Zobrazeno 1 - 8
of 8
pro vyhledávání: '"M. D. Perrin"'
Autor:
R. Pourcelot, E. H. Por, M. N’Diaye, H. Benard, G. Brady, L. Canas, M. Carbillet, K. Dohlen, I. Laginja, J. Lugten, J. Noss, M. D. Perrin, P. Petrone, L. Pueyo, S. F. Redmond, A. Sahoo, A. Vigan, S. D. Will, R. Soummer
Context. Wavefront sensing and control (WFSC) will play a key role in improving the stability of future large segmented space telescopes while relaxing the thermo-mechanical constraints on the observatory structure. Coupled with a coronagraph to reje
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::728cf23b2312600ce2f04879a69a9864
http://arxiv.org/abs/2301.03242
http://arxiv.org/abs/2301.03242
Autor:
R. Pourcelot, M. N’Diaye, E. H. Por, I. Laginja, M. Carbillet, H. Benard, G. Brady, L. Canas, K. Dohlen, J. Fowler, O. Lai, M. Maclay, E. McChesney, J. Noss, M. D. Perrin, P. Petrone, L. Pueyo, S. F. Redmond, A. Sahoo, A. Vigan, S. D. Will, R. Soummer
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, pp.A49. ⟨10.1051/0004-6361/202243145⟩
Astronomy and Astrophysics-A&A, 2022, 663, pp.A49. ⟨10.1051/0004-6361/202243145⟩
Context.The combination of large segmented space telescopes, coronagraphy, and wavefront control methods is a promising solution for producing a dark hole (DH) region in the coronagraphic image of an observed star in order to study planetary companio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c00dbd45da480958756a1d7ae961055
https://hal-insu.archives-ouvertes.fr/insu-03780768
https://hal-insu.archives-ouvertes.fr/insu-03780768
Autor:
C. H. Chen, A. Boccaletti, Abhijith Rajan, C. del Burgo, Dimitri Mawet, J. C. Augereau, Anne-Marie Lagrange, Christophe Pinte, Julien Milli, Steve Ertel, Elena Gofas-Salas, S. Wolff, J. B. Hagan, Aki Roberge, Dean C. Hines, Mamadou N'Diaye, Rémi Soummer, M. D. Perrin, Z. Wahhaj, David A. Golimowski, Olivier Absil, W. R. F. Dent, Elodie Choquet, Julien Girard, P. Hibon, Glenn Schneider, Mark Booth, David Mouillet, Mark C. Wyatt, Luca Matrà, Laurent Pueyo, Grant M. Kennedy, John H. Debes, C. A. Gomez Gonzalez
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 834 (12), pp.1-7. ⟨10.3847/2041-8213/834/2/L12⟩
The Astrophysical journal letters, 2017, 834 (12), pp.1-7. ⟨10.3847/2041-8213/834/2/L12⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 834 (12), pp.1-7. ⟨10.3847/2041-8213/834/2/L12⟩
The Astrophysical journal letters, 2017, 834 (12), pp.1-7. ⟨10.3847/2041-8213/834/2/L12⟩
We present the first scattered-light images of the debris disk around 49 ceti, a ~40 Myr A1 main sequence star at 59 pc, famous for hosting two massive dust belts as well as large quantities of atomic and molecular gas. The outer disk is revealed in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c05a3171acf48bf27e408ad713ef894b
https://resolver.caltech.edu/CaltechAUTHORS:20170110-072851219
https://resolver.caltech.edu/CaltechAUTHORS:20170110-072851219
Autor:
Francois Menard, D. L. Padgett, Gaspard Duchêne, John Krist, C. Pinte, M. D. Perrin, K. R. Stapelfeldt, Schuyler Wolff
Publikováno v:
Proceedings of the International Astronomical Union. 8:99-103
Edge-on, optically thick circumstellar disks have been previously imaged at subarcsecond resolution around about a dozen nearby young stellar objects. In these systems the central star is occulted from direct view, bright star image artifacts are abs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9c053fbcb1377dbace99996aaef85bde
https://doi.org/10.1017/s1743921313008004
https://doi.org/10.1017/s1743921313008004
Autor:
Patrick Ingraham, Andrew Serio, Stephen J. Goodsell, Schuyler Wolff, Markus Hartung, Alexandra Z. Greenbaum, M. D. Perrin, Lisa Poyneer, Anthony Cheetham, Naru Sadakuni, Anand Sivaramakrishnan, Peter Tuthill, Laurent Pueyo, B. Norris, Andrew Cardwell, Fredrik T. Rantakyrö, Dmitry Savransky, Sandrine Thomas, Pascale Hibon, Bruce Macintosh
The Gemini Planet Imager (GPI) Extreme Adaptive Optics Coronograph contains an interferometric mode: a 10-hole non-redundant mask (NRM) in its pupil wheel. GPI operates at $Y, J, H$, and $K$ bands, using an integral field unit spectrograph (IFS) to o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2f416678cd7341def51d3a2f2f4863c
Autor:
É. Choquet, G. Bryden, M. D. Perrin, R. Soummer, J.-C. Augereau, C. H. Chen, J. H. Debes, E. Gofas-Salas, J. B. Hagan, D. C. Hines, D. Mawet, F. Morales, L. Pueyo, A. Rajan, B. Ren, G. Schneider, C. C. Stark, S. Wolff
Publikováno v:
Astrophysical Journal; 2/10/2018, Vol. 854 Issue 1, p1-1, 1p
Autor:
J. B. Hornbeck, J. R. Swearingen, C. A. Grady, G. M. Williger, A. Brown, M. L. Sitko, J. P. Wisniewski, M. D. Perrin, J. T. Lauroesch, G. Schneider, D. Apai, S. Brittain, J. M. Brown, E. H. Champney, K. Hamaguchi, Th. Henning, D. K. Lynch, R. Petre, R. W. Russell, F. M. Walter
Publikováno v:
Astrophysical Journal; 10/1/2016, Vol. 829 Issue 2, p1-1, 1p
Autor:
J. Mazoyer, A. Boccaletti, É. Choquet, M. D. Perrin, L. Pueyo, J.-C. Augereau, A.-M. Lagrange, J. Debes, S. G. Wolff
Publikováno v:
Astrophysical Journal; 2/20/2016, Vol. 818 Issue 2, p1-1, 1p