+-----------------------+--------------------+-------------------+-------------------+----------------+---------------------+---------------------+-------------+------------+------------------------+ | Name | NH | Gamma | kT | kT2 | Abs. Flux | Unabs. Flux | Energy Band | References | 2-10 keV Flux [1] | | | (10^22 cm^-2) | | (keV) | (keV) | (10^-12 erg/s/cm^2) | (10^-12 erg/s/cm^2) | (keV) | | (10^-12 erg/s/cm^2) | +-----------------------+--------------------+-------------------+-------------------+----------------+---------------------+---------------------+-------------+------------+------------------------+ | CXOU J010043.1-721134 | 0.063 0.020 0.016 | | 0.30 0.02 0.02 | 0.68 0.09 0.07 | 0.14 | 0.14 | 2--10 | 1 | 0.14 | | 4U 0142+61 | 1.00 0.01 0.01 | 3.88 0.01 0.01 | 0.410 0.004 0.002 | | 58 1 1 | | 2--10 | 2 | 67.9 | | SGR 0418+5729 | 0.115 0.006 0.006 | | 0.32 0.05 0.05 | | 0.012 0.001 0.001 | | 0.5--10 | 3 | 0.0020 0.0014 0.0010 | | SGR 0501+4516 | 0.88 0.01 0.01 | 3.84 0.06 0.06 | 0.50 0.02 0.02 | | 3.0 0.2 0.2 | 19 1 1 | 0.5--10 | 4 | 1.7 | | SGR 0526-66 | 0.604 0.058 0.059 | 2.50 0.11 0.12 | 0.44 0.02 0.02 | | 1.01 0.08 0.13 | 1.58 0.13 0.20 | 0.5--10 | 5 | 0.55 | | 1E 1048.1-5937 | 0.97 0.01 0.01 | 3.14 0.11 0.11 | 0.56 0.01 0.01 | | | 5.1 0.1 0.1 | 2--10 | 6 | 5.1 0.1 0.1 | | 1E 1547.0-5408 | 3.2 0.2 0.2 | 4.0 0.2 0.2 | 0.43 0.03 0.03 | | 0.37 0.01 0.03 | | 0.5--10 | 7 | 0.54 | | PSR J1622-4950 | 5.4 1.6 1.4 | | 0.5 0.1 0.1 | | 0.030 0.008 0.006 | 0.11 0.09 0.04 | 0.3--10 | 8 | 0.045 0.063 0.028 | | SGR 1627-41 | 10 2 2 | 2.9 0.8 0.8 | | | 0.10 0.03 0.02 | 0.25 0.17 0.10 | 2--10 | 9, 10 | 0.25 0.17 0.10 | | CXOU J164710.2-455216 | 2.39 0.05 0.05 | 3.86 0.22 0.22 | 0.59 0.06 0.06 | | | 0.25 0.04 0.04 | 2--10 | 11 | 0.25 0.04 0.04 | | 1RXS J170849.0-400910 | 1.36 0.04 0.04 | 2.792 0.008 0.012 | 0.456 0.007 0.004 | | | 87.0 0.4 0.2 | 0.5--10 | 12 | 24.3 | | CXOU J171405.7-381031 | 3.95 0.15 0.14 | 3.45 0.09 0.08 | | | 1.51 0.03 0.03 | 2.68 0.09 0.09 | 2--10 | 13 | 2.68 0.09 0.09 | | SGR J1745-2900 | | | | | | < 0.013 | 2--10 | 14 | < 0.013 | | SGR 1806-20 | 6.9 0.4 0.4 | 1.6 0.1 0.1 | 0.55 0.07 0.07 | | | 18 1 1 | 2--10 | 15 | 18 1 1 | | XTE J1810-197 | 0.63 0.05 0.05 | | 0.18 0.02 0.02 | | 0.75 | 4.6 | 0.5--10 | 16 | 0.029 | | Swift J1818.0-1607 | | | | | | | | | | | Swift J1822.3-1606 | 0.453 0.008 0.008 | | 0.12 0.02 0.02 | | 0.09 0.20 0.09 | | 0.1--2.4 | 17 | < 0.0013 | | SGR 1833-0832 | | | | | < 0.02 | < 0.2 | 2--10 | 18 | < 0.2 | | Swift J1834.9-0846 | | | | | | < 0.004 | 2--10 | 19 | < 0.004 | | 1E 1841-045 | 2.2 0.1 0.1 | 1.9 0.2 0.2 | 0.45 0.03 0.03 | | | 43 9 12 | 0.5--10 | 20 | 21.3 | | 3XMM J185246.6+003317 | | | | | | < 0.4 | bolometric | 21 | < 0.001 | | SGR 1900+14 | 2.12 0.08 0.08 | 1.9 0.1 0.1 | 0.47 0.02 0.02 | | | 4.8 0.2 0.2 | 2--10 | 22 | 4.8 0.2 0.2 | | SGR 1935+2154 | 1.6 0.2 0.2 | 1.8 0.5 0.5 | 0.47 0.02 0.02 | | | | 1--10 | 23 | | | 1E 2259+586 | 1.012 0.007 0.007 | 3.75 0.04 0.04 | 0.37 0.01 0.01 | | 11.5 0.2 0.2 | 14.1 0.3 0.3 | 2--10 | 24 | 14.1 0.3 0.3 | | | | | | | | | | | | | SGR 0755-2933 # | | | | | | | | | | | SGR 1801-23 # | | | | | | | | | | | SGR 1808-20 # | | | | | | | | | | | AX J1818.8-1559 # | 3.6 0.5 0.5 | 1.17 0.17 0.17 | | | 1.37 0.07 0.07 | | 2--10 | 25 | 1.68 0.16 0.15 | | AX J1845.0-0258 # | 7.8 2.3 1.8 | 1.0 0.5 0.3 | | | 0.28 0.02 0.02 | 0.33 0.07 0.08 | 2--10 | 26 | 0.33 0.07 0.08 | | SGR 2013+34 # | | | | | | | | | | | | | | | | | | | | | | PSR J1846-0258 ## | 4.0 0.1 0.1 | 1.1 0.1 0.1 | | | 3.6 0.5 0.5 | 5.2 0.7 0.7 | 0.5--10 | 27, 28 | 4.3 0.7 0.7 | +-----------------------+--------------------+-------------------+-------------------+----------------+---------------------+---------------------+-------------+------------+------------------------+ 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] We used WebPIMMS to convert the flux found in the literature to the 2-10 keV range if necessary. Likewise, if only the absorbed flux was given, WebPIMMS was used to estimate the unabsorbed flux. 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