| thick disc | 56 | 11 | 5.5 | 0.007868 | 2101.01187,2101.01360,etc |
| flux rope | 366 | 22 | 17.095 | 0.005438 | 2101.00011,2101.01020,etc |
| gravitational wave observation | 26 | 13 | 2.083 | 0.005417 | 2101.02217,2101.05144,etc |
| grain size distribution | 116 | 12 | 10.273 | 0.004827 | 2101.01012,2101.01182,etc |
| secondary peak | 77 | 15 | 5.357 | 0.004377 | 2101.00248,2101.02290,etc |
| thermal conduction | 126 | 17 | 7.812 | 0.004115 | 2101.01019,2101.01020,etc |
| SNe Ia | 273 | 20 | 13.105 | 0.004049 | 2101.00283,2101.02407,etc |
| Sun-like star | 59 | 21 | 2.25 | 0.003445 | 2101.00663,2101.02043,etc |
| reference image | 54 | 13 | 4.333 | 0.003401 | 2101.00800,2101.01293,etc |
| mass-loss rate | 256 | 33 | 7.969 | 0.003317 | 2101.00042,2101.00045,etc |
| Hubble tension | 49 | 15 | 3.429 | 0.00323 | 2101.01244,2101.01372,etc |
| scalar spectral index | 54 | 13 | 3.917 | 0.003181 | 2101.00825,2101.01684,etc |
| gas-phase metallicity | 114 | 15 | 7.5 | 0.003164 | 2101.01706,2101.02220,etc |
| flat CDM model | 36 | 12 | 3.0 | 0.003069 | 2101.02765,2101.02978,etc |
| tensor-to-scalar ratio | 108 | 28 | 3.815 | 0.002993 | 2101.00034,2101.00825,etc |
| Taylor expansion | 84 | 24 | 3.609 | 0.002969 | 2101.02156,2101.03074,etc |
| phase speed | 40 | 12 | 3.182 | 0.00294 | 2101.01220,2101.02241,etc |
| neutral fraction | 67 | 12 | 6.0 | 0.002816 | 2101.01205,2101.06273,etc |
| background model | 45 | 17 | 2.5 | 0.002528 | 2101.03105,2101.04188,etc |
| flux tube | 120 | 24 | 4.696 | 0.002506 | 2101.00273,2101.01019,etc |
| Gaia parallax | 57 | 11 | 5.6 | 0.002482 | 2101.01726,2101.02707,etc |
| energy resolution | 92 | 23 | 4.0 | 0.002464 | 2101.00696,2101.00815,etc |
| maximum mass | 119 | 35 | 3.441 | 0.00244 | 2101.00209,2101.00951,etc |
| thin disc | 34 | 15 | 2.286 | 0.002404 | 2101.00209,2101.00768,etc |
| matter power spectrum | 83 | 23 | 3.727 | 0.002388 | 2101.00298,2101.01198,etc |
| disk wind | 70 | 14 | 5.308 | 0.002356 | 2101.00899,2101.01596,etc |
| Doppler velocity | 88 | 12 | 5.818 | 0.002337 | 2101.00011,2101.00768,etc |
| mass accretion rate | 183 | 40 | 4.667 | 0.002319 | 2101.01194,2101.01198,etc |
| star-formation history | 60 | 15 | 4.143 | 0.002297 | 2101.01937,2101.02228,etc |
| transmission spectrum | 86 | 14 | 6.538 | 0.002293 | 2101.00042,2101.00045,etc |
| two-component model | 83 | 24 | 3.174 | 0.002271 | 2101.00013,2101.00372,etc |
| spectral slope | 79 | 21 | 3.85 | 0.002224 | 2101.00830,2101.01440,etc |
| energetic electron | 52 | 11 | 5.1 | 0.002222 | 2101.00189,2101.01526,etc |
| magnetic field strength | 337 | 116 | 2.922 | 0.002185 | 2101.00213,2101.00248,etc |
| ray emission | 149 | 23 | 6.727 | 0.002177 | 2101.02738,2101.02964,etc |
| black hole mass | 248 | 58 | 4.333 | 0.002172 | 2101.00209,2101.00502,etc |
| short GRBs | 85 | 11 | 8.2 | 0.002135 | 2101.03082,2101.03084,etc |
| dark energy equation | 44 | 16 | 2.867 | 0.002131 | 2101.01184,2101.01542,etc |
| radiative efficiency | 56 | 13 | 4.583 | 0.002117 | 2101.00209,2101.01219,etc |
| color code | 33 | 12 | 2.909 | 0.00207 | 2101.01183,2101.02890,etc |
| hard state | 87 | 13 | 7.083 | 0.002051 | 2101.01187,2101.01569,etc |
| Paper I | 155 | 16 | 8.267 | 0.002016 | 2101.00045,2101.00158,etc |
| mass-radius relation | 64 | 24 | 2.696 | 0.002016 | 2101.00663,2101.01183,etc |
| pebble accretion | 52 | 11 | 5.1 | 0.002011 | 2101.01331,2101.01728,etc |
| massive disk | 40 | 11 | 3.9 | 0.001961 | 2101.01728,2101.01888,etc |
| Earth-like planet | 66 | 16 | 4.0 | 0.00189 | 2101.00696,2101.01225,etc |
| orbital solution | 76 | 15 | 5.357 | 0.001885 | 2101.00663,2101.04232,etc |
| background field | 103 | 19 | 5.667 | 0.001879 | 2101.00830,2101.01478,etc |
| kick velocity | 44 | 12 | 3.364 | 0.001872 | 2101.03670,2101.05288,etc |
| electric field | 171 | 36 | 4.571 | 0.001869 | 2101.00011,2101.01343,etc |
