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  • Detector Array  (1)
  • space instrumentation  (1)
  • 1
    ISSN: 1572-9508
    Keywords: FIR detectors ; MIPS ; SIRTF ; space instrumentation
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We present data from a 16×32 array of unstressed Ge:Gadetectors, showing the long time constant responses and hook effectcharacteristic of these devices. This array is half the size of the70 μm imaging array planned for MIPS, the Multiband ImagingPhotometer for SIRTF. We present simulations of the FIR (farinfrared) sky as viewed by a MIPS array, including realistic noiseeffects and extraction of point sources with a standard photometrypackage, showing that the photometric goals of MIPS are attainablewith the current array performance and using standard analysistechniques. Previous calculations by Heim et al. (1998) haddetermined that MIPS would achieve 5-σ detections of ≤1 mJy at 70 μm in 2000 s; the simulations presented hereobtain results consistent with those calculations.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    International journal of infrared and millimeter waves 12 (1991), S. 859-884 
    ISSN: 1572-9559
    Keywords: Spectrometer ; Infrared Astronomy ; Infrared Techniques ; Detector Array ; Cryogenic Electronics ; Fabry-Perot ; Cryogenic ; Imaging ; Instrument Function
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract FIFI is an imaging spectrometer with two or three Fabry-Perot interferometers (FPI) in series for airborne astronomical observations in the far-infrared range (λ=40...200μm). It employs 5×5 arrays of photoconducting detectors and offers spectral resolutions as small as 2km/s. Resolution and bandwidth can be set over a wide range to match a variety of astronomical sources. Cryogenic optics minimizes thermal background radiation and provides for in-flight step tunable spatial resolution. At 158 μm wavelength the background-limited NEP is 3 × 10-15W/ℚHz at 40 km/s resolution and with two FPI's; with three FPI's the expected NEP is ≤10-15W√Hz at 5 km/s resolution. The frequency-chopping mode of the high-resolution Fabry-Perot allows for line detection in extended objects. Absolute internal flux calibration ensures adequate “flat fielding” of the array elements.
    Type of Medium: Electronic Resource
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