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dc.contributor.authorDesidera, S.en
dc.contributor.authorChauvin, G.en
dc.contributor.authorBonavita, M.en
dc.contributor.authorMessina, S.en
dc.contributor.authorLecoroller, H.en
dc.contributor.authorSchmidt, T.en
dc.contributor.authorGratton, R.en
dc.contributor.authorLazzoni, C.en
dc.contributor.authorMeyer, M.en
dc.contributor.authorSchlieder, J.en
dc.contributor.authorCheetham, A.en
dc.contributor.authorHagelberg, J.en
dc.contributor.authorBonnefoy, M.en
dc.contributor.authorFeldt, M.en
dc.contributor.authorLagrange, A. -M.en
dc.contributor.authorLanglois, M.en
dc.contributor.authorVigan, A.en
dc.contributor.authorTan, T. G.en
dc.contributor.authorHambsch, F. -J.en
dc.contributor.authorMillward, M.en
dc.contributor.authorAlcalá, J.en
dc.contributor.authorBenatti, S.en
dc.contributor.authorBrandner, W.en
dc.contributor.authorCarson, J.en
dc.contributor.authorCovino, E.en
dc.contributor.authorDelorme, P.en
dc.contributor.authorD'Orazi, V.en
dc.contributor.authorJanson, M.en
dc.contributor.authorRigliaco, E.en
dc.contributor.authorBeuzit, J. -L.en
dc.contributor.authorBiller, B.en
dc.contributor.authorBoccaletti, A.en
dc.contributor.authorDominik, C.en
dc.contributor.authorCantalloube, F.en
dc.contributor.authorFontanive, C.en
dc.contributor.authorGalicher, R.en
dc.contributor.authorHenning, T.en
dc.contributor.authorLagadec, E.en
dc.contributor.authorLigi, R.en
dc.contributor.authorMaire, A. -L.en
dc.contributor.authorMenard, F.en
dc.contributor.authorMesa, D.en
dc.contributor.authorMüller, A.en
dc.contributor.authorSamland, M.en
dc.contributor.authorSchmid, H. M.en
dc.contributor.authorSissa, E.en
dc.contributor.authorTuratto, M.en
dc.contributor.authorUdry, S.en
dc.contributor.authorZurlo, A.en
dc.contributor.authorAsensio-Torres, R.en
dc.contributor.authorKopytova, T.en
dc.contributor.authorRickman, E.en
dc.contributor.authorAbe, L.en
dc.contributor.authorAntichi, J.en
dc.contributor.authorBaruffolo, A.en
dc.contributor.authorBaudoz, P.en
dc.contributor.authorBaudrand, J.en
dc.contributor.authorBlanchard, P.en
dc.contributor.authorBazzon, A.en
dc.contributor.authorBuey, T.en
dc.contributor.authorCarbillet, M.en
dc.contributor.authorCarle, M.en
dc.contributor.authorCharton, J.en
dc.contributor.authorCascone, E.en
dc.contributor.authorClaudi, R.en
dc.contributor.authorCostille, A.en
dc.contributor.authorDeboulbé, A.en
dc.contributor.authorDe Caprio, V.en
dc.contributor.authorDohlen, K.en
dc.contributor.authorFantinel, D.en
dc.contributor.authorFeautrier, P.en
dc.contributor.authorFusco, T.en
dc.contributor.authorGigan, P.en
dc.contributor.authorGiro, E.en
dc.contributor.authorGisler, D.en
dc.contributor.authorGluck, L.en
dc.contributor.authorHubin, N.en
dc.contributor.authorHugot, E.en
dc.contributor.authorJaquet, M.en
dc.contributor.authorKasper, M.en
dc.contributor.authorMadec, F.en
dc.contributor.authorMagnard, Y.en
dc.contributor.authorMartinez, P.en
dc.contributor.authorMaurel, D.en
dc.contributor.authorLe Mignant, D.en
dc.contributor.authorMöller-Nilsson, O.en
dc.contributor.authorLlored, M.en
dc.contributor.authorMoulin, T.en
dc.contributor.authorOrigné, A.en
dc.contributor.authorPavlov, A.en
dc.contributor.authorPerret, D.en
dc.contributor.authorPetit, C.en
dc.contributor.authorPragt, J.en
dc.contributor.authorPuget, P.en
dc.contributor.authorRabou, P.en
dc.contributor.authorRamos, J.en
dc.contributor.authorRigal, F.en
dc.contributor.authorRochat, S.en
dc.contributor.authorRoelfsema, R.en
dc.contributor.authorRousset, G.en
dc.contributor.authorRoux, A.en
dc.contributor.authorSalasnich, B.en
dc.contributor.authorSauvage, J. -F.en
dc.contributor.authorSevin, A.en
dc.contributor.authorSoenke, C.en
dc.contributor.authorStadler, E.en
dc.contributor.authorSuarez, M.en
dc.contributor.authorWeber, L.en
dc.contributor.authorWildi, F.en
dc.date.accessioned2022-05-12T08:18:57Z-
dc.date.available2022-05-12T08:18:57Z-
dc.date.issued2021-
