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Table 5:

Upper limits in mK as a function of angular size on the sky from the spectral surveys observations during 2006/07 (deep searches are not included) using 1, 4 and 16 MHz channel spacings.
    1 MHz channel spacing  
Position 2-5$^\prime$ Peak intensity 5-10$^\prime$ Peak intensity 10-15$^\prime$ Peak intensity 15-30$^\prime$ Peak intensity
  1$\sigma $ [mK] [$\sigma $] 1$\sigma $ [mK] [$\sigma $] 1$\sigma $ [mK] [$\sigma $] 1$\sigma $ [mK] [$\sigma $]
A 16 (23) 3.0 (3.3) 21 (31) 3.2 (3.4) 21 (31) 3.2 (3.4) 21 (31) 3.2 (3.4)
B 17 (26) 3.1 (2.9) 23 (34) 3.3 (3.2) 23 (34) 3.3 (3.2) - -
C 19 (26) 3.3 (3.0) 19 (26) 3.3 (3.0) 25 (35) 3.1 (3.2) - -
D 15 (25) 3.1 (2.9) 15 (25) 3.1 (2.9) 20 (33) 3.2 (3.1) 20 (33) 3.2 (3.1)
    4 MHz channel spacing  
A 10 (15) 3.0 (2.8) 13 (20) 3.0 (2.9) 13 (20) 3.0 (2.9) 13 (20) 3.0 (2.9)
B 11 (17) 2.7 (3.0) 15 (23) 2.9 (3.1) 15 (23) 2.9 (3.1) - -
C 12 (16) 3.0 (2.9) 12 (16) 3.0 (2.9) 16 (22) 2.9 (3.0) - -
D 10 (15) 2.9 (3.1) 10 (15) 2.9 (3.1) 13 (20) 3.1 (3.0) 13 (20) 3.1 (3.0)
    16 MHz channel spacing  
A 5 (8) 2.7 (2.8) 6 (11) 3.0 (2.9) 6 (11) 3.0 (2.9) 6 (11) 3.0 (2.9)
B 6 (9) 2.8 (3.0) 8 (12) 2.7 (3.1) 8 (12) 2.7 (3.1) - -
C 6 (11) 2.7 (2.8) 6 (11) 2.7 (2.8) 8 (14) 3.0 (2.9) - -
D 5 (8) 2.9 (3.0) 5 (8) 2.9 (3.0) 7 (11) 2.8 (3.1) 7 (11) 2.8 (3.1)

Notes. The limits are for the data taken with the AOS(AC) and for frequency ranges 542.0-547.5 (486.5-492) GHz.


Source LaTeX | All tables | In the text

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