October 10, 2021 Poster Open Access

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

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{
  "description": "<p>Well-characterized multiplanetary systems offer a unique opportunity for comparative planetology, allowing for investigations of the formation and evolution processes.&nbsp;I will present the analysis of a new multiplanetary system, TOI-561, initially discovered by the&nbsp;TESS&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).&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.</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "Universit\u00e0 degli Studi di Padova, INAF-OAPD", 
      "@id": "https://orcid.org/0000-0002-4197-7374", 
      "@type": "Person", 
      "name": "Lacedelli Gaia"
    }, 
    {
      "affiliation": "Universit\u00e0 degli Studi di Padova, INAF-OAPD", 
      "@id": "https://orcid.org/0000-0002-6492-2085", 
      "@type": "Person", 
      "name": "Malavolta Luca"
    }, 
    {
      "affiliation": "INAF-OAPD", 
      "@id": "https://orcid.org/0000-0003-0066-9268", 
      "@type": "Person", 
      "name": "Borsato Luca"
    }, 
    {
      "affiliation": "Universit\u00e0 degli Studi di Padova, INAF-OAPD", 
      "@id": "https://orcid.org/0000-0002-9937-6387", 
      "@type": "Person", 
      "name": "Piotto Giampaolo"
    }, 
    {
      "affiliation": "Laboratoire d'Astrophysique de Marseille", 
      "@id": "https://orcid.org/0000-0003-1149-3659", 
      "@type": "Person", 
      "name": "Nardiello Domenico"
    }, 
    {
      "@type": "Person", 
      "name": "the HARPS-N team"
    }, 
    {
      "@type": "Person", 
      "name": "the CHEOPS team"
    }
  ], 
  "sameAs": [
    "https://doi.org/10.5281/zenodo.5123553"
  ], 
  "datePublished": "2021-10-10", 
  "url": "https://zenodo.org/record/5559862", 
  "@type": "CreativeWork", 
  "keywords": [
    "Exoplanets", 
    "Exoplanets Detection And Characterization", 
    "Transits", 
    "Radial Velocity", 
    "TOI-561"
  ], 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5559862", 
  "@id": "https://doi.org/10.5281/zenodo.5559862", 
  "workFeatured": {
    "@type": "Event", 
    "name": "PLATO Mission Conference 2021"
  }, 
  "name": "CHEOPS, HARPS-N and TESS: a joint effort to characterize the unexpected planetary system around TOI-561"
}