| 1 | flux tube | 42 | 14 | 3.154 | 0.007171 | 1805.01466,1805.09377,etc |
| 2 | explosion energy | 221 | 24 | 9.391 | 0.005126 | 1805.11501,1805.07268,etc |
| 3 | slit width | 55 | 17 | 3.312 | 0.004454 | 1805.00620,1805.06715,etc |
| 4 | wavelength dependence | 60 | 12 | 5.364 | 0.004097 | 1805.03598,1805.06715,etc |
| 5 | SNe Ia | 223 | 28 | 7.704 | 0.004077 | 1805.04521,1805.07268,etc |
| 6 | ray source | 37 | 13 | 3.0 | 0.00396 | 1805.03641,1805.11112,etc |
| 7 | black hole mass | 212 | 51 | 4.16 | 0.003823 | 1805.07873,1805.11785,etc |
| 8 | dust particle | 207 | 19 | 11.389 | 0.003539 | 1805.04521,1805.06722,etc |
| 9 | diffuse emission | 118 | 29 | 4.179 | 0.003536 | 1805.11112,1805.08870,etc |
| 10 | line list | 93 | 16 | 6.133 | 0.003411 | 1805.11744,1805.00929,etc |
| 11 | model A | 81 | 12 | 6.182 | 0.003356 | 1805.11314,1805.10301,etc |
| 12 | primordial power spectrum | 66 | 23 | 2.455 | 0.003324 | 1805.11210,1805.11527,etc |
| 13 | two-point correlation function | 48 | 15 | 3.357 | 0.00325 | 1805.05643,1805.11527,etc |
| 14 | gravity model | 119 | 25 | 4.917 | 0.003171 | 1805.09918,1805.04716,etc |
| 15 | magnetic structure | 75 | 22 | 3.524 | 0.003143 | 1805.08980,1805.00916,etc |
| 16 | intrinsic variability | 75 | 17 | 4.625 | 0.003129 | 1805.00300,1805.08843,etc |
| 17 | background field | 48 | 17 | 2.938 | 0.003072 | 1805.11172,1805.02160,etc |
| 18 | jet power | 63 | 15 | 4.429 | 0.003019 | 1805.11785,1805.01902,etc |
| 19 | size distribution | 145 | 44 | 3.349 | 0.003002 | 1805.05489,1805.04521,etc |
| 20 | metal-poor star | 195 | 30 | 6.655 | 0.002977 | 1805.05841,1805.04347,etc |
| 21 | contamination rate | 24 | 11 | 2.3 | 0.002946 | 1805.08985,1805.04162,etc |
| 22 | first star | 120 | 25 | 2.417 | 0.002906 | 1805.09599,1805.11044,etc |
| 23 | diffuse ISM | 42 | 13 | 3.25 | 0.0029 | 1805.03598,1805.11105,etc |
| 24 | flux rope | 60 | 13 | 4.917 | 0.002791 | 1805.00916,1805.12314,etc |
| 25 | gamma ray | 166 | 29 | 5.857 | 0.002765 | 1805.08379,1805.10305,etc |
| 26 | Paper I | 341 | 33 | 10.594 | 0.002705 | 1805.00283,1805.04709,etc |
| 27 | Fe line | 69 | 14 | 5.231 | 0.002587 | 1805.11396,1805.05810,etc |
| 28 | hard state | 90 | 14 | 6.846 | 0.002537 | 1805.07873,1805.06076,etc |
| 29 | halo property | 85 | 16 | 5.6 | 0.002531 | 1805.06397,1805.00033,etc |
| 30 | binary component | 47 | 20 | 2.368 | 0.002496 | 1805.02012,1805.00494,etc |
| 31 | telluric correction | 50 | 13 | 4.083 | 0.002475 | 1805.02720,1805.03212,etc |
| 32 | Galactocentric radius | 65 | 11 | 6.3 | 0.002462 | 1805.03706,1805.03212,etc |
| 33 | peak flux density | 56 | 14 | 4.0 | 0.002364 | 1805.02012,1805.05540,etc |
| 34 | cold gas | 178 | 40 | 4.513 | 0.00231 | 1805.06076,1805.12251,etc |
