| response function | 127 | 13 | 10.5 | 0.008917 | 1906.11272,1906.08266,etc |
| grain size distribution | 88 | 11 | 8.5 | 0.005541 | 1906.09277,1906.11308,etc |
| neutron star merger | 61 | 23 | 2.727 | 0.005212 | 1906.09647,1906.05002,etc |
| SNe Ia | 350 | 25 | 14.5 | 0.005069 | 1906.09040,1906.09980,etc |
| scalar spectral index | 29 | 12 | 2.455 | 0.004846 | 1906.11572,1906.11697,etc |
| flux tube | 82 | 12 | 7.182 | 0.004341 | 1906.02317,1906.03964,etc |
| surface mass density | 28 | 11 | 2.7 | 0.003378 | 1906.02209,1906.11728,etc |
| dust component | 45 | 11 | 4.4 | 0.003359 | 1906.03216,1906.06338,etc |
| Gaussian component | 126 | 17 | 7.562 | 0.003286 | 1906.06846,1906.11305,etc |
| debris disk | 59 | 11 | 5.8 | 0.003175 | 1906.04195,1906.11106,etc |
| quark matter | 74 | 11 | 7.3 | 0.003141 | 1906.00175,1906.10393,etc |
| multiple image | 122 | 12 | 10.455 | 0.003036 | 1906.11055,1906.05469,etc |
| gamma-ray emission | 76 | 18 | 4.412 | 0.003026 | 1906.10954,1906.09647,etc |
| primordial curvature perturbation | 34 | 12 | 3.0 | 0.00298 | 1906.00721,1906.01336,etc |
| overdense region | 73 | 16 | 4.533 | 0.002863 | 1906.04298,1906.07959,etc |
| radiative efficiency | 66 | 20 | 3.421 | 0.002831 | 1906.05865,1906.10130,etc |
| Paper I | 193 | 26 | 7.52 | 0.002739 | 1906.10630,1906.05155,etc |
| inflaton field | 79 | 20 | 4.105 | 0.002728 | 1906.01336,1906.09648,etc |
| dark matter mass | 57 | 16 | 3.733 | 0.0027 | 1906.08327,1906.10739,etc |
| astrophysical neutrino | 32 | 13 | 2.5 | 0.002611 | 1906.07209,1906.07419,etc |
| frequency bin | 44 | 12 | 2.273 | 0.002543 | 1906.07750,1906.00153,etc |
| effective mass | 141 | 27 | 5.346 | 0.002453 | 1906.09475,1906.00967,etc |
| fiducial cosmology | 64 | 14 | 4.769 | 0.002399 | 1906.01018,1906.04730,etc |
| fitting formula | 83 | 30 | 2.828 | 0.00238 | 1906.10690,1906.04730,etc |
| hard state | 46 | 12 | 3.091 | 0.002331 | 1906.10960,1906.01000,etc |
| particle size | 55 | 14 | 3.923 | 0.00231 | 1906.04265,1906.11400,etc |
| Planck scale | 70 | 22 | 3.286 | 0.002308 | 1906.11572,1906.00721,etc |
| dark matter particle | 154 | 51 | 3.06 | 0.002297 | 1906.05920,1906.09277,etc |
| black hole mass | 222 | 55 | 4.093 | 0.002217 | 1906.05865,1906.10130,etc |
| microlensing event | 73 | 11 | 7.1 | 0.002205 | 1906.11268,1906.08264,etc |
| sample star | 67 | 17 | 4.125 | 0.002196 | 1906.04195,1906.11911,etc |
| tensor-to-scalar ratio | 64 | 18 | 3.647 | 0.002156 | 1906.11572,1906.01336,etc |
| neural network | 67 | 19 | 3.5 | 0.002141 | 1906.10425,1906.08826,etc |
| gamma ray | 78 | 32 | 2.419 | 0.002018 | 1906.10954,1906.00357,etc |
| relic abundance | 52 | 15 | 3.5 | 0.002013 | 1906.09269,1906.00967,etc |
| dark matter density | 70 | 21 | 3.45 | 0.001999 | 1906.10690,1906.08749,etc |
| basis function | 51 | 11 | 4.2 | 0.001979 | 1906.10421,1906.05285,etc |
| dust-to-gas ratio | 89 | 13 | 7.333 | 0.001972 | 1906.11491,1906.09277,etc |
| soft state | 37 | 11 | 2.5 | 0.001967 | 1906.10960,1906.01000,etc |
| size distribution | 89 | 30 | 3.034 | 0.001965 | 1906.05804,1906.11308,etc |
| power law slope | 35 | 13 | 2.833 | 0.001942 | 1906.09656,1906.03493,etc |
| linear matter power spectrum | 42 | 15 | 2.786 | 0.001939 | 1906.01018,1906.08680,etc |
| denser region | 31 | 14 | 2.308 | 0.001874 | 1906.08327,1906.06846,etc |
| two-point correlation function | 42 | 21 | 2.05 | 0.001859 | 1906.04298,1906.00516,etc |
| detection rate | 89 | 27 | 3.385 | 0.001846 | 1906.02209,1906.07376,etc |
| keV band | 26 | 11 | 2.4 | 0.001812 | 1906.04744,1906.01964,etc |
| dark sector | 86 | 24 | 3.652 | 0.0018 | 1906.04989,1906.09269,etc |
| magnetic field structure | 24 | 12 | 2.091 | 0.0018 | 1906.10650,1906.09782,etc |
| single power law | 45 | 18 | 2.529 | 0.001795 | 1906.03493,1906.02519,etc |
| outflowing gas | 43 | 12 | 3.818 | 0.001785 | 1906.05865,1906.07364,etc |
