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Photometric characterization of the U.S. Naval Observatory HgCdTe IR camera

机译:美国海军天文台HgCdTe红外热像仪的光度表征

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Abstract: An IR camera based on a Rockwell 256 $MUL 256 HgCdTe (NICMOS III) array has been recently acquired by the U.S. Naval Observatory as part of a program to evaluate the astrometric characteristics of current-generation IR arrays. Results of a pixel-by-pixel photometric evaluation of this HgCdTe device are presented. Overall, the array is of extremely high quality with less than 100 (0.2%) photometrically unusable pixels. With a fairly stringent photometric selection based on linearity and full well, the bad pixel count is about 420. The average pixel photometric response is linear to within about 1.6% rms over a range of 0 - 120,000 e$+$MIN$/; using a quadratic relation reduces the calibration errors to under 1% rms. For comparison, the results of a similar test with a Texas Instruments TI800 $MUL 800 CCD (a prototype of the HST WF/PC 1) are shown. !7
机译:摘要:美国海军天文台最近购买了一种基于Rockwell 256 $ MUL 256 HgCdTe(NICMOS III)阵列的红外摄像机,作为评估当前IR阵列天体特性的程序的一部分。给出了此HgCdTe器件逐个像素的光度评估结果。总体而言,该阵列具有极高的质量,不到100个(0.2%)的光度学无法使用的像素。通过基于线性度和完全良好的相当严格的光度选择,不良像素数约为420。在0-120,000 e $ + $ MIN $ /的范围内,平均像素光度响应在rms范围内呈线性,约为1.6%。使用二次关系可将校准误差降低到1%rms以下。为了进行比较,显示了使用德州仪器TI800 $ MUL 800 CCD(HST WF / PC 1的原型)进行的类似测试的结果。 !7

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