ner_tags: O O O O O O O O O O O O O O B-Software O O O O B-Observatory I-Observatory I-Observatory O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O O O B-Grant I-Grant I-Grant B-Grant O B-Organization O B-Grant O O B-ComputingFacility I-ComputingFacility B-ComputingFacility O O B-Observatory I-Observatory I-Observatory I-Observatory I-Observatory I-Observatory O O O O O O O O O O O O O O O O B-Grant I-Grant I-Grant I-Grant I-Grant B-Grant O B-Organization O O B-Organization O B-Organization O O O O O O O B-Organization B-Collaboration O O O O O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization B-Organization O O O O O B-Grant I-Grant O O O B-Grant O O B-Person I-Person O B-Person I-Person O O O O O O O B-Grant I-Grant
tokens: We thank the referee for their comments that helped us to improve the manuscript. PLUTO is developed at the Turin Astronomical Observatory in collaboration with the Department of Physics of Turin University. We acknowledge the “Accordo Quadro INAF-CINECA (2017)” the CINECA Award HP10B1GLGV and the HPC facility (SCAN) of the INAF – Osservatorio Astronomico di Palermo, for the availability of high performance computing resources and support. This work was supported by the Programme National de Physique Stellaire (PNPS) of CNRS/INSU, co-funded by CEA and CNES. This work has been done within the LABEX Plas@par project, and received financial state aid managed by the Agence Nationale de la Recherche (ANR), as part of the programme “Investissements d’avenir” under the reference ANR-11-IDEX-0004-02. The authors (R. B. and C. A.) acknowledge modest financial contribution from the agreement ASI-INAF n.2017-14.H.O.