Computational single photon counting for non-line-of-sight, light in flight, and photon flux imaging

2020 ◽  
Author(s):  
Martin Laurenzis
Keyword(s):  
Single Photon ◽  
Photon Counting ◽  
Photon Flux ◽  
Line Of Sight ◽  
Single Photon Counting ◽  
Non Line Of Sight

scholarly journals A Single-Shot Non-Line-of-Sight Range-Finder

Sensors ◽  
2019 ◽  
Vol 19 (21) ◽  
pp. 4820 ◽  
Author(s):  
James Brooks ◽  
Daniele Faccio
Keyword(s):  
Autonomous Vehicles ◽  
Arrival Time ◽  
Single Photon ◽  
Photon Counting ◽  
Line Of Sight ◽  
Single Shot ◽  
Single Photon Counting ◽  
Range Finding ◽  
Finding Method ◽  
Non Line Of Sight

The ability to locate a target around a corner is crucial in situations where it is impractical or unsafe to physically move around the obstruction. However, current techniques are limited to long acquisition times as they rely on single-photon counting for precise arrival time measurements. Here, we demonstrate a single-shot non-line-of-sight range-finding method operating at 10 Hz and capable of detecting a moving human target up to distances of 3 m around a corner. Due to the potential data acquisition speeds, this technique will find applications in search and rescue and autonomous vehicles.

scholarly journals Fast-Gated 16 × 1 SPAD Array for Non-Line-of-Sight Imaging Applications

Instruments ◽  
2020 ◽  
Vol 4 (2) ◽  
pp. 14
Author(s):  
Marco Renna ◽  
Ji Hyun Nam ◽  
Mauro Buttafava ◽  
Federica Villa ◽  
Andreas Velten ◽  
...  
Keyword(s):  
Single Photon ◽  
Photon Counting ◽  
Complementary Metal Oxide Semiconductor ◽  
Oxide Semiconductor ◽  
Line Of Sight ◽  
Single Photon Detector ◽  
Single Photon Counting ◽  
Timing Resolution ◽  
Fast Gating ◽  
Non Line Of Sight

In this paper we present a novel single-photon detector specifically designed for Non-Line-Of-Sight (NLOS) imaging applications within the framework of the DARPA REVEAL program. The instrument is based on a linear 16 × 1 Complementary Metal-Oxide-Semiconductor (CMOS) Single-Photon Avalanche Diode (SPAD) array operated in fast-gated mode by a novel fast-gating Active Quenching Circuit (AQC) array, which enables the detectors with sub-ns transitions thanks to a SPAD-dummy approach. The detector exhibits a timing resolution better than 50 ps (Full Width at Half Maximum - FWHM) at a measurement repetition rate up to 40 MHz, and provides 16 independent outputs compatible with commercial Time-Correlated Single-Photon Counting (TCSPC) instrumentation. The instrument has been experimentally characterized and operated in preliminary NLOS imaging acquisitions where a 40 × 60 cm hidden object is successfully reconstructed by scanning over a grid of 150 × 150 positions.

Study of single photon counting for non-line-of-sight vision

2015 ◽  
Author(s):  
Martin Laurenzis ◽  
Frank Christnacher ◽  
Jonathan Klein ◽  
Matthias B. Hullin ◽  
Andreas Velten
Keyword(s):  
Single Photon ◽  
Photon Counting ◽  
Line Of Sight ◽  
Single Photon Counting ◽  
Non Line Of Sight

Single Point PICA Probing with an Avalanche Photo-Diode

2001 ◽  
Author(s):  
Mike Bruce ◽  
Rama R. Goruganthu ◽  
Shawn McBride ◽  
David Bethke ◽  
J.M. Chin
Keyword(s):  
Single Photon ◽  
Single Point ◽  
Photon Counting ◽  
Ring Oscillator ◽  
Time Resolved ◽  
Single Photon Counting ◽  
Photo Diode ◽  
Avalanche Photo Diode ◽  
Photo Multiplier Tube ◽  
Channel Plate

Abstract For time resolved hot carrier emission from the backside, an alternate approach is demonstrated termed single point PICA. The single point approach records time resolved emission from an individual transistor using time-correlated-single-photon counting and an avalanche photo-diode. The avalanche photo-diode has a much higher quantum efficiency than micro-channel plate photo-multiplier tube based imaging cameras typically used in earlier approaches. The basic system is described and demonstrated from the backside on a ring oscillator circuit.

scholarly journals UVscope and its application aboard the ASTRI-Horn telescope

2021 ◽  
Author(s):  
Maria Concetta Maccarone ◽  
Giovanni La Rosa ◽  
Osvaldo Catalano ◽  
Salvo Giarrusso ◽  
Alberto Segreto ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Single Photon ◽  
Photon Counting ◽  
Light Flux ◽  
Cosmic Ray ◽  
High Energy ◽  
Wide Field ◽  
High Energy Astrophysics ◽  
Single Photon Counting ◽  
Photon Counting Mode

AbstractUVscope is an instrument, based on a multi-pixel photon detector, developed to support experimental activities for high-energy astrophysics and cosmic ray research. The instrument, working in single photon counting mode, is designed to directly measure light flux in the wavelengths range 300-650 nm. The instrument can be used in a wide field of applications where the knowledge of the nocturnal environmental luminosity is required. Currently, one UVscope instrument is allocated onto the external structure of the ASTRI-Horn Cherenkov telescope devoted to the gamma-ray astronomy at very high energies. Being co-aligned with the ASTRI-Horn camera axis, UVscope can measure the diffuse emission of the night sky background simultaneously with the ASTRI-Horn camera, without any interference with the main telescope data taking procedures. UVscope is properly calibrated and it is used as an independent reference instrument for test and diagnostic of the novel ASTRI-Horn telescope.

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