J1031-6117 2012-07-18 05:13:39 07 0.12   306.411  506.8  10.5   12.7 Weak, close to beam FWHM, but unambiguous in ephemeris fold.
J1233-6344 2012-04-01 10:19:04 02 0.094  756.892  495.0  11.7   12.4 Weak, but unambiguous in ephemeris fold.
J1301-6310 2011-12-22 15:34:56 09 0.075  663.830   86.1  17.8   15.1 XRS (Prinz & Becker 2015arXiv151107713P). Unambiguous in ephemeris fold.
J1309-6526 2012-04-14 10:01:12 03 0.091  398.292  340.0  20.3   10.8 Weak detection.
J1322-6329 2012-04-05 14:47:06 10 0.096 2764.209  659.   26.6   13.0 Significant RFI contamination. Pulsar only detectable in ephemeris fold after additional cleaning.
J1501-5637 2011-12-13 18:40:47 11 0.11   782.949  258.0  18.2   11.0 Significant RFI contamination.
J1509-5850 2012-04-03 19:16:00 03 0.094   88.922  140.6  13.4    9.4 HE pulsar (Weltevrede et al. 2010ApJ...708.1426W). Weakly detected in ephemeris fold, close to S/N_min_.
J1524-5819 2012-08-01 10:10:14 07 0.096  961.043  406.6  15.9    8.8 Weakly detected in ephemeris fold, below S/N_min_.
J1550-5418 2011-07-14 05:40:23 01 0.022 2069.833  830.0 114.0 a      Magnetar, AXP 1E 1547.0-5408 (Camilo et al. 2007ApJ...666L..93C).
J1611-4811 2011-12-27 19:03:07 08 0.047 1296.850  221.0  12.4    8.6 Weakly detected in ephemeris fold, below S/N_min_.
J1633-4805 2011-12-30 19:34:06 13 0.096  710.830 1120.0  15.0   14.4 Unambiguous in ephemeris fold.
J1709-4342 2011-12-12 05:16:53 02 0.10  1735.898  281.0  15.7   17.0 RFI contamination.
J1709-4401 2012-09-24 06:43:27 01 0.026  865.235  225.8 233.0        Described as 'intermittent' (Tiburzi et al. 2013MNRAS.436.3557T).
J1733-2837 2011-12-07 03:42:23 03 0.070  768.185  225.0  14.4   15.5 Significant RFI contamination.
J1738-3107 2011-12-22 22:10:51 03 0.10   549.498  735.0  19.3   12.3 Weak, but unambiguous in ephemeris fold.
J1747-2958 2012-08-03 09:31:42 08 0.061   98.814  101.5  21.0        Discovered by Camilo et al. (2007ApJ...666L..93C) with S_1400_=0.25mJy. Associated with the Mouse Nebula, with flux variability likely due to interstellar scintillation. Also undetected by Ng et al. (2015MNRAS.450.2922N).
J1755-2534 2012-07-26 12:48:29 02 0.12   233.541  590.0  10.6   11.6 Weak, close to beam FWHM, but unambiguous in ephemeris fold.
J1801-2115 2012-03-30 22:36:23 01 0.078  438.113  778.8  14.3   10.2 Weak detection.
J1819-1131 2012-08-05 08:17:44 02 0.069 1388.137  578.0  17.7   11.4 Weak, but unambiguous in ephemeris fold. Possible red noise confusion.
J1819-1717 2012-07-26 14:01:59 03 0.12   393.522  405.0  14.9   14.6 Unambiguous in ephemeris fold.
J1822-1617 2012-07-25 14:25:48 12 0.064  831.156  647.0  11.3   10.2 Wide pulse profile with {delta}~14 per cent, appears to be scattered.