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Detector Linearity and Noise

Both the response and the noise of the detectors have been characterized as function of signal strength. Tab. 5.1 summarizes the overall properties of the detectors.

For sensitivity calculations, the noise  per reset interval may be summarized as

equation275

with S the signal in tex2html_wrap_inline2404 V/s and tex2html_wrap_inline2408 dimensionless (happens to be equal to the reset time in seconds). The empirically determined noise parameters tex2html_wrap_inline2710 (read noise, in tex2html_wrap_inline2404 V/s) tex2html_wrap_inline2714 (dark current noise, in tex2html_wrap_inline2404 V/s), and tex2html_wrap_inline2718 (signal shot noise, tex2html_wrap_inline2404 V tex2html_wrap_inline2722 /s tex2html_wrap_inline2722 ) have been obtained by forcing a fit through this function, and are summarized in Tab. 5.2. For the SW grating and the FP detectors the function works well up to a tex2html_wrap_inline2726 sec. For the LW grating detectors the function does not work well in describing the tex2html_wrap_inline2408 dependency, and the resulting values are not necessarily directly to be associated with read noise and dark noise. Parameter values are chosen in such a way that they give the best description for the short reset intervals.

For Band 4, test measurements show consistently a very poor increase of SNR for tex2html_wrap_inline2730 sec. The parameters listed apply to tex2html_wrap_inline2408 = 1 sec and tex2html_wrap_inline2408 = 2 sec. For longer tex2html_wrap_inline2408 no improvement in noise should be expected, but the tex2html_wrap_inline2738 function still applies.

 

 
detector T bias minimum int. tex2html_wrap_inline2742 average response min. system
system noise tex2html_wrap_inline2744 tex2html_wrap_inline2746 tex2html_wrap_inline2744
(K) (V) ( tex2html_wrap_inline2404 V/s) (electrons) ( tex2html_wrap_inline2404 V/s) ( tex2html_wrap_inline2404 V/s/Jy) (W/ tex2html_wrap_inline2756 )
gain=16 tex2html_wrap_inline2758
Gr-InSb 3 - 0.7 35 0.32 3.0 tex2html_wrap_inline2760
Gr-Si:Ga 3 12 1.5 75 0.32 1.6 tex2html_wrap_inline2760
Gr-Si:As 4.5 3.0 3.0 150 0.40 tex2html_wrap_inline2764 1.5 tex2html_wrap_inline2766
Gr-Ge:Be 2 0.6 2.0 100 1.00 1.3 tex2html_wrap_inline2768
F-P-Si:Sb 10 1.1 1.1 tex2html_wrap_inline2770 70 0.40 0.007 tex2html_wrap_inline2772
F-P-Ge:Be 2 0.6 3.0 200 0.40 0.0037 tex2html_wrap_inline2774
Table 5.1: Summary of SWS-FM detector properties for a reset time tex2html_wrap_inline2402 sec


Notes to Tab. 5.1:
All minimum noise and NEP's are conservative values for tex2html_wrap_inline2402 sec and gain=16 . tex2html_wrap_inline2746 's include the transmissions of the instrument (i.e., directly relate to tex2html_wrap_inline2784 's).
1) values listed for element 2; noise = 0.7 tex2html_wrap_inline2404 V/s for element 1
2) excess photon noise at tex2html_wrap_inline2788 V/s
3) measured at a signal power at which photon noise is negligible; except FP-Ge:Be where still some photon-noise is suspected; estimated photon-noise free tex2html_wrap_inline2746 = tex2html_wrap_inline2792 W/ tex2html_wrap_inline2756
4) int. is intercept: photon noise at signal = 10 tex2html_wrap_inline2404 V/s
5) 1 Jy = tex2html_wrap_inline2798 WHz tex2html_wrap_inline2800 , ISO telescope area taken as 0.28 m tex2html_wrap_inline2764

 

   

Band 1 2 3 4
detector InSb Si:Ga Si:As Ge:Be
range ( tex2html_wrap_inline2404 m)2.38-4.05 4.05-12.012.0-29.529.5-45.2
tex2html_wrap_inline2710 0.75 0.75 1.00 1.56
tex2html_wrap_inline2714 0.70 1.50 3.00 2.00
tex2html_wrap_inline2718 0.10 0.13 0.14 0.32
Table 5.2: Grating noise parameters


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Next: Saturation Up: Grating Sections Previous: Grating Spectral Response and

SWS Consortium
Wed Aug 7 17:20:29 MET DST 1996