PyFOSC

Please note: This program is under active development. The documentation may be inconsistent with the latest codes.

PyFOSC is a pipeline toolbox for long-slit spectroscopy data reduction written in Python. It can be used for FOSC (Faint Object Spectrograph and Camera) data from Xinglong/Lijiang 2-meter telescopes.

BFOSC (Beijing-Faint Object Spectrograph and Camera) is an instrument of the 2.16-m Telescope in Xinglong Observatory, National Astronomical Observatories, Chinese Academy of Sciences (NAOC) (IAU code: 327, coordinates: 40°23′39″ N, 117°34′30″ E). For more information about BFOSC, please see http://www.xinglong-naoc.org/html/en/gcyq/216/detail-18.html.

YFOSC (Yunnan-Faint Object Spectrograph and Camera) is an instrument of the 2.4-m Telescope in Lijiang Observatory, Yunnan Observatories, Chinese Academy of Sciences (YNAO) (IAU code: O44, coordinates: 26°42′33.1″ N, 100°1′51.6″ E). For more information about YFOSC, please see http://wiki.gmg.org.cn/pages/viewpage.action?pageId=557106.

1. Installation

conda install -c astropy ccdproc

1.1. Dependencies

IRAF
PyRAF
pandas

This package depends on IRAF and PyRAF. Although these two softwares will no longer be supported by their developers, you can still download and install the IRAF Community Distribution.

1.2. Install the IRAF/PyRAF Community Distribution

For detailed description on how to install IRAF and PyRAF, visit:

• https://iraf-community.github.io/install.html
• https://iraf-community.github.io/x11iraf.html
• https://iraf-community.github.io/pyraf.html

1.3. Download PyFOSC and set environment variable for it.

You can use git clone to download this package.

git clone https://github.com/rudolffu/pyfosc.git

To checkout the current branch (py3dev), use

git checkout py3dev

In order to run PyFOSC commands in the terminal, you need to add the path of PyFOSC and its sub-directory src to $PATH, by editing ~/.bashrc (Linux, e.g., Ubuntu) or ~/.bash_profile (Mac OS). An example of this can be:

export PATH=/Your/Path/to/pyfosc:$PATH
export PATH=/Your/Path/to/pyfosc/src:$PATH

2. Usage

2.1 Preparation

2.1.1 Run pyfosc_init to begin

First go to the working directory which contains FOSC spectroscopic data. Run pyfosc_init from the terminal:

pyfosc_init

2.1.2 Generate lists of files

As PyFOSC pipeline reduce data grouped by different types (bias, flat, object, etc), make sure you have lists of fits files as follows:

zero.list --------------- List of bias files (e.g. bias*.fits).
flat.list --------------- List of flat field files (e.g. flat*.fits).
objall.list ------------- List of 2d spectra images of all objects (science targets and standard stars).
lampall.list ------------ List of all 2d lamp spectra images.
flatnall.list ----------- List of 2d images that need zero correction (flat.list + lampall.list + objall.list).
specall.list ------------ List of all 2d spectra images (objall.list + lampall.list).

2.2 Running the pipeline

You can run pyfosc_run.sh from the terminal:

pyfosc_run.sh

Alternatively, you can run the scripts step by step, following the order as:

makezero_ccdp.py     # Combine zero(bias) frames.
ccdotz.py         # Do zero(bias), overscan correction and trimming.
makeflat2m_ccdp.py     # Combine flat fields.
makereflat2m.py   # Do (illumination) normalization and get perfect flat.
divideflat2m.py   # Do flat correction.
removecr_ccdp.py  # Remove cosmic rays in two-d images. Please go to 3. Credits for more information.
doapall.py        # Extract spectra.
reidentlamp2m.py  # Reidentify lamp spectra with previously stored ones.
#Can use identlamp2m.py instead to identify lamp by oneself.
wavecal2m.py      # Do wavelength calibration, flux calibration.
telluric_base2m.py # Telluric correction and one-d spectra extraction.

Plot all final 1d spectra with:

plotonedsp.py

Move some intermediate files into INTMD directory:

mvintmd.sh

3. Credits

This software uses BSD 3-Clause License.

Copyright (c) 2019, Yuming Fu
All rights reserved.

This software contains sources from third-party softwares.

The pyfosc$iraf_data/onedstds directory is from IRAF, and it contains standard calibration data for extinction and sensitivity calibration.

The pyfosc$iraf_task/lacos_im.cl script is the IRAF version for Laplacian Cosmic Ray Identification by Pieter G. van Dokkum (Yale) from http://www.astro.yale.edu/dokkum/lacosmic/. L.A.Cosmic is an algorithm for robust cosmic ray identification. It detects cosmic rays of arbitrary shapes and sizes, and distinguishes between undersampled point sources and cosmic rays. If you use this program please refer to P. G. van Dokkum, 2001, PASP, 113, 1420.

Please see COPYRIGHT file and pyfosc$doc/LICENSES directory for detailed copyright information.

4. How to cite

Yuming Fu. (2020, June 29). PyFOSC: a pipeline toolbox for BFOSC/YFOSC long-slit spectroscopy data reduction (Version v1.0.1). Zenodo. https://doi.org/10.5281/zenodo.3915021

Cite the current version (v1.0.1) with bibtex:

@software{yuming_fu_2020_3915021,
  author       = {Yuming Fu},
  title        = {{PyFOSC: a pipeline toolbox for BFOSC/YFOSC long-slit spectroscopy data reduction}},
  month        = jun,
  year         = 2020,
  publisher    = {Zenodo},
  version      = {v1.0.1},
  doi          = {10.5281/zenodo.3915021},
  url          = {https://doi.org/10.5281/zenodo.3915021}
}