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Table 2.

Overview of the upper limits from both time and imaging domain.

L-band S1-band
Target D Lmean FSP FIm LIm FULP LULP Lmean FSP FIm LIm FULP LULP
Prefactor – 1013 1013 10−3 1013 10−3 1013 1013 1013 10−3 1013 10−3 1013
Units kpc erg Hz Mathematical equation: $ \frac{erg}{Hz} $ erg Hz s Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz\ s}}} $ Jy erg Hzs Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz\ s}}} $ Jy s erg Hz Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz}}} $ erg Hz Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz}}} $ erg Hz s Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz\ s}}} $ Jy erg Hz s Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz\ s}}} $ Jy s erg Hz Mathematical equation: $ \frac{\mathrm{{erg}}}{\mathrm{{Hz}}} $
1E 1048.1-5937 9.0 5.29 6.92 0.60 60.56 2.50 254.5 3.97 5.29 1.34 136.1 0.90 91.61
1E 1841-045 8.5 4.72 6.17 6.30 572 0.60 54.48 3.54 4.72 0.41 37.24 0.40 36.32
1RXS J170849.0 3.8 0.94 1.23 0.43 7.76 0.80 14.52 – – – – – –
3XMM J185246.6 7.1 3.29 4.31 2.45 155.2 0.60 38.01 2.47 3.29 0.70 44.25 0.30 19.00
CXOU J164710.2 3.9 0.99 1.30 0.47 9.00 0.60 11.47 – – – – – –
CXOU J171405.7 13.2 – – – – – – 8.54 11.4 – – – –
SGR 1627-41 11.0 – – – – – – 5.93 7.91 – – – –
SGR 1806-20 8.7 4.95 6.47 11.8 1119 1.00 95.11 3.71 4.95 – – – –
SGR 1833-0832 10.0 6.53 8.55 0.11 14.43 1.00 125.7 4.90 6.53 – – – –
SGR 1900+14 12.5 10.2 13.35 0.42 82.47 0.50 98.17 7.66 10.21 0.16 32.16 0.20 39.27
SGR 1935+2154 9.0 5.29 6.92 0.67 68.33 0.40 40.72 3.97 5.29 0.17 17.60 0.20 20.36
Swift J1822.3-1606 1.6 0.17 0.22 3.79 12.21 1.30 4.18 – – – – – –
Swift J1834.9-0846 4.2 1.15 1.51 1.47 32.59 0.40 8.87 0.86 1.15 1.01 1.40 0.50 11.08
ASKAP J1935+2148 5 – – 0.34 10.64 0.4 12.57 – – 0.17 0.33 0.20 6.28
SGR1808-20 10 – – 0.77 96.76 0.8 100.5 – – – – – –

Notes. For each target the assumed distance (from the magnetar catalogue and Caleb et al. (2024)), the spectral luminosity Lmean for the folded profile, the spectral single pulse fluence FSP, the flux density limits from the total intensity FIm, and the corresponding spectral luminosity LIm, as well as the flux density upper limits from the light curves FULP and the corresponding spectral luminosity LULP, are given for both the L and S1-band observations. Due to the offset of the S1-band imaging observation, SGR 1627-41 and CXOU J171405.7 do not have any imaging upper limits, and the time domain ones are only for epoch 2.

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