dc.identifier.citationThe SPHERE Infrared Survey for Exoplanets (SHINE): I. Sample Definition and Target Characterization / S. Desidera, G. Chauvin, M. Bonavita et al. — DOI 10.1117/12.2207781 // Astronomy and Astrophysics. — 2021. — Vol. 651. — A70.en
dc.identifier.issn0004-6361-
dc.identifier.otherAll Open Access, Green3
dc.identifier.urihttp://elar.urfu.ru/handle/10995/111539-
dc.description.abstractLarge surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from ~5 to 300 au. A careful assessment of the stellar properties is crucial for a proper understanding of when, where, and how frequently planets form, and how they evolve. The sensitivity of detection limits to stellar age makes this a key parameter for direct imaging surveys. Aims. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the context of the SPHERE Guaranteed Time Observations of the SPHERE consortium. In this first paper we present the selection and the properties of the complete sample of stars surveyed with SHINE, focusing on the targets observed during the first phase of the survey (from February 2015 to February 2017). This early sample composed of 150 stars is used to perform a preliminary statistical analysis of the SHINE data, deferred to two companion papers presenting the survey performance, main discoveries, and the preliminary statistical constraints set by SHINE. Methods. Based on a large database collecting the stellar properties of all young nearby stars in the solar vicinity (including kinematics, membership to moving groups, isochrones, lithium abundance, rotation, and activity), we selected the original sample of 800 stars that were ranked in order of priority according to their sensitivity for planet detection in direct imaging with SPHERE. The properties of the stars that are part of the early statistical sample wererevisited, including for instance measurements from the Gaia Data Release 2. Rotation periods were derived for the vast majority of the late-type objects exploiting TESS light curves and dedicated photometric observations. Results. The properties of individual targets and of the sample as a whole are presented. © ESO 2021.en
dc.description.sponsorshipSPHERE is an instrument designed and built by a consortium consisting of IPAG (Grenoble, France), MPIA (Heidelberg, Germany), LAM (Marseille, France), LESIA (Paris, France), Laboratoire Lagrange (Nice, France), INAF – Osservatorio di Padova (Italy), Observatoire de Genève (Switzerland), ETH Zürich (Switzerland), NOVA (Netherlands), ONERA (France) and ASTRON (Netherlands) in collaboration with ESO. SPHERE was funded by ESO, with additional contributions from CNRS (France), MPIA (Germany), INAF (Italy), FINES (Switzerland) and NOVA (Netherlands). SPHERE also received funding from the European Commission Sixth and Seventh Framework Programmes as part of the Optical Infrared Coordination Network for Astronomy (OPTICON) under grant number RII3-Ct-2004-001566 for FP6 (2004–2008), grant number 226 604 for FP7 (2009–2012) and grant number 312430 for FP7 (2013–2016). This research has made use of the SIMBAD database and Vizier services, operated at CDS, Strasbourg, France and of the Washington Double Star Catalog maintained at the US Naval Observatory. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. This paper has made use of data products available in ESO archive. Program ID: 60.A-9036(A); 072.C-0488(E) (PI Mayor), 074.C-0364(A) (PI Robichon), 074.C-0037(A) (PI Gunther), 075.C-0202(A) (PI Gunther), 075.C-0689(A) (PI Galland), 076.C-0010(A) (PI Gunther), 077.C-0012(A) (PI Gunther), 077.C-0295(D) (PI Galland), 078.D-0245(C) (PI Dall), 079.C-0046(A) (PI Gunther), 080.D-0151(A) (PI Hatzes), 080.C-0712(A) (PI Desort), 180.C-0886(A) (PI Bonfils), 082.C-0718(B) (PI Bonfils), 082.C-0427(A) (PI Doellinger), 082.C-0390(A) (PI Weise), 183.C-0437(A) (PI Bonfils), 083.C-0794(A) (PI Chauvin), 084.C-1039(A) (PI Chauvin), 184.C-0815(B) (PI Desort), 089.C-0732(A) (PI Lo Curto), 191.C-0873(D) (PI Bonfils), 192.C-0224(A) (PI