Version of chemevol used in Forgan et al 2017

This version of the code includes the planet formation process in the dust and metal evolution. This includes three new parameters (f_disc, f_wind, f_debris) which account for the fact that not all metals and dust are lost per unit star formation (classical astration) due to the planet formation process which can return some material back to the ISM.

All the equations and rationale can be found in Forgan et al 2017, MNRAS 10.1093/mnras/stx2162

Version of chemevol used in de Vis et al 2017

This release is based on the version of the chemevol code developed as part of the ERC CosmicDust grant by H L Gomez, E L Gomez, P De Vis with contributions from S Schofield and K Rowlands. If you use this code please include the url to this release and cite the following papers

1. De Vis, P, Gomez H L, et al, Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies, 2017, MNRAS, https://doi.org/10.1093/mnras/stx981

Get the paper here:
Open source: http://cdsads.u-strasbg.fr/abs/2017arXiv170502340D
Journal: https://academic.oup.com/mnras/article/doi/10.1093/mnras/stx981/3800703/Using-dust-gas-and-stellar-mass-selected-samples

2. Rowlands, K, Gomez H L, et al, The dust budget crisis in high-redshift submillimetre galaxies, 2014, MNRAS, 441, 1040

Get the paper here:
Open source: http://cdsads.u-strasbg.fr/abs/2014MNRAS.441.1040R
Journal: https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stu605