| 35 | Alfv'en wave | 80 | 11 | 7.9 | 0.002306 | 1805.00285,1805.11220,etc |
| 36 | relative difference | 108 | 34 | 3.242 | 0.002197 | 1805.09918,1805.10530,etc |
| 37 | maximum mass | 95 | 33 | 2.938 | 0.002193 | 1805.00547,1805.12143,etc |
| 38 | hot Jupiters | 190 | 26 | 6.72 | 0.002177 | 1805.01903,1805.00029,etc |
| 39 | gas particle | 178 | 31 | 5.7 | 0.002166 | 1805.12271,1805.04521,etc |
| 40 | lens galaxy | 36 | 12 | 3.0 | 0.00216 | 1805.08640,1805.00027,etc |
| 41 | control sample | 96 | 14 | 7.308 | 0.002148 | 1805.05003,1805.03604,etc |
| 42 | Sgr A* | 73 | 11 | 6.8 | 0.002128 | 1805.04669,1805.00474,etc |
| 43 | energy threshold | 47 | 18 | 2.647 | 0.002121 | 1805.02472,1805.01847,etc |
| 44 | halo mass | 486 | 73 | 6.736 | 0.002117 | 1805.05489,1805.10944,etc |
| 45 | X-ray source | 127 | 39 | 3.316 | 0.002099 | 1805.05489,1805.06076,etc |
| 46 | small body | 133 | 15 | 9.357 | 0.002089 | 1805.00929,1805.06159,etc |
| 47 | peak position | 83 | 23 | 3.727 | 0.002056 | 1805.12251,1805.05146,etc |
| 48 | high-redshift galaxy | 93 | 31 | 3.067 | 0.002051 | 1805.05481,1805.09351,etc |
| 49 | radiative efficiency | 35 | 13 | 2.833 | 0.002048 | 1805.11785,1805.06076,etc |
| 50 | Gaia DR2 | 92 | 28 | 3.37 | 0.002004 | 1805.00482,1805.01448,etc |
| 51 | central velocity dispersion | 45 | 13 | 3.583 | 0.001978 | 1805.05226,1805.06894,etc |
| 52 | red clump star | 40 | 12 | 2.364 | 0.001978 | 1805.12199,1805.00275,etc |
| 53 | single power law | 35 | 17 | 2.125 | 0.001963 | 1805.10475,1805.00474,etc |
| 54 | oscillation frequency | 42 | 20 | 2.105 | 0.001957 | 1805.12522,1805.09385,etc |
| 55 | polarization degree | 51 | 13 | 4.167 | 0.001956 | 1805.00494,1805.02674,etc |
| 56 | stellar rotation period | 47 | 13 | 2.083 | 0.001933 | 1805.09352,1805.07044,etc |
| 57 | absorption signal | 40 | 12 | 3.182 | 0.001916 | 1805.11210,1805.03254,etc |
| 58 | ambient medium | 93 | 23 | 4.182 | 0.001915 | 1805.06614,1805.00014,etc |
| 59 | magnetic field line | 172 | 58 | 2.895 | 0.001907 | 1805.02012,1805.00494,etc |
| 60 | inflaton field | 61 | 16 | 3.667 | 0.001895 | 1805.11527,1805.04550,etc |
| 61 | flux distribution | 47 | 21 | 2.25 | 0.001881 | 1805.11512,1805.05481,etc |
| 62 | soft state | 58 | 11 | 4.7 | 0.001875 | 1805.07873,1805.06076,etc |
| 63 | initial abundance | 24 | 11 | 2.3 | 0.00187 | 1805.00498,1805.03618,etc |
| 64 | baryonic mass | 82 | 25 | 3.25 | 0.001868 | 1805.00122,1805.04528,etc |
| 65 | outflow rate | 125 | 14 | 9.231 | 0.001868 | 1805.00474,1805.06614,etc |
| 66 | redshift-space distortion | 40 | 13 | 3.25 | 0.001866 | 1805.00934,1805.10178,etc |
| 67 | poloidal field | 37 | 13 | 3.0 | 0.001854 | 1805.00494,1805.02478,etc |
