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# Contributed material
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# Contributed material
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## pyCloudy
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## pyCloudy
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... | @@ -14,27 +12,31 @@ Morisset created [pyCloudy](https://sites.google.com/site/pycloudy/). This allo |
... | @@ -14,27 +12,31 @@ Morisset created [pyCloudy](https://sites.google.com/site/pycloudy/). This allo |
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They have a [discussion forum](https://groups.google.com/forum/#!forum/pycloudy) to answer questions.
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They have a [discussion forum](https://groups.google.com/forum/#!forum/pycloudy) to answer questions.
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Morisset and Stasinska created [Cloudy 3D](http://sites.google.com/site/cloudy3d/).
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This uses IDL scripts to drive Cloudy
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as a subprogram and create simulations of complex geometries.
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Morisset and Stasinska created [Cloudy 3D](http://sites.google.com/site/cloudy3d/).\
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This uses IDL scripts to drive Cloudy as a subprogram and create simulations of complex geometries.
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Nebular emission is included in the *Flexible Stellar Population Synthesis* (FSPS; Conroy+2009) code using Cloudy (v13.03). The nebular model is described in
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Nebular emission is included in the _Flexible Stellar Population Synthesis_ (FSPS; Conroy+2009) code using Cloudy (v13.03). The nebular model is described in [Byler+2017](http://adsabs.harvard.edu/abs/2017ApJ...840...44B) which predicts nebular line and continuum emission for complex stellar populations. The model was generated using the code cloudyFSPS, which is available at http://nell-byler.github.io/cloudyfsps/. Users can (a) download the pre-computed FSPS SSP ascii tables and (b) find usage examples for how to use FSPS to generate SEDs for complex stellar populations that include nebular line and continuum emission. More generally, users can also (c) use cloudyFSPS to generate their own ascii tables for use within Cloudy, and format the output for use within FSPS.
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[Byler+2017](http://adsabs.harvard.edu/abs/2017ApJ...840...44B) which predicts nebular line and continuum emission for complex stellar populations. The model was generated using the code cloudyFSPS, which is available at http://nell-byler.github.io/cloudyfsps/. Users can (a) download the pre-computed FSPS SSP ascii tables and (b) find usage examples for how to use FSPS to generate SEDs for complex stellar populations that include nebular line and continuum emission. More generally, users can also (c) use cloudyFSPS to generate their own ascii tables for use within Cloudy, and format the output for use within FSPS.
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*WARPFIELD solves the acceleration* against gravity accounting for feedback from winds, radiation, and SNe. More information is [here](https://bitbucket.org/drahner/warpfield) and a paper
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describing it is [here](https://arxiv.org/abs/1704.04240).
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_WARPFIELD solves the acceleration_ against gravity accounting for feedback from winds, radiation, and SNe. More information is [here](https://bitbucket.org/drahner/warpfield) and a paper describing it is [here](https://arxiv.org/abs/1704.04240).
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*Wang Ye's helper scripts* for extracting information related to the gas cooling are given [here](https://github.com/wangye0206/Cloudy_Helper).
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---
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Kyujin Kwak's grids of *radiation fields from turbulent mixing layer* simulations, suitable for use in the `interpolate` command,
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_Wang Ye's helper scripts_ for extracting information related to the gas cooling are given [here](https://github.com/wangye0206/Cloudy_Helper).
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are [here](http://www.physast.uga.edu/~kkwak/index.files/Page863.htm).
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------
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Kyujin Kwak's grids of _radiation fields from turbulent mixing layer_ simulations, suitable for use in the `interpolate` command, are [here](http://www.physast.uga.edu/\~kkwak/index.files/Page863.htm).
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---
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Return to [main](Home) page
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Return to [main](Home) page
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------
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\ No newline at end of file |