| 1 | SNe Ia | 304 | 26 | 12.12 | 0.008186 | 1710.05440,1710.00963,etc |
| 2 | flux tube | 202 | 14 | 7.154 | 0.004982 | 1710.08926,1710.10937,etc |
| 3 | young massive star | 33 | 13 | 2.667 | 0.004627 | 1710.02099,1710.06902,etc |
| 4 | arrival direction | 86 | 15 | 4.714 | 0.004511 | 1710.00890,1710.00247,etc |
| 5 | short GRBs | 228 | 43 | 5.405 | 0.004187 | 1710.07436,1710.05851,etc |
| 6 | debris disk | 99 | 13 | 8.083 | 0.00382 | 1710.10269,1710.06209,etc |
| 7 | dark matter mass | 49 | 17 | 3.0 | 0.003707 | 1710.02865,1710.06170,etc |
| 8 | interaction term | 42 | 11 | 4.1 | 0.003461 | 1710.00713,1710.01853,etc |
| 9 | black hole mass | 230 | 57 | 4.089 | 0.003356 | 1710.02865,1710.01399,etc |
| 10 | molecular gas mass | 88 | 15 | 6.143 | 0.003345 | 1710.10181,1710.04224,etc |
| 11 | axion field | 95 | 11 | 7.4 | 0.003173 | 1710.09198,1710.07269,etc |
| 12 | dust attenuation | 92 | 23 | 4.136 | 0.003128 | 1710.10472,1710.06628,etc |
| 13 | toroidal field | 91 | 17 | 5.312 | 0.003123 | 1710.09227,1710.05897,etc |
| 14 | event rate | 123 | 32 | 3.839 | 0.003102 | 1710.03020,1710.10765,etc |
| 15 | transmission spectrum | 145 | 14 | 9.231 | 0.003073 | 1710.10269,1710.04946,etc |
| 16 | linear model | 50 | 21 | 2.4 | 0.003025 | 1710.08342,1710.04707,etc |
| 17 | line shape | 60 | 22 | 2.667 | 0.002977 | 1710.03336,1710.03535,etc |
| 18 | inner disk | 232 | 36 | 6.6 | 0.002843 | 1710.03153,1710.01323,etc |
| 19 | gas metallicity | 100 | 16 | 6.6 | 0.002841 | 1710.03315,1710.08726,etc |
| 20 | mass-loss rate | 170 | 29 | 5.893 | 0.002772 | 1710.09590,1710.07780,etc |
| 21 | halo mass | 409 | 75 | 5.5 | 0.002764 | 1710.01324,1710.07637,etc |
| 22 | average spectrum | 53 | 22 | 2.476 | 0.002705 | 1710.05834,1710.08345,etc |
| 23 | neutrino signal | 36 | 11 | 3.5 | 0.002629 | 1710.03020,1710.02155,etc |
| 24 | old population | 47 | 16 | 3.067 | 0.002595 | 1710.09403,1710.04053,etc |
| 25 | hot Jupiters | 165 | 26 | 6.56 | 0.002582 | 1710.10269,1710.10863,etc |
| 26 | single pulse | 39 | 13 | 3.167 | 0.002572 | 1710.05834,1710.11114,etc |
| 27 | stellar mass range | 45 | 15 | 3.143 | 0.002508 | 1710.07637,1710.08421,etc |
| 28 | magnetic field line | 178 | 56 | 2.527 | 0.002478 | 1710.04598,1710.08501,etc |
| 29 | tidal dissipation | 65 | 16 | 4.267 | 0.002422 | 1710.04707,1710.01737,etc |
| 30 | magnetic field amplification | 42 | 11 | 2.9 | 0.002332 | 1710.06992,1710.05859,etc |
| 31 | Eddington ratio | 97 | 27 | 3.692 | 0.002326 | 1710.09590,1710.02525,etc |
| 32 | analytic model | 140 | 44 | 3.209 | 0.002309 | 1710.05302,1710.08564,etc |
| 33 | sharp peak | 29 | 13 | 2.333 | 0.002187 | 1710.05851,1710.06279,etc |
| 34 | local source | 32 | 11 | 3.1 | 0.002161 | 1710.10937,1710.10266,etc |
