| PSR | S350 (mJy) | S1380 (mJy) | S2273 (mJy) | SI |
| J1721-2457 | 0.58(2) | 0.28(3) | -1.5(2) | |
| J1745-0952 | 1.8(3) | 0.38(3) | -1.14(12) | |
| J1810-2005 | 1.33(2) | 0.95(4) | -0.67(3) | |
| J1918-0642 | 5.9(6) | 0.58(2) | -1.67(6) |
Notes. These numbers correspond to the WSRT profiles in Fig. 1. Measurements of flux densities at 350 and 2273 MHz, and PSR J1918-0642 at 1380 MHz are based on one or two 50 min observations, and therefore should be regarded as indicative of the intensities of the pulsars at the observed frequencies only. The ranges in flux densities, and consequently, SI calculations, are now based on the uncertainties in duty cycles.
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