+-----------------------+---------------+---------------------+---------------------+------------------------------+----------------------------------+---------------+------------+---------------------+-----------+ | Name | Telescope [1] | Gamma (Pulsed) | Pulsed Flux [2] | Gamma (Total) | Total Flux [2] | Cutoff Energy | References | Gamma-ray Flux [3] | Reference | | | | | (10^-11 erg/s/cm^2) | | (10^-11 erg/s/cm^2) | (keV) | | (10^-11 erg/s/cm^2) | | +-----------------------+---------------+---------------------+---------------------+------------------------------+----------------------------------+---------------+------------+---------------------+-----------+ | CXOU J010043.1-721134 | | | | | | | | | | | 4U 0142+61 | I, R | 0.40 | 2.68 | 0.93 | 9.09 | 279 65 41 | 1 | < 0.9 | 18 | | 4U 0142+61 | S | | | 0.89 | 10.3 | | 2 | | | | SGR 0418+5729 | | | | | | | | < 0.4 | 18 | | SGR 0501+4516 | I | | | 0.8 | <3.5 | >100 | 3 | < 1.9 | 18 | | SGR 0501+4516 | S | | | 0.79 | 8.4 | | 4 | | | | SGR 0526-66 | | | | | | | | | | | 1E 1048.1-5937 | | | | | | | | < 5.3 | 18 | | 1E 1547.0-5408 | I, R | -0.37, -0.59, -1.55 | 6.9, 7.5, 4.1 | 1.41, 1.45, 1.27, 1.22, 0.87 | <1.5, 25.2, 18.5, 21.5, 8.4, 8.0 | >200 | 5 | <10.0 | 18 | | 1E 1547.0-5408 | S | | | 1.54 | 17.4 | | 6 | | | | PSR J1622-4950 | | | | | | | | | | | SGR 1627-41 | | | | | | | | <20.0 | 18 | | CXOU J164710.2-455216 | | | | | | | | <10.0 | 18 | | 1RXS J170849.0-400910 | I, R | 0.86 | 2.60 | 1.46, 1.13 | 5.2, 6.61 | >300 | 7, 8 | <10.0 | 18 | | CXOU J171405.7-381031 | | | | | | | | | | | SGR J1745-2900 | N | | | 1.47 | 0.67 | > 50 | 9 | | | | SGR 1806-20 | I | | | 1.9, 1.5 | 6.0, 11 | >160 | 10 | < 0.6 | 18 | | SGR 1806-20 | S | | | 1.7, 1.2, 1.6 | 4.70, 9.89, 3.83 | | 11 | | | | XTE J1810-197 | | | | | | | | < 5.0 | 18 | | Swift J1822.3-1606 | | | | | | | | | | | SGR 1833-0832 | | | | | | | | | | | Swift J1834.9-0846 | | | | | | | | | | | 1E 1841-045 | | | | | | | | | | | 1E 1841-045 | I, R | 0.72 | 4.00 | 1.32 | 6.88 | | 12 | | | | 1E 1841-045 | S | 1.35 | 2.67 | 1.62 | 4.59 | | 13 | | | | 3XMM J185246.6+003317 | N | 0.99 | 3.03 | 1.33 | 7.99 | >140 | 14 | < 3.0 | 18 | | SGR 1900+14 | | | | | | | | | | | SGR 1900+14 | I | | | 3.1 | 1.6 | | 15 | | | | SGR 1935+2154 | S | | | 1.2, 1.4 | 3.24, 1.42 | >100 | 11 | < 0.4 | 18 | | 1E 2259+586 | I | | | 0.7 | | | 16 | | | | 1E 2259+586 | R | -1.02 | 5.95 | | | | 12 | | | | | | | | | | | | | | | SGR 0755-2933 # | S | | | | <2.0 | | 11 | < 1.7 | 18 | | SGR 1801-23 # | | | | | | | | | | | SGR 1808-20 # | | | | | | | | | | | AX J1818.8-1559 # | | | | | | | | | | | AX J1845.0-0258 # | | | | | | | | | | | SGR 2013+34 # | | | | | | | | | | | | | | | | | | | | | | PSR J1846-0258 ## | | | | | | | | | | | | | | | | | | | | | | Swift J1818.0-1607 | | | | 3.05 | | | 17 | | | +-----------------------+---------------+---------------------+---------------------+------------------------------+----------------------------------+---------------+------------+---------------------+-----------+ 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] R = RXTE I = Integral S = Suzaku N = NuSTAR [2] The pulsed and total hard X-ray fluxes are given for the 20-150 keV range. If these fluxes could only be found at a different energy range in the literature, then we used WebPIMMS to estimate the 20-150 keV fluxes. [3] Gamma-ray flux is given for the 0.1-10 GeV range. References: 1 den Hartog et al. 2008, A&A, 489, 245 2 Enoto et al. 2011, PASJ, 63, 387 3 Rea et al. 2009, MNRAS, 396, 2419 4 Enoto et al. 2010, ApJ, 715, 665 5 Kuiper et al. 2012, ApJ, 748, 133 6 Enoto et al. 2010, PASJ, 62, 475 7 Gotz et al. 2007, A&A, 475, 317 8 den Hartog et al. 2008, A&A, 489, 263 9 Mori et al. 2013, ApJL, 770, L23 10 Mereghetti et al. 2005, A&A, 433, L9 11 Enoto et al. 2010, ApJL, 722, L162 12 Kuiper et al. 2006, ApJ, 645, 556 13 Morii et al. 2010, PASJ, 62, 1249 14 An et al. 2013, ApJ, 779, 163 15 Gotz et al. 2006, A&A, 449, L31 16 Mereghetti et al. 2020, ApJL, 898, L29 17 Laha et al. 2020, GCN, 28193, 1 18 Abdo et al. 2010, ApJL, 725, L73