Readout Techniques for Drift and Low Frequency Noise Rejection in Infrared Arrays
Three different methods are presented to subtract thermal drifts and low-frequency noise from the signal of infrared array. The first is dead pixels with open Indium bumps, the second is reference output as implemented on the Hawaii2 multiplexer, and the third is dark pixels to emulate reference cel...
Saved in:
Published in | Scientific Detectors for Astronomy pp. 435 - 444 |
---|---|
Main Authors | , , , , , , |
Format | Book Chapter |
Language | English |
Published |
Dordrecht
Springer Netherlands
2004
|
Series | Astrophysics and Space Science Library |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | Three different methods are presented to subtract thermal drifts and low-frequency noise from the signal of infrared array. The first is dead pixels with open Indium bumps, the second is reference output as implemented on the Hawaii2 multiplexer, and the third is dark pixels to emulate reference cells having a capacity connected to the gate of the unit cell field-effect transistor (FET). The third method is the most effective and yields a reduction in readout noise from 15.4-9.4 erms. A novel method will be described to extend this readout technique to the Aladdin 1K×1K InSb array. |
---|---|
Bibliography: | European Southern Observatory Raytheon Infrared Operations |
ISBN: | 9781402017889 140201788X |
DOI: | 10.1007/1-4020-2527-0_56 |