| nebular emission | 104 | 15 | 7.357 | 0.007515 | 1310.5809,1310.3917,etc |
| radiative efficiency | 107 | 16 | 7.067 | 0.005238 | 1310.0313,1310.4317,etc |
| stellar core | 103 | 14 | 7.846 | 0.004389 | 1310.3198,1310.0049,etc |
| thick disc | 89 | 11 | 8.8 | 0.00432 | 1310.6939,1310.5145,etc |
| distant observer | 48 | 11 | 4.7 | 0.004086 | 1310.4869,1310.8376,etc |
| hard state | 89 | 20 | 3.947 | 0.003959 | 1310.6939,1310.3037,etc |
| neutrino mass | 109 | 15 | 7.714 | 0.003899 | 1310.8642,1310.1859,etc |
| high energy emission | 35 | 15 | 2.429 | 0.003844 | 1310.1837,1310.6318,etc |
| dust attenuation | 138 | 16 | 9.133 | 0.003787 | 1310.3497,1310.7388,etc |
| soft state | 65 | 18 | 3.235 | 0.003572 | 1310.3037,1310.1186,etc |
| Sgr A* | 91 | 11 | 8.9 | 0.003222 | 1310.7022,1310.8177,etc |
| SNe Ia | 170 | 19 | 9.056 | 0.003082 | 1310.5188,1310.4184,etc |
| thermal conduction | 82 | 20 | 4.263 | 0.003062 | 1310.4286,1310.2940,etc |
| magnetic field vector | 24 | 11 | 2.3 | 0.003057 | 1310.0257,1310.1823,etc |
| dark matter mass | 51 | 19 | 2.778 | 0.003012 | 1310.2938,1310.3280,etc |
| total stellar mass | 115 | 30 | 3.931 | 0.002982 | 1310.3819,1310.2938,etc |
| Fe abundance | 42 | 12 | 3.636 | 0.002964 | 1310.3270,1310.2461,etc |
| nonumber && | 87 | 24 | 3.739 | 0.002911 | 1310.8177,1310.3021,etc |
| mass accretion rate | 182 | 51 | 3.52 | 0.002833 | 1310.6318,1310.6939,etc |
| water vapor | 73 | 12 | 3.273 | 0.00282 | 1310.7030,1310.4286,etc |
| stellar disc | 56 | 16 | 3.667 | 0.002719 | 1310.5562,1310.7022,etc |
| jet power | 61 | 13 | 5.0 | 0.002595 | 1310.0462,1310.5450,etc |
| large separation | 90 | 21 | 4.45 | 0.002587 | 1310.8178,1310.5048,etc |
| radio continuum emission | 31 | 11 | 2.5 | 0.00253 | 1310.8229,1310.8144,etc |
| mass-to-light ratio | 79 | 31 | 2.567 | 0.002524 | 1310.5867,1310.2389,etc |
| outer disk | 177 | 33 | 5.5 | 0.002424 | 1310.5069,1310.0044,etc |
| open field line | 35 | 11 | 3.4 | 0.002392 | 1310.7012,1310.1134,etc |
| early-type star | 47 | 12 | 4.182 | 0.002287 | 1310.2209,1310.6616,etc |
| low-mass star | 142 | 60 | 2.356 | 0.002284 | 1310.0175,1310.1017,etc |
| gas giant | 80 | 12 | 7.182 | 0.002225 | 1310.8581,1310.7800,etc |
| refractory element | 27 | 12 | 2.273 | 0.002214 | 1310.6297,1310.2596,etc |
| primordial non-Gaussianity | 66 | 13 | 5.333 | 0.002205 | 1310.8617,1310.7023,etc |
| abundance pattern | 85 | 20 | 4.368 | 0.002174 | 1310.3276,1310.6373,etc |
| cold gas | 253 | 51 | 5.04 | 0.002163 | 1310.7572,1310.6616,etc |
| dust formation | 53 | 16 | 3.467 | 0.002156 | 1310.3034,1310.3497,etc |
| spiral density wave | 29 | 12 | 2.545 | 0.002132 | 1310.2852,1310.6697,etc |
| Einstein frame | 103 | 16 | 6.533 | 0.00213 | 1310.6743,1310.5058,etc |
| velocity shift | 95 | 13 | 5.917 | 0.002124 | 1310.3074,1310.8297,etc |
| dark sector | 86 | 19 | 4.556 | 0.002116 | 1310.8642,1310.3278,etc |
| grain size distribution | 45 | 14 | 3.077 | 0.002097 | 1310.4679,1310.2600,etc |
| flux tube | 66 | 20 | 3.368 | 0.002089 | 1310.7756,1310.5940,etc |
| best-fitting model | 102 | 29 | 2.607 | 0.00208 | 1310.2966,1310.7101,etc |
| recent star formation | 53 | 21 | 2.6 | 0.00207 | 1310.5693,1310.5424,etc |
| X-ray flare | 31 | 12 | 2.545 | 0.00206 | 1310.0487,1310.1367,etc |
| post-AGB star | 47 | 12 | 4.182 | 0.002054 | 1310.7711,1310.3142,etc |
| source spectrum | 48 | 22 | 2.19 | 0.002035 | 1310.1248,1310.8355,etc |
| black hole mass | 216 | 56 | 3.909 | 0.002017 | 1310.7022,1310.7936,etc |
| direct detection experiment | 38 | 12 | 3.364 | 0.002006 | 1310.8642,1310.5718,etc |
| toroidal field | 61 | 17 | 2.375 | 0.001955 | 1310.5562,1310.8178,etc |
| neutrino flux | 68 | 18 | 3.941 | 0.001882 | 1310.8642,1310.7488,etc |
