Near-Infrared InGaAs Detectors for Background-limited Imaging and
Photometry
P. Sullivan, B. Croll, and R. Simcoe. (2014)cite arxiv:1406.2695Comment: Submitted to Proc. SPIE, Astronomical Telescopes + Instrumentation (2014).
Abstract
Originally designed for night-vision equipment, InGaAs detectors are
beginning to achieve background-limited performance in broadband imaging from
the ground. The lower cost of these detectors can enable multi-band
instruments, arrays of small telescopes, and large focal planes that would be
uneconomical with high-performance HgCdTe detectors. We developed a camera to
operate the FLIR AP1121 sensor using deep thermoelectric cooling and
up-the-ramp sampling to minimize noise. We measured a dark current of 163$~e$-
s$^-1$ pix$^-1$, a read noise of 87$~e$- up-the-ramp, and a well depth of
80k$~e$-. Laboratory photometric testing achieved a stability of 230 ppm
hr$^-1/2$, which would be required for detecting exoplanet transits. InGaAs
detectors are also applicable to other branches of near-infrared time-domain
astronomy, ranging from brown dwarf weather to gravitational wave follow-up.
Description
[1406.2695] Near-Infrared InGaAs Detectors for Background-limited Imaging and Photometry
%0 Generic
%1 sullivan2014nearinfrared
%A Sullivan, Peter W.
%A Croll, Bryce
%A Simcoe, Robert A.
%D 2014
%K detectors infrared
%T Near-Infrared InGaAs Detectors for Background-limited Imaging and
Photometry
%U http://arxiv.org/abs/1406.2695
%X Originally designed for night-vision equipment, InGaAs detectors are
beginning to achieve background-limited performance in broadband imaging from
the ground. The lower cost of these detectors can enable multi-band
instruments, arrays of small telescopes, and large focal planes that would be
uneconomical with high-performance HgCdTe detectors. We developed a camera to
operate the FLIR AP1121 sensor using deep thermoelectric cooling and
up-the-ramp sampling to minimize noise. We measured a dark current of 163$~e$-
s$^-1$ pix$^-1$, a read noise of 87$~e$- up-the-ramp, and a well depth of
80k$~e$-. Laboratory photometric testing achieved a stability of 230 ppm
hr$^-1/2$, which would be required for detecting exoplanet transits. InGaAs
detectors are also applicable to other branches of near-infrared time-domain
astronomy, ranging from brown dwarf weather to gravitational wave follow-up.
@misc{sullivan2014nearinfrared,
abstract = {Originally designed for night-vision equipment, InGaAs detectors are
beginning to achieve background-limited performance in broadband imaging from
the ground. The lower cost of these detectors can enable multi-band
instruments, arrays of small telescopes, and large focal planes that would be
uneconomical with high-performance HgCdTe detectors. We developed a camera to
operate the FLIR AP1121 sensor using deep thermoelectric cooling and
up-the-ramp sampling to minimize noise. We measured a dark current of 163$~e$-
s$^{-1}$ pix$^{-1}$, a read noise of 87$~e$- up-the-ramp, and a well depth of
80k$~e$-. Laboratory photometric testing achieved a stability of 230 ppm
hr$^{-1/2}$, which would be required for detecting exoplanet transits. InGaAs
detectors are also applicable to other branches of near-infrared time-domain
astronomy, ranging from brown dwarf weather to gravitational wave follow-up.},
added-at = {2014-06-12T09:43:08.000+0200},
author = {Sullivan, Peter W. and Croll, Bryce and Simcoe, Robert A.},
biburl = {https://www.bibsonomy.org/bibtex/2e6f7a7159c498bb5cc2b2098eb219791/miki},
description = {[1406.2695] Near-Infrared InGaAs Detectors for Background-limited Imaging and Photometry},
interhash = {c53714ceaa27090e15c28bc3063a8654},
intrahash = {e6f7a7159c498bb5cc2b2098eb219791},
keywords = {detectors infrared},
note = {cite arxiv:1406.2695Comment: Submitted to Proc. SPIE, Astronomical Telescopes + Instrumentation (2014)},
timestamp = {2014-06-12T09:43:08.000+0200},
title = {Near-Infrared InGaAs Detectors for Background-limited Imaging and
Photometry},
url = {http://arxiv.org/abs/1406.2695},
year = 2014
}