ner_tags: O O O O O O O B-Organization I-Organization I-Organization I-Organization O O B-Grant I-Grant I-Grant O B-Grant O O B-Fellowship I-Fellowship I-Fellowship I-Fellowship B-Person O B-Person O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O O B-Grant I-Grant I-Grant B-Grant O B-Grant O O B-Grant I-Grant O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Person B-Person O O O O O B-Fellowship I-Fellowship I-Fellowship I-Fellowship O O B-Organization I-Organization I-Organization I-Organization O O O O O O O O O B-Organization I-Organization I-Organization B-Organization O B-Telescope O B-URL O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Organization B-URL O O O O B-Organization O O O O O O O O O O O O B-Collaboration I-Collaboration I-Collaboration O O O B-Location O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O O B-Organization B-Grant I-Grant O B-Grant I-Grant O B-Grant I-Grant I-Grant O O B-Organization I-Organization I-Organization I-Organization O O O O O O O B-Telescope O O O O B-Telescope O B-Mission O O O O O B-Organization I-Organization I-Organization I-Organization O B-Telescope B-Mission O O O O O O O O O B-Archive I-Archive I-Archive I-Archive I-Archive B-Archive B-Organization O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O B-Organization O B-Grant O O B-Archive O B-Telescope O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization O O B-Grant O O O O O O O O B-Person I-Person O O O O O B-Person I-Person O O O O O O B-Software I-Software
tokens: Acknowledgements This research received funding from the Hungarian Academy of Sciences through the Lendület grants LP2014-17 and LP2018-7, and the János Bolyai Research Scholarship (L.M. and E.P.); the Hungarian National Research, Development, and Innovation Office through the NKFIH grants K-115709, PD-116175, and PD-121203; and the ÚNKP-17-3 program of the Ministry of Human Capacities of Hungary (Á.L.J.). L.M. has been supported by the Premium Postdoctoral Research Program of the Hungarian Academy of Sciences. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, some of which participate in the Gaia Multilateral Agreement, which include, for Switzerland, the Swiss State Secretariat for Education, Research and Innovation through the ESA Prodex program, the “Mesures d’accompagnement”, the “Activités Nationales Complémentaires”, and the Swiss National Science Foundation. This paper includes data collected by the Kepler mission. Funding for the Kepler and K2 missions are provided by the NASA Science Mission Directorate. The Kepler/ K2 data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. We thank Carolyn Doherty for proofreading the manuscript, and Benjamin Montet for the fruitful discussions about the f3 code.