| size distribution | 142 | 39 | 3.5 | 0.001865 | 2101.00032,2101.00273,etc |
| neural network | 145 | 34 | 4.364 | 0.001853 | 2101.00011,2101.00750,etc |
| central galaxy | 237 | 34 | 7.0 | 0.001848 | 2101.00113,2101.00844,etc |
| paper I | 68 | 13 | 5.5 | 0.001847 | 2101.00045,2101.00506,etc |
| cluster field | 35 | 13 | 2.833 | 0.001843 | 2101.01640,2101.01644,etc |
| gas fraction | 122 | 35 | 3.559 | 0.001833 | 2101.00209,2101.01729,etc |
| gamma-ray emission | 70 | 20 | 3.632 | 0.001813 | 2101.00372,2101.00610,etc |
| density gradient | 50 | 18 | 2.824 | 0.001796 | 2101.00639,2101.01349,etc |
| training sample | 66 | 14 | 4.923 | 0.00179 | 2101.02228,2101.02532,etc |
| lookback time | 41 | 11 | 3.6 | 0.001787 | 2101.01734,2101.04157,etc |
| donor star | 55 | 15 | 3.429 | 0.001774 | 2101.00815,2101.01967,etc |
| galactic outflow | 33 | 12 | 2.909 | 0.001764 | 2101.00032,2101.05016,etc |
| gas inflow | 34 | 13 | 2.75 | 0.001758 | 2101.01196,2101.01729,etc |
| dust-to-gas ratio | 107 | 20 | 5.579 | 0.001738 | 2101.01193,2101.01888,etc |
| source size | 75 | 24 | 3.174 | 0.001724 | 2101.00128,2101.00680,etc |
| redshift distribution | 128 | 43 | 3.0 | 0.001716 | 2101.00113,2101.00298,etc |
| number count | 98 | 25 | 4.042 | 0.001698 | 2101.01183,2101.01205,etc |
| first stage | 50 | 25 | 2.042 | 0.001697 | 2101.01019,2101.02290,etc |
| hardness ratio | 64 | 18 | 3.706 | 0.001695 | 2101.00724,2101.00815,etc |
| matter model | 32 | 13 | 2.5 | 0.001684 | 2101.00013,2101.01828,etc |
| hot Jupiters | 96 | 25 | 3.917 | 0.001684 | 2101.00045,2101.01470,etc |
| soft state | 75 | 13 | 6.167 | 0.001654 | 2101.00696,2101.01187,etc |
| star-forming region | 179 | 63 | 2.806 | 0.001639 | 2101.00248,2101.01182,etc |
| primordial magnetic field | 33 | 12 | 2.909 | 0.001637 | 2101.03644,2101.05284,etc |
| inner heliosphere | 24 | 12 | 2.091 | 0.00163 | 2101.00830,2101.01440,etc |
| density field | 169 | 41 | 4.175 | 0.001612 | 2101.00273,2101.00844,etc |
| new source | 49 | 15 | 3.429 | 0.001606 | 2101.01649,2101.02077,etc |
| disk surface | 55 | 13 | 4.417 | 0.001596 | 2101.00899,2101.01596,etc |
| quiescent state | 38 | 11 | 3.7 | 0.001588 | 2101.00042,2101.04692,etc |
| total stellar mass | 91 | 37 | 2.5 | 0.001588 | 2101.01219,2101.01522,etc |
| tidal field | 65 | 14 | 4.077 | 0.001568 | 2101.00951,2101.01455,etc |
| solar-like star | 34 | 11 | 3.3 | 0.001553 | 2101.00663,2101.04448,etc |
| polarization signal | 80 | 15 | 5.643 | 0.001549 | 2101.00034,2101.00506,etc |
| halo mass | 369 | 66 | 5.662 | 0.001541 | 2101.00113,2101.00253,etc |
| stellar effective temperature | 52 | 14 | 3.923 | 0.00153 | 2101.00750,2101.01202,etc |
| tidal deformability | 35 | 11 | 3.1 | 0.001526 | 2101.00951,2101.01201,etc |
| maximum light | 77 | 13 | 6.333 | 0.001521 | 2101.02738,2101.02756,etc |
| reference model | 42 | 16 | 2.733 | 0.001513 | 2101.00506,2101.00639,etc |
| dynamical system | 38 | 12 | 3.364 | 0.001507 | 2101.00402,2101.06652,etc |
| accretion rate | 385 | 95 | 4.085 | 0.001481 | 2101.00209,2101.00518,etc |
| Stokes profile | 59 | 12 | 4.636 | 0.001471 | 2101.00506,2101.00899,etc |
| plasma flow | 42 | 13 | 2.75 | 0.001469 | 2101.02065,2101.03768,etc |
| Bayesian analysis | 69 | 27 | 2.615 | 0.001465 | 2101.01201,2101.02043,etc |
| double peak | 22 | 11 | 2.1 | 0.001458 | 2101.02738,2101.02801,etc |
| body simulation | 166 | 40 | 4.154 | 0.001442 | 2101.00113,2101.01198,etc |
| group environment | 65 | 11 | 6.4 | 0.001441 | 2101.00032,2101.01734,etc |
| synthetic datum | 48 | 14 | 3.462 | 0.001432 | 2101.00011,2101.00034,etc |
| eccentricity distribution | 30 | 12 | 2.636 | 0.001416 | 2101.01202,2101.01360,etc |
| mass model | 61 | 16 | 4.0 | 0.001411 | 2101.01740,2101.01937,etc |
| bottom boundary | 39 | 13 | 2.417 | 0.001402 | 2101.01019,2101.01020,etc |
|