Lagrange), 097.C-0864(B) (PI Lannier), 098.C-0739(A) (PI Lagrange), 099.C-0205(A) (PI Lagrange), 099.C-0458(A) (PI Lo Curto), 1101.C-0557(A) (PI Lagrange). We have used data from the WASP public archive in this research. The WASP consortium comprises of the University of Cambridge, Keele University, University of Leicester, The Open University, The Queen’s University Belfast, St. Andrews University and the Isaac Newton Group. Funding for WASP comes from the consortium universities and from the UK’s Science and Technology Facilities Council. Based on data retrieved from the SOPHIE archive at Observatoire de Haute-Provence (OHP), available at http://atlas.obs-hp.fr/sophie/. We thank the anonymous referee for useful comments. S.D., V.D., D.M. and R.G. acknowledge the support by INAF/Frontiera through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research, the PRIN-INAF 2019 “Planetary systems at young ages” (PLATEA) and the ASI-INAF agreement n.2018-16-HH.0. AV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 757561). A.M.L. acknowledges funding from Agence Nationale de la Recherche (France) under contract number ANR-14-CE33-0018. J.C. was supported by SC Space Grant and Fulbright Colombia. M.B. acknowledges funding by the UK Science and Technology Facilities Council (STFC) grant no. ST/M001229.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherEDP Sciencesen1
dc.publisherEDP Sciencesen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceAstron. Astrophys.2
dc.sourceAstronomy and Astrophysicsen
dc.subjectPLANETS AND SATELLITES: GENERALen
dc.subjectSTARS: ACTIVITYen
dc.subjectSTARS: FUNDAMENTAL PARAMETERSen
dc.subjectSTARS: KINEMATICS AND DYNAMICSen
dc.subjectSTARS: PRE-MAIN SEQUENCEen
dc.subjectSTARS: ROTATIONen
dc.subjectEXTRASOLAR PLANETSen
dc.subjectSPHERESen
dc.subjectSURVEYSen
dc.subjectDETECTION LIMITSen
dc.subjectHIGH CONTRAST IMAGINGen
dc.subjectORIGINAL SAMPLEen
dc.subjectPLANET DETECTIONen
dc.subjectROTATION PERIODen
dc.subjectSTATISTICAL CONSTRAINTSen
dc.subjectSTATISTICAL SAMPLESen
dc.subjectTARGET CHARACTERIZATIONen
dc.subjectSTARSen
dc.titleThe SPHERE Infrared Survey for Exoplanets (SHINE): I. Sample Definition and Target Characterizationen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.typeinfo:eu-repo/semantics/submittedVersionen
dc.identifier.rsi46910314-
dc.identifier.doi10.1117/12.2207781-
dc.identifier.scopus85110441170-
local.contributor.employeeDesidera, S., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Chauvin, G., Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Bonavita, M., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy, Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom, Centre for Exoplanet Science, University of Edinburgh, Edinburgh, EH9 3HJ, United Kingdom; Messina, S., Inaf - Osservatorio Astrofisico di Catania, Via S. Sofia 78, Catania, 95123, Italy; Lecoroller, H., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Schmidt, T., Hamburger Sternwarte, Gojenbergsweg 112, Hamburg, 21029, Germany, Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Gratton, R., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Lazzoni, C., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy, Dipartimento di Fisica e Astronomia Galileo Galilei, Universitá di Padova, Vicolo dell'Osservatorio 3, Padova, 35122, Italy; Meyer, M., Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, United States, Institute for Particle Physics and Astrophysics, Eth Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland; Schlieder, J., Exoplanets and Stellar Astrophysics Laboratory, Code 667, Nasa Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, United States, Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Cheetham, A., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany, Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Hagelberg, J., Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Bonnefoy, M., Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Feldt, M., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Lagrange, A.