You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
22 July 2008Teledyne Imaging Sensors: infrared imaging technologies for astronomy and civil space
James W. Beletic,1 Richard Blank,1 David Gulbransen,1 Donald Lee,1 Markus Loose,1 Eric C. Piquette,1 Thomas Sprafke,1 William E. Tennant,1 Majid Zandian,1 Joseph Zino1
Teledyne Imaging Sensors develops and produces high performance infrared sensors, electronics and packaging for
astronomy and civil space. These IR sensors are hybrid CMOS arrays, with HgCdTe used for light detection and a
silicon integrated circuit for signal readout. Teledyne manufactures IR sensors in a variety of sizes and formats.
Currently, the most advanced sensors are based on the Hawaii-2RG (H2RG), 2K×2K array with 18 μm pixel pitch. The
HgCdTe detector achieves very low dark current (<0.01 e-/pixel/sec) and high quantum efficiency (80-90%) over a wide
bandpass. Substrate-removed HgCdTe can simultaneously detect visible and infrared light, enabling spectrographs to
use a single focal plane array (FPA) for Visible-IR sensitivity. The SIDECARTM ASIC provides focal plane electronics
on a chip, operating in cryogenic environments with very low power (<11 mW). The H2RG and SIDECARTM have been
qualified to NASA Technology Readiness Level 6 (TRL-6). Teledyne continues to advance the state-of-the-art and is
producing a high speed, low noise array designed for IR wavefront sensing. Teledyne is also developing a 4K×4K, 15
µm pixel infrared array that will be a cost effective module for the large focal planes of the Extremely Large Telescopes
and future generation space astronomy missions.
The alert did not successfully save. Please try again later.
James W. Beletic, Richard Blank, David Gulbransen, Donald Lee, Markus Loose, Eric C. Piquette, Thomas Sprafke, William E. Tennant, Majid Zandian, Joseph Zino, "Teledyne Imaging Sensors: infrared imaging technologies for astronomy and civil space," Proc. SPIE 7021, High Energy, Optical, and Infrared Detectors for Astronomy III, 70210H (22 July 2008); https://doi.org/10.1117/12.790382