+-----------------------+------------------------------+-----------------------+-----------+---------------+------------+------------+--------------------+-------------------+-------------------+----------------+------------------------+------------+---------------+-----------+---------------+--------------------------------+------------+---------+------------+--------------+-------------------------+-------------------------+-----------+ | Name | Period | dP/dt | B | dE/dt | Age | References | NH | Gamma | kT | kT2 | Flux [1] | References | Distance | Reference | Luminosity | Proposed Associations [2] | References | Opt/IR? | Bands? [3] | Activity [4] | Right Ascension | Declination | Reference | | | (s) | (10^-11 s/s) | (10^14 G) | (10^33 erg/s) | (kyr) | | (10^22 cm^-2) | | (keV) | (keV) | (10^-12 erg/s/cm^2) | | (kpc) | | (10^33 erg/s) | | | | | | (J2000) | (J2000) | | +-----------------------+------------------------------+-----------------------+-----------+---------------+------------+------------+--------------------+-------------------+-------------------+----------------+------------------------+------------+---------------+-----------+---------------+--------------------------------+------------+---------+------------+--------------+-------------------------+-------------------------+-----------+ | CXOU J010043.1-721134 | 8.020392 0.000009 | 1.88 0.08 | 3.93 | 1.44 | 6.76 | 1 | 0.063 0.020 0.016 | | 0.30 0.02 0.02 | 0.68 0.09 0.07 | 0.14 | 26 | 62.4 1.6 1.6 | 45 | 65 | SMC | 64 | maybe | X | | 01 00 43.14 0.13 | -72 11 33.8 0.6 | 64 | | 4U 0142+61 | 8.68869249 0.00000005 | 0.2022 0.0004 | 1.34 | 0.122 | 68.1 | 2 | 1.00 0.01 0.01 | 3.88 0.01 0.01 | 0.410 0.004 0.002 | | 67.9 | 27 | 3.6 0.4 0.4 | 46 | 110 | | | yes | HXOI | BG | 01 46 22.407 0.028 | +61 45 03.19 0.20 | 82 | | SGR 0418+5729 | 9.07838822 0.00000005 | 0.0004 0.0001 | 0.0610 | 0.000211 | 36000 | 3 | 0.115 0.006 0.006 | | 0.32 0.05 0.05 | | 0.0020 0.0014 0.0010 | 3 | ~ 2 | 47 | 0.00096 | | | no | X | BT | 04 18 33.867 0.043 | +57 32 22.91 0.35 | 47 | | SGR 0501+4516 | 5.7620695 0.0000001 | 0.594 0.002 | 1.87 | 1.23 | 15.4 | 4 | 0.88 0.01 0.01 | 3.84 0.06 0.06 | 0.50 0.02 0.02 | | 1.7 | 4 | ~ 2 | 48 | 0.81 | SNR HB 9? | 65 | yes | HXO | B | 05 01 06.76 0.01 | +45 16 33.92 0.11 | 83 | | SGR 0526-66 | 8.0544 0.0002 | 3.8 0.1 | 5.60 | 2.87 | 3.36 | 5 | 0.604 0.058 0.059 | 2.50 0.11 0.12 | 0.44 0.02 0.02 | | 0.55 | 28 | 53.6 1.2 1.2 | 49 | 190 | LMC, SNR N49?, SL 463 | 66, 67 | no | X | BF | 05 26 00.89 0.10 | -66 04 36.3 0.6 | 84 | | 1E 1048.1-5937 | 6.457875 0.000003 | 2.25 | 3.86 | 3.30 | 4.54 | 6 | 0.97 0.01 0.01 | 3.14 