Reference : Planet formation imager: Project update
Scientific congresses and symposiums : Paper published in a journal
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/228659
Planet formation imager: Project update
English
Monnier, J. D. [Univ. of Michigan, United States]
Ireland, M. [Australian National Univ., Australia]
Kraus, S. [Univ. of Exeter, United Kingdom]
Alonso-Herrero, A. [Centro de Astrobiologia (CSIC-INTA), Spain]
Bonsor, A. [Univ. of Cambridge, United Kingdom]
Baron, Fabien [> >]
Bayo, A. [Univ. de Valparaso, Chile, Núcleo Milenio Formación Planetaria (NPF), Chile]
Berger, J.-P. [Univ. Grenoble Alpes, France]
Boyajian, T. [Louisiana State Univ., United States]
Chiavassa, A. [Observatoire de la Côte d'Azur, France]
Ciardi, D. [Infrared Processing and Analysis Ctr., United States]
Creech-Eakman, M. [New Mexico Institute of Mining and Technology, United States]
De Wit, W.-J. [European Southern Observatory, Chile]
Defrere, Denis mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > ISSPSILAB >]
Dong, R. [Univ. of Arizona, United States]
Duchêne, G. [Univ. Grenoble Alpes, France, Univ. of California, Berkeley, United States]
Espaillat, C. [Boston Univ., United States]
Gallenne, A. [European Southern Observatory, Chile]
Gandhi, P. [Univ. of Southampton, United Kingdom]
Gonzalez, J.-F. [Univ. de Lyon, France]
Haniff, C. [Univ. of Cambridge, United Kingdom]
Hoenig, S. [Univ. of Southampton, United Kingdom]
Ilee, J. [Univ. of Cambridge, United Kingdom]
Isella, A. [Rice Univ., United States]
Jensen, E. [Swarthmore College, United States]
Juhasz, A. [Univ. of Cambridge, United Kingdom]
Kane, S. [Univ. of California, Riverside, United States]
Kishimoto, M. [Kyoto Sangyo Univ., Japan]
Kley, W. [Eberhard Karls Univ. Tübingen, Germany]
Kral, Q. [Univ. of Cambridge, United Kingdom]
Kratter, K. [Univ. of Arizona, United States]
Labadie, L. [Univ. zu Köln, Germany]
Lacour, S. [Observatoire de Paris, France]
Laughlin, G. [Yale Univ., United States]
Le Bouquin, J.-B. [Univ. Grenoble Alpes, France]
Michael, E. [Univ. de Chile, Chile]
Meru, F. [Univ. of Cambridge, United Kingdom]
Millan-Gabet, R. [GMTO Corp., United States]
Millour, F. [Observatoire de la Côte d'Azur, France]
Minardi, S. [Institute of Applied Physics, Friedrich-Schiller-Univ. Jena, Germany]
Morbidelli, A. [Observatoire de la Côte d'Azur, France]
Mordasini, C. [Univ. Bern, Switzerland]
Morlok, A. [Westische Wilhelms-Univ. Münster, Germany]
Mozurkewich, D. [Seabrook Engineering, United States]
Nelson, R. [Queen Mary Univ. of London, United Kingdom]
Olofsson, J. [Univ. de Valparaso, Chile, Núcleo Milenio Formación Planetaria (NPF), Chile]
Oudmaijer, R. [Univ. of Leeds, United Kingdom]
Packham, C. [Univ. of Texas at San Antonio, United States]
Paladini, C. [European Southern Observatory, Chile]
Panic, O. [Univ. of Leeds, United Kingdom]
Petrov, R. [Observatoire de la Côte d'Azur, France]
Pope, B. [New York Univ., United States]
Pott, J.-U. [Max-Planck-Institut für Astronomie, Germany]
Quiroga-Nunez, L. H. [Leiden Univ., Netherlands]
Ramos Almeida, C. [Instituto de Astrofsica de Canarias, Spain]
Raymond, S. N. [Lab. d'Astrophysique de Bordeaux, France]
Regaly, Z. [Konkoly Observatory, Hungary]
Reynolds, M. [Univ. of Michigan, United States]
Ridgway, S. [National Optical Astronomy Observatory, United States]
Rinehart, S. [NASA Goddard Space Flight Ctr., United States]
Schreiber, M. [Univ. de Valparaso, Chile, Núcleo Milenio Formación Planetaria (NPF), Chile]
Smith, M. [Univ. of Kent, United Kingdom]
Stassun, K. [Vanderbilt Univ., United States]
Surdej, Jean mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Ten Brummelaar, T. [Georgia State Univ., United States]
Tristram, K. [European Southern Observatory, Chile]
Turner, N. [Jet Propulsion Lab., United States]
Tuthill, P. [Univ. of Sydney, Australia]
Van Belle, G. [Lowell Observatory, United States]
Vasisht, G. [Jet Propulsion Lab., United States]
Wallace, A. [Australian National Univ., Australia]
Weigelt, G. [Max-Planck-Institut für Radioastronomie, Germany]
Wishnow, E. [Space Sciences Lab., United States]
Wittkowski, M. [European Southern Observatory, Germany]
Wolf, S. [Christian-Albrechts-Univ. zu Kiel, Germany]
Young, J. [Univ. of Cambridge, United Kingdom]
Zhao, M. [New York Times Co., United States]
Zhu, Z. [Univ. of Nevada, Las Vegas, United States]
Zúñiga-Fernández, S. [Univ. de Valparaso, Chile, Núcleo Milenio Formación Planetaria (NPF), Chile]
Tuthill, P. G. [> >]
Creech [> >]
Eakman, M. J. [> >]
Merand, A. [> >]
1-Jul-2018
Proceedings of SPIE: The International Society for Optical Engineering
SPIE
10701
No
International
0277-786X
1996-756X
2018 Optical and Infrared Interferometry and Imaging VI
11 June 2018 through 15 June 2018
[en] Infrared interferometry ; PFI ; Planet formation ; Extrasolar planets ; Telescopes ; Dust structure ; Large aperture telescopes ; Protoplanetary disks ; Quantitative detection ; Space interferometry ; Technology development ; Interferometry
[en] The Planet Formation Imager (PFI) is a near- and mid-infrared interferometer project with the driving science goal 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 dust structures during the assembly phase of planet formation and quantitative detection efficiencies for accreting and non-accreting young exoplanets as a function of mass and age. We use these results to motivate two reference PFI designs consisting of a) twelve 3m telescopes with a maximum baseline of 1.2km focused on young exoplanet imaging and b) twelve 8m telescopes optimized for a wider range of young exoplanets and protoplanetary disk imaging out to the 150K H2O ice line. Armed with 4 x 8m telescopes, the ESO/VLTI can already 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 make PFI more affordable, including progress towards new designs for inexpensive, small field-of-view, large aperture telescopes and prospects for Cubesat-based space interferometry. © 2018 SPIE.
4D Technology;Andor Technology, Ltd.;Astronomical Consultants and Equipment, Inc.;et al.;Giant Magellan Telescope;The Society of Photo-Optical Instrumentation Engineers (SPIE)
http://hdl.handle.net/2268/228659
10.1117/12.2312683
138926
9781510619555

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