.. jjmodel documentation master file, created by sphinx-quickstart on Thu Mar 24 16:00:37 2022. You can adapt this file completely to your liking, but it should at least contain the root `toctree` directive. Acknowledgements **************** If you use the **jjmodel** code in your work, please cite our paper describing the latest version of the JJ model - `Sysoliatina and Just (2022) in prep (link will be added soon). Optionally, cite some of our other papers: - `Just and Jahreiß (2010), Towards a fully consistent Milky Way disc model - I. The local model based on kinematic and photometric data `_ - `Just et al. (2011), Towards a fully consistent Milky Way disc model - II. The local disc model and SDSS data of the NGP region `_ - `Rybizki and Just (2015), Towards a fully consistent Milky Way disc model - III. Constraining the initial mass function `_ - `Sysoliatina et al. (2018), Local disc model in view of Gaia DR1 and RAVE data `_ - `Sysoliatina and Just (2021), Towards a fully consistent Milky Way disk model -- IV. The impact of Gaia DR2 and APOGEE `_ If you used **jjmodel** facilities for the stellar population synthesis with isochrones, we also kindly ask you to cite papers of the corresponding research groups: 1. PARSEC (Padova): `Bressan et al. (2012) `_, optionally `Marigo et al. (2013) `_, `Marigo et al. (2017) `_. 2. MIST: `Dotter (2016) `_ and `Choi et al. (2016) `_, optionally some of `Paxton et al. (2011) `_, `Paxton et al. (2013) `_, `Paxton et al. (2015) `_, `Paxton et al. (2018) `_. 3. BaSTI: `Hidalgo et al. (2018) `_. If you use our separately published isochrone sets not in the framework of the JJ model, please refer to them as following: Sysoliatina, Kseniia, 2022, "JJ-model isochrone set: PARSEC, MIST, and BaSTI stellar evolution", ``_, heiDATA, V1.