0.11 0.11 | 0.56 0.01 0.01 | | 5.1 0.1 0.1 | 29 | 9.0 1.7 1.7 | 46 | 49 | GSH 288.3-0.5-28? | 68 | yes | HXO | BG | 10 50 07.14 0.08 | -59 53 21.4 0.6 | 85 | | 1E 1547.0-5408 | 2.0721255 0.0000001 | 4.77 | 3.18 | 211 | 0.689 | 7 | 3.2 0.2 0.2 | 4.0 0.2 0.2 | 0.43 0.03 0.03 | | 0.54 | 30 | 4.5 0.5 0.5 | 50 | 1.3 | SNR G327.24-0.13 | 69 | maybe | HXR | BT | 15 50 54.12386 0.00064 | -54 18 24.1141 0.0020 | 86 | | PSR J1622-4950 | 4.3261 0.0001 | 1.7 0.1 | 2.74 | 8.29 | 4.03 | 8 | 5.4 1.6 1.4 | | 0.5 0.1 0.1 | | 0.045 0.063 0.028 | 31 | ~ 9 | 8 | 0.44 | SNR G333.9+0.0 | 31 | no | XR | | 16 22 44.89 0.08 | -49 50 52.7 0.8 | 31 | | SGR 1627-41 | 2.594578 0.000006 | 1.9 0.4 | 2.25 | 42.9 | 2.16 | 9, 10 | 10 2 2 | 2.9 0.8 0.8 | | | 0.25 0.17 0.10 | 32, 33 | 11.0 0.3 0.3 | 51 | 3.6 | CTB 33, MC -71, SNR G337.0-0.1 | 51, 70 | no | X | BT | 16 35 51.844 0.020 | -47 35 23.31 0.20 | 87 | | CXOU J164710.2-455216 | 10.610644 0.000017 | < 0.04 | < 0.659 | < 0.0132 | > 420 | 11 | 2.39 0.05 0.05 | 3.86 0.22 0.22 | 0.59 0.06 0.06 | | 0.25 0.04 0.04 | 11 | 3.9 0.7 0.7 | 52 | 0.45 | Westerlund 1 | 71 | no | X | BT | 16 47 10.20 0.03 | -45 52 16.90 0.30 | 71 | | 1RXS J170849.0-400910 | 11.00502461 0.00000017 | 1.9455 0.0013 | 4.68 | 0.576 | 8.96 | 2 | 1.36 0.04 0.04 | 2.792 0.008 0.012 | 0.456 0.007 0.004 | | 24.3 | 34 | 3.8 0.5 0.5 | 46 | 42 | | | maybe | HX | G | 17 08 46.87 0.06 | -40 08 52.44 0.70 | 88 | | CXOU J171405.7-381031 | 3.825352 0.000004 | 6.40 0.05 | 5.01 | 45.1 | 0.947 | 12 | 3.95 0.15 0.14 | 3.45 0.09 0.08 | | | 2.68 0.09 0.09 | 12 | ~13.2 | 53 | 56 | SNR CTB 37B | 72 | no | X | | 17 14 05.74 0.05 | -38 10 30.9 0.6 | 89 | | SGR J1745-2900 | 3.76363824 0.00000013 | 1.385 0.015 | 2.31 | 10.3 | 4.31 | 13 | | | | | < 0.013 | 35 | 8.3 0.3 0.3 | 54 | < 0.11 | Galactic Center | 35 | no | HXR | BT | 17 45 40.164 0.002 | -29 00 29.818 0.090 | 90 | | SGR 1806-20 | 7.54773 0.00002 | 49.5 | 19.6 | 45.5 | 0.242 | 14 | 6.9 0.4 0.4 | 1.6 0.1 0.1 | 0.55 0.07 0.07 | | 18 1 1 | 36 | 8.7 1.8 1.5 | 55 | 160 | W31, Star cluster, MC 13A | 73-75 | yes | HXO | BF | 18 08 39.337 0.004 | -20 24 39.85 0.06 | 91 | | XTE J1810-197 | 5.5403537 0.0000002 | 0.777 0.003 | 2.10 | 1.80 | 11.3 | 15 | 0.63 0.05 0.05 | | 0.18 0.02 0.02 | | 0.029 | 37 | 3.5 0.5 0.4 | 56 | 0.043 | | | yes | XOR | BT | 18 09 51.08696 0.00028 | -19 43 51.9315 0.0040 | 92 | | Swift J1818.0-1607 | 1.363490 0.000003 | 9 1 | 3.54 | 1400 | 0.240 | 16, 17 | | | | | | | ~ 4.8 | 16 | | | | no | GR | B | 18 18 03.7 11.2 | -16 07 31.8 162.0 | 93 | | Swift J1822.3-1606 | 8.43772106 0.00000006 | 0.0021 0.0002 | 0.136 | 0.00140 | 6260 | 18 | 0.453 0.008 0.008 | | 0.12 0.02 0.02 | | < 0.0013 | 38 | 1.6 0.3 0.3 | 38 | < 0.00040 | M17 | 38 | no | X | BT | 18 22 18.00 0.12 | -16 04 26.8 1.8 | 94 | | SGR 1833-0832 | 7.5654084 0.0000004 | 0.35 0.03 | 1.65 | 0.319 | 34.2 | 19 | | | | | < 0.2 | 19 | | | | | | no | X | B | 18 33 44.37 0.03 | -08 31 07.5 0.4 | 95 | | Swift J1834.9-0846 | 2.4823018 0.0000001 | 0.796 0.012 | 1.42 | 20.5 | 4.94 | 20 | | | | | < 0.004 | 39 | 4.2 0.3 0.3 | 57 | < 0.0084 | SNR W41 | 20 | no | X | BT | 18 34 52.118 0.040 | -08 45 56.02 0.60 | 20 | | 1E 1841-045 | 11.788978 0.000001 | 4.092 0.015 | 7.03 | 0.986 | 4.57 | 2 | 2.2 0.1 0.1 | 1.9 0.2 0.2 | 0.45 0.03 0.03 | | 21.3 | 40 | 8.5 1.3 1.0 | 58 | 180 | SNR Kes 73 | 76 | maybe | HX | BG | 18 41 19.343 0.020 | -04 56 11.16 0.30 | 87 | | 3XMM J185246.6+003317 | 11.55871346 0.00000006 | < 0.014 | < 0.407 | < 0.00358 | > 1310 | 21 | | | | | < 0.001 | 21 | ~ 7.1 | 59 | < 0.0060 | | | no | X | T | 18 52 46.67 0.02 | +00 33 17.8 0.3 | 59 | | SGR 1900+14 | 5.19987 0.00007 | 9.2 0.4 | 7.00 | 25.8 | 0.896 | 22 | 2.12 0.08 0.08 | 1.9 0.1 0.1 | 0.47 0.02 0.02 | | 4.8 0.2 0.2 | 22 | 12.5 1.7 1.7 | 60 | 90 | Star cluster | 77 | maybe | HX | BF | 19 07 14.33 0.01 | +09 19 20.1 0.2 | 96 | | SGR 1935+2154 | 3.2450650 0.0000001 | 1.43 0.01 | 2.18 | 16.5 | 3.60 | 23 | 1.6 0.2 0.2 | 1.8 0.5 0.5 | 0.47 0.02 0.02 | | | 23 | | | | SNR G57.2+0.8 | 78 | no | HXR | B | 19 34 55.5978 0.0503 | +21 53 47.7864 0.7000 | 23 | | 1E 2259+586 | 6.9790427250 0.0000000015 | 0.0483695 0.0000063 | 0.588 | 0.0562 | 229 | 2 | 1.012 0.007 0.007 | 3.75 0.04 0.04 | 0.37 0.01 0.01 | | 14.1 0.3 0.3 | 41 | 3.2 0.2 0.2 | 61 | 17 | SNR CTB 109 | 79 | yes | HXOI | BGA | 23 01 08.295 0.077 | +58 52 44.45 0.60 | 97 | | | | | | | | | | | | | | | | | | | | | | | | | | | SGR 0755-2933 # | | | | | | | | | | | | | | | | | | no | X | BT | 07 55 42.48 0.15 | -29 33 49.2 2.0 | 98 | | SGR 1801-23 # | | | | | | | | | | | | | | | | | | no | | B | 18 00 59 | -22 56 48 | 99 | | SGR 1808-20 # | | | | | | | | | | | | | | | | | | no | | B | 18 08 11.2 29.5 | -20 38 49 414 | 100 | | AX J1818.8-1559 # | | | | | | | 3.6 0.5 0.5 | 1.17 0.17 0.17 | | | 1.68 0.16 0.15 | 42 | | | | | | no | X | B | 18 18 51.38 0.04 | -15 59 22.62 0.60 | 42 | | AX J1845.0-0258 # | 6.97127 0.00028 | | | | | 24 | 7.8 2.3 1.8 | 1.0 0.5 0.3 | | | 0.33 0.07 0.08 | 43 | ~ 8.5 | 24 | 2.9 | SNR G29.6+0.1 | 80 | no | X | T | 18 44 54.68 0.04 | -02 56 53.1 0.6 | 43 | | SGR 2013+34 # | | | | | | | | | | | | | ~ 8.8 | 62 | | W58 | 62 | no | | B | 20 13 56.9 7.3 | +34 19 48 90 | 62 | | | | | | | | | | | | | | | | | | | | | | | | | | | PSR J1846-0258 ## | 0.32657128834 0.00000000004 | 0.7107450 0.0000002 | 0.488 | 8060 | 0.728 | 25 | 4.0 0.1 0.1 | 1.1 0.1 0.1 | | | 4.3 0.7 0.7 | 25, 44 | 6.0 1.5 0.9 | 63 | 19 | SNR Kes 75 | 81 | no | HX | BG | 18 46 24.94 0.01 | -02 58 30.1 0.2 | 101 | +-----------------------+------------------------------+-----------------------+-----------+---------------+------------+------------+--------------------+-------------------+-------------------+----------------+------------------------+------------+---------------+-----------+---------------+--------------------------------+------------+---------+------------+--------------+-------------------------+-------------------------+-----------+ Notes: # This candidate is unconfirmed. ## This source is often classified as a young, rotation-powered pulsar, but it was seen to undergo a magnetar-like outburst in 2006 (see Gavriil et al. 2008, Science, 319, 1802). [1] Flux is given for the 2-10 keV range. If only the absorbed flux was given in the literature, or if it was not given in the 2-10keV band, we used WebPIMMS to estimate the 2-10keV unabsorbed flux. [2] Associations followed by a question mark have been disputed. [3] Only wavebands in which persistent emission has been confirmed are included. H = soft gamma rays/hard X-rays (>10 keV) X = X-rays (1-10 keV) O = optical/near-infrared I = mid to far infrared R = radio [4] B = bursts F = giant flare G = glitch A = anti-glitch T = transient magnetar References: 1 McGarry et al. 2005, ApJL, 627, L137 2 Dib & Kaspi 2014, ApJ, 784, 37 3 Rea et al. 2013, ApJ, 770, 65 4 Camero et al. 2014, MNRAS, 438, 3291 5 Tiengo et al. 2009, MNRAS, 399, L74 6 Dib et al. 2009, ApJ, 702, 614 7 Dib et al. 2012, ApJ, 748, 3 8 Levin et al. 2010, ApJL, 721, L33 9 Esposito et al. 2009, ApJL, 690, L105 10 Esposito et al. 2009, MNRAS, 399, L44 11 An et al. 2013, ApJ, 763, 82 12 Sato et al. 2010, PASJ, 62, L33 13 Kaspi et al. 2014, ApJ, 786, 84 14 Woods et al. 2007, ApJ, 654, 470 15 Camilo et al. 2007, ApJ, 663, 497 16 Karuppusamy et al. 2020, ATel, 13553, 1 17 Esposito et al. 2020, ApJL, 896, L30 18 Scholz et al. 2014, ApJ, 786, 62 19 Esposito et al. 2011, MNRAS, 416, 205 20 Kargaltsev et al. 2012, ApJ, 748, 26 21 Rea et al. 2014, ApJL, 781, L17 22 Mereghetti et al. 2006, ApJ, 653, 1423 23 Israel et al. 2016, MNRAS, 457, 3448 24 Torii et al. 1998, ApJ, 503, 843 25 Livingstone et al. 2011, ApJ, 730, 66 26 Tiengo et al. 2008, ApJL, 680, L133 27 Rea et al. 2007, MNRAS, 381, 293 28 Park et al. 2012, ApJ, 748, 117 29 Tam et al. 2008, ApJ, 677, 503 30 Bernardini et al. 2011, A&A, 529, 19 31 Anderson et al. 2012, ApJ, 751, 53 32 Esposito et al. 2008, MNRAS, 390, L34 33 An et