+-----------------------+--------------------------------+-------------------+------------+---------------+------------------+-----------+----------------------+----------------+ | Name | Proposed Associations [1] | SNR Age | References | Distance | Measured To | Reference | Gal. Height [2] | Luminosity [3] | | | | (kyr) | | (kpc) | | | (pc) | (10^33 erg/s) | +-----------------------+--------------------------------+-------------------+------------+---------------+------------------+-----------+----------------------+----------------+ | CXOU J010043.1-721134 | SMC | | 1 | 62.4 1.6 1.6 | SMC | 31 | | 65 | | 4U 0142+61 | | | | 3.6 0.4 0.4 | 0142+61 | 32 | -27.1 3.0 3.0 | 110 | | SGR 0418+5729 | | | | ~ 2 | Perseus Arm | 33 | ~ 180 | 0.00096 | | SGR 0501+4516 | SNR HB 9? | 6.6 0.4 2.6 | 2, 3 | ~ 2 | Perseus Arm | 34 | ~ 68 | 0.81 | | SGR 0526-66 | LMC, SNR N49?, SL 463 | ~ 4.8 | 4-6 | 53.6 1.2 1.2 | LMC | 35 | | 190 | | 1E 1048.1-5937 | GSH 288.3-0.5-28? | | 7 | 9.0 1.7 1.7 | 1048.1-5937 | 32 | -82 15 15 | 49 | | 1E 1547.0-5408 | SNR G327.24-0.13 | | 8 | 4.5 0.5 0.5 | 1547.0-5408 | 36 | -10.3 1.1 1.1 | 1.3 | | PSR J1622-4950 | SNR G333.9+0.0 | < 6 | 9 | ~ 9 | J1622-4950 | 37 | ~ -16 | 0.44 | | SGR 1627-41 | CTB 33, MC -71, SNR G337.0-0.1 | | 10, 11 | 11.0 0.3 0.3 | G337.0-0.1 | 10 | -21.41 0.58 0.58 | 3.6 | | CXOU J164710.2-455216 | Westerlund 1 | | 12 | 3.9 0.7 0.7 | Westerlund 1 | 38 | -29.3 5.3 5.3 | 0.45 | | 1RXS J170849.0-400910 | | | | 3.8 0.5 0.5 | J170849.0-400910 | 32 | 2.39 0.31 0.31 | 42 | | CXOU J171405.7-381031 | SNR CTB 37B | 0.65 2.50 0.30 | 13, 14 | ~13.2 | CTB 37B | 39 | ~ 86 | 56 | | SGR J1745-2900 | Galactic Center | | 15 | 8.3 0.3 0.3 | Galactic Center | 40 | -6.78 0.25 0.25 | < 0.11 | | SGR 1806-20 | W31, Star cluster, MC 13A | | 16-18 | 8.7 1.8 1.5 | Star cluster | 41 | -36.7 6.3 7.6 | 160 | | XTE J1810-197 | | | | 3.5 0.5 0.4 | J1810-197 | 42 | -9.7 1.1 1.4 | 0.043 | | Swift J1818.0-1607 | | | | ~ 4.8 | J1818.0-1607 | 43 | ~ -12 | | | Swift J1822.3-1606 | M17 | | 19 | 1.6 0.3 0.3 | M17 | 19 | -28.5 5.3 5.3 | < 0.00040 | | SGR 1833-0832 | | | | | | | ~ 3.6 | < 2.4 | | Swift J1834.9-0846 | SNR W41 | ~100 | 20, 21 | 4.2 0.3 0.3 | W41 | 44 | -25.0 1.8 1.8 | < 0.0084 | | 1E 1841-045 | SNR Kes 73 | 0.75 0.25 0.25 | 22, 23 | 8.5 1.3 1.0 | Kes 73 | 23 | -0.97 0.11 0.15 | 180 | | 3XMM J185246.6+003317 | | | | ~ 7.1 | Kes 79 | 45 | ~ -5.6 | < 0.0060 | | SGR 1900+14 | Star cluster | | 24 | 12.5 1.7 1.7 | Star cluster | 46 | 167 23 23 | 90 | | SGR 1935+2154 | SNR G57.2+0.8 | | 25 | | | | ~ 140 | | | 1E 2259+586 | SNR CTB 109 | 14 2 2 | 26, 27 | 3.2 0.2 0.2 | CTB 109 | 47 | -55.6 3.5 3.5 | 17 | | | | | | | | | | | | SGR 0755-2933 # | | | | | | | ~-110 | | | SGR 1801-23 # | | | | | | | ~ 12 | | | SGR 1808-20 # | | | | | | | ~ -45 | | | AX J1818.8-1559 # | | | | | | | ~ -44 | 20 | | AX J1845.0-0258 # | SNR G29.6+0.1 | < 8 | 28 | ~ 8.5 | Scutum Arm | 48 | ~ 16 | 2.9 | | SGR 2013+34 # | W58 | | 29 | ~ 8.8 | W58 | 29 | ~ -16 | | | | | | | | | | | | | PSR J1846-0258 ## | SNR Kes 75 | | 30 | 6.0 1.5 0.9 | Kes 75 | 49 | -25.1 3.8 6.3 | 19 | +-----------------------+--------------------------------+-------------------+------------+---------------+------------------+-----------+----------------------+----------------+ 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] Associations followed by a question mark have been disputed. [2] The height above the Galactic plane is calculated from the Galactic latitudes given in Table 1, assuming a distance of 10 kpc if none is known. [3] Luminosity is in the 2-10 keV range and is calculated using the fluxes given in Table 3, assuming a distance of 10 kpc if none is known. References: 1 Lamb et al. 2002, ApJL, 574, L29 2 Gaensler & Chatterjee 2008, GCN, 8149, 1 3 Leahy & Tian 2007, A&A, 461, 1013 4 Cline et al. 1982, ApJL, 255, L45 5 Klose et al. 2004, ApJL, 609, L13 6 Park et al. 2012, ApJ, 748, 117 7 Gaensler et al. 2005, ApJL, 620, L95 8 Gelfand & Gaensler 2007, ApJ, 667, 1111 9 Anderson et al. 2012, ApJ, 751, 53 10 Corbel et al. 1999, ApJL, 526, L29 11 Woods et al. 1999, ApJL, 519, L139 12 Muno et al. 2006, ApJL, 636, L41 13 Halpern & Gotthelf 2010, ApJ, 710, 941 14 Nakamura et al. 2009, PASJ, 61, 197 15 Mori et al. 2013, ApJL, 770, L23 16 Corbel et al. 1997, ApJ, 478, 624 17 Fuchs et al. 1999, A&A, 350, 891 18 Corbel & Eikenberry 2004, A&A, 419, 191 19 Scholz et al. 2012, ApJ, 761, 66 20 Kargaltsev et al. 2012, ApJ, 748, 26 21 Tian et al. 2007, ApJL, 657, L25 22 Vasisht & Gotthelf 1997, ApJL, 486, L129 23 Tian & Leahy 2008, ApJ, 677, 292 24 Vrba et al. 2000, ApJL, 533, L17 25 Gaensler 2014, GCN, 16533, 1 26 Fahlman & Gregory 1981, Nature, 293, 202 27 Sasaki et al. 2013, A&A, 552, 45 28 Gaensler et al. 1999, ApJL, 526, L37 29 Sakamoto et al. 2011, AdSpR, 47, 1346 30 Gotthelf et al. 2000, ApJL, 542, L37 31 Haschke et al. 2012, AJ, 144, 107 32 Durant & van Kerkwijk 2006, ApJ, 650, 1070 33 van der Horst et al. 2010, ApJL, 711, L1 34 Lin et al. 2011, ApJ, 739, 87 35 Haschke et al. 2012, AJ, 144, 106 36 Tiengo et al. 2010, ApJ, 710, 227 37 Levin et al. 2010, ApJL, 721, L33 38 Kothes & Dougherty 2007, A&A, 468, 993 39 Tian & Leahy 2012, MNRAS, 421, 2593 40 Bower et al. 2014, ApJL, 780, L2 41 Bibby et al. 2008, MNRAS, 386, L23 42 Minter et al. 2008, ApJ, 676, 1189 43 Karuppusamy et al. 2020, ATel, 13553, 1 44 Leahy & Tian 2008, AJ, 135, 167 45 Zhou et al. 2014, ApJL, 781, L16 46 Davies et al. 2009, ApJ, 707, 844 47 Kothes & Foster 2012, ApJL, 746, L4 48 Torii et al. 1998, ApJ, 503, 843 49 Leahy & Tian 2008, A&A, 480, L25