The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry

Supporting data of the peer-reviewed paper "The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry" published in MNRAS in 2026. For the purpose of open access, the authors have applied a CC BY licence to the author accepted manuscript version: https://arxiv.org/abs/2608.03383 The TESS data used in this work are publicly available via the MAST website: https://archive.stsci.edu/missions-and-data/tess. The HERMES data used in this work are publicly available via the Mercator Observatory Archive website: https://www.mercator.iac.es/instruments/hermes/archive/. The GAIA data used in this work are publicly available via the Gaia website: https://gea.esac.esa.int/archive/, processed by the Gaia Data Processing and Analysis Consortium (DPAC). This work was supported by UK Research and Innovation (UKRI) in the form of a Frontier Research grant under the UK government’s ERC Horizon Europe funding guarantee (SYMPHONY; PI Bowman; grant number: EP/Y031059/1), and a Royal Society University Research Fellowship (PI Bowman; grant number: URF\R1\231631). This project received support from the “La Caixa” Foundation (ID 100010434) under the fellowship code LCF/BQ/PI23/11970035, by an NWO Veni fellowship (VI.Veni.242.199), by the Polish National Center for Science (NCN) through grant 2021/43/B/ST9/02972, from the Israel Science Foundation (grant number 2752/19), from the Pazy foundation (grant number 216312), from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement number 852097), from the Israel Science Foundation (ISF) under grant number 0603225041 and from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement 101164755/METAL), from the State Research Agency (AEI) of the Spanish Ministry of Science and Innovation (MICIN) and the European Regional Development Fund, FEDER under grants PRODUCTOS DE LA INTERACCION DE ESTRELLAS MASIVAS REVELADOS POR GRANDES SONDEOS ESPECTROSCOPICOS, with reference PID2024-159329NB-C21, from the European Commission (EC) under Project OCEANS - Over-coming challenges in the evolution and nature of massive stars, HORIZON-MSCA-2023-SE-01, No G.A 101183150 funded by the European Union, from the BELgian federal Science Policy Office (BELSPO) through PRODEX grant PLATO (ZKE8588), from the Flemish Government under the long-term structural Methusalem funding program by means of the project SOUL: Stellar evolution in full glory, grant METH/24/012 at KU Leuven, and from the Research Foundation – Flanders (FWO) (grantagreement G0ABL24N). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them.