ar X iv : a st ro - p h / 96 07 10 7 v 1 2 2 Ju l 1 99 6 An SSPM - Based High - Speed Near - Infrared Photometer for Astronomy

Received ; accepted – 2 – ABSTRACT We describe the design, operation, and performance of a new high-speed infrared photometer using the Solid-State Photomultiplier (SSPM) detector. single-photon counting capability over the 0.4-28 micron wavelength range, intrinsic time response of order 1 ns, and low detector noise (Petroff, et al., 1987). We have operated a 200x200-micron back-illuminated SSPM in a liquid-helium cooled dewar with a room-temperature transimpedance amplifier output. Single photon pulses can be easily distinguished above the amplifier noise. The individual photon pulses are binned at a selectable time resolution ranging from 5µs to 64 ms, and then written to Exabyte tape. In the first astronomical application of such a device, we have made observations of the Crab Nebula pulsar and Her X-1 at near-infrared wavelengths (J-, Hand nd K-bands), and we present the instrument sensitivities established by these observations. We discuss other astronomical observations which are either planned or currently underway. Finally, we present design specifications and predicted performances for a second-generation SSPM high-speed infrared photometer. – 3 –