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Optimizing the subwavelength grating of L-band annular groove phase masks for high coronagraphic performance

Vargas Catalán, E. and Huby, E. and Forsberg, P. and Jolivet, A. and Baudoz, P. and Carlomagno, B. and Delacroix, C. and Habraken, S. and Mawet, D. and Surdej, J. and Absil, O. and Karlsson, M. (2016) Optimizing the subwavelength grating of L-band annular groove phase masks for high coronagraphic performance. Astronomy and Astrophysics, 595 . Art. No. A127. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20161222-104537389

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Abstract

Context. The annular groove phase mask (AGPM) is one possible implementation of the vector vortex coronagraph, where the helical phase ramp is produced by a concentric subwavelength grating. For several years, we have been manufacturing AGPMs by etching gratings into synthetic diamond substrates using inductively coupled plasma etching. Aims. We aim to design, fabricate, optimize, and evaluate new L-band AGPMs that reach the highest possible coronagraphic performance, for applications in current and forthcoming infrared high-contrast imagers. Methods. Rigorous coupled wave analysis (RCWA) is used for designing the subwavelength grating of the phase mask. Coronagraphic performance evaluation is performed on a dedicated optical test bench. The experimental results of the performance evaluation are then used to accurately determine the actual profile of the fabricated gratings, based on RCWA modeling. Results. The AGPM coronagraphic performance is very sensitive to small errors in etch depth and grating profile. Most of the fabricated components therefore show moderate performance in terms of starlight rejection (a few 100:1 in the best cases). Here we present new processes for re-etching the fabricated components in order to optimize the parameters of the grating and hence significantly increase their coronagraphic performance. Starlight rejection up to 1000:1 is demonstrated in a broadband L filter on the coronagraphic test bench, which corresponds to a raw contrast of about 10-5 at two resolution elements from the star for a perfect input wave front on a circular, unobstructed aperture. Conclusions. Thanks to their exquisite performance, our latest L-band AGPMs are good candidates for installation in state of the art and future high-contrast thermal infrared imagers, such as METIS for the E-ELT.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201628739DOIArticle
http://www.aanda.org/articles/aa/abs/2016/11/aa28739-16/aa28739-16.htmlPublisherArticle
https://arxiv.org/abs/1610.05065arXivDiscussion Paper
ORCID:
AuthorORCID
Mawet, D.0000-0002-8895-4735
Surdej, J.0000-0002-7005-1976
Absil, O.0000-0002-4006-6237
Karlsson, M.0000-0002-2011-0851
Additional Information:© ESO, 2016. Received 19 April 2016 / Accepted 4 August 2016. The authors are grateful to Jérôme Parisot (LESIA, Observatoire de Paris), who manages the YACADIRE test bench, for his availability and help during every AGPM test campaigns. The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (ERC Grant Agreement No. 337569), the French Community of Belgium through an ARC grant for Concerted Research Action, and the Swedish Research Council (VR) through project grant 621-2014-5959.
Funders:
Funding AgencyGrant Number
European Research Council (ERC)337569
Communauté française de Belgique – Actions de recherche concertéesUNSPECIFIED
Swedish Research Council621-2014-5959
Subject Keywords:instrumentation: high angular resolution / planetary systems / planets and satellites: detection
Record Number:CaltechAUTHORS:20161222-104537389
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161222-104537389
Official Citation:Optimizing the subwavelength grating of L-band annular groove phase masks for high coronagraphic performance E. Vargas Catalán, E. Huby, P. Forsberg, A. Jolivet, P. Baudoz, B. Carlomagno, C. Delacroix, S. Habraken, D. Mawet, J. Surdej, O. Absil and M. Karlsson A&A, 595 (2016) A127 DOI: http://dx.doi.org/10.1051/0004-6361/201628739
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:73144
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:22 Dec 2016 19:11
Last Modified:14 Oct 2019 23:16

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