+-----------------------+---------------+-----------------+--------------------------+----------------+---------------------+---------------+-----------+ | Name | Cutoff Energy | Gamma (Pulsed) | Pulsed Flux [1] | Gamma (Total) | Total Flux [1] | Telescope [2] | Reference | | | (keV) | | (10^-11 erg/s/cm^2) | | (10^-11 erg/s/cm^2) | | | +-----------------------+---------------+-----------------+--------------------------+----------------+---------------------+---------------+-----------+ | 4U 0142+61 | 279 65 41 | 0.40 0.15 0.15 | 2.68 1.34 1.34 | 0.93 0.06 0.06 | 9.09 0.35 0.35 | I, R | 1 | | 4U 0142+61 | | | | 0.89 0.11 0.10 | 10.3 | S | 2 | | | | | | | | | | | SGR 0501+4516 | >100 | | | 0.8 0.2 0.2 | | I | 3 | | SGR 0501+4516 | | | | | < 3.5 | I | 3 | | SGR 0501+4516 | | | | 0.79 0.20 0.18 | 8.4 2.0 1.5 | S | 4 | | | | | | | | | | | 1E 1547.0-5408 | >200 | | | 1.54 0.06 0.05 | 17.4 1.4 1.8 | S | 5 | | 1E 1547.0-5408 | | -0.37 0.28 0.20 | 6.9 1.2 1.0 | | | R | 6 | | 1E 1547.0-5408 | | -0.59 0.25 0.19 | 7.5 0.9 1.0 | | | R | 6 | | 1E 1547.0-5408 | | -1.55 0.42 0.26 | 4.1 0.9 0.9 | | | R | 6 | | 1E 1547.0-5408 | | | | | < 1.5 | I | 6 | | 1E 1547.0-5408 | | | | 1.41 0.06 0.06 | 25.2 3.7 3.7 | I | 6 | | 1E 1547.0-5408 | | | | 1.45 0.04 0.04 | 18.5 1.8 1.8 | I | 6 | | 1E 1547.0-5408 | | | | 1.27 0.11 0.11 | 21.5 1.4 1.4 | I | 6 | | 1E 1547.0-5408 | | | | 1.22 0.10 0.10 | 8.4 2.7 2.7 | I | 6 | | 1E 1547.0-5408 | | | | 0.87 0.07 0.07 | 8.0 2.2 2.2 | I | 6 | | | | | | | | | | | 1RXS J170849.0-400910 | >300 | | | 1.46 0.21 0.21 | 5.2 1.0 1.0 | I | 7 | | 1RXS J170849.0-400910 | | 0.86 0.16 0.16 | 2.60 0.35 0.35 | 1.13 0.06 0.06 | 6.61 0.23 0.23 | I, R | 8 | | | | | | | | | | | SGR J1745-2900 | > 50 | | | 1.47 0.46 0.37 | 0.67 0.20 0.26 | N | 9 | | | | | | | | | | | SGR 1806-20 | >160 | | | 1.9 0.2 0.2 | 6.0 0.9 0.9 | I | 10 | | SGR 1806-20 | | | | 1.5 0.3 0.3 | 11 2 2 | I | 10 | | SGR 1806-20 | | | | 1.7 0.1 0.1 | 4.70 | S | 11 | | SGR 1806-20 | | | | 1.2 0.1 0.1 | 9.89 | S | 11 | | SGR 1806-20 | | | | 1.6 0.2 0.2 | 3.83 | S | 11 | | | | | | | | | | | 1E 1841-045 | >140 | | 62000 9000 9000 | | | N | 12 | | 1E 1841-045 | | 0.72 0.15 0.15 | 4.00 | 1.32 0.11 0.11 | 6.88 | I, R | 13 | | 1E 1841-045 | | 1.35 0.30 0.25 | 2.67 | 1.62 0.21 0.22 | 4.59 | S | 14 | | | | | | | | | | | SGR 1900+14 | >100 | 0.99 0.36 0.36 | 3.03 | 1.33 0.03 0.03 | 7.99 | N | 15 | | SGR 1900+14 | | | | 3.1 0.5 0.5 | 1.6 0.4 0.4 | I | 16 | | SGR 1900+14 | | | | 1.2 0.5 0.5 | 3.24 | S | 11 | | | | | | | | | | | SGR 1935+2154 | | | | 1.4 0.3 0.3 | 1.42 | S | 11 | | | | | | | | | | | 1E 2259+586 | | | | 0.7 0.4 0.2 | | I | 17 | | 1E 2259+586 | | -1.02 0.24 0.13 | 5.95 | | | R | 13 | | | | | | | | | | | PSR J1846-0258 ## | | | | | < 2.0 | S | 11 | | PSR J1846-0258 ## | | | | 3.05 0.28 0.28 | | | 18 | | | | | | | | | | | Swift J1818.0-1607 | | | | | | | 18 | +-----------------------+---------------+-----------------+--------------------------+----------------+---------------------+---------------+-----------+ 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] 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. [2] R = RXTE I = Integral S = Suzaku N = NuSTAR 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 Enoto et al. 2010, PASJ, 62, 475 6 Kuiper et al. 2012, ApJ, 748, 133 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 Esposito et al. 2020, ApJL, 896, L30 13 Kuiper et al. 2006, ApJ, 645, 556 14 Morii et al. 2010, PASJ, 62, 1249 15 An et al. 2013, ApJ, 779, 163 16 Gotz et al. 2006, A&A, 449, L31 17 Mereghetti et al. 2020, ApJL, 898, L29 18 Laha et al. 2020, GCN, 28193, 1