Planet formation imager: project update

Autor: Gerd Weigelt, Ernest A. Michael, Florentin Millour, Andrea Isella, Edward H. Wishnow, Kaitlin M. Kratter, Eric L. N. Jensen, Jean Baptiste Le Bouquin, Stephen T. Ridgway, Jean François Gonzalez, Rafael Millan-Gabet, Farzana Meru, David R. Ciardi, Neal J. Turner, Greg Laughlin, Cristina Ramos Almeida, Almudena Alonso-Herrero, S. F. Hoenig, Ming Zhao, Claudia Paladini, Zhaohuan Zhu, Amy Bonsor, O. Panić, L. H. Quiroga-Nuñez, Stephen R. Kane, Ruobing Dong, Stefano Minardi, Andrea Chiavassa, Stephen A. Rinehart, Amelia Bayo, T. ten Brummelaar, Jean Surdej, Alexander Wallace, Attila Juhasz, John D. Ilee, Benjamin J. S. Pope, Matthias R. Schreiber, Konrad R. W. Tristram, Jean Philippe Berger, Gerard T. van Belle, Willem Jan De Wit, Richard P. Nelson, Johan Olofsson, Joerg Uwe Pott, Michael J. Ireland, John Young, Fabien Baron, Mark Reynolds, Sean N. Raymond, Wilhelm Kley, Alessandro Morbidelli, Sebastian Wolf, Tabetha S. Boyajian, Michelle Creech-Eakman, Peter G. Tuthill, Gaspard Duchene, Chris Packham, S. Zúñiga-Fernández, Rene D. Oudmaijer, Sylvestre Lacour, Quentin Kral, Makoto Kishimoto, Lucas Labadie, G. Vasisht, Catherine Espaillat, Poshak Gandhi, Michael D. Smith, Denis Defrere, Andreas Morlok, Chris Mordasini, D. Mozurkewich, Keivan G. Stassun, John D. Monnier, Alexandre Gallenne, Zsolt Regaly, Stefan Kraus, Christopher A. Haniff, Romain Petrov, Markus Wittkowski

Publikováno v: Optical 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
Optical 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, Jun 2018, Austin, United States. ⟨10.1117/12.2312683⟩

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 o

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::958ba94228d19c54e059636f5e6907d2
https://hal.archives-ouvertes.fr/hal-01901978

Review and scientific prospects of high-contrast optical stellar interferometry

Autor: Romain Laugier, Sylvestre Lacour, John D. Monnier, Marc A. Martinod, Joerg Uwe Pott, Frank Eisenhauer, Steve Ertel, Barnaby Norris, Eugene Serabyn, Guillermo Martin, Denis Defrere, Michael J. Ireland, Olivier Absil, Lucas Labadie, Adrian M. Glauser, Michael Nowak, Jordan Stone, Julien Woillez, William C. Danchi, Bertrand Mennesson, Jens Kammerer, Sascha P. Quanz, F. Martinache, Tyler Gardner, Jean-Philippe Berger, Stefan Kraus, Colin Dandumont, Peter G. Tuthill, Jerôme Loicq, Philip Hinz

Publikováno v: Optical and Infrared Interferometry and Imaging VII
Proceedings of the SPIE: The International Society for Optical Engineering

High-contrast optical stellar interferometry generally refers to instruments able to detect circumstellar emission at least a few hundred times fainter than the host star at high-angular resolution (typically within a few λ/D). While such contrast l

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d718e963cba518d4013f5486ed84456d