-M., Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Langlois, M., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France, Cral, Cnrs, Université Lyon 1, Université de Lyon, Ens, 9 avenue Charles Andre, Saint Genis Laval, 69561, France; Vigan, A., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Tan, T.G., Perth Exoplanet Survey TelescopeWA, Australia; Hambsch, F.-J., Remote Observatory Atacama Desert, Chile; Millward, M., York Creek Observatory, Georgetown, TN, Australia; Alcalá, J., Inaf - Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, Napoli, 80131, Italy; Benatti, S., Inaf - Osservatorio Astronomico di Palermo, Piazza del Parlamento, 1, Palermo, 90134, Italy; Brandner, W., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Carson, J., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany, College of Charleston, Department of Physics and Astronomy, 66 George St, Charleston, SC 29424, United States; Covino, E., Inaf - Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, Napoli, 80131, Italy; Delorme, P., Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; D'Orazi, V., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Janson, M., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany, Department of Astronomy, Stockholm University, Stockholm, 10691, Sweden; Rigliaco, E., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Beuzit, J.-L., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Biller, B., Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom, Centre for Exoplanet Science, University of Edinburgh, Edinburgh, EH9 3HJ, United Kingdom, Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Boccaletti, A., Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Dominik, C., Anton Pannekoek Institute for Astronomy, Science Park 9, XH Amsterdam, 1098, Netherlands; Cantalloube, F., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Fontanive, C., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy, Center for Space and Habitability, University of Bern, Bern, 3012, Switzerland; Galicher, R., Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Henning, T., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Lagadec, E., Université Cote d'Azur, Oca, Cnrs, Lagrange, France; Ligi, R., Inaf - Osservatorio Astronomico di Brera, Via E. Bianchi 46, Merate, 23807, Italy; Maire, A.-L., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany, Star Institute, University of Liège, Allée du Six Août 19c, Liège, 4000, Belgium; Menard, F., Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Mesa, D., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Müller, A., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Samland, M., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Schmid, H.M., Institute for Particle Physics and Astrophysics, Eth Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland; Sissa, E., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Turatto, M., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Udry, S., Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Zurlo, A., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France, Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. 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Ejercito 441, Santiago, Chile; Asensio-Torres, R., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Kopytova, T., Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany, Dkfz, Heidelberg, Germany, Ural Federal University, Yekaterinburg, 620002, Russian Federation; Rickman, E., Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Abe, L., Université Cote d'Azur, Oca, Cnrs, Lagrange, France; Antichi, J., Inaf - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi 5, Firenze, 50125, Italy; Baruffolo, A., Inaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Baudoz, P., Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Baudrand, J., Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Blanchard, P., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Bazzon, A., Institute for Particle Physics and Astrophysics, Eth Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland; Buey, T., Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Carbillet, M., Université Cote d'Azur, Oca, Cnrs, Lagrange, France; Carle, M., Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Charton, J., Univ. 