| 1 | flux rope | 178 | 12 | 16.091 | 0.006478 | 1707.04421,1707.06198,etc |
| 2 | flux tube | 203 | 19 | 11.111 | 0.006439 | 1707.09419,1707.08846,etc |
| 3 | magnetic field amplification | 37 | 13 | 3.0 | 0.005354 | 1707.06147,1707.09419,etc |
| 4 | spatial curvature | 37 | 12 | 3.0 | 0.004873 | 1707.00588,1707.01948,etc |
| 5 | neutrino mass | 174 | 25 | 7.0 | 0.004264 | 1707.07684,1707.00588,etc |
| 6 | SNe Ia | 304 | 25 | 12.583 | 0.004057 | 1707.00696,1707.00588,etc |
| 7 | linear perturbation | 63 | 22 | 2.952 | 0.003953 | 1707.09419,1707.06929,etc |
| 8 | control sample | 166 | 13 | 12.25 | 0.0039 | 1707.02840,1707.01559,etc |
| 9 | polarization degree | 103 | 12 | 8.727 | 0.00363 | 1707.05540,1707.09764,etc |
| 10 | magnetic field line | 218 | 50 | 4.429 | 0.003172 | 1707.06147,1707.08846,etc |
| 11 | mass accretion rate | 257 | 40 | 6.564 | 0.003056 | 1707.09479,1707.00540,etc |
| 12 | black hole mass | 241 | 49 | 4.979 | 0.002882 | 1707.06249,1707.01411,etc |
| 13 | orbital solution | 35 | 11 | 2.1 | 0.002753 | 1707.00591,1707.08263,etc |
| 14 | mass-metallicity relation | 42 | 14 | 3.077 | 0.002701 | 1707.05293,1707.07991,etc |
| 15 | grid point | 92 | 25 | 3.792 | 0.002671 | 1707.01411,1707.06640,etc |
| 16 | cluster sample | 71 | 18 | 4.118 | 0.002665 | 1707.05318,1707.09126,etc |
| 17 | Sgr A* | 72 | 13 | 5.083 | 0.002619 | 1707.03416,1707.02378,etc |
| 18 | polarization fraction | 59 | 13 | 4.833 | 0.002538 | 1707.03827,1707.00066,etc |
| 19 | galactic scale | 41 | 18 | 2.353 | 0.002536 | 1707.06147,1707.04001,etc |
| 20 | semimajor axis | 63 | 16 | 4.0 | 0.002362 | 1707.03026,1707.08127,etc |
| 21 | halo mass | 541 | 66 | 7.938 | 0.002331 | 1707.01108,1707.00568,etc |
| 22 | X-ray flare | 75 | 13 | 6.167 | 0.002318 | 1707.07903,1707.09831,etc |
| 23 | ray emission | 138 | 28 | 5.074 | 0.002273 | 1707.08473,1707.00136,etc |
| 24 | iron abundance | 83 | 15 | 5.857 | 0.002225 | 1707.05318,1707.04399,etc |
| 25 | gamma ray | 112 | 33 | 3.469 | 0.002222 | 1707.00176,1707.06147,etc |
| 26 | central galaxy | 283 | 40 | 7.128 | 0.002218 | 1707.01108,1707.07691,etc |
| 27 | radiation domination | 27 | 12 | 2.364 | 0.002218 | 1707.06929,1707.03417,etc |
| 28 | active neutrino | 31 | 11 | 2.9 | 0.002186 | 1707.07684,1707.00588,etc |
| 29 | overdense region | 57 | 13 | 4.667 | 0.002184 | 1707.02879,1707.04259,etc |
| 30 | mass-radius relation | 42 | 12 | 3.727 | 0.002181 | 1707.06460,1707.03161,etc |
| 31 | stellar feedback | 87 | 24 | 3.739 | 0.00218 | 1707.02879,1707.01108,etc |
| 32 | dark matter mass | 29 | 12 | 2.545 | 0.002135 | 1707.07691,1707.03400,etc |
| 33 | molecular gas mass | 53 | 14 | 3.846 | 0.002121 | 1707.05329,1707.06329,etc |
