The TESS camera: modeling and measurements with deep depletion devices

The Transiting Exoplanet Survey Satellite, a NASA Explorer-class mission in development, will discover planets around nearby stars, most notably Earth-like planets with potential for follow up characterization. The all-sky survey requires a suite of four wide field-of-view cameras with sensitivity a...

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Main Authors: Woods, Deborah F., Vanderspek, Roland K, MacDonald, Robert E., Morgan, Edward H, Villasenor, Jesus Noel Samonte, Thayer, Carolyn T., Burke, Barry E., Chesbrough, Christian D., Chrisp, Michael P., Clark, Kristin E., Gonzales, Alexandria, Nguyen, Tam, Prigozhin, Gregory, Primeau, Brian, Sauerwein, Timothy A, Furesz, Gabor, Ricker, George R, Suntharalingam, Vyshnavi
Other Authors: Lincoln Laboratory
Format: Article
Published: SPIE 2018
Online Access:http://hdl.handle.net/1721.1/115318
https://orcid.org/0000-0001-7149-2792
https://orcid.org/0000-0003-2058-6662
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author Woods, Deborah F.
Vanderspek, Roland K
MacDonald, Robert E.
Morgan, Edward H
Villasenor, Jesus Noel Samonte
Thayer, Carolyn T.
Burke, Barry E.
Chesbrough, Christian D.
Chrisp, Michael P.
Clark, Kristin E.
Gonzales, Alexandria
Nguyen, Tam
Prigozhin, Gregory
Primeau, Brian
Sauerwein, Timothy A
Furesz, Gabor
Ricker, George R
Suntharalingam, Vyshnavi
author2 Lincoln Laboratory
author_facet Lincoln Laboratory
Woods, Deborah F.
Vanderspek, Roland K
MacDonald, Robert E.
Morgan, Edward H
Villasenor, Jesus Noel Samonte
Thayer, Carolyn T.
Burke, Barry E.
Chesbrough, Christian D.
Chrisp, Michael P.
Clark, Kristin E.
Gonzales, Alexandria
Nguyen, Tam
Prigozhin, Gregory
Primeau, Brian
Sauerwein, Timothy A
Furesz, Gabor
Ricker, George R
Suntharalingam, Vyshnavi
author_sort Woods, Deborah F.
collection MIT
description The Transiting Exoplanet Survey Satellite, a NASA Explorer-class mission in development, will discover planets around nearby stars, most notably Earth-like planets with potential for follow up characterization. The all-sky survey requires a suite of four wide field-of-view cameras with sensitivity across a broad spectrum. Deep depletion CCDs with a silicon layer of 100 μm thickness serve as the camera detectors, providing enhanced performance in the red wavelengths for sensitivity to cooler stars. The performance of the camera is critical for the mission objectives, with both the optical system and the CCD detectors contributing to the realized image quality. Expectations for image quality are studied using a combination of optical ray tracing in Zemax and simulations in Matlab to account for the interaction of the incoming photons with the 100 μm silicon layer. The simulations include a probabilistic model to determine the depth of travel in the silicon before the photons are converted to photo-electrons, and a Monte Carlo approach to charge diffusion. The charge diffusion model varies with the remaining depth for the photo-electron to traverse and the strength of the intermediate electric field. The simulations are compared with laboratory measurements acquired by an engineering unit camera with the TESS optical design and deep depletion CCDs. In this paper we describe the performance simulations and the corresponding measurements taken with the engineering unit camera, and discuss where the models agree well in predicted trends and where there are differences compared to observations.
