Please use this identifier to cite or link to this item: http://hdl.handle.net/1942/40470
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dc.date.accessioned2023-06-26T10:08:40Z-
dc.date.available2023-06-26T10:08:40Z-
dc.date.issued2023-
dc.date.submitted2023-06-26T10:07:11Z-
dc.identifier.citationZenodo. 10.5281/zenodo.7816728 https://zenodo.org/record/7816728-
dc.identifier.urihttp://hdl.handle.net/1942/40470-
dc.description.abstractMESA and GYRE inlists, opacity tables, and supplementary material for the paper "Internal mixing of rotating stars inferred from dipole gravity modes" by Pedersen et al. (2021), Nature Astronomy, Volume 5, p. 715-722, DOI:10.1038/s41550-021-01351-x-
dc.description.sponsorshipEuropean Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 670519: MAMSIE)-
dc.description.sponsorshipNational Science Foundation (grant number NSF PHY-1748958)-
dc.description.sponsorshipKU Leuven Research Council (grant number C16/18/005: PARADISE)-
dc.description.sponsorshipResearch Foundation Flanders (FWO) by means of PhD Fellowships to M.M. and S. Gebruers under contract numbers 11F7120N and 11E5620N and a senior post-doctoral fellowship to D.M.B. under grant agreement number 1286521N-
dc.description.sponsorshipunding for the Kepler Mission was provided by NASA’s Science Mission Directorate.-
dc.language.isoen-
dc.publisherZenodo-
dc.subject.classificationStellar astrophysics-
dc.subject.otherAstronomy and astrophysics-
dc.subject.otherSeismology-
dc.subject.otherStars-
dc.subject.otherStellar Evolution-
dc.titleInternal mixing of rotating stars inferred from dipole gravity modes-
dc.typeDataset-
local.bibliographicCitation.jcatDS-
dc.description.version1.0-
dc.rights.licenseCreative Commons Attribution 4.0 International (CC-BY-4.0)-
dc.identifier.doi10.5281/zenodo.7816728-
dc.identifier.urlhttps://zenodo.org/record/7816728-
dc.description.otherWe thank the MESA and GYRE code developers for their efforts, public dissemination and training initiatives to make their software so accessible to the worldwide astrophysics community. We thank S. Ekström of the Geneva Observatory for providing mixing profiles from Georgy et al.4 in electronic format. We acknowledge the work of the teams behind the NASA Kepler and ESA Gaia space missions. This work is based on observations with the HERMES spectrograph at the Mercator Telescope, which is operated at La Palma, Spain, by the Flemish Community. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, and NASA’s Astrophysics Data System. The research leading to these results has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 670519: MAMSIE), from the National Science Foundation (grant number NSF PHY-1748958), from the KU Leuven Research Council (grant number C16/18/005: PARADISE) and from the Research Foundation Flanders (FWO) by means of PhD Fellowships to M.M. and S. Gebruers under contract numbers 11F7120N and 11E5620N and a senior post-doctoral fellowship to D.M.B. under grant agreement number 1286521N. Funding for the Kepler Mission was provided by NASA’s Science Mission Directorate. Gaia data are being processed by the Gaia Data Processing and Analysis Consortium (DPAC); funding for the DPAC is provided by national institutions, in particular the institutions participating in the Gaia MultiLateral Agreement (MLA).-
local.provider.typedatacite-
local.uhasselt.internationalyes-
local.contributor.datacreatorPedersen, May G.-
local.contributor.datacreatorAerts, Conny-
local.contributor.datacreatorPápics, Péter I.-
local.contributor.datacreatorMichielsen, Mathias-
local.contributor.datacreatorGebruers, Sarah-
local.contributor.datacreatorRogers, Tamara M.-
local.contributor.datacreatorMOLENBERGHS, Geert-
local.contributor.datacreatorBurssens, Siemen-
local.contributor.datacreatorGarcia, Stefano-
local.contributor.datacreatorBowman, Dominic M.-
local.contributor.datacuratorPedersen, May G.-
local.contributor.rightsholderPedersen, May G.-
local.format.extent127.4 Mb-
local.format.mimetypezip-
local.format.mimetypetxt-
local.format.mimetypepdf-
local.contributororcid.datacreator0000-0002-7950-0061-
local.contributororcid.datacreator0000-0003-1822-7126-
local.contributororcid.datacreator0000-0001-9097-3655-
local.contributororcid.datacreator0000-0001-8426-4158-
local.contributororcid.datacreator0000-0002-6453-5448-
local.contributororcid.datacreator0000-0002-1593-0863-
local.contributororcid.datacreator0000-0001-7354-711X-
local.contributororcid.datacreator0000-0001-7402-3852-
local.contributororcid.datacurator0000-0002-7950-0061-
local.contributororcid.rightsholder0000-0002-7950-0061-
local.publication.doi10.1038/s41550-021-01351-x-
local.contributingorg.datacreatorKU Leuven-
local.contributingorg.datacreatorUniversity of California, Santa Barbara-
local.contributingorg.datacreatorRadboud University Nijmegen-
local.contributingorg.datacreatorMax Planck Institute for Astronomy, Heidelberg-
local.contributingorg.datacreatorNewcastle University-
local.contributingorg.datacreatorPlanetary Science Institute, Tucson-
local.contributingorg.datacreatorHasselt University-
local.contributingorg.datacuratorKU Leuven-
local.contributingorg.datacuratorUniversity of California, Santa Barbara-
local.contributingorg.rightsholderKU Leuven-
local.contributingorg.rightsholderUniversity of California, Santa Barbara-
dc.rights.accessOpen Access-
item.fulltextNo Fulltext-
item.accessRightsClosed Access-
item.contributorPedersen, May G.-
item.contributorAerts, Conny-
item.contributorPápics, Péter I.-
item.contributorMichielsen, Mathias-
item.contributorGebruers, Sarah-
item.contributorRogers, Tamara M.-
item.contributorMOLENBERGHS, Geert-
item.contributorBurssens, Siemen-
item.contributorGarcia, Stefano-
item.contributorBowman, Dominic M.-
item.fullcitationPedersen, May G.; Aerts, Conny; Pápics, Péter I.; Michielsen, Mathias; Gebruers, Sarah; Rogers, Tamara M.; MOLENBERGHS, Geert; Burssens, Siemen; Garcia, Stefano & Bowman, Dominic M. (2023) Internal mixing of rotating stars inferred from dipole gravity modes. Zenodo. 10.5281/zenodo.7816728 https://zenodo.org/record/7816728.-
crisitem.license.codeCC-BY-4.0-
crisitem.license.nameCreative Commons Attribution 4.0 International (CC-BY-4.0)-
crisitem.discipline.code01030115-
crisitem.discipline.nameStellar astrophysics-
crisitem.discipline.pathNatural sciences > Physical sciences > Astronomy and space sciences > Stellar astrophysics-
crisitem.discipline.pathandcodeNatural sciences > Physical sciences > Astronomy and space sciences > Stellar astrophysics (01030115)-
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