October 10, 2021 Poster Open Access

Lacedelli Gaia; Malavolta Luca; Borsato Luca; Piotto Giampaolo; Nardiello Domenico; the HARPS-N team; the CHEOPS team

MARC21 XML Export

<?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">Exoplanets</subfield>
  </datafield>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">Exoplanets Detection And Characterization</subfield>
  </datafield>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">Transits</subfield>
  </datafield>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">Radial Velocity</subfield>
  </datafield>
  <datafield tag="653" ind1=" " ind2=" ">
    <subfield code="a">TOI-561</subfield>
  </datafield>
  <controlfield tag="005">20211011014836.0</controlfield>
  <controlfield tag="001">5559862</controlfield>
  <datafield tag="711" ind1=" " ind2=" ">
    <subfield code="d">11-15 October, 2021</subfield>
    <subfield code="a">PLATO Mission Conference 2021</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">Università degli Studi di Padova, INAF-OAPD</subfield>
    <subfield code="0">(orcid)0000-0002-6492-2085</subfield>
    <subfield code="a">Malavolta Luca</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">INAF-OAPD</subfield>
    <subfield code="0">(orcid)0000-0003-0066-9268</subfield>
    <subfield code="a">Borsato Luca</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">Università degli Studi di Padova, INAF-OAPD</subfield>
    <subfield code="0">(orcid)0000-0002-9937-6387</subfield>
    <subfield code="a">Piotto Giampaolo</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="u">Laboratoire d'Astrophysique de Marseille</subfield>
    <subfield code="0">(orcid)0000-0003-1149-3659</subfield>
    <subfield code="a">Nardiello Domenico</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">the HARPS-N team</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">the CHEOPS team</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">4479075</subfield>
    <subfield code="z">md5:9b34bd4d23ab051f95be340c672ab78a</subfield>
    <subfield code="u">https://zenodo.org/record/5559862/files/poster_PLATO_Lacedelli.pdf</subfield>
  </datafield>
  <datafield tag="542" ind1=" " ind2=" ">
    <subfield code="l">open</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2021-10-10</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:5559862</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="u">Università degli Studi di Padova, INAF-OAPD</subfield>
    <subfield code="0">(orcid)0000-0002-4197-7374</subfield>
    <subfield code="a">Lacedelli Gaia</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">CHEOPS, HARPS-N and TESS: a joint effort to characterize the unexpected planetary system around TOI-561</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">&lt;p&gt;Well-characterized multiplanetary systems offer a unique opportunity for comparative planetology, allowing for investigations of the formation and evolution processes.&amp;nbsp;I will present the analysis of a new multiplanetary system, TOI-561, initially discovered by the&amp;nbsp;TESS&amp;nbsp;mission through photometric observations, and further characterized using high-precision RV data collected with the HARPS-N spectrograph, that allowed us to obtain precise masses for all the four planets in the system, namely an ultra-short period super-Earth and three mini-Neptunes (Lacedelli et al. 2021).&amp;nbsp; I will show how in this case combining photometric and RV data has been essential to discriminate between various possible architectures, highlighting the importance of combining different techniques to obtain a better characterization of a planetary system. Additional insights on the planetary architecture and internal structure are coming from the ultra-high precision photometry of the CHEOPS satellite (Lacedelli et al., in prep), which additionally stresses the importance of synergies between various techniques and instruments.&lt;/p&gt;</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="n">doi</subfield>
    <subfield code="i">isIdenticalTo</subfield>
    <subfield code="a">10.5281/zenodo.5123553</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="n">doi</subfield>
    <subfield code="i">isDocumentedBy</subfield>
    <subfield code="a">10.1093/mnras/staa3728</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="n">doi</subfield>
    <subfield code="i">isVersionOf</subfield>
    <subfield code="a">10.5281/zenodo.5559861</subfield>
  </datafield>
  <datafield tag="024" ind1=" " ind2=" ">
    <subfield code="a">10.5281/zenodo.5559862</subfield>
    <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">poster</subfield>
  </datafield>
</record>