| 34 | sample galaxy | 45 | 12 | 3.909 | 0.002114 | 1707.05293,1707.07991,etc |
| 35 | dust mass | 157 | 34 | 4.727 | 0.002047 | 1707.07281,1707.02997,etc |
| 36 | hot Jupiters | 70 | 18 | 4.059 | 0.002039 | 1707.08328,1707.04262,etc |
| 37 | maximum mass | 84 | 22 | 3.952 | 0.00203 | 1707.09475,1707.01108,etc |
| 38 | accretion rate | 334 | 91 | 3.7 | 0.002 | 1707.01542,1707.00591,etc |
| 39 | central BH | 88 | 16 | 5.733 | 0.001957 | 1707.08822,1707.05334,etc |
| 40 | light nucleus | 50 | 11 | 4.7 | 0.001922 | 1707.06147,1707.03852,etc |
| 41 | nonlinear regime | 42 | 12 | 3.545 | 0.001885 | 1707.09194,1707.01863,etc |
| 42 | Sun-like star | 64 | 20 | 3.316 | 0.001849 | 1707.06192,1707.06249,etc |
| 43 | axion mass | 59 | 14 | 4.385 | 0.001849 | 1707.06929,1707.03400,etc |
| 44 | magnetic field strength | 260 | 77 | 3.132 | 0.001847 | 1707.00176,1707.03827,etc |
| 45 | mass-loss rate | 123 | 23 | 5.545 | 0.001834 | 1707.00611,1707.06003,etc |
| 46 | half-mass radius | 70 | 17 | 4.312 | 0.001824 | 1707.01094,1707.09153,etc |
| 47 | source region | 71 | 21 | 3.5 | 0.001803 | 1707.01542,1707.01367,etc |
| 48 | completeness limit | 28 | 12 | 2.455 | 0.001747 | 1707.09126,1707.02636,etc |
| 49 | stellar velocity dispersion | 51 | 25 | 2.042 | 0.001735 | 1707.03570,1707.01411,etc |
| 50 | dust temperature | 231 | 56 | 4.164 | 0.001729 | 1707.03827,1707.07281,etc |
| 51 | underdense region | 45 | 11 | 4.0 | 0.001716 | 1707.07535,1707.01906,etc |
| 52 | slow-roll parameter | 49 | 18 | 2.824 | 0.001706 | 1707.01300,1707.03023,etc |
| 53 | Alfv'en wave | 117 | 16 | 3.8 | 0.00166 | 1707.06147,1707.00485,etc |
| 54 | triple system | 31 | 11 | 2.8 | 0.001652 | 1707.06249,1707.01942,etc |
| 55 | transition point | 46 | 15 | 3.071 | 0.001643 | 1707.08846,1707.01802,etc |
| 56 | tensor-to-scalar ratio | 101 | 23 | 4.409 | 0.001642 | 1707.01300,1707.09841,etc |
| 57 | dust particle | 51 | 21 | 2.5 | 0.001641 | 1707.05293,1707.00696,etc |
| 58 | maximum light | 121 | 22 | 5.714 | 0.001618 | 1707.00696,1707.03954,etc |
| 59 | best-fit model | 155 | 53 | 2.942 | 0.001607 | 1707.05318,1707.04671,etc |
| 60 | distance estimate | 62 | 15 | 4.357 | 0.001602 | 1707.04554,1707.00696,etc |
| 61 | lens galaxy | 65 | 11 | 5.5 | 0.001591 | 1707.09159,1707.04590,etc |
| 62 | photometric variability | 44 | 17 | 2.688 | 0.00158 | 1707.05788,1707.04292,etc |
| 63 | Paper I | 163 | 31 | 5.167 | 0.001578 | 1707.03570,1707.09419,etc |
| 64 | grain growth | 47 | 15 | 3.214 | 0.001566 | 1707.00591,1707.08697,etc |
| 65 | response function | 44 | 13 | 3.583 | 0.001556 | 1707.08042,1707.07019,etc |
| 66 | red sequence | 96 | 19 | 5.278 | 0.001555 | 1707.00568,1707.07991,etc |
| 67 | ambient medium | 83 | 23 | 3.273 | 0.001553 | 1707.00485,1707.04706,etc |
