Modeling the e-APD SAPHIRA/C-RED ONE camera at low flux level An attempt to count photons in the near-infrared with the MIRC-X interferometric combiner

10Citations
Citations of this article
8Readers
Mendeley users who have this article in their library.
Get full text

Abstract

Context. We implement an electron avalanche photodiode (e-APD) in the MIRC-X instrument, which is an upgrade of the sixtelescope near-infrared imager MIRC, at the CHARA array. This technology should improve the sensitivity of near-infrared interferometry. Aims. We aim to characterize a near-infrared C-RED ONE camera from First Light Imaging (FLI) using an e-APD from Leonardo (previously SELEX). Methods. We first used the classical mean-variance analysis to measure the system gain and the amplification gain. We then developed a physical model of the statistical distribution of the camera output signal. This model is based on multiple convolutions of the Poisson statistic, the intrinsic avalanche gain distribution, and the observed distribution of the background signal. At low flux level, this model independently constrains the incident illumination level, the total gain, and the excess noise factor of the amplification. Results. We measure a total transmission of 48 ± 3% including the cold filter and the Quantum Efficiency. We measure a system gain of 0.49ADU/e, a readout noise of 10 ADU, and amplification gains as high as 200. These results are consistent between the two methods and therefore validate our modeling approach. The measured excess noise factor based on the modeling is 1:47 ± 0:03, with no obvious dependency with flux level or amplification gain. Conclusions. The presented model allows the characteristics of the e-APD array to be measured at low flux level independently of a preexisting calibration.With <0:3 electron equivalent readout noise at kilohertz frame rates, we confirm the revolutionary performances of the camera with respect to the PICNIC or Hawaii technologies. However, the measured excess noise factor is significantly higher than what is claimed in the literature (<1.25), and explains why counting multiple photons remains challenging with this camera.

References Powered by Scopus

First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer

360Citations
N/AReaders
Get full text

PIONIER: A 4-telescope visitor instrument at VLTI

264Citations
N/AReaders
Get full text

An avalanchephotodiode-based photon-number-resolving detector

217Citations
N/AReaders
Get full text

Cited by Powered by Scopus

MIRC-X: A Highly Sensitive Six-telescope Interferometric Imager at the CHARA Array

79Citations
N/AReaders
Get full text

Recent hotspots and innovative trends of infrared photon detectors

27Citations
N/AReaders
Get full text

MYSTIC: a high angular resolution K-band imager at CHARA

24Citations
N/AReaders
Get full text

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Cite

CITATION STYLE

APA

Lanthermann, C., Anugu, N., Le Bouquin, J. B., Monnier, J. D., Kraus, S., & Perraut, K. (2019). Modeling the e-APD SAPHIRA/C-RED ONE camera at low flux level An attempt to count photons in the near-infrared with the MIRC-X interferometric combiner. Astronomy and Astrophysics, 625. https://doi.org/10.1051/0004-6361/201935043

Readers' Seniority

Tooltip

Researcher 3

75%

PhD / Post grad / Masters / Doc 1

25%

Readers' Discipline

Tooltip

Physics and Astronomy 5

83%

Business, Management and Accounting 1

17%

Save time finding and organizing research with Mendeley

Sign up for free