General purpose and references
GLAM is a Python software that will allow you to derive the gas density, metallicity, and deviations from the Kennicutt-Schmidt relation of a galaxy with known star formation rate surface density (Sigma_SFR), known [CII] surface brightness, and known surface brightness of an ionized gas tracer (e.g. Halpha, [OIII]5007, [OIII]88um, ...). Details on the rationale, the model implementation, and on the equations are discussed in the following papers:
Requirements
The code is tested for Python >3.9. It requires Pyneb, emcee, corner.
Acknowledging this code in Scientific Publications
@ARTICLE{Ferrara:2019,
author = { {Ferrara}, A. and {Vallini}, L. and {Pallottini}, A. and {Gallerani}, S. and {Carniani}, S.
and {Kohandel}, M. and {Decataldo}, D. and {Behrens}, C.},
title = "{A physical model for [C II] line emission from galaxies}",
journal = {\mnras},
year = 2019,
month = oct,
volume = {489},
number = {1},
pages = {1-12},
doi = {10.1093/mnras/stz2031},
archivePrefix = {arXiv},
eprint = {1908.07536},
primaryClass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.489....1F},
}
@ARTICLE{Vallini2021,
author = {{Vallini}, L. and {Ferrara}, A. and {Pallottini}, A. and {Carniani}, S. and {Gallerani}, S.},
title = "{High [OIII]/[CII] surface brightness ratios trace early starburst galaxies}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Astrophysics of Galaxies},
year = 2021,
month = jun,
eid = {arXiv:2106.05279},
pages = {arXiv:2106.05279},
archivePrefix = {arXiv},
eprint = {2106.05279},
primaryClass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210605279V},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
Funding
This work is supported by the ERC Advanced Grant INTERSTELLAR H2020/740120 (PI: Ferrara).
Part of the work of LV has been supported by funding from the EU Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant agreement No. 746119.
Metadata
Release files for astroglam 0.1.0
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
|---|---|---|---|
| astroglam-0.1.0.tar.gz | 14.2 kB | Details |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Reset |
|---|---|---|---|---|
| astroglam-0.1.0-py3-none-any.whl | Python 3 | none | any | Details |
Total release size: 28.5 kB
Release files / astroglam-0.1.0.tar.gz
| Download URL | astroglam-0.1.0.tar.gz |
|---|---|
| Size | 14.2 kB |
| Tags | Source |
|
SHA-256 checksum How to use checksums |
a6696c891f12e789f710e2f14c95a6d6da29583c3c4746cdac0246d0768b9301
|
|
BLAKE2b-256 checksum How to use checksums |
1621ded65857ce33bc07c27db440099230d478d036ce255acdaa1f4e27c74513
|
| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/5.1.1 CPython/3.12.7
|
Release files / astroglam-0.1.0-py3-none-any.whl
| Download URL | astroglam-0.1.0-py3-none-any.whl |
|---|---|
| Size | 14.3 kB |
| Tags | Python 3 |
|
SHA-256 checksum How to use checksums |
4fb67ae2571358c7d210e9d1dd6f72c86ef76c025142ca42388c6a4a0eff1664
|
|
BLAKE2b-256 checksum How to use checksums |
838877428af705eb28341a9c8d119ac49da11fbe685514c91e2c0e61750cc223
|
| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/5.1.1 CPython/3.12.7
|