| 68 | redshift distribution | 135 | 42 | 3.268 | 0.001547 | 1707.01411,1707.00804,etc |
| 69 | nitrogen abundance | 85 | 15 | 6.0 | 0.001531 | 1707.06236,1707.03456,etc |
| 70 | reheating temperature | 47 | 14 | 3.154 | 0.001514 | 1707.06277,1707.03830,etc |
| 71 | aperture correction | 52 | 16 | 3.4 | 0.001509 | 1707.03954,1707.03828,etc |
| 72 | type Ia supernova | 35 | 17 | 2.062 | 0.001498 | 1707.00588,1707.00111,etc |
| 73 | direct detection experiment | 46 | 16 | 3.0 | 0.001494 | 1707.06277,1707.08571,etc |
| 74 | stellar particle | 51 | 17 | 3.0 | 0.00147 | 1707.01094,1707.01108,etc |
| 75 | polarization map | 27 | 11 | 2.6 | 0.001459 | 1707.03827,1707.04076,etc |
| 76 | parameter region | 29 | 11 | 2.8 | 0.001458 | 1707.06929,1707.08571,etc |
| 77 | tidal heating | 68 | 13 | 5.583 | 0.001448 | 1707.01108,1707.04262,etc |
| 78 | cosmological evolution | 67 | 24 | 2.87 | 0.001422 | 1707.06147,1707.01480,etc |
| 79 | X-ray variability | 35 | 16 | 2.267 | 0.001415 | 1707.04671,1707.03200,etc |
| 80 | significance level | 32 | 12 | 2.727 | 0.001415 | 1707.03658,1707.06651,etc |
| 81 | cosmological signal | 34 | 12 | 3.0 | 0.001408 | 1707.04102,1707.02288,etc |
| 82 | arrival direction | 36 | 14 | 2.692 | 0.001404 | 1707.06147,1707.07684,etc |
| 83 | paper I | 63 | 19 | 3.444 | 0.001402 | 1707.09419,1707.01108,etc |
| 84 | size distribution | 89 | 30 | 3.034 | 0.001375 | 1707.03570,1707.00696,etc |
| 85 | analytic model | 65 | 24 | 2.783 | 0.001359 | 1707.02302,1707.09356,etc |
| 86 | temperature map | 29 | 14 | 2.154 | 0.001355 | 1707.04102,1707.04259,etc |
| 87 | planet radius | 51 | 16 | 3.333 | 0.001341 | 1707.04253,1707.06192,etc |
| 88 | transit depth | 48 | 14 | 3.0 | 0.00134 | 1707.08328,1707.04262,etc |
| 89 | dark sector | 74 | 21 | 3.65 | 0.001339 | 1707.06277,1707.09246,etc |
| 90 | dense gas | 67 | 30 | 2.241 | 0.001336 | 1707.02879,1707.03827,etc |
| 91 | galaxy mass | 99 | 28 | 3.63 | 0.001336 | 1707.01094,1707.07991,etc |
| 92 | source plane | 69 | 11 | 6.2 | 0.001334 | 1707.02454,1707.09159,etc |
| 93 | strong magnetic field | 102 | 48 | 2.106 | 0.001324 | 1707.09419,1707.07854,etc |
| 94 | gas surface density | 39 | 15 | 2.714 | 0.001312 | 1707.02302,1707.04001,etc |
| 95 | comparison sample | 58 | 19 | 2.889 | 0.001302 | 1707.01542,1707.08328,etc |
| 96 | spectral distortion | 39 | 11 | 3.7 | 0.001295 | 1707.01300,1707.08129,etc |
| 97 | density contrast | 82 | 32 | 2.613 | 0.00129 | 1707.08697,1707.01480,etc |
| 98 | energy injection | 70 | 29 | 2.393 | 0.001262 | 1707.01300,1707.05529,etc |
| 99 | binary separation | 42 | 12 | 3.727 | 0.001255 | 1707.05989,1707.08127,etc |
| 100 | adiabatic cooling | 38 | 14 | 2.846 | 0.001243 | 1707.01300,1707.01906,etc |
|