al. 2012, ApJ, 757, 68 34 Rea et al. 2007, Ap&SS, 308, 505 35 Mori et al. 2013, ApJL, 770, L23 36 Esposito et al. 2007, A&A, 476, 321 37 Gotthelf et al. 2004, ApJ, 605, 368 38 Scholz et al. 2012, ApJ, 761, 66 39 Younes et al. 2012, ApJ, 757, 39 40 Kumar & Safi-Harb 2010, ApJL, 725, L191 41 Zhu et al. 2008, ApJ, 686, 520 42 Mereghetti et al. 2012, A&A, 546, 30 43 Tam et al. 2006, ApJ, 652, 548 44 Ng et al. 2008, ApJ, 686, 508 45 Haschke et al. 2012, AJ, 144, 107 46 Durant & van Kerkwijk 2006, ApJ, 650, 1070 47 van der Horst et al. 2010, ApJL, 711, L1 48 Lin et al. 2011, ApJ, 739, 87 49 Haschke et al. 2012, AJ, 144, 106 50 Tiengo et al. 2010, ApJ, 710, 227 51 Corbel et al. 1999, ApJL, 526, L29 52 Kothes & Dougherty 2007, A&A, 468, 993 53 Tian & Leahy 2012, MNRAS, 421, 2593 54 Bower et al. 2014, ApJL, 780, L2 55 Bibby et al. 2008, MNRAS, 386, L23 56 Minter et al. 2008, ApJ, 676, 1189 57 Leahy & Tian 2008, AJ, 135, 167 58 Tian & Leahy 2008, ApJ, 677, 292 59 Zhou et al. 2014, ApJL, 781, L16 60 Davies et al. 2009, ApJ, 707, 844 61 Kothes & Foster 2012, ApJL, 746, L4 62 Sakamoto et al. 2011, AdSpR, 47, 1346 63 Leahy & Tian 2008, A&A, 480, L25 64 Lamb et al. 2002, ApJL, 574, L29 65 Gaensler & Chatterjee 2008, GCN, 8149, 1 66 Cline et al. 1982, ApJL, 255, L45 67 Klose et al. 2004, ApJL, 609, L13 68 Gaensler et al. 2005, ApJL, 620, L95 69 Gelfand & Gaensler 2007, ApJ, 667, 1111 70 Woods et al. 1999, ApJL, 519, L139 71 Muno et al. 2006, ApJL, 636, L41 72 Halpern & Gotthelf 2010, ApJ, 710, 941 73 Corbel et al. 1997, ApJ, 478, 624 74 Fuchs et al. 1999, A&A, 350, 891 75 Corbel & Eikenberry 2004, A&A, 419, 191 76 Vasisht & Gotthelf 1997, ApJL, 486, L129 77 Vrba et al. 2000, ApJL, 533, L17 78 Gaensler 2014, GCN, 16533, 1 79 Fahlman & Gregory 1981, Nature, 293, 202 80 Gaensler et al. 1999, ApJL, 526, L37 81 Gotthelf et al. 2000, ApJL, 542, L37 82 Hulleman et al. 2004, A&A, 416, 1037 83 Gogus et al. 2010, ApJ, 722, 899 84 Kulkarni et al. 2003, ApJ, 585, 948 85 Wang & Chakrabarty 2002, ApJL, 579, L33 86 Deller et al. 2012, ApJL, 748, L1 87 Wachter et al. 2004, ApJ, 615, 887 88 Israel et al. 2003, ApJL, 589, L93 89 Halpern & Gotthelf 2010, ApJ, 725, 1384 90 Shannon & Johnston 2013, MNRAS, 435, L29 91 Israel et al. 2005, A&A, 438, L1 92 Helfand et al. 2007, ApJ, 662, 1198 93 Stamatikos et al. 2020, GCN, 27384, 1 94 Pagani et al. 2011, ATel, 3493, 1 95 Gogus et al. 2010, ApJ, 718, 331 96 Frail et al. 1999, Nature, 398, 127 97 Hulleman et al. 2001, ApJL, 563, L49 98 Barthelmy et al. 2016, ATel, 8831, 1 99 Cline et al. 2000, ApJ, 531, 407 100 Lamb et al. 2003, GCN, 2351, 1 101 Helfand et al. 2003, ApJ, 582, 783