% Spatial matches of all known pulsars with Toby 4-year DC TS>10 sources. Removed SMC. Removed J1856+0245 (Edot = 4.6e+36), which matches same source as J1858+0241, see 2PC Table 13. Removed J1717-5800, folded, and intriguing: https://confluence.slac.stanford.edu/display/SCIGRPS/PSUE+J1717m5800 Removed J1811-1925,J2022+3842 (Edot > 6e+36), see 2PC Table 13. Moved MSPs to bottom of list. "ellps" is Conf_95_SemiMajor. The catalog association pipeline result "ID_Name" is a variable-length list. A Fermi source can "match" >1 pulsars -- added blank lines for readability. Non-MSPs PSRJ angsep ellps ts P0 EDOT DIST Gb NickName ID_Name J1022-5813 0.08 0.15 14 1.6437 1.3e+33 7.24 -0.83 P7R41447P 1AGLJ1022-5822 2CG 284-00 J1210-5226 0.14 0.16 30 0.4241 1.2e+31 1.3 9.92 P7R41747 G296.5+10.0 J1542-5133 0.17 0.18 37 1.7839 4.1e+30 5.13 2.83 P7R42323G J1617-4216 0.03 0.09 14 3.4285 1.8e+31 3.6 5.92 P7R42419A 2FGL J1617.6-4219 J1653-4854 0.22 0.40 24 3.0595 4.8e+30 6.8 -3.26 P7R42547 J1711-4322 0.13 0.15 17 0.1026 9.7e+32 3.84 -2.24 P7R42599G J1725-3546 0.16 0.17 14 1.0325 5.4e+32 8.73 -0.15 P7R42647P 1FGL J1724.0-3611c J1733-2533 0.25 0.30 31 0.6598 2.9e+32 4.96 4.09 P7R42673 J1810-1441 0.17 0.21 13 0.2172 9.2e+31 5.0 2.03 P7R42804H J1818-1556 0.42 0.83 67 0.9527 3.2e+31 3.89 -0.23 P7R42830BP ERC030 G015.05-00.70 1FGL J1818.7-1557c 2FGL J1819.3-1523 G015.4+00.1 G015.1-01.6 J1821-1432 0.06 0.07 45 1.9151 3.0e+31 6.48 -0.17 P7R42830AH 1AGLJ1823-1454 0FGLJ1821.4-1444 J1822-1606 0.47 0.83 67 8.4377 2.0e+31 * -1.02 P7R42830BP ERC030 G015.05-00.70 1FGL J1818.7-1557c 2FGL J1819.3-1523 G015.4+00.1 G015.1-01.6 J1822-1617 0.56 0.83 67 0.8312 1.3e+32 9.39 -1.19 P7R42830BP ERC030 G015.05-00.70 1FGL J1818.7-1557c 2FGL J1819.3-1523 G015.4+00.1 G015.1-01.6 J1839-0643 0.08 0.08 54 0.4495 1.6e+33 6.65 -0.35 P7R42901 J1840-1419 0.27 0.54 20 6.5976 8.7e+29 0.84 -4.12 P7R42907P 1FGL J1842.0-1409 J1841-0456 0.09 0.16 25 11.7789 1.1e+33 9.6 -0.01 P7R42906P 2FGL J1841.2-0459c G027.4+00.0 G027.8+00.6 J1841-0500 0.15 0.16 25 0.9130 1.8e+33 7.01 -0.03 P7R42906P 2FGL J1841.2-0459c G027.4+00.0 G027.8+00.6 J1841-1404 0.41 0.54 20 1.3346 1.1e+31 6.45 -4.23 P7R42907P 1FGL J1842.0-1409 J1852+0008 0.13 0.15 47 0.4679 2.2e+33 5.7 -0.22 P7R42943 1FGL J1853.1+0032c G033.2-00.6 J1858+0241 0.51 0.57 11 4.6932 9.3e+30 6.55 -0.43 P7R42956 J1858+0313 EGRJ1856+0235 2FGL J1859.3+0312c G036.6-00.7 HESS J1857+026 J1923+1706 0.09 0.09 19 0.5472 1.0e+31 5.12 0.96 P7R43030G J2301+5852 0.03 0.05 79 6.9791 5.5e+31 3.3 -1.0 P7R43557 J2301+5852 G109.1-01.0 From this list, we could favor those where (angsep << ellps) and abs(Gb) > 1. For example, PSRJ angsep ellps ts P0 EDOT DIST Gb NickName ID_Name J1617-4216 0.03 0.09 14 3.4285 1.8e+31 3.6 5.92 P7R42419A 2FGL J1617.6-4219 J1653-4854 0.22 0.40 24 3.0595 4.8e+30 6.8 -3.26 P7R42547 J1733-2533 0.25 0.30 31 0.6598 2.9e+32 4.96 4.09 P7R42673 J1810-1441 0.17 0.21 13 0.2172 9.2e+31 5.0 2.03 P7R42804H J1822-1606 0.47 0.83 67 8.4377 2.0e+31 * -1.02 P7R42830BP ERC030 G015.05-00.70 1FGL J1818.7-1557c 2FGL J1819.3-1523 G015.4+00.1 G015.1-01.6 J1822-1617 0.56 0.83 67 0.8312 1.3e+32 9.39 -1.19 P7R42830BP ERC030 G015.05-00.70 1FGL J1818.7-1557c 2FGL J1819.3-1523 G015.4+00.1 G015.1-01.6 (multiple radio pulsars could be timed with one pointing in search mode) J1840-1419 0.27 0.54 20 6.5976 8.7e+29 0.84 -4.12 P7R42907P 1FGL J1842.0-1409 (SIX second period??) J1841-1404 0.41 0.54 20 1.3346 1.1e+31 6.45 -4.23 P7R42907P 1FGL J1842.0-1409 J2301+5852 0.03 0.05 79 6.9791 5.5e+31 3.3 -1.0 P7R43557 J2301+5852 G109.1-01.0 (these slowpokes keep popping up... discovery?) MSPs only PSRJ angsep ellps ts P0 EDOT DIST Gb NickName ID_Name J1125-6014 0.05 0.06 39 0.0026 8.7e+33 1.49 0.89 P7R41640G J1125-6014 J1400-1438 0.05 0.12 99 0.0031 0.0e+00 0.48 45.0 P7R42068 2FGL J1400.7-1438 J1543-5149 0.18 0.18 37 0.0021 7.3e+34 2.42 2.48 P7R42323G J1628-3205 0.03 0.09 115 0.0032 1.8e+34 1.25 11.51 P7R42458 J1628-32 1FGL J1627.8-3204 2FGL J1628.3-3206