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'?> <record xmlns="http://www.loc.gov/MARC21/slim"> <leader>00000nam##2200000uu#4500</leader> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">stars: low-mass</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">stars: rotation</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">stars: activity</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">starspots</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">techniques: photometric</subfield> </datafield> <controlfield tag="005">20211011180317.0</controlfield> <controlfield tag="001">5552872</controlfield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Instituto de Astrofísica de Canarias</subfield> <subfield code="0">(orcid)0000-0002-0129-0316</subfield> <subfield code="a">Mathur, Savita</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">CEA, Université Paris-Saclay</subfield> <subfield code="0">(orcid)0000-0002-8854-3776</subfield> <subfield code="a">García, Rafael A.</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Instituto de Astrofísica e Ciências do Espaço</subfield> <subfield code="0">(orcid)0000-0001-8237-7343</subfield> <subfield code="a">Cunha, Margarida S.</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Instituto de Astrofísica e Ciências do Espaço</subfield> <subfield code="0">(orcid)0000-0002-1440-6963</subfield> <subfield code="a">Avelino, Pedro P.</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Department of Physics, University of Warwick</subfield> <subfield code="0">(orcid)0000-0002-5209-9378</subfield> <subfield code="a">Broomhall, Anne-Marie</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">NASA Johnson Space Center</subfield> <subfield code="0">(orcid)0000-0002-4996-0753</subfield> <subfield code="a">Egeland, Ricky</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">CEA, Université Paris-Saclay</subfield> <subfield code="0">(orcid)0000-0003-0377-0740</subfield> <subfield code="a">Breton, Sylvain N.</subfield> </datafield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="s">2589439</subfield> <subfield code="z">md5:642d7f244232bc708e628044ade6f469</subfield> <subfield code="u">https://zenodo.org/record/5552872/files/poster_ARGSantos.pdf</subfield> </datafield> <datafield tag="542" ind1=" " ind2=" "> <subfield code="l">open</subfield> </datafield> <datafield tag="260" ind1=" " ind2=" "> <subfield code="c">2021-10-06</subfield> </datafield> <datafield tag="909" ind1="C" ind2="O"> <subfield code="p">openaire</subfield> <subfield code="p">user-plato2021</subfield> <subfield code="o">oai:zenodo.org:5552872</subfield> </datafield> <datafield tag="100" ind1=" " ind2=" "> <subfield code="u">Department of Physics, University of Warwick</subfield> <subfield code="0">(orcid)0000-0001-7195-6542</subfield> <subfield code="a">Santos, Angela R. G.</subfield> </datafield> <datafield tag="245" ind1=" " ind2=" "> <subfield code="a">Photometric magnetic activity and active-region lifetimes of solar-like stars</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">user-plato2021</subfield> </datafield> <datafield tag="540" ind1=" " ind2=" "> <subfield code="u">https://creativecommons.org/licenses/by/4.0/legalcode</subfield> <subfield code="a">Creative Commons Attribution 4.0 International</subfield> </datafield> <datafield tag="650" ind1="1" ind2="7"> <subfield code="a">cc-by</subfield> <subfield code="2">opendefinition.org</subfield> </datafield> <datafield tag="520" ind1=" " ind2=" "> <subfield code="a"><p>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 <em>Kepler</em> (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 S<sub>ph</sub>, as well as the characteristic timescale of active-regions in solar-like stars.</p></subfield> </datafield> <datafield tag="773" ind1=" " ind2=" "> <subfield code="n">doi</subfield> <subfield code="i">isVersionOf</subfield> <subfield code="a">10.5281/zenodo.5552867</subfield> </datafield> <datafield tag="024" ind1=" " ind2=" "> <subfield code="a">10.5281/zenodo.5552872</subfield> <subfield code="2">doi</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">poster</subfield> </datafield> </record>
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