Precision of a Low-Cost InGaAs Detector for Near Infrared Photometry

Abstract

We have designed, constructed, and tested an InGaAs near-infrared camera to explore whether low-cost detectors can make small (≤1 m) telescopes capable of precise (<1 mmag) infrared photometry of relatively bright targets. The camera is constructed around the 640 × 512 pixel APS640C sensor built by FLIR Electro-Optical Components. We designed custom analog-to-digital electronics for maximum stability and minimum noise. The InGaAs dark current halves with every 7°C of cooling, and we reduce it to 840 e[superscript -]s[superscript -1]pixel[superscript -1] (with a pixel-to-pixel variation of ±200 e[superscript -]s[superscript -1]pixel[superscript -1]) by cooling the array to 20°C. Beyond this point, glow from the readout dominates. The single-sample read noise of 149 [superscript -]e is reduced to 54 [superscript -]e through up-the-ramp sampling. Laboratory testing with a star field generated by a lenslet array shows that two-star differential photometry is possible to a precision of 631 ± 205 ppm (0.68 mmag) hr[superscript -1/2] at a flux of 2.4 × 10[superscript 4] e[superscript -]s[superscript -1]. Employing three comparison stars and decorrelating reference signals further improves the precision to 483 ± 161 ppm (0.52 mmag) hr[superscript -1/2]. Photometric observations of HD80606 and HD80607 (J - 7.7 and 7.8) in the Y band shows that differential photometry to a precision of 415 ppm (0.45 mmag) hr[superscript -1/2] is achieved with an effective telescope aperture of 0.25 m. Next-generation InGaAs detectors should indeed enable Poisson-limited photometry of brighter dwarfs with particular advantage for late-M and L types. In addition, one might acquire near-infrared photometry simultaneously with optical photometry or radial velocity measurements to maximize the return of exoplanet searches with small telescopes.