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Performance Figures AOT SWS06

Table and figures presented in this section are derived either from data taken during the Performance Verification phase or with the current version of the logic.

   figure959
Figure: Sensitivity of AOT SWS06. Spectral flux density vs. wavelength, detectable at SNR = 20 per resolution element. It is assumed that a pure integration time of 120 sec is used for the wavelength range of 30 scanner steps covered by AOT SWS06

 

Band tex2html_wrap_inline3222 tex2html_wrap_inline3224 6 tex2html_wrap_inline2948
0.1 Jy 0.3 Jy 1 Jy 3 Jy 10 Jy 30 Jy 100 Jy
1A 2.381 2.489 21677 3124 566 384 384 384
2.489 2.600 6324 956 392 392 392 392
1B 2.600 2.749 14953 1680 566 384 384 384
2.749 2.898 33617 6124 928 386 386 386 386
2.883 3.020 20221 2924 542 372 372 372 372
1D 3.021 3.167 18661 3124 566 384 384 384 384
3.167 3.312 31141 6124 572 386 386 386 386
3.312 3.455 28021 3124 572 386 386 386 386
3.455 3.520 24485 2924 536 300 300 300 300
1E 3.520 3.746 12053 1680 566 384 384 384
3.746 3.972 28021 3124 572 386 386 386 386
3.836 4.050 20845 3024 548 376 376 376 376
2A 4.051 4.305 7681 3809 408 408 408
4.305 4.556 31177 3809 616 408 408
4.556 4.805 24089 3705 600 400 408
4.805 5.050 31177 3809 616 408 408
5.050 5.291 31177 3809 616 408 408
5.074 5.300 27301 3601 590 396 396
2B 5.302 5.824 27301 3809 616 408 408
5.824 6.343 17681 3809 408 408 408
6.343 6.860 25003 3809 616 408 408
6.498 7.000 18461 3705 608 404 404
2C 7.000 7.511 5459 1032 408 408 408
7.511 8.023 5561 1032 408 408 408
8.023 8.531 5561 1032 408 408 408
8.531 9.035 7409 1032 408 408 408
9.035 9.533 11513 1957 408 408 408
9.533 10.025 13349 1957 408 408 408
10.025 10.509 18893 3809 408 408 408
10.509 10.985 23009 3809 616 408 408
10.985 11.400 35189 4949 572 386 386
11.400 11.860 7513 1032 408 408
11.544 12.000 7409 1032 408 408
Table 6.7: AOT SWS06 grating scan observing times for wavelength intervals corresponding to tex2html_wrap_inline2438 80 resolution elements of sources of 0.3, 1, 3, 10, 30, and 100 Jy. In all cases a SNR = 20 per resolution element was requested, but may be exceeded.  

 

Band tex2html_wrap_inline3222 tex2html_wrap_inline3224 6 tex2html_wrap_inline2948
0.1 Jy 0.3 Jy 1 Jy 3 Jy 10 Jy 30 Jy 100 Jy
3A 12.000 12.889 4121 648 424
12.889 13.773 27509 4121 648 424 424
13.773 14.652 12377 2093 424 424 424
14.652 15.524 20297 4017 424 424 424
15.176 16.000 16029 1993 412 424 424
16.000 16.500 5765 720 332 332
3C 16.500 16.840 7929 1721 300 300 300
16.840 17.669 18577 4017 420 420 420
17.669 18.484 35069 4017 640 420 420
18.484 19.285 5765 1080 420 420
18.726 19.500 9979 1048 412 412
3D 19.500 21.272 24209 4017 640 420 420
21.272 23.029 14573 2027 420 420 420
23.029 24.773 7825 1080 420 420 420
24.773 26.509 7825 1080 420 420 420
26.509 27.5 10529 1293 326 326 326
3E 27.500 28.235 4225 942 300 300 300
28.235 28.999 5969 1164 300 300 300
4 29.000 31.462 20081 2977 624 412
31.462 33.565 7305 928 384 384
33.565 35.634 7305 928 384 384
35.634 37.662 7305 928 384 384
37.662 39.644 7409 928 384 384
39.644 41.576 10309 928 384 384
41.576 43.460 10309 1393 384 384
43.460 45.199 17121 2457 548 374
Table 6.8: Continuation of AOT SWS06 grating scan observing times


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Next: AOT SWS07: Combined Fabry-Pérot Up: AOT SWS06: Grating Scan Previous: Raster observations with AOT

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