| long GRBs | 70 | 17 | 4.25 | 0.004277 | 1506.07801,1506.05899,etc |
| primordial gravitational wave | 42 | 12 | 3.545 | 0.004051 | 1506.02671,1506.01011,etc |
| gravity model | 87 | 20 | 4.474 | 0.003877 | 1506.08859,1506.04977,etc |
| tidal field | 111 | 17 | 6.125 | 0.003477 | 1506.00957,1506.07366,etc |
| stellar population property | 63 | 13 | 4.667 | 0.003323 | 1506.05315,1506.01037,etc |
| Einstein frame | 69 | 15 | 3.5 | 0.003276 | 1506.00186,1506.00988,etc |
| log g | 90 | 12 | 7.727 | 0.003111 | 1506.07517,1506.03615,etc |
| hard state | 147 | 13 | 12.083 | 0.003066 | 1506.06780,1506.01102,etc |
| pulsar magnetosphere | 33 | 11 | 3.0 | 0.002928 | 1506.00182,1506.05507,etc |
| main halo | 62 | 11 | 6.1 | 0.00292 | 1506.05877,1506.01724,etc |
| tensor-to-scalar ratio | 124 | 20 | 6.368 | 0.0029 | 1506.01410,1506.09172,etc |
| control sample | 95 | 11 | 9.0 | 0.002897 | 1506.01380,1506.05521,etc |
| wavelength solution | 61 | 12 | 5.273 | 0.002815 | 1506.08864,1506.07525,etc |
| line list | 57 | 16 | 3.0 | 0.002811 | 1506.08864,1506.06095,etc |
| third body | 48 | 11 | 4.7 | 0.00278 | 1506.03029,1506.01441,etc |
| spin-down rate | 32 | 11 | 3.1 | 0.002706 | 1506.06700,1506.00182,etc |
| quark matter | 68 | 12 | 6.0 | 0.002698 | 1506.08645,1506.05552,etc |
| mass-loss rate | 158 | 20 | 7.895 | 0.002688 | 1506.05176,1506.04238,etc |
| small body | 45 | 14 | 3.154 | 0.002668 | 1506.03029,1506.06569,etc |
| SNe Ia | 90 | 18 | 5.176 | 0.00264 | 1506.08212,1506.08957,etc |
| donor star | 117 | 20 | 6.105 | 0.002609 | 1506.03219,1506.08604,etc |
| electron energy | 62 | 13 | 5.0 | 0.002592 | 1506.07926,1506.02358,etc |
| maximum mass | 96 | 31 | 3.133 | 0.002497 | 1506.08585,1506.01765,etc |
| stellar surface density | 45 | 12 | 3.727 | 0.00234 | 1506.05289,1506.03845,etc |
| free-free emission | 47 | 17 | 2.688 | 0.002196 | 1506.06582,1506.01907,etc |
| background evolution | 33 | 14 | 2.462 | 0.002186 | 1506.08575,1506.04543,etc |
| dark matter mass | 53 | 16 | 2.8 | 0.002177 | 1506.05119,1506.06767,etc |
| broad component | 63 | 14 | 4.769 | 0.002174 | 1506.03454,1506.01276,etc |
| non-thermal emission | 68 | 20 | 3.526 | 0.00212 | 1506.08043,1506.05916,etc |
| energy band | 136 | 38 | 3.649 | 0.002102 | 1506.00593,1506.05899,etc |
| nonumber && | 60 | 15 | 4.071 | 0.002099 | 1506.03524,1506.06596,etc |
| mass accretion rate | 157 | 47 | 3.37 | 0.002097 | 1506.07170,1506.06780,etc |
| low mass end | 36 | 14 | 2.615 | 0.002092 | 1506.00655,1506.05931,etc |
| detection probability | 33 | 12 | 2.818 | 0.002061 | 1506.04035,1506.01515,etc |
| radio power | 67 | 11 | 6.1 | 0.002053 | 1506.08043,1506.05916,etc |
| magnetic field strength | 190 | 54 | 3.566 | 0.002027 | 1506.07170,1506.06780,etc |
| black hole mass | 211 | 51 | 3.84 | 0.002022 | 1506.07170,1506.06780,etc |
| thermal conduction | 50 | 16 | 3.267 | 0.002012 | 1506.04674,1506.08356,etc |
| quiescent state | 53 | 21 | 2.6 | 0.001982 | 1506.00593,1506.03219,etc |
| jet component | 39 | 11 | 3.8 | 0.001945 | 1506.05899,1506.08043,etc |
| model spectrum | 76 | 26 | 3.0 | 0.001942 | 1506.05315,1506.01037,etc |
| Starobinsky model | 63 | 12 | 2.909 | 0.00194 | 1506.07433,1506.03253,etc |
| diffuse ISM | 42 | 12 | 3.727 | 0.001938 | 1506.06503,1506.06782,etc |
| accretion rate | 305 | 77 | 4.0 | 0.001884 | 1506.05877,1506.01772,etc |
| cluster mass | 94 | 22 | 4.286 | 0.001831 | 1506.01400,1506.00957,etc |
| progenitor system | 51 | 13 | 4.083 | 0.00182 | 1506.00636,1506.03367,etc |
| soft state | 92 | 12 | 7.909 | 0.00174 | 1506.03219,1506.01102,etc |
| host halo | 163 | 34 | 4.909 | 0.001731 | 1506.05877,1506.00957,etc |
| progenitor mass | 37 | 12 | 3.182 | 0.001727 | 1506.00106,1506.03891,etc |
| cross-correlation function | 52 | 17 | 3.125 | 0.001689 | 1506.06780,1506.05899,etc |
