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", https://doi.org/10.11588/data/ZCXHOE, heiDATA, V1.