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TRIDENT: an infrared camera optimized for the detection of methanated substellar companions around nearby stars

C. Marois·R. Doyon·D. Nadeau·R. Racine·M. Riopel·P. Vallee
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Abstract

A near-infrared (0.85-2.5 microns) camera in use at the Canada-France-Hawaii Telescope and at the 1.6m telescope of the Observatoire du Mont-Megantic is described. The camera is based on a Hawaii-1 1024x1024 HgCdTe array detector. Its main feature is to acquire three simultaneous images at three wavelengths (simultaneous differential imaging) across the methane absorption bandhead at 1.6 micron, enabling an accurate subtraction of the stellar point spread function (PSF) and the detection of faint close methanated companions. The instrument has no coronagraph and features a fast (1 MHz) data acquisition system without reset anomaly, yielding high observing efficiencies on bright stars. The performance of the instrument is described, and it is illustrated by CFHT images of the nearby star Ups And. TRIDENT can detect (3 sigma) a methanated companion with DeltaH=10 at 0.5 arcsec from the star in one hour of observing time. Non-common path aberrations between the three optical paths are the limiting factors preventing further PSF attenuation. Reference star subtraction and instrument rotation improve the detection limit by one order of magnitude.

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C. Marois, R. Doyon, D. Nadeau, R. Racine, M. Riopel, P. Vallee. 2002-12-02. TRIDENT: an infrared camera optimized for the detection of methanated substellar companions around nearby stars. https://doi.org/10.1117/12.457844

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