The kilopixel array pathfinder project (KAPPa), a 16-pixel integrated heterodyne focal plane array: characterization of the single pixel prototype

Abstract

We report on the laboratory testing of KAPPa, a 16-pixel proof-of-concept array to enable the creation THz imaging spectrometer with ~1000 pixels. Creating an array an order of magnitude larger than the existing state of the art of 64 pixels requires a simple and robust design as well as improvements to mixer selection, testing, and assembly.Our testing employs a single pixel test bench where a novel 2D array architecture is tested. The minimum size of the footprint is dictated by the diameter of the drilled feedhorn aperture. In the adjoining detector block, a 6mm × 6mm footprint houses the SIS mixer, LNA, matching and bias networks, and permanent magnet. We present an initial characterization of the single pixel prototype using a computer controlled test bench to determine Y-factors for a parameter space of LO power, LO frequency, IF bandwidth, magnet field strength, and SIS bias voltage. To reduce the need to replace poorly preforming pixels that are already mounted in a large format array, we show techniques to improve SIS mixer selection prior to mounting in the detector block.The 2D integrated 16-pixel array design has been evolved as we investigate the properties of the single pixel prototype. Carful design of the prototype has allowed for rapid translation of single pixel design improvements to be easily incorporated into the 16-pixel model.

Automated reduction of sub-millimetre single-dish heterodyne data from the James Clerk Maxwell Telescope using orac-dr

“…As heterodyne receivers have progressed from single-detector instruments (Padman et al 1992;Davies et al 1992;Cunningham et al 1992) to small focal-plane arrays (Graf et al 2003;Schuster et al 2004) to 16-element arrays such as HARP at JCMT (Buckle et al 2009), and beyond (Kloosterman et al 2012;Hurtado et al 2014), and correlators have improved such that we can easily obtain spectra at 10 Hz with 8192 channels, data rates have increased substantially such that it is now common-place to take a short observation resulting in thousands of spectra. This is only going to become more challenging with the advent of instruments with 64,000 channels and dual-waveband arrays each of which consist of 128 detectors, such as the CHAI instrument proposed for CCAT or KAPPa successors (Wheeler et al 2014).…”