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Planet Formation Imager: project update

hal.structure.identifierUniversity of Michigan [Ann Arbor]
dc.contributor.authorMONNIER, John
hal.structure.identifierDepartment of Astronomy [Ann Arbor]
dc.contributor.authorKRAUS, Stefan
hal.structure.identifierInstitut de Planétologie et d'Astrophysique de Grenoble [IPAG]
dc.contributor.authorBONSOR, Amy
hal.structure.identifierCavendish Laboratory
dc.contributor.authorBARON, Fabien
dc.contributor.authorBERGER, Jean-Philippe
dc.contributor.authorBOYAJIAN, Tabetha
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorCHIAVASSA, Andrea
dc.contributor.authorCIARDI, David
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorDE WIT, Willem-Jan
dc.contributor.authorDONG, Ruobing
dc.contributor.authorESPAILLAT, Catherine
hal.structure.identifierUniversidad de Concepción - University of Concepcion [Chile]
dc.contributor.authorGALLENNE, Alexandre
hal.structure.identifierSchool of Physics and Astronomy [Southampton]
dc.contributor.authorGANDHI, Poshak
hal.structure.identifierCentre de Recherche Astrophysique de Lyon [CRAL]
dc.contributor.authorGONZALEZ, Jean-François
dc.contributor.authorHANIFF, Chris
dc.contributor.authorHOENIG, Sebastian
dc.contributor.authorILEE, John
dc.contributor.authorISELLA, Andrea
dc.contributor.authorJENSEN, Eric
dc.contributor.authorJUHASZ, Attila
dc.contributor.authorKANE, Stephen
dc.contributor.authorKISHIMOTO, Makoto
dc.contributor.authorKLEY, Wilhelm
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA (UMR_8109)]
dc.contributor.authorKRAL, Quentin
dc.contributor.authorKRATTER, Kaitlin
dc.contributor.authorLABADIE, Lucas
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorLACOUR, Sylvestre
dc.contributor.authorLAUGHLIN, Greg
dc.contributor.authorLE BOUQUIN, Jean
hal.structure.identifierUniversity of Cyprus [Nicosia] [UCY]
dc.contributor.authorMICHAEL, Michael
dc.contributor.authorMERU, Farzana
hal.structure.identifierMichelson Science Center [MSC]
dc.contributor.authorMILLAN-GABET, Rafaël
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorMILLOUR, Florentin
hal.structure.identifierFriedrich-Schiller-Universität = Friedrich Schiller University Jena [Jena, Germany]
dc.contributor.authorMINARDI, Stefano
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorMORBIDELLI, Alessandro
dc.contributor.authorMORDASINI, Chris
hal.structure.identifierCentre de Recherches Pétrographiques et Géochimiques [CRPG]
dc.contributor.authorMORLOK, Andreas
dc.contributor.authorMOZURKEWICH, Dave
hal.structure.identifierQueen Mary University of London [QMUL]
dc.contributor.authorNELSON, Richard
dc.contributor.authorOUDMAIJER, Rene
dc.contributor.authorPACKHAM, Chris
hal.structure.identifierInstitut für Astronomie, Universität Wien [IFA]
dc.contributor.authorPALADINI, Claudia
dc.contributor.authorPANIC, Olja
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorPETROV, Romain
dc.contributor.authorPOPE, Benjamin
dc.contributor.authorPOTT, Joerg-Uwe
dc.contributor.authorQUIROGA-NUÑEZ, Luis Henry
dc.contributor.authorRAMOS ALMEIDA, Cristina
hal.structure.identifierECLIPSE 2018
dc.contributor.authorRAYMOND, Sean N.
