cmos imagers
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Author(s):  
Martín Pérez ◽  
Juan Jerónimo Blostein ◽  
Fabricio Alcalde Bessia ◽  
Aureliano Tartaglione ◽  
Iván Sidelnik ◽  
...  

2017 ◽  
Vol 12 (1) ◽  
pp. 47-55
Author(s):  
R. A. Souza ◽  
L. G. M. Ventura ◽  
A. R. S. Martins ◽  
D. W. de Lima Monteiro ◽  
L. P. Salles

The Active Pixel Sensor (APS) has been a vastly used integrated circuit topology in CMOS imagers. Mismatch of physical parameters among pixels, caused by process variations, introduces Fixed-Pattern Noise (FPN) at the array output. Correlated Double Sampling (CDS) in voltage mode is a commonly used method to suppress the offset caused FPN. However, it increases the complexity as well as the demanded silicon area of either the pixel or the external circuitry, besides having its signal swing restricted by the supply voltage. An alternative CDS circuit operating in current mode to reduce FPN is presented in this paper. The correlated current signals are sampled and subtracted using a simpler circuitry, leading to a more efficient relation of FPN reduction for the required silicon area. Furthermore, this technique does not change the APS topology or basic operation cycle. A simulated and tested CDS alternative is presented, and a simulated further improved version is proposed. Simulation and experiments showed a 40% FPN reduction with the fabricated CDS, whereas the improved simulated version ensures 90% FPN reduction.


2017 ◽  
Vol 14 (S339) ◽  
pp. 193-196
Author(s):  
M. J. Lehner ◽  
S-Y. Wang ◽  
M. Reyes-Ruiz ◽  
Z-W. Zhang ◽  
L. Figueroa ◽  
...  

AbstractTAOS II is a next-generation occultation survey with the goal of measuring the size distribution of the small end of the Kuiper Belt (objects with diameters 0.5–30 km). Such objects have magnitudes r > 30, and are thus undetectable by direct imaging. The project will operate three telescopes at San Pedro Mártir Observatory in Baja California, México. Each telescope will be equipped with a custom-built camera comprised of a focal-plane array of CMOS imagers. The cameras will be capable of reading out image data from 10,000 stars at a cadence of 20 Hz. The telescopes will monitor the same set of stars simultaneously to search for coincident occultation detections, thus minimising the false-positive rate. This talk described the project, and reported on the progress of the development of the survey infrastructure.


2017 ◽  
Author(s):  
James Janesick ◽  
Tom Elliott ◽  
James Andrews ◽  
John Tower
Keyword(s):  

2017 ◽  
Vol 53 (1) ◽  
pp. 16-18 ◽  
Author(s):  
M.‐K. Kim ◽  
S.‐K. Hong ◽  
J. Gou ◽  
O.‐K. Kwon
Keyword(s):  

2016 ◽  
Author(s):  
Mark Downing ◽  
Johann Kolb ◽  
Bart Dierickx ◽  
Arnaud Defernez ◽  
Philippe Feautrier ◽  
...  

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