Rupert H. Dodkins
First Principle Simulator of a Stochastically Varying Image Plane for Photon-counting High Contrast Applications
Dodkins, Rupert H.; Davis, Kristina K.; Lewis, Briley; Mahashabde, Sumedh; Mazin, Benjamin A.; Lipartito, Isabel A.; Fruitwala, Neelay; O’Brien, Kieran; Thatte, Niranjan
Authors
Kristina K. Davis
Briley Lewis
Sumedh Mahashabde
Benjamin A. Mazin
Isabel A. Lipartito
Neelay Fruitwala
Professor Kieran Obrien kieran.s.obrien@durham.ac.uk
Professor
Niranjan Thatte
Abstract
Optical and near-infrared Microwave Kinetic Inductance Detectors, or MKIDs are low-temperature detectors with inherent spectral resolution that are able to instantly register individual photons with potentially no false counts or readout noise. These properties make MKIDs transformative for exoplanet direct imaging by enabling photon-statistics-based planet-discrimination techniques as well as performing conventional noise-subtraction techniques on shorter timescales. These detectors are in the process of rapid development, and as such, the full extent of their performance enhancing potential has not yet be quantified. MKID Exoplanet Direct Imaging Simulator, or MEDIS, is a general-purpose end-to-end numerical simulator for high-contrast observations with MKIDs. The simulator exploits current optical propagation libraries and augments them with a new MKIDs simulation module to provide a pragmatic model of many of the degradation effects present during the detection process. We use MEDIS to demonstrate how changes in various MKID properties affect the contrast-separation performance when conventional differential imaging techniques are applied to low-flux, short duration observations. We show that to improve performance at close separations will require increasing the maximum count rate or pixel sampling when there is high residual flux after the coronagraph. We predict that taking pixel yield from the value achieved by current instruments of 80% and increasing it to 100% would result in an improvement in contrast of a factor of ~4 at 3λ/D and ~8 at 6λ/D. Achieving better contrast performance in this low flux regime would then require exploiting the information encoded in the photon arrival time statistics.
Citation
Dodkins, R. H., Davis, K. K., Lewis, B., Mahashabde, S., Mazin, B. A., Lipartito, I. A., Fruitwala, N., O’Brien, K., & Thatte, N. (2020). First Principle Simulator of a Stochastically Varying Image Plane for Photon-counting High Contrast Applications. Publications of the Astronomical Society of the Pacific, 132(1016), Article 104503. https://doi.org/10.1088/1538-3873/aba9e4
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 28, 2020 |
Online Publication Date | Sep 16, 2020 |
Publication Date | 2020-10 |
Deposit Date | Oct 13, 2020 |
Publicly Available Date | Sep 16, 2021 |
Journal | Publications of the Astronomical Society of the Pacific |
Print ISSN | 0004-6280 |
Publisher | Astronomical Society of the Pacific |
Peer Reviewed | Peer Reviewed |
Volume | 132 |
Issue | 1016 |
Article Number | 104503 |
DOI | https://doi.org/10.1088/1538-3873/aba9e4 |
Public URL | https://durham-repository.worktribe.com/output/1260290 |
Files
Accepted Journal Article
(1.2 Mb)
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Copyright Statement
The deposited manuscript is available under a CC BY-NC-ND 4.0 licence.
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