Table 3.
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The values of rms/mean estimated from the light curves of highly inclined SMBH binary systems, based on the flare emission profiles in DD18. Listed here are values for two selected values of mass ratio, four selected values of NE, the fraction of an Einstein radius separating the lens and the source at closest approach, and two wavebands, NUV and V. Also listed, in parentheses, are estimates of log(Prat) assuming a mixture of a Q = 30 QPO at the MF QPO frequency, 8.0 × 10−7 Hz, and a continuum PSD with β = 2.3 and a normalization of 20 Hz−1 at 10−6 Hz.

Mass ratio q = 0.05Mass ratio q = 0.5
NENUVVNUVV
0.050.752 (5.67)0.471 (5.27)0.784 (5.70)0.504 (5.33)
0.10.471 (5.27)0.281 (4.82)0.504 (5.33)0.307 (4.89)
0.50.095 (3.87)0.074 (3.66)0.105 (3.96)0.082 (3.75)
1.00.030 (2.88)0.030 (2.88)0.033 (2.96)0.033 (2.96)
Mass ratio q = 0.05Mass ratio q = 0.5
NENUVVNUVV
0.050.752 (5.67)0.471 (5.27)0.784 (5.70)0.504 (5.33)
0.10.471 (5.27)0.281 (4.82)0.504 (5.33)0.307 (4.89)
0.50.095 (3.87)0.074 (3.66)0.105 (3.96)0.082 (3.75)
1.00.030 (2.88)0.030 (2.88)0.033 (2.96)0.033 (2.96)
Table 3.
Open in new tab

The values of rms/mean estimated from the light curves of highly inclined SMBH binary systems, based on the flare emission profiles in DD18. Listed here are values for two selected values of mass ratio, four selected values of NE, the fraction of an Einstein radius separating the lens and the source at closest approach, and two wavebands, NUV and V. Also listed, in parentheses, are estimates of log(Prat) assuming a mixture of a Q = 30 QPO at the MF QPO frequency, 8.0 × 10−7 Hz, and a continuum PSD with β = 2.3 and a normalization of 20 Hz−1 at 10−6 Hz.

Mass ratio q = 0.05Mass ratio q = 0.5
NENUVVNUVV
0.050.752 (5.67)0.471 (5.27)0.784 (5.70)0.504 (5.33)
0.10.471 (5.27)0.281 (4.82)0.504 (5.33)0.307 (4.89)
0.50.095 (3.87)0.074 (3.66)0.105 (3.96)0.082 (3.75)
1.00.030 (2.88)0.030 (2.88)0.033 (2.96)0.033 (2.96)
Mass ratio q = 0.05Mass ratio q = 0.5
NENUVVNUVV
0.050.752 (5.67)0.471 (5.27)0.784 (5.70)0.504 (5.33)
0.10.471 (5.27)0.281 (4.82)0.504 (5.33)0.307 (4.89)
0.50.095 (3.87)0.074 (3.66)0.105 (3.96)0.082 (3.75)
1.00.030 (2.88)0.030 (2.88)0.033 (2.96)0.033 (2.96)
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