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MEC: the MKID exoplanet camera for high contrast astronomy at Subaru (Conference Presentation)

Walter, Alex and Mazin, Benjamin A. and Bockstiegel, Clint and Fruitwala, Neelay and Szypryt, Paul and Lipartito, Isabel and Meeker, Seth and Zobrist, Nicholas and Collura, Giulia and Coiffard, Grégoire and Strader, Paschal and Guyon, Olivier and Lozi, Julien and Jovanovic, Nemanja (2018) MEC: the MKID exoplanet camera for high contrast astronomy at Subaru (Conference Presentation). In: Ground-based and Airborne Instrumentation for Astronomy VII. Proceedings of SPIE. No.10702. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 107020V . ISBN 9781510619579. https://resolver.caltech.edu/CaltechAUTHORS:20190823-134013267

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Abstract

Direct Imaging of exoplanets is one of the most technically difficult techniques used to study exoplanets, but holds immense promise for not just detecting but characterizing planets around the nearest stars. Ambitious instruments at the world’s largest telescopes have been built to carry out this science: the Gemini Planet Imager (GPI), SPHERE at VLT, SCExAO at Subaru, and the P1640 and Stellar Double Coronagraph (SDC) at Palomar. These instruments share a common archetype consisting of an extreme AO system feeding a coronagraph for on-axis stellar light rejection followed by a focal plane Integral Field Spectrograph (IFS). They are currently limited by uncontrolled scattered and diffracted light which produces a coherent speckle halo in the image plane. A number of differential imaging schemes exist to mitigate these issues resulting in star-planet contrast ratios as deep as ~10^-6 at low angular separations. Surpassing this contrast limit requires high speed active speckle nullification from a focal plane wavefront sensor (FPWS) and new processing techniques. MEC, the Microwave Kinetic Inductance Detector (MKID) Exoplanet Camera, is a J-band IFS module behind Subaru Telescope’s SCExAO system. MEC is capable of producing an image cube several thousand times a second without the read noise that dominates conventional high speed IFUs. This enables it to integrate with SCExAO as an extremely fast FPWS while eliminating non-common path aberrations by doubling as a science camera. Key science objectives can be further explored if longer wavelengths (H and K band) are simultaneously sent to CHARIS for high resolution spectroscopy. MEC, to be commissioned at Subaru in early 2018, is the second MKID IFS for high contrast imaging following DARKNESS’ debut at Palomar in July 2016. MEC will follow up on young planets and debris disks discovered in the SEEDS survey or by Project 1640 as well as discover self-luminous massive planets. The increased sensitivity, combined with the advanced coronagraphs in SCExAO which have inner working angles (IWAs) as small as 0.03” at 1.2 μm, allows young Jupiter-sized objects to be imaged as close as 4 AU from their host star. If the wavefront control enabled by MEC is fully realized, it may begin to probe the reflected light of giant planets around some nearby stars, opening a new parameter space for direct imaging targeting older stars. While direct imaging of reflected light exoplanets is the most challenging of the scientific goals, it is a promising long-term path towards characterization of habitable planets around nearby stars using Extremely Large Telescopes (ELTs). With diameters of about 30-m, an ELT can resolve the habitable zones of nearby M-type stars, for which an Earth-sized planet would be at ~10^(-7) contrast at 1 μm. This will complement future space-based high contrast optical imaging targeting the wider habitable zones of sun-like stars for ~10^(-10) contrast earth analogs. We will present lessons learned from the first few months of MEC’s operation including initial lab and on-sky (weather permitting) results. We already have preliminary data from Palomar testing a new statistical speckle discrimination post-processing technique using the photon arrival time measured with MKIDs. Residual stellar light in the form of a speckle masquerading as a planetary companion is pulled from a modified Rician distribution and can be statistically discerned from a true off-axis Poisson point source. Additionally, the progress of active focal plane wavefront control will be briefly discussed.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.2311586DOIArticle
ORCID:
AuthorORCID
Guyon, Olivier0000-0002-1097-9908
Lozi, Julien0000-0002-3047-1845
Additional Information:© 2018 Society of Photo-Optical Instrumentation Engineers (SPIE).
Series Name:Proceedings of SPIE
Issue or Number:10702
Record Number:CaltechAUTHORS:20190823-134013267
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190823-134013267
Official Citation:Alex Walter, Benjamin B. Mazin, Clint Bockstiegel, Neelay Fruitwala, Paul Szypryt, Isabel Lipartito, Seth Meeker, Nicholas Zobrist, Giulia Collura, Grégoire Coiffard, Paschal Strader, Olivier Guyon, Julien Lozi, and Nemanja Jovanovic "MEC: the MKID exoplanet camera for high contrast astronomy at Subaru (Conference Presentation)", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107020V (9 July 2018); https://doi.org/10.1117/12.2311586
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:98182
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 Aug 2019 21:42
Last Modified:03 Oct 2019 21:38

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