Name | DustyGlow JSON |
Version |
0.0.1
JSON |
| download |
home_page | https://github.com/neutrinomuon/DustyGlow |
Summary | DustyGlow is a standalone python library with Fortran legacy routines for absorption (attenuation) and python scripts for remission of dust in the IR. IMPORTANT: It uses the optically thin limit. |
upload_time | 2023-09-25 11:47:42 |
maintainer | |
docs_url | None |
author | Jean Gomes |
requires_python | |
license | |
keywords |
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VCS |
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bugtrack_url |
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requirements |
No requirements were recorded.
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Travis-CI |
No Travis.
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coveralls test coverage |
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# DustyGlow - Absorption (Attenuation) and Reemission of Dust Particles
**Authors:** Jean Gomes, Catarina Lobo
**Student:** André Pinheiro
**Contact:**
- Jean Gomes: [antineutrinomuon@gmail.com](mailto:antineutrinomuon@gmail.com), [jean@astro.up.pt](mailto:jean@astro.up.pt)
last stable version: 0.0.1
## About
DustyGlow is a software program designed for absorption (ATTENUATION) and reemission analysis. This README file provides essential information about the project.
## Contributors
- Jean Gomes (Software Developer, Advisor): Jean is primarily responsible for
the software development and implementation of DustyGlow. He provided
guidance and served as an advisor throughout the project.
- Catarina Lobo (Co-Advisor): Catarina provided valuable assistance during the
project. She also help guided in the selection of the sample. She co-advised
the project, offering insights and expertise.
- André Pinheiro (MSc Student): André contributed to the project as a Master's
student. He actively participated in the research and test of the code
DustyGlow.
![Barnard 68](figures/Barnard-68.jpeg)
Barnard 68 is a molecular cloud, dark absorption nebula or Bok globule.
<table>
<tr><td align='center'><img width=50 src="https://github.com/neutrinomuon/PyDust/blob/main/figures/logs.jpg?raw=true"></td><td>LOGS</td></tr>
<tr><td>19/12/2022</td>
<td>J.G. changed nomenclature from Remission to Reemission. All directories and routines were affected</td></tr>
<tr><td>18/11/2022</td>
<td>A.P. added photometric and output directories to PyDust</td></tr>
<tr><td>24/10/2022</td>
<td>J.G. added new format for LOGs added. Verification and change of directory structure</td></tr>
<tr><td>16/10/2021</td>
<td>J.G. uploaded the routines concerning absorption in the UV/Optical. Try to plot them as a function of wavelength from 91 to 15000 Angstroms to see the different behavior of extinction laws.</td></tr>
<tr><td>15/01/2022</td>
<td>J.G. uploaded correction for the reddening laws. We can use as well to compare the extinction package, but it is limited to a few extinction laws.<p>
J.G. added a directory called Literature. Please feel free to include papers of interest.
</td></tr>
<tr><td>14/01/2022</td>
<td>J.G. uploaded the recorded video from our joint meeting on 13/01/2022. The purpose of this meeting was to have a first grasp of the PyDust.py module.</td></tr>
<tr><td>12/01/2022</td>
<td>J.G. uploaded the PyDust module written in Python.</td></tr>
<tr><td>05/06/2023</td>
<td>J.G. modified the PyDust module in order to implement optimisation</td></tr>
<tr><td>25/09/2023</td> <td>J.G. modified the name PyDust to DustyGlow, since
there was during this year a registration of the PyDust package on the PyPI
library, which is not related to astronomy.</td></tr>
<tr><td>25/09/2023</td> <td>J.G. registered the name DustyGlow in the PyPI
platform.</td></tr>
</table>
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