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3 changes: 2 additions & 1 deletion pyproject.toml
Original file line number Diff line number Diff line change
@@ -1,13 +1,14 @@
[project]
name = "astro-ssptools"
version = "2.1.3"
version = "2.1.4"
description = "Simple Stellar Population Tools"
authors = [
{name = "Eduardo Balbinot", email = "eduardo.balbinot@gmail.com"},
{name = "Nolan Dickson", email = "nolan.dickson@smu.ca"},
{name = "Peter Smith", email = "smith.peter.902@gmail.com"},
{name = "Mark Gieles", email = "m.gieles@surrey.ac.uk"},
{name = "Miklos Peuten", email = "m.peuten@surrey.ac.uk"},
{name = "Daniel Marin Pina", email = "daniel.marin@uni-heidelberg.de"},
]
readme = "README.md"
requires-python = ">=3.10"
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2 changes: 1 addition & 1 deletion ssptools/__init__.py
Original file line number Diff line number Diff line change
Expand Up @@ -4,7 +4,7 @@

__author__ = """Eduardo Balbinot"""
__email__ = "eduardo.balbinot@gmail.com"
__version__ = "2.0.1"
__version__ = "2.1.4"

from .evolve_mf import *
from .sev import *
14 changes: 14 additions & 0 deletions ssptools/data/ifmr/README.md
Original file line number Diff line number Diff line change
Expand Up @@ -107,3 +107,17 @@ Models are computed using the following BSE parameters:

All other parameters are left as defaults (see `ifmr._DEFAULT_BSEDICT`).


## `SEVN_rapid/`

SEVN (`sevncodes.gitlab.io/sevn`) IFMR, assuming the Fryer+2012
rapid supernovae prescription.


## `SEVN_delayed/`

SEVN (`sevncodes.gitlab.io/sevn`) IFMR, assuming the Fryer+2012
delayed supernovae prescription.

All parameters used to run SEVN are listed in the
`SEVN_delayed/used_params.svpar` file.
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