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Laboratory demonstration of a mid-infrared AGPM vector vortex coronagraph

Delacroix, Christian (författare)
Hololab, Université de Liège
Absil, Olivier (författare)
IAGL, Université de Liège
Forsberg, Pontus, 1981- (författare)
Uppsala universitet,Mikrosystemteknik
visa fler...
Mawet, Dimitri (författare)
European Southern Observatory
Christiaens, Valentin (författare)
IAGL, Université de Liège
Karlsson, Mikael (författare)
Uppsala universitet,Mikrosystemteknik
Boccaletti, Anthony (författare)
LESIA-Observatoire de Paris
Baudoz, Pierre (författare)
LESIA-Observatoire de Paris
Kuittinen, Markku (författare)
Department of Physics and Mathematics, University of Eastern Finland
Vartiainen, Ismo (författare)
Paul Scherrer Institut
Surdej, Jean (författare)
IAGL, Université de Liège
Habraken, Serge (författare)
IAGL, Université de Liège
visa färre...
 (creator_code:org_t)
2013-05-16
2013
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 553, s. A98-
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. Coronagraphy is a powerful technique to achieve high contrast imaging, hence to image faint companions around bright targets. Various concepts have been used in the visible and near-infrared regimes, while coronagraphic applications in the mid-infrared nowadays remain largely unexplored. Vector vortex phase masks based on concentric subwavelength gratings show great promise for such applications.Aims. We aim at producing and validating the first high-performance broadband focal plane phase mask coronagraphs for applications in the mid-infrared regime, and in particular the L band with a fractional bandwidth of  ~16% (3.5–4.1 μm).Methods. Based on rigorous coupled wave analysis, we designed an annular groove phase mask (AGPM) producing a vortex effect in the L band, and etched it onto a series of diamond substrates. The grating parameters were measured by means of scanning electron microscopy. The resulting components were then tested on a mid-infrared coronagraphic test bench.Results. A broadband raw null depth of 2 × 10-3 was obtained for our best L-band AGPM after only a few iterations between design and manufacturing. This corresponds to a raw contrast of about 6 × 10-5 (10.5 mag) at 2λ/D. This result is fully in line with our projections based on rigorous coupled wave analysis modelling, using the measured grating parameters. The sensitivity to tilt and focus has also been evaluated.Conclusions. After years of technological developments, mid-infrared vector vortex coronagraphs have finally become a reality and live up to our expectations. Based on their measured performance, our L-band AGPMs are now ready to open a new parameter space in exoplanet imaging at major ground-based observatories.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

coronagraph diamond
Teknisk fysik med inriktning mot mikrosystemteknik
Engineering Science with specialization in Microsystems Technology

Publikations- och innehållstyp

ref (ämneskategori)
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