under the BSD 3-clause licence. See the licenses folder for more information.
Metadata
Release files for aesop-arces 0.5
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
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| aesop_arces-0.5.tar.gz | 342.8 kB | Details |
Release files / aesop_arces-0.5.tar.gz
| Download URL | aesop_arces-0.5.tar.gz |
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