| absorption system | 51 | 13 | 3.333 | 0.001845 | 1310.8297,1310.5859,etc |
| metal-poor star | 118 | 23 | 4.864 | 0.00183 | 1310.3276,1310.0011,etc |
| upper mass limit | 25 | 12 | 2.182 | 0.001823 | 1310.4497,1310.2255,etc |
| ray source | 40 | 13 | 3.083 | 0.00182 | 1310.1837,1310.1565,etc |
| poloidal field | 64 | 14 | 4.846 | 0.001811 | 1310.5562,1310.7012,etc |
| planet radius | 44 | 13 | 3.333 | 0.001804 | 1310.7942,1310.7952,etc |
| dark energy equation | 32 | 12 | 2.727 | 0.001793 | 1310.7517,1310.0085,etc |
| effective mass | 48 | 16 | 3.133 | 0.00179 | 1310.3742,1310.5627,etc |
| band light curve | 52 | 16 | 3.0 | 0.001785 | 1310.7630,1310.6579,etc |
| microlensing event | 48 | 13 | 3.833 | 0.001785 | 1310.6579,1310.4824,etc |
| velocity amplitude | 37 | 12 | 3.273 | 0.00178 | 1310.2209,1310.6743,etc |
| magnetic field line | 209 | 69 | 3.044 | 0.001762 | 1310.7756,1310.0257,etc |
| binary separation | 47 | 15 | 2.643 | 0.001747 | 1310.0487,1310.0627,etc |
| Jordan frame | 73 | 14 | 5.538 | 0.001746 | 1310.6743,1310.3950,etc |
| hot dust | 62 | 12 | 5.545 | 0.001742 | 1310.3034,1310.7711,etc |
| peak intensity | 63 | 22 | 2.952 | 0.001728 | 1310.7017,1310.0257,etc |
| two-point correlation function | 52 | 21 | 2.55 | 0.001722 | 1310.7388,1310.1605,etc |
| Sun-like star | 53 | 23 | 2.364 | 0.001719 | 1310.5562,1310.7952,etc |
| fundamental parameter | 66 | 33 | 2.031 | 0.001719 | 1310.2966,1310.1017,etc |
| accretion rate | 339 | 103 | 3.314 | 0.001716 | 1310.6318,1310.4728,etc |
| oxygen abundance | 116 | 29 | 4.107 | 0.001705 | 1310.7020,1310.2253,etc |
| false positive | 70 | 18 | 3.882 | 0.001669 | 1310.4207,1310.5048,etc |
| Kepler datum | 48 | 13 | 3.833 | 0.001666 | 1310.3019,1310.5048,etc |
| phase speed | 42 | 13 | 3.417 | 0.001643 | 1310.2135,1310.7939,etc |
| radiative transfer model | 36 | 17 | 2.125 | 0.001642 | 1310.0487,1310.3074,etc |
| hot gas | 113 | 44 | 2.558 | 0.001641 | 1310.7017,1310.2253,etc |
| halo gas | 28 | 11 | 2.7 | 0.001626 | 1310.5711,1310.7944,etc |
| ejecta mass | 36 | 12 | 3.182 | 0.001624 | 1310.2950,1310.6356,etc |
| photometric variability | 55 | 19 | 3.0 | 0.001608 | 1310.3034,1310.1367,etc |
| local value | 35 | 16 | 2.267 | 0.001597 | 1310.0535,1310.7012,etc |
| detection rate | 61 | 27 | 2.308 | 0.001579 | 1310.3819,1310.7711,etc |
| point function | 62 | 11 | 3.0 | 0.001567 | 1310.8133,1310.8617,etc |
| short orbital period | 38 | 15 | 2.643 | 0.001563 | 1310.2209,1310.4037,etc |
| inflaton field | 27 | 11 | 2.6 | 0.001552 | 1310.4988,1310.3950,etc |
| gas phase | 119 | 36 | 3.286 | 0.001542 | 1310.4679,1310.0011,etc |
| mass-loss rate | 140 | 35 | 4.059 | 0.001535 | 1310.0449,1310.0487,etc |
| bulk Lorentz factor | 58 | 19 | 3.167 | 0.00153 | 1310.2481,1310.4893,etc |
| time variation | 76 | 30 | 2.586 | 0.001525 | 1310.8177,1310.8150,etc |
| grain growth | 60 | 13 | 4.917 | 0.001524 | 1310.4679,1310.5154,etc |
| pulsar magnetosphere | 41 | 12 | 3.636 | 0.00152 | 1310.2531,1310.1823,etc |
| contact discontinuity | 44 | 14 | 2.769 | 0.001511 | 1310.0487,1310.2481,etc |
| cluster mass | 122 | 34 | 3.636 | 0.001506 | 1310.2938,1310.3142,etc |
| disk wind | 46 | 16 | 3.0 | 0.001502 | 1310.6318,1310.6745,etc |
| Paper I | 298 | 34 | 9.0 | 0.001497 | 1310.4207,1310.1336,etc |
| body simulation | 168 | 38 | 4.216 | 0.001495 | 1310.3280,1310.3631,etc |
| energy bin | 63 | 21 | 3.05 | 0.001492 | 1310.6093,1310.5718,etc |
| large angular scale | 24 | 11 | 2.2 | 0.00149 | 1310.0469,1310.2989,etc |
| preferred direction | 29 | 14 | 2.154 | 0.001485 | 1310.8150,1310.1513,etc |
| activity cycle | 22 | 11 | 2.1 | 0.001472 | 1310.5562,1310.8178,etc |
| hot Jupiters | 87 | 20 | 4.158 | 0.001469 | 1310.7952,1310.5048,etc |
|