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Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Suarez, M., Onera Office National DEtudes et de Recherches Arospatiales, B.P.72, Chatillon, 92322, France; Weber, L., Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Wildi, F., Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerlanden
local.volume651-
dc.identifier.wos000756538900003-
local.contributor.departmentInaf - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, 35122, Italy; Univ. Grenoble Alpes, Cnrs, Ipag, Grenoble, 38000, France; Supa, Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, United Kingdom; Centre for Exoplanet Science, University of Edinburgh, Edinburgh, EH9 3HJ, United Kingdom; Inaf - Osservatorio Astrofisico di Catania, Via S. Sofia 78, Catania, 95123, Italy; Aix Marseille Univ, Cnrs, Cnes, Lam, Marseille, France; Hamburger Sternwarte, Gojenbergsweg 112, Hamburg, 21029, Germany; Lesia Observatoire de Paris, Université Psl, Cnrs, Sorbonne Université, Université de Paris, 5 place Jules Janssen, Meudon, 92195, France; Dipartimento di Fisica e Astronomia Galileo Galilei, Universitá di Padova, Vicolo dell'Osservatorio 3, Padova, 35122, Italy; Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, United States; Institute for Particle Physics and Astrophysics, Eth Zurich, Wolfgang-Pauli-Strasse 27, Zurich, 8093, Switzerland; Exoplanets and Stellar Astrophysics Laboratory, Code 667, Nasa Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, United States; Max Planck Institute for Astronomy, Königstuhl 17, Heidelberg, 69117, Germany; Geneva Observatory, University of Geneva, Chemin des Mailettes 51, Versoix, 1290, Switzerland; Cral, Cnrs, Université Lyon 1, Université de Lyon, Ens, 9 avenue Charles Andre, Saint Genis Laval, 69561, France; Perth Exoplanet Survey TelescopeWA, Australia; Remote Observatory Atacama Desert, Chile; York Creek Observatory, Georgetown, TN, Australia; Inaf - Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, Napoli, 80131, Italy; Inaf - Osservatorio Astronomico di Palermo, Piazza del Parlamento, 1, Palermo, 90134, Italy; College of Charleston, Department of Physics and Astronomy, 66 George St, Charleston, SC 29424, United States; Department of Astronomy, Stockholm University, Stockholm, 10691, Sweden; Anton Pannekoek Institute for Astronomy, Science Park 9, XH Amsterdam, 1098, Netherlands; Center for Space and Habitability, University of Bern, Bern, 3012, Switzerland; Université Cote d'Azur, Oca, Cnrs, Lagrange, France; Inaf - Osservatorio Astronomico di Brera, Via E. Bianchi 46, Merate, 23807, Italy; Star Institute, University of Liège, Allée du Six Août 19c, Liège, 4000, Belgium; Núcleo de Astronomía, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejercito 441, Santiago, Chile; Escuela de Ingeniería Industrial, Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Av. Ejercito 441, Santiago, Chile; Dkfz, Heidelberg, Germany; Ural Federal University, Yekaterinburg, 620002, Russian Federation; Inaf - Osservatorio Astrofisico di Arcetri Largo Enrico Fermi 5, Firenze, 50125, Italy; Onera Office National DEtudes et de Recherches Arospatiales, B.P.72, Chatillon, 92322, France; European Southern Observatory (ESO), Karl-Schwarzschild-Str. 2, Garching, 85748, Germany; Nova Optical Infrared Instrumentation Group, Oude Hoogeveensedijk 4, Dwingeloo, 7991 PD, Netherlandsen
local.identifier.pure23003805-
local.description.orderA70-
local.identifier.eid2-s2.0-85110441170-
local.fund.cordisH2020: 757561-
local.identifier.wosWOS:000756538900003-
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