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Releases: kpolsen/SIGAME_v2

SÍGAME v2.0.1

14 Jan 17:07
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SImulator of GAlaxy Millimeter/submillimeter Emission

A code to simulate the far-IR emission lines of the ISM in galaxies from hydrodynamical codes for the interpretation and prediction of observations.


UPDATES from previous release

  • Small correction to sigame/init.py to make z=0 the default selection.

REQUIREMENTS

The code has been tested with:

  • iPython v3.6.5
  • numpy v1.16.4
  • pandas v0.24.2
  • matplotlib v3.1.0
  • PyTables v3.5.2

You may also have to install periodictable with e.g. pip install periodictable.


MORE INFO

For a description of the underlying assumptions and methods adopted by SÍGAME, see the most recent publication Olsen et al. 2017 and references therein.

Main contributors to this release are:

  • Karen Olsen
  • Daisy Leung
  • Lily Whitler

Enjoy and let us know if you find any bugs or have suggestions for improvements!

SÍGAME v2.0.0

15 Jun 21:33
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SImulator of GAlaxy Millimeter/submillimeter Emission

A code to simulate the far-IR emission lines of the ISM in galaxies from hydrodynamical codes for the interpretation and prediction of observations.


UPDATES

  • The code is now compatible with Python3.
  • A test galaxy at z=0 from the MUFASA simulation comes with the release.
  • 5 tutorials as jupyter notebooks have been added.

REQUIREMENTS

The code has been tested with:

  • iPython v3.6.5
  • numpy v1.16.4
  • pandas v0.24.2
  • matplotlib v3.1.0
  • PyTables v3.5.2

MORE INFO

For a description of the underlying assumptions and methods adopted by SÍGAME, see the most recent publication Olsen et al. 2017 and references therein.

Main contributors to this release are:

  • Karen Olsen
  • Daisy Leung
  • Lily Whitler

Enjoy and let us know if you find any bugs or have suggestions for improvements!

SÍGAME v1.0.0

01 Oct 22:22
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The very first public release of SÍGAME, including data for a galaxy at z~6 and a very limited version of the parent code. By downloading the source code and following the README, you can derive the [CII], [OI] and [OIII] line emission from this test galaxy. In addition, the galaxy can be studied with 9 different plots - a subset of what was used in this 2017 paper. Please enjoy and let us know of any bugs!