| 68 | ray flare | 43 | 11 | 3.0 | 0.001832 | 1805.02750,1805.04588,etc |
| 69 | third body | 33 | 11 | 2.9 | 0.00182 | 1805.04952,1805.00798,etc |
| 70 | detector response | 37 | 11 | 3.6 | 0.001813 | 1805.08980,1805.12562,etc |
| 71 | redshift distribution | 159 | 41 | 3.875 | 0.001775 | 1805.05481,1805.00934,etc |
| 72 | light travel time | 26 | 11 | 2.5 | 0.001758 | 1805.05051,1805.00046,etc |
| 73 | weighting function | 37 | 15 | 2.571 | 0.001751 | 1805.09385,1805.09881,etc |
| 74 | source size | 61 | 25 | 2.458 | 0.001749 | 1805.09789,1805.11499,etc |
| 75 | electron distribution | 51 | 17 | 3.125 | 0.001724 | 1805.08773,1805.04603,etc |
| 76 | Poynting flux | 42 | 11 | 3.9 | 0.001682 | 1805.11785,1805.03010,etc |
| 77 | transmission spectrum | 58 | 15 | 4.0 | 0.001681 | 1805.11744,1805.00029,etc |
| 78 | multi-planet system | 53 | 13 | 4.333 | 0.001678 | 1805.01903,1805.00956,etc |
| 79 | ionised gas | 39 | 13 | 2.917 | 0.001677 | 1805.11512,1805.05341,etc |
| 80 | axion mass | 58 | 12 | 5.091 | 0.001675 | 1805.10533,1805.12147,etc |
| 81 | different environment | 107 | 36 | 3.029 | 0.001665 | 1805.06397,1805.00929,etc |
| 82 | central galaxy | 143 | 32 | 4.581 | 0.001661 | 1805.10944,1805.06938,etc |
| 83 | gamma-ray flux | 39 | 14 | 2.769 | 0.001654 | 1805.08379,1805.10305,etc |
| 84 | joint distribution | 27 | 12 | 2.364 | 0.00165 | 1805.00283,1805.00934,etc |
| 85 | gravity theory | 47 | 15 | 3.286 | 0.001643 | 1805.05146,1805.08731,etc |
| 86 | progenitor mass | 66 | 17 | 3.625 | 0.001633 | 1805.04521,1805.01213,etc |
| 87 | central density | 111 | 43 | 2.619 | 0.00162 | 1805.09918,1805.00122,etc |
| 88 | polarization fraction | 48 | 11 | 4.6 | 0.001594 | 1805.00494,1805.06131,etc |
| 89 | spatial correlation | 33 | 14 | 2.462 | 0.001587 | 1805.12188,1805.07157,etc |
| 90 | local density | 73 | 29 | 2.571 | 0.001583 | 1805.06473,1805.06397,etc |
| 91 | photometric selection | 28 | 11 | 2.3 | 0.00158 | 1805.05332,1805.03665,etc |
| 92 | microlensing event | 86 | 20 | 4.421 | 0.001569 | 1805.01898,1805.04347,etc |
| 93 | ray emission | 99 | 27 | 3.731 | 0.001569 | 1805.04588,1805.06319,etc |
| 94 | electric field | 119 | 38 | 3.054 | 0.001569 | 1805.09348,1805.07257,etc |
| 95 | dark matter mass | 40 | 19 | 2.167 | 0.001561 | 1805.10305,1805.02472,etc |
| 96 | star particle | 188 | 28 | 6.926 | 0.001552 | 1805.12271,1805.05643,etc |
| 97 | numerical resolution | 55 | 19 | 3.0 | 0.001547 | 1805.11755,1805.01249,etc |
| 98 | galactocentric radius | 65 | 20 | 3.368 | 0.001542 | 1805.05353,1805.06894,etc |
| 99 | donor star | 64 | 16 | 4.2 | 0.001504 | 1805.00482,1805.04952,etc |
| 100 | finite temperature | 25 | 12 | 2.182 | 0.001495 | 1805.10530,1805.07186,etc |
|