Table 2
List of the most prominent peaks in Fig. 5.
| ν [nHz] | Pgw [d] | parameters affected | k | l | m | ν − νk, l,m [nHz] | |
|---|---|---|---|---|---|---|---|
| 4.3 | 2663.8 | pm | 0 | 0 | 1 | −0.1 | |
| 20.1 | 574.9 | pm | −5 | 1 | −1 | −0.8 | |
| 26.1 | 442.9 | pos | −5 | 1 | 0 | +0.7 | |
| 29.0 | 398.1 | pm | −5 | 1 | 1 | −0.7 | |
| 32.3 | 357.9 | plx | 1 | 0 | 0 | +0.6 | |
| 51.1 | 226.0 | pm | −4 | 1 | −1 | −1.5 | |
| 57.2 | 202.2 | plx | −4 | 1 | 0 | +0.1 | |
| 59.6 | 194.0 | pm | { | −4 | 1 | 1 | −1.8 |
| 2 | 0 | −1 | +0.6 | ||||
| 63.6 | 181.7 | pos | 2 | 0 | 0 | +0.2 | |
| 68.0 | 170.0 | pm | 2 | 0 | 1 | +0.2 | |
| 84.5 | 136.9 | pm | −3 | 1 | −1 | +0.1 | |
| 88.5 | 130.8 | pos, plx | −3 | 1 | 0 | −0.2 | |
| 93.3 | 123.9 | pm | −3 | 1 | 1 | +0.2 | |
| 96.0 | 120.4 | plx | 3 | 0 | 0 | +0.9 | |
| 115.6 | 100.0 | pm | −2 | 1 | −1 | −0.4 | |
| 119.8 | 96.6 | pos, plx | −2 | 1 | 0 | −0.6 | |
| 123.9 | 93.3 | pm | { | −2 | 1 | 1 | −0.9 |
| 4 | 0 | −1 | +1.5 | ||||
| 128.3 | 90.1 | pos | 4 | 0 | 0 | +1.5 | |
| 131.4 | 88.0 | pm | 4 | 0 | 1 | +0.3 | |
| 147.8 | 78.2 | pm | −1 | 1 | −1 | +0.0 | |
| 152.4 | 75.9 | pos, plx | −1 | 1 | 0 | +0.3 | |
| 156.5 | 73.9 | pm | −1 | 1 | 1 | −0.0 | |
| 183.4 | 63.0 | plx | 0 | 1 | 0 | −0.4 | |
| 186.4 | 62.0 | pm | 6 | 0 | −1 | +0.7 | |
| 190.0 | 60.8 | pos | 6 | 0 | 0 | −0.1 | |
| 195.0 | 59.3 | pm | 6 | 0 | 1 | +0.5 | |
| 211.1 | 54.8 | pm | 1 | 1 | −1 | +0.0 | |
| 215.5 | 53.7 | pos, plx | 1 | 1 | 0 | +0.0 | |
| 219.9 | 52.6 | pm | 1 | 1 | 1 | -0.0 |
Notes. Columns 1–2 give the peak frequency as measured from the simulations and the corresponding period. Column 3 shows the astrometric parameters for which the peak was detected in the data at that frequency (pos = α and/or δ; plx = ϖ; pm = µα* and/or µδ). When the peak was detected in both position and parallax errors, the mean frequency is given. Columns 4–6 give our interpretation of the frequency in terms of the integers k, l, and m in Eq. (13). The last column gives the difference between the measured and calculated frequency. As discussed in the text, the peaks at ν = 59.6 and 123.9 nHz may be blends of νk,l,m for the given combinations of k, l, and m. The GW frequencies and periods given in this table are shown by red vertical tick marks on the left pictures of Fig. 5.
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