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Table 1
Optimal signal-to-noise ratio obtained by correlating interferometer pairs for the l = m = 2,3,4f-modes and supernova-derived NSs with the HB06 CSFR (see Sect. 2).
| Pair | l = m = 2 | l = m = 3 | l = m = 4 |
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| aL/aV | 9.80 | 1.53 | 6.07 × 10-2 |
| ET | 1130 | 193 | 10.6 |
Notes. Here 10% of the NS population becomes f-mode unstable and 100% of the rotational energy lost during the instability is due to GWs.
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