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spelling mit-1721.1/1153182022-09-28T08:58:20Z The TESS camera: modeling and measurements with deep depletion devices Woods, Deborah F. Vanderspek, Roland K MacDonald, Robert E. Morgan, Edward H Villasenor, Jesus Noel Samonte Thayer, Carolyn T. Burke, Barry E. Chesbrough, Christian D. Chrisp, Michael P. Clark, Kristin E. Gonzales, Alexandria Nguyen, Tam Prigozhin, Gregory Primeau, Brian Sauerwein, Timothy A Furesz, Gabor Ricker, George R Suntharalingam, Vyshnavi Lincoln Laboratory Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences MIT Kavli Institute for Astrophysics and Space Research Woods, Deborah F. Vanderspek, Roland K MacDonald, Robert E. Morgan, Edward H Villasenor, Jesus Noel Samonte Thayer, Carolyn T. Burke, Barry E. Chesbrough, Christian D. Chrisp, Michael P. Clark, Kristin E. Gonzales, Alexandria Nguyen, Tam Prigozhin, Gregory Primeau, Brian Sauerwein, Timothy A Furesz, Gabor Ricker, George R Suntharalingam, Vyshnavi The Transiting Exoplanet Survey Satellite, a NASA Explorer-class mission in development, will discover planets around nearby stars, most notably Earth-like planets with potential for follow up characterization. The all-sky survey requires a suite of four wide field-of-view cameras with sensitivity across a broad spectrum. Deep depletion CCDs with a silicon layer of 100 μm thickness serve as the camera detectors, providing enhanced performance in the red wavelengths for sensitivity to cooler stars. The performance of the camera is critical for the mission objectives, with both the optical system and the CCD detectors contributing to the realized image quality. Expectations for image quality are studied using a combination of optical ray tracing in Zemax and simulations in Matlab to account for the interaction of the incoming photons with the 100 μm silicon layer. The simulations include a probabilistic model to determine the depth of travel in the silicon before the photons are converted to photo-electrons, and a Monte Carlo approach to charge diffusion. The charge diffusion model varies with the remaining depth for the photo-electron to traverse and the strength of the intermediate electric field. The simulations are compared with laboratory measurements acquired by an engineering unit camera with the TESS optical design and deep depletion CCDs. In this paper we describe the performance simulations and the corresponding measurements taken with the engineering unit camera, and discuss where the models agree well in predicted trends and where there are differences compared to observations. 2018-05-11T15:04:57Z 2018-05-11T15:04:57Z 2016-06 2018-03-16T19:01:18Z Article http://purl.org/eprint/type/ConferencePaper http://hdl.handle.net/1721.1/115318 Woods, Deborah F., et al. "The TESS Camera: Modeling and Measurements with Deep Depletion Devices." Proceedings Volume 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 26 June - 1 July, 2016, Edinburgh, United Kingdom, edited by Howard A. MacEwen et al., 2016, p. 99042C. © 2016 SPIE https://orcid.org/0000-0001-7149-2792 https://orcid.org/0000-0003-2058-6662 http://dx.doi.org/10.1117/12.2231296 Proceedings Volume 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE SPIE
spellingShingle Woods, Deborah F.
Vanderspek, Roland K
MacDonald, Robert E.
Morgan, Edward H
Villasenor, Jesus Noel Samonte
Thayer, Carolyn T.
Burke, Barry E.
Chesbrough, Christian D.
Chrisp, Michael P.
Clark, Kristin E.
Gonzales, Alexandria
Nguyen, Tam
Prigozhin, Gregory
Primeau, Brian
Sauerwein, Timothy A
Furesz, Gabor
Ricker, George R
Suntharalingam, Vyshnavi
The TESS camera: modeling and measurements with deep depletion devices
title The TESS camera: modeling and measurements with deep depletion devices
title_full The TESS camera: modeling and measurements with deep depletion devices
title_fullStr The TESS camera: modeling and measurements with deep depletion devices
title_full_unstemmed The TESS camera: modeling and measurements with deep depletion devices
title_short The TESS camera: modeling and measurements with deep depletion devices
title_sort tess camera modeling and measurements with deep depletion devices
url http://hdl.handle.net/1721.1/115318
https://orcid.org/0000-0001-7149-2792
https://orcid.org/0000-0003-2058-6662
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