Abstract
We explore the feasibility of using current generation, off-the-shelf, indium gallium arsenide (InGaAs) near-infrared (NIR) detectors for astronomical observations. Light-weight InGaAs cameras, developed for the night vision industry and operated at or near room temperature, enable cost-effective new paths for observing the NIR sky, particularly when paired with small telescopes. We have tested an InGaAs camera in the laboratory and on the sky using 12 and 18 inch telescopes. The camera is a small-format, 320×240 pixels of 40 μm pitch, shortwave infrared (SWIR) device from Sensors Unlimited. Although the device exhibits a room-temperature dark current of 5.7×104 e- s-1 per pixel, we find observations of bright sources and low-positional-resolution observations of faint sources remain feasible. We can record unsaturated images of bright (J=3.9) sources due to the large pixel well-depth and resulting high dynamic range. When mounted on an 18 inch telescope, the sensor is capable of achieving milli-magnitude precision for sources brighter than J=8. Faint sources can be sky-background-limited with modest thermoelectric cooling. We can detect faint sources (J=16.4 at 10σ) in a one-minute exposure when mounted to an 18 inch telescope. From laboratory testing, we characterize the noise properties, sensitivity, and stability of the camera in a variety of different operational modes and at different operating temperatures. Through sky testing, we show that the (unfiltered) camera can enable precise and accurate photometry, operating like a filtered J-band detector, with small color corrections. In the course of our sky testing, we successfully measured sub-percent flux variations in an exoplanet transit. We have demonstrated an ability to detect transient sources in dense fields using image subtraction of existing reference catalogs.
Original language | English (US) |
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Article number | 095001 |
Journal | Publications of the Astronomical Society of the Pacific |
Volume | 130 |
Issue number | 991 |
DOIs | |
State | Published - Sep 2018 |
Externally published | Yes |
Bibliographical note
Funding Information:This paper makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
Funding Information:
Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts.
Publisher Copyright:
© 2018. The Astronomical Society of the Pacific. All rights reserved.
Keywords
- Instrumentation: detectors