Characterization of a 15 $\mu m$ Cutoff HgCdTe Detector Array for Astronomy

The University of Rochester infrared detector group is working together with Teledyne Imaging Sensors to develop HgCdTe 15 $\mu m$ cutoff wavelength detector arrays for future space missions. To reach the 15 $\mu m$ cutoff goal, we took an intermediate step by developing four $\sim$13 $\mu m$ cutoff wavelength arrays to identify any unforeseen effects related to increasing the cutoff wavelength from the extensively characterized 10 $\mu m$ cutoff wavelength detector arrays developed for the NEOCam mission. The characterization of the $\sim$13 $\mu m$ cutoff wavelength HgCdTe arrays at the University of Rochester allowed us to determine the key dark current mechanisms that limit the performance of these HgCdTe detector arrays at different temperatures and bias when the cutoff wavelength is increased. We present initial dark current and well depth measurements of a 15 $\mu m$ cutoff array which shows dark current values two orders of magnitude smaller at large reverse bias than would be expected from our previous best structures.