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FIRST, a fibered aperture masking instrument: on-sky results

Authors :
Gaspard Duchene
Elodie Choquet
Franck Marchis
Takayuki Kotani
Guy Perrin
Elinor L. Gates
Elsa Huby
Olivier Lai
Julien Woillez
Sylvestre Lacour
Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Haute résolution angulaire en astrophysique
Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
SETI Institute (United States)
Institute of Space and Astronautical Science (ISAS)
University of California (UCBerkeley)
University of California, Department of Astronomy and Astrophysics, Observatories, Lick Observatory
W. M. Keck Observatory
Canada-France-Hawaii Telescope Corporation (CFHT)
National Research Council of Canada (NRC)-Centre National de la Recherche Scientifique (CNRS)-University of Hawai'i [Honolulu] (UH)
Source :
Proceedings of the SPIE, Ground-based and Airborne Instrumentation for Astronomy IV, Ground-based and Airborne Instrumentation for Astronomy IV, Jul 2012, Amsterdam, Netherlands. ⟨10.1117/12.925615⟩
Publication Year :
2012
Publisher :
HAL CCSD, 2012.

Abstract

We present on-sky results obtained with the visible light prototype of the Fibered Imager foR Single Telescope(FIRST) mounted on the 3-m Shane Telescope at Lick Observatory and using its Adaptive Optics system. Thisinstrument is dedicated to high angular resolution and high dynamic range imaging. Its principle combines bothtechniques of single-mode “ber interferometry and pupil remapping. Simulations predict a dynamic range upto 10 6 at /D , or at a few tens of milliarcseconds at 630nm using an 8-m telescope. Laboratory experimentsbased on a 9-“ber prototype working in the 600nm 900nm spectral band successfully demonstrated the powerof the concept. The same prototype has been set-up on the 3-m Shane telescope in July 2010. In this paper, wepresent the on-sky results obtained in October 2011 with an improved version of the instrument using 18 “bers.They clearly show the detection of the binary star Capella at the diraction limit of the telescope.Keywords: high dynamic range imaging, high angular resolution, aperture masking, pupil remapping, “berinterferometer, Cap ella, exoplanets

Details

Language :
English
Database :
OpenAIRE
Journal :
Proceedings of the SPIE, Ground-based and Airborne Instrumentation for Astronomy IV, Ground-based and Airborne Instrumentation for Astronomy IV, Jul 2012, Amsterdam, Netherlands. ⟨10.1117/12.925615⟩
Accession number :
edsair.doi.dedup.....0e7545a354abd3800acfda90ce0d3901
Full Text :
https://doi.org/10.1117/12.925615⟩