Metadata-Version: 2.1
Name: pyird
Version: 0.3.0
Summary: Python IRD
Home-page: 
Author: Yui Kasagi, Hajime Kawahara, Kento Masuda
Author-email: divrot@gmail.com
Maintainer: Yui Kasagi, Hajime Kawahara, Kento Masuda
Maintainer-email: divrot@gmail.com
License: UNKNOWN
Platform: UNKNOWN
Classifier: Programming Language :: Python
Description-Content-Type: text/x-rst
Requires-Dist: numpy
Requires-Dist: matplotlib
Requires-Dist: tqdm
Requires-Dist: scipy
Requires-Dist: astroquery
Requires-Dist: sep
Requires-Dist: gpkron
Requires-Dist: pandas

PYIRD
===========

Free from messy directory and file management of IRD analysis.
Currently under heavily construction. Use develop branch for dev.


Core Pipelines
------------------

- pyird.utils -- setting us free from file name managements
- pyird.image -- reducing systematics in the image level and extracting raw spectra
- pyird.spec -- assigning wavelength reference (wavref) to pixel coordinates in the raw spectra


Classes
------------------

- fitsset.FitsSet --  sets of fits files
- irdstream.Stream2D -- 2D fits stream from raw images
- aperture.TraceAperture -- aperture class for trace
- image_widget.image_1Dand2D -- interactive figures of 1D spectrum and 2D detector image

Aperture
------------------------------

Mask: n=42 (H), 102 (YJ) apertures extracted from FLAT for aperture mask.

Star: `aperture.TraceAperture.mmf2()` sets n=21 (H) apertures of star fiber.

Comb: `aperture.TraceAperture.mmf1()` sets n=51 (YJ) apertures of comb fiber.