| 35 | inner Galaxy | 36 | 15 | 2.286 | 0.00215 | 1710.10703,1710.03535,etc |
| 36 | direct detection experiment | 30 | 13 | 2.417 | 0.002105 | 1710.03658,1710.06170,etc |
| 37 | core mass | 94 | 25 | 3.875 | 0.002102 | 1710.05504,1710.03134,etc |
| 38 | chemical evolution model | 49 | 11 | 4.8 | 0.002102 | 1710.11014,1710.03657,etc |
| 39 | electron fraction | 152 | 32 | 4.871 | 0.002079 | 1710.04254,1710.11114,etc |
| 40 | Kelvin-Helmholtz instability | 35 | 11 | 3.4 | 0.002078 | 1710.01345,1710.05932,etc |
| 41 | delay time distribution | 34 | 11 | 3.0 | 0.002076 | 1710.05504,1710.04222,etc |
| 42 | disc galaxy | 74 | 17 | 4.562 | 0.002026 | 1710.00415,1710.04064,etc |
| 43 | triple system | 64 | 14 | 4.846 | 0.001998 | 1710.03153,1710.05030,etc |
| 44 | axis ratio | 106 | 24 | 4.478 | 0.001996 | 1710.04598,1710.03241,etc |
| 45 | neutron star surface | 31 | 11 | 3.0 | 0.001973 | 1710.10118,1710.03536,etc |
| 46 | high-mass star formation | 26 | 11 | 2.5 | 0.001967 | 1710.08564,1710.04595,etc |
| 47 | redshift distribution | 215 | 62 | 3.508 | 0.001947 | 1710.01733,1710.01569,etc |
| 48 | broad component | 106 | 21 | 5.05 | 0.001939 | 1710.10211,1710.03230,etc |
| 49 | energy-momentum tensor | 83 | 26 | 2.84 | 0.001922 | 1710.02865,1710.06086,etc |
| 50 | outer disk | 195 | 34 | 5.879 | 0.001921 | 1710.05049,1710.07051,etc |
| 51 | accretion rate | 472 | 103 | 4.618 | 0.001916 | 1710.05504,1710.03134,etc |
| 52 | neutron star merger | 113 | 41 | 2.6 | 0.001881 | 1710.05454,1710.04964,etc |
| 53 | hot gas | 145 | 40 | 3.692 | 0.001877 | 1710.00963,1710.07286,etc |
| 54 | scalar spectral index | 42 | 13 | 3.25 | 0.001877 | 1710.05793,1710.02477,etc |
| 55 | upper mass limit | 52 | 14 | 3.846 | 0.001863 | 1710.01138,1710.00823,etc |
| 56 | kilonova model | 72 | 21 | 3.5 | 0.001841 | 1710.05440,1710.05865,etc |
| 57 | reference model | 51 | 17 | 3.125 | 0.001819 | 1710.10987,1710.02084,etc |
| 58 | water vapor | 62 | 11 | 6.0 | 0.001798 | 1710.03134,1710.04707,etc |
| 59 | X-ray light curve | 34 | 13 | 2.667 | 0.001788 | 1710.06992,1710.02456,etc |
| 60 | type I | 65 | 14 | 4.923 | 0.001771 | 1710.05448,1710.08935,etc |
| 61 | large angular scale | 45 | 20 | 2.316 | 0.00177 | 1710.10987,1710.07652,etc |
| 62 | low mass end | 42 | 14 | 3.154 | 0.001762 | 1710.07637,1710.05029,etc |
| 63 | energy scale | 87 | 30 | 2.966 | 0.001738 | 1710.08342,1710.05413,etc |
| 64 | massive progenitor | 29 | 14 | 2.154 | 0.001738 | 1710.04712,1710.08421,etc |
| 65 | seed photon | 57 | 16 | 3.667 | 0.00173 | 1710.01748,1710.09910,etc |
| 66 | magnetic field strength | 266 | 99 | 2.704 | 0.001723 | 1710.09227,1710.04712,etc |