dc.contributor.authorREGALY, Zsolt
hal.structure.identifierSchool of Computer Science and Software Engineering [Australia]
dc.contributor.authorREYNOLDS, Mark
hal.structure.identifierNational Optical Astronomy Observatory [NOAO]
dc.contributor.authorRIDGWAY, Stephen
dc.contributor.authorRINEHART, Stephen
dc.contributor.authorSMITH, Michael
dc.contributor.authorSTASSUN, Keivan
hal.structure.identifierInstitut d'Astrophysique et de Géophysique [Liège]
dc.contributor.authorSURDEJ, Jean
dc.contributor.authorTURNER, Neal
dc.contributor.authorVAN BELLE, Gerard
dc.contributor.authorVASISHT, Gautum
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWEIGELT, Gerd
dc.contributor.authorWISHNOW, Edward
hal.structure.identifierDepartment of Materials Science and Engineering
dc.contributor.authorWOLF, Sebastian
hal.structure.identifierHarbin University of Commerce [Heilongjiang]
dc.contributor.authorZHAO, Ming
dc.contributor.authorZHU, Zhaohuan
dc.contributor.authorSCHREIBER, Matthias
dc.contributor.authorDUCHÊNE, Gaspard
dc.contributor.authorBAYO, Amelia
dc.contributor.authorOLOFSSON, Johan
hal.structure.identifierCenter for High Angular Resolution Astronomy [CHARA]
dc.contributor.authorTEN BRUMMELAAR, Theo
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorTRISTRAM, Konrad
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorWITTKOWSKI, Markus
hal.structure.identifierCavendish Laboratory
dc.contributor.authorYOUNG, John
dc.contributor.authorWALLACE, Alexander
hal.structure.identifierSpace Sciences, Technologies and Astrophysics Research Institute [STAR]
dc.contributor.authorDEFRÈRE, Denis
dc.contributor.authorALONSO-HERRERO, Almudena
dc.contributor.authorZ'U~NIGA-FERN'ANDEZ, Sebasti'An
hal.structure.identifierCenter for High Angular Resolution Astronomy [CHARA]
dc.contributor.authorMÉRAND, Antoine
dc.contributor.authorCREECH-EAKMAN, Michelle
dc.contributor.authorTUTHILL, Peter
dc.date.issued2018
dc.date.conference2018-06-10
dc.description.abstractEnThe Planet Formation Imager (PFI) is a near- and mid-infrared interferometer project with the driving sciencegoal of imaging directly the key stages of planet formation, including the young proto-planets themselves. Here,we will present an update on the work of the Science Working Group (SWG), including new simulations of duststructures during the assembly phase of planet formation and quantitative detection efficiencies for accretingand non-accreting young exoplanets as a function of mass and age. We use these results to motivate tworeference PFI designs consisting of a) twelve 3 m telescopes with a maximum baseline of 1.2 km focused onyoung exoplanet imaging and b) twelve 8 m telescopes optimized for a wider range of young exoplanets andprotoplanetary disk imaging out to the 150 K H2O ice line. Armed with 4×8 m telescopes, the ESO/VLTI canalready detect young exoplanets in principle and projects such as MATISSE, Hi-5 and Heimdallr are important PFI pathfinders to make this possible. We also discuss the state of technology development needed to makePFI more affordable, including progress towards new designs for inexpensive, small field-of-view, large aperturetelescopes and prospects for Cubesat-based space interferometry
dc.language.isoen
dc.publisherSPIE
dc.subject.enInfrared interferometry
dc.subject.enPlanet formation
dc.subject.enPFI
dc.title.enPlanet Formation Imager: project update
dc.typeCommunication dans un congrès
dc.identifier.doi10.1117/12.2312683
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1807.11555
bordeaux.conference.titleOptical and Infrared Interferometry and Imaging VI - Proceedings of the SPIE, Volume 10701, id. 1070118 17 pp. (2018). 10-15 June 2018 Austin, Texas, United States
bordeaux.countryUS
bordeaux.conference.cityAustin
bordeaux.peerReviewedoui
hal.identifierhal-01901978
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2018-06-15
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01901978v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=MONNIER,%20John&KRAUS,%20Stefan&BONSOR,%20Amy&BARON,%20Fabien&BERGER,%20Jean-Philippe&rft.genre=unknown


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