Poster Open Access
Santos, Angela R. G.;
Mathur, Savita;
García, Rafael A.;
Cunha, Margarida S.;
Avelino, Pedro P.;
Broomhall, Anne-Marie;
Egeland, Ricky;
Breton, Sylvain N.
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>Santos, Angela R. G.</dc:creator> <dc:creator>Mathur, Savita</dc:creator> <dc:creator>García, Rafael A.</dc:creator> <dc:creator>Cunha, Margarida S.</dc:creator> <dc:creator>Avelino, Pedro P.</dc:creator> <dc:creator>Broomhall, Anne-Marie</dc:creator> <dc:creator>Egeland, Ricky</dc:creator> <dc:creator>Breton, Sylvain N.</dc:creator> <dc:date>2021-10-06</dc:date> <dc:description>Rotational modulation due to dark spots co-rotating with the stellar surface allows us to constrain rotation and magnetic properties of solar-like stars. The long-term observations collected by Kepler (and those that will be collected by PLATO) are preferred for a better characterization of magnetic activity. In this work, we investigate the temporal variability of the photometric magnetic activity proxy Sph, as well as the characteristic timescale of active-regions in solar-like stars.</dc:description> <dc:description>Part of the results, particularly on the ACF for artificial date, are published and can be found here: https://ui.adsabs.harvard.edu/abs/2021MNRAS.508..267S/abstract The rotation and average S_ph catalog can be found here: https://ui.adsabs.harvard.edu/abs/2019ApJS..244...21S/abstract https://ui.adsabs.harvard.edu/abs/2021ApJS..255...17S/abstract The machine learning algorithm for rotation, ROOSTER, is described here: https://ui.adsabs.harvard.edu/abs/2021A%26A...647A.125B/abstract</dc:description> <dc:identifier>https://zenodo.org/record/5552868</dc:identifier> <dc:identifier>10.5281/zenodo.5552868</dc:identifier> <dc:identifier>oai:zenodo.org:5552868</dc:identifier> <dc:relation>doi:10.5281/zenodo.5552867</dc:relation> <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights> <dc:subject>stars: low-mass</dc:subject> <dc:subject>stars: rotation</dc:subject> <dc:subject>stars: activity</dc:subject> <dc:subject>starspots</dc:subject> <dc:subject>techniques: photometric</dc:subject> <dc:title>Photometric magnetic activity and active-region lifetimes of solar-like stars</dc:title> <dc:type>info:eu-repo/semantics/conferencePoster</dc:type> <dc:type>poster</dc:type> </oai_dc:dc>
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