| planetary mass | 45 | 16 | 2.867 | 0.001782 | 1906.05254,1906.11491,etc |
| neutrino luminosity | 64 | 13 | 5.083 | 0.001778 | 1906.05002,1906.08787,etc |
| toy model | 60 | 28 | 2.185 | 0.001765 | 1906.10421,1906.10690,etc |
| hot Jupiters | 88 | 15 | 6.214 | 0.001751 | 1906.05254,1906.11491,etc |
| matter power spectrum | 118 | 29 | 4.143 | 0.001747 | 1906.00968,1906.04730,etc |
| tidal field | 36 | 13 | 2.917 | 0.001717 | 1906.10690,1906.03264,etc |
| energy resolution | 71 | 23 | 3.182 | 0.001716 | 1906.08037,1906.05002,etc |
| disk mass | 35 | 15 | 2.429 | 0.001699 | 1906.01237,1906.03266,etc |
| dust particle | 74 | 23 | 3.318 | 0.001688 | 1906.11491,1906.07111,etc |
| scalar-tensor theory | 26 | 12 | 2.182 | 0.001684 | 1906.12333,1906.10791,etc |
| dark matter distribution | 33 | 15 | 2.143 | 0.001682 | 1906.10421,1906.03264,etc |
| nuclear region | 72 | 19 | 3.944 | 0.001677 | 1906.09656,1906.06638,etc |
| central galaxy | 131 | 29 | 4.25 | 0.00166 | 1906.03272,1906.04298,etc |
| dynamical system | 39 | 16 | 2.533 | 0.001651 | 1906.04482,1906.06306,etc |
| halo mass | 286 | 63 | 4.565 | 0.001632 | 1906.02209,1906.06955,etc |
| abundance pattern | 78 | 15 | 5.214 | 0.001623 | 1906.04195,1906.09137,etc |
| sequence star | 84 | 18 | 4.882 | 0.001613 | 1906.01066,1906.08788,etc |
| water vapor | 36 | 11 | 3.5 | 0.001608 | 1906.07111,1906.02820,etc |
| fitting function | 43 | 21 | 2.1 | 0.001602 | 1906.10690,1906.00968,etc |
| metal-poor star | 93 | 21 | 4.5 | 0.001542 | 1906.05653,1906.01072,etc |
| gas component | 66 | 19 | 3.611 | 0.001539 | 1906.04265,1906.04744,etc |
| light ray | 43 | 13 | 3.5 | 0.001525 | 1906.05920,1906.09040,etc |
| local measurement | 31 | 13 | 2.5 | 0.001511 | 1906.11697,1906.11814,etc |
| early-type galaxy | 71 | 28 | 2.556 | 0.00151 | 1906.04744,1906.01237,etc |
| explosion energy | 88 | 21 | 4.35 | 0.001503 | 1906.07249,1906.03493,etc |
| rotation velocity | 70 | 27 | 2.5 | 0.001498 | 1906.01201,1906.06245,etc |
| ray emission | 74 | 24 | 3.087 | 0.001491 | 1906.06055,1906.03493,etc |
| primary mass | 68 | 17 | 3.938 | 0.001481 | 1906.08219,1906.09251,etc |
| dust mass | 131 | 26 | 5.2 | 0.001461 | 1906.09277,1906.03216,etc |
| median redshift | 27 | 11 | 2.6 | 0.001444 | 1906.00008,1906.04707,etc |
| radiative loss | 57 | 15 | 4.0 | 0.001441 | 1906.02317,1906.01746,etc |
| stellar velocity dispersion | 67 | 24 | 2.87 | 0.001436 | 1906.02209,1906.08779,etc |
| mass-loss rate | 147 | 26 | 5.84 | 0.001434 | 1906.03189,1906.01066,etc |
| protoplanetary disc | 52 | 15 | 3.643 | 0.0014 | 1906.11491,1906.08219,etc |
| donor star | 85 | 17 | 5.188 | 0.001397 | 1906.07767,1906.06055,etc |
| progenitor system | 37 | 12 | 3.273 | 0.001392 | 1906.00812,1906.08749,etc |
| stellar variability | 52 | 17 | 3.125 | 0.001392 | 1906.11911,1906.02820,etc |
| mass growth | 37 | 12 | 2.455 | 0.001367 | 1906.10130,1906.00967,etc |
| gas phase | 160 | 38 | 4.27 | 0.001357 | 1906.09656,1906.08779,etc |
| neutrino event | 44 | 11 | 3.5 | 0.001352 | 1906.07209,1906.07419,etc |
| maximum light | 40 | 13 | 3.167 | 0.001344 | 1906.00812,1906.02023,etc |
| bimodal distribution | 27 | 13 | 2.167 | 0.001344 | 1906.01647,1906.04197,etc |
| gas mass | 197 | 58 | 3.368 | 0.001342 | 1906.07804,1906.11491,etc |
| thin disc | 52 | 15 | 3.643 | 0.00134 | 1906.09853,1906.08187,etc |
| high-energy neutrino | 40 | 14 | 3.0 | 0.001336 | 1906.07209,1906.07419,etc |
| self-similar solution | 49 | 11 | 4.0 | 0.001333 | 1906.09420,1906.11830,etc |
| magnetic field strength | 172 | 59 | 2.879 | 0.001328 | 1906.06570,1906.03189,etc |
| small radius | 87 | 34 | 2.606 | 0.001326 | 1906.05865,1906.10421,etc |
| primordial power spectrum | 39 | 18 | 2.118 | 0.001321 | 1906.04730,1906.01421,etc |
| progenitor mass | 56 | 16 | 3.333 | 0.00132 | 1906.00812,1906.04727,etc |
|