SuperCam: A 64 pixel superheterodyne camera

Christopher Groppi, Christopher Walker, Craig Kulesa, Dathon Golish, Patrick Putz, Paul Gensheimer, Abby Hedden, Shane Bussmann, Sander Weinreb, Glenn Jones, Joseph Barden, Hamdi Mani, Tom Kuiper, Jacob Kooi, Art Lichtenberger, Thomas Cecil, Gopal Narayanan, Narayanan Gopal Narayanan

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Scopus citations

Abstract

We report on the development of SuperCam, a 64 pixel, superheterodyne camera designed for operation in the astrophysically important 870 μm atmospheric window. SuperCam will be used to answer fundamental questions about the physics and chemistry of molecular clouds in the Galaxy and their direct relation to star and planet formation. The advent of such a system will provide an order of magnitude increase in mapping speed over what is now available and revolutionize how observational astronomy is performed in this important wavelength regime. SuperCam is constructed by stacking eight, 1x8 rows of tunerless, SIS mixers. The SIS junctions use SOI (Silicon on Insulator) technology, with beamleads for device positioning and IF and ground electrical connections. The mixer modules are fabricated using a Kern MMP-2522 micromilling machine purchased specifically for this task. The IF output of each SIS device is directly connected to a low-noise, broadband MMIC amplifier module integrated into the mixer block. The instantaneous IF bandwidth of each pixel is 2 GHz, with a center frequency of 5 GHz. An IF processor constructed of eight 8-channel modules provides IF amplification, total power monitoring and baseband downconversion. A spectrum of the central 250 MHz or 500 MHz of each IF band is provided by the Omnisys real-time FFT spectrometer system, based on Xilinx Virtex 4 FPGAs. This spectrometer can operate in either 32 channel mode (500 MHz/channel) or 64 channel mode (250 MHz/channel). Local oscillator power is provided by a Virginia Diodes solid-state multiplier chain whose output is divided between the pixels with a matrix of waveguide power dividers. The mixer array is cooled to 4K by a closed-cycle cryostat with two cryocoolers. SuperCam will reside at the Cassegrain focus of the 10m Heinrich Hertz telescope (HHT) with a dedicated reimaging optics system. All subsystems of SuperCam have completed the development stage, and are undergoing testing. We present test results for the SuperCam LNA modules, integration of LNAs in a test mixer, IF processor performance, spectrometer performance, cryogenic system verification, and end-to-end measurements of the IF chain and backend. Results from the fabrication, construction and testing of prototype SOI mixers, in both single pixel and 8 pixel versions will be shown. We will enter the final fabrication stage in early 2007, with expected completion in late 2007. Science operations are expected to begin in Spring, 2008.

Original languageEnglish (US)
Title of host publicationProceedings of the Eighteenth International Symposium on Space Terahertz Technology 2007, ISSTT 2007
Pages264-269
Number of pages6
StatePublished - 2007
Externally publishedYes
Event18th International Symposium on Space Terahertz Technology 2007, ISSTT 2007 - Pasadena, CA, United States
Duration: Mar 21 2007Mar 23 2007

Other

Other18th International Symposium on Space Terahertz Technology 2007, ISSTT 2007
CountryUnited States
CityPasadena, CA
Period3/21/073/23/07

Keywords

  • Submillimeter heterodyne array

ASJC Scopus subject areas

  • Computer Networks and Communications
  • Space and Planetary Science
  • Electrical and Electronic Engineering
  • Atomic and Molecular Physics, and Optics
  • Radiation

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