SPHERE on-sky performance compared with budget predictions

Author:

Dohlen Kjetil1,Vigan Arthur1,Mouillet David2,Wildi François3,Sauvage Jean-François1,Fusco Thierry1,Beuzit Jean-Luc2,Puget Pascal2,Le Mignant David1,Roelfsema Ronald4,Pragt Johan4,Schmid Hans Martin5,Gratton Raffaele6,Mesa Dino6,Claudi Riccardo6,Langlois Maud7,Costille Anne1,Hugot Emmanuel1,O'Neil Jared8,Guerra Juan Carlos8,N'Diaye Mamadou9,Girard Julien8,Mawet Dimitri10,Zins Gerard8

Affiliation:

1. Lab. d'Astrophysique de Marseille (France)

2. Institut de Planétologie et d’Astrophysique de Grenoble (France)

3. Observatoire de Genève (Switzerland)

4. ASTRON (Netherlands)

5. ETH Zürich (Switzerland)

6. INAF - Osservatorio Astronomico di Padova (Italy)

7. Ctr. de Recherche Astrophysique de Lyon, Univ. Lyon, Univ. Lyon 1, CNRS (France)

8. European Southern Observatory (Chile)

9. Space Telescope Science Institute (United States)

10. California Institute of Technology (United States)

Publisher

SPIE

Reference18 articles.

1. SPHERE: a 'Planet Finder' instrument for the VLT

2. Fast-moving features in the debris disk around AU Microscopii

3. Active optics methods for exoplanet direct imaging. Stress polishing of supersmooth aspherics for VLT-SPHERE planet finder;Hugot,2012

4. The ZIMPOL high contrast imaging polarimeter for SPHERE: system test results;Roelfsema,2014

5. The infra-red dual imaging and spectrograph for SPHERE: design and performance

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