| magnetic fluctuation | 42 | 11 | 4.1 | 0.00168 | 1506.02034,1506.03087,etc |
| low velocity | 49 | 20 | 2.526 | 0.001673 | 1506.06605,1506.06569,etc |
| dark matter particle | 107 | 45 | 2.295 | 0.00166 | 1506.05877,1506.03924,etc |
| star-forming galaxy | 222 | 60 | 3.746 | 0.001649 | 1506.08205,1506.08821,etc |
| gamma ray | 83 | 28 | 2.963 | 0.001638 | 1506.05119,1506.08202,etc |
| emission region | 97 | 27 | 3.692 | 0.001638 | 1506.04827,1506.03947,etc |
| dynamical system | 54 | 17 | 3.312 | 0.001637 | 1506.03221,1506.01496,etc |
| selection method | 29 | 12 | 2.545 | 0.001588 | 1506.08043,1506.01765,etc |
| mass transfer rate | 42 | 12 | 3.727 | 0.00158 | 1506.02526,1506.05972,etc |
| density gradient | 47 | 18 | 2.706 | 0.001576 | 1506.02426,1506.03875,etc |
| gas fraction | 107 | 24 | 4.609 | 0.001573 | 1506.08957,1506.03819,etc |
| pixel value | 51 | 20 | 2.632 | 0.001563 | 1506.01400,1506.08205,etc |
| explosion energy | 79 | 15 | 2.714 | 0.001561 | 1506.05802,1506.08827,etc |
| density contrast | 58 | 20 | 2.842 | 0.001558 | 1506.04977,1506.07526,etc |
| Jordan frame | 51 | 13 | 3.333 | 0.001554 | 1506.00186,1506.06313,etc |
| neutrino mass | 70 | 16 | 4.6 | 0.001548 | 1506.07493,1506.08124,etc |
| dust temperature | 127 | 36 | 3.6 | 0.001538 | 1506.05176,1506.07037,etc |
| halo mass | 222 | 52 | 4.314 | 0.001534 | 1506.00957,1506.01100,etc |
| X-ray flare | 41 | 14 | 3.0 | 0.001528 | 1506.05899,1506.03079,etc |
| mass estimate | 79 | 34 | 2.364 | 0.001511 | 1506.00635,1506.01387,etc |
| Paper I | 285 | 41 | 7.0 | 0.001509 | 1506.05125,1506.04508,etc |
| positional uncertainty | 31 | 12 | 2.545 | 0.001505 | 1506.07373,1506.01424,etc |
| fluid element | 49 | 14 | 3.692 | 0.00148 | 1506.08598,1506.07195,etc |
| chemical species | 37 | 12 | 3.273 | 0.001466 | 1506.01265,1506.06740,etc |
| short GRBs | 57 | 20 | 2.789 | 0.00145 | 1506.07801,1506.05899,etc |
| target star | 116 | 22 | 5.429 | 0.001418 | 1506.07517,1506.06095,etc |
| grain size | 86 | 18 | 4.941 | 0.001404 | 1506.07170,1506.00430,etc |
| angular momentum loss | 37 | 18 | 2.118 | 0.001397 | 1506.00182,1506.05298,etc |
| ambient medium | 80 | 24 | 3.304 | 0.001392 | 1506.04508,1506.03079,etc |
| outer disk | 123 | 28 | 4.481 | 0.00139 | 1506.06780,1506.00430,etc |
| average spectrum | 31 | 12 | 2.727 | 0.001376 | 1506.01276,1506.01102,etc |
| dynamical interaction | 52 | 17 | 3.188 | 0.00136 | 1506.01400,1506.01147,etc |
| oxygen abundance | 54 | 15 | 3.786 | 0.001353 | 1506.06959,1506.04238,etc |
| overlap region | 39 | 13 | 3.167 | 0.001352 | 1506.05931,1506.08864,etc |
| count rate | 177 | 58 | 3.07 | 0.00134 | 1506.05899,1506.01515,etc |
| matter power spectrum | 71 | 27 | 2.692 | 0.001331 | 1506.05877,1506.07493,etc |
| annihilation rate | 42 | 13 | 3.417 | 0.001331 | 1506.01529,1506.06767,etc |
| Chabrier IMF | 38 | 14 | 2.846 | 0.001322 | 1506.01037,1506.01518,etc |
| low-mass star | 95 | 41 | 2.35 | 0.001304 | 1506.05176,1506.02704,etc |
| parameter estimation | 77 | 24 | 3.13 | 0.001302 | 1506.07366,1506.03926,etc |
| stellar feedback | 80 | 17 | 4.75 | 0.001289 | 1506.08205,1506.06503,etc |
| second generation | 44 | 14 | 3.231 | 0.001288 | 1506.01037,1506.01529,etc |
| gas mass | 127 | 45 | 2.864 | 0.001287 | 1506.04144,1506.05888,etc |
| energetic electron | 29 | 14 | 2.154 | 0.001285 | 1506.04674,1506.05119,etc |
| star formation history | 141 | 52 | 2.725 | 0.001284 | 1506.01323,1506.05315,etc |
| large angular scale | 24 | 12 | 2.091 | 0.001283 | 1506.01907,1506.07135,etc |
| atomic datum | 67 | 23 | 3.0 | 0.001272 | 1506.07753,1506.06095,etc |
| statistical isotropy | 56 | 16 | 3.667 | 0.001267 | 1506.06596,1506.03926,etc |
| spectral indices | 138 | 42 | 3.268 | 0.001262 | 1506.05899,1506.08043,etc |
| paper I | 74 | 16 | 4.867 | 0.001257 | 1506.05125,1506.04508,etc |
|