| 67 | expansion history | 74 | 26 | 2.84 | 0.001703 | 1710.05877,1710.08875,etc |
| 68 | Galactic centre | 43 | 19 | 2.278 | 0.001702 | 1710.08927,1710.10937,etc |
| 69 | model selection | 32 | 15 | 2.214 | 0.001697 | 1710.02947,1710.09808,etc |
| 70 | control sample | 53 | 15 | 3.714 | 0.001696 | 1710.04224,1710.10843,etc |
| 71 | coherent oscillation | 29 | 12 | 2.364 | 0.001691 | 1710.09198,1710.05606,etc |
| 72 | baryonic mass | 56 | 23 | 2.5 | 0.001688 | 1710.09380,1710.05834,etc |
| 73 | protoplanetary disc | 60 | 11 | 5.8 | 0.001682 | 1710.10863,1710.07846,etc |
| 74 | Gaia DR1 | 25 | 12 | 2.182 | 0.001672 | 1710.08875,1710.11625,etc |
| 75 | paper I | 76 | 21 | 3.75 | 0.001665 | 1710.00142,1710.09604,etc |
| 76 | lensed image | 36 | 11 | 3.5 | 0.001648 | 1710.02947,1710.05029,etc |
| 77 | reaction rate | 65 | 17 | 3.438 | 0.001641 | 1710.04712,1710.04254,etc |
| 78 | chemical model | 40 | 13 | 3.25 | 0.001633 | 1710.09380,1710.02993,etc |
| 79 | source model | 39 | 14 | 2.846 | 0.001628 | 1710.05049,1710.05029,etc |
| 80 | dark matter particle | 68 | 34 | 2.03 | 0.001625 | 1710.09380,1710.06170,etc |
| 81 | gas fraction | 155 | 39 | 3.605 | 0.00162 | 1710.09380,1710.01569,etc |
| 82 | high-mass star | 60 | 28 | 2.185 | 0.001614 | 1710.08564,1710.02364,etc |
| 83 | process element | 78 | 24 | 3.348 | 0.001612 | 1710.05865,1710.03544,etc |
| 84 | dark energy equation | 41 | 18 | 2.235 | 0.001604 | 1710.02947,1710.10876,etc |
| 85 | thin disc | 55 | 16 | 2.467 | 0.001599 | 1710.05635,1710.00415,etc |
| 86 | gas surface density | 60 | 23 | 2.5 | 0.001597 | 1710.10863,1710.01737,etc |
| 87 | Paper I | 265 | 37 | 7.111 | 0.001578 | 1710.01569,1710.03544,etc |
| 88 | mass outflow rate | 93 | 15 | 6.5 | 0.001573 | 1710.03230,1710.02525,etc |
| 89 | grid resolution | 52 | 16 | 3.4 | 0.001572 | 1710.08689,1710.10269,etc |
| 90 | dynamical ejecta | 143 | 29 | 4.893 | 0.001571 | 1710.00142,1710.05865,etc |
| 91 | opening angle | 186 | 57 | 3.179 | 0.001565 | 1710.03241,1710.05834,etc |
| 92 | Poynting flux | 72 | 15 | 5.071 | 0.00156 | 1710.05834,1710.02132,etc |
| 93 | massive particle | 31 | 12 | 2.545 | 0.001557 | 1710.05556,1710.06170,etc |
| 94 | instrumental noise | 63 | 17 | 3.875 | 0.001557 | 1710.07118,1710.01714,etc |
| 95 | massive star formation | 39 | 18 | 2.235 | 0.001551 | 1710.08564,1710.02456,etc |
| 96 | neutrino flux | 67 | 23 | 3.0 | 0.001542 | 1710.04712,1710.03020,etc |
| 97 | acceleration region | 54 | 16 | 3.533 | 0.001526 | 1710.09385,1710.11322,etc |
| 98 | galaxy center | 74 | 26 | 2.88 | 0.001517 | 1710.03241,1710.09590,etc |
| 99 | post-AGB star | 43 | 12 | 3.727 | 0.001516 | 1710.03730,1710.04368,etc |
| 100 | stellar core | 58 | 21 | 2.85 | 0.001511 | 1710.05504,1710.04712,etc |
|