| flux rope | 180 | 19 | 9.278 | 0.004011 | 2103.01213,2103.02352,etc |
| Hubble tension | 267 | 21 | 13.0 | 0.004006 | 2103.00248,2103.00943,etc |
| structure function | 114 | 17 | 6.938 | 0.003779 | 2103.01424,2103.01839,etc |
| flux tube | 87 | 18 | 5.059 | 0.003432 | 2103.00374,2103.01993,etc |
| variability amplitude | 84 | 21 | 4.15 | 0.003395 | 2103.01233,2103.01424,etc |
| line list | 120 | 17 | 5.938 | 0.003018 | 2103.01246,2103.01601,etc |
| false alarm probability | 32 | 12 | 2.818 | 0.002995 | 2103.00062,2103.01641,etc |
| tidal field | 100 | 16 | 5.667 | 0.002964 | 2103.00730,2103.01522,etc |
| background event | 63 | 25 | 2.583 | 0.002906 | 2103.01175,2103.02161,etc |
| multi-planet system | 43 | 13 | 3.5 | 0.002826 | 2103.01239,2103.01974,etc |
| ray spectrum | 34 | 13 | 2.75 | 0.002793 | 2103.00727,2103.01557,etc |
| SNe Ia | 171 | 25 | 7.0 | 0.002788 | 2103.01923,2103.02117,etc |
| starless core | 108 | 11 | 10.5 | 0.002779 | 2103.03324,2103.03499,etc |
| third body | 37 | 12 | 3.273 | 0.002722 | 2103.00062,2103.00568,etc |
| scale parameter | 42 | 11 | 4.1 | 0.002605 | 2103.00292,2103.02988,etc |
| quasar sample | 58 | 15 | 3.929 | 0.002533 | 2103.01277,2103.01424,etc |
| mass-loss rate | 371 | 39 | 9.053 | 0.002516 | 2103.01227,2103.01317,etc |
| primordial power spectrum | 55 | 20 | 2.526 | 0.002513 | 2103.01056,2103.01183,etc |
| magnetic field strength | 339 | 95 | 3.564 | 0.002512 | 2103.00267,2103.00332,etc |
| gas disc | 86 | 14 | 6.538 | 0.00251 | 2103.00016,2103.01236,etc |
| Einstein frame | 75 | 13 | 5.75 | 0.002479 | 2103.06855,2103.10890,etc |
| quantum mechanic | 53 | 14 | 4.0 | 0.002478 | 2103.02797,2103.03824,etc |
| Gaia datum | 44 | 14 | 3.308 | 0.002447 | 2103.00196,2103.01142,etc |
| reaction rate | 128 | 22 | 5.81 | 0.002442 | 2103.03760,2103.03810,etc |
| time-averaged spectrum | 44 | 11 | 4.2 | 0.002415 | 2103.02558,2103.04994,etc |
| chemical model | 48 | 18 | 2.765 | 0.002341 | 2103.01125,2103.02666,etc |
| metal-poor star | 93 | 22 | 3.81 | 0.002335 | 2103.00568,2103.01643,etc |
| telluric absorption | 42 | 18 | 2.412 | 0.002312 | 2103.01336,2103.01699,etc |
| massive star formation | 38 | 13 | 2.75 | 0.002298 | 2103.01635,2103.02531,etc |
| outer disc | 84 | 21 | 3.0 | 0.00227 | 2103.00211,2103.01236,etc |
| dust mass | 222 | 33 | 5.938 | 0.002259 | 2103.01236,2103.02610,etc |
| Advanced LIGO | 63 | 19 | 3.444 | 0.002238 | 2103.00826,2103.01641,etc |
| band light curve | 62 | 20 | 2.526 | 0.002199 | 2103.01557,2103.02005,etc |
| ray emission | 87 | 23 | 3.909 | 0.002171 | 2103.00292,2103.00727,etc |
| halo mass | 437 | 67 | 6.606 | 0.002132 | 2103.01227,2103.01231,etc |
| main peak | 50 | 15 | 3.5 | 0.002122 | 2103.00292,2103.01952,etc |
| Alfv'en wave | 58 | 12 | 5.182 | 0.002099 | 2103.00470,2103.01993,etc |
| nonumber && | 62 | 14 | 2.385 | 0.002077 | 2103.03627,2103.11756,etc |
| paper I | 113 | 21 | 5.4 | 0.002055 | 2103.00478,2103.01233,etc |
| second peak | 63 | 24 | 2.652 | 0.002046 | 2103.00995,2103.01968,etc |
| wind speed | 76 | 18 | 4.353 | 0.002029 | 2103.04740,2103.05263,etc |
| iron line | 62 | 17 | 3.812 | 0.002022 | 2103.02422,2103.03880,etc |
| baryonic mass | 62 | 21 | 3.05 | 0.002015 | 2103.00211,2103.01072,etc |
| exponential growth | 42 | 18 | 2.412 | 0.002014 | 2103.00470,2103.01016,etc |
| direct method | 76 | 14 | 5.538 | 0.001986 | 2103.01505,2103.01514,etc |
| photospheric radius | 66 | 11 | 6.4 | 0.001977 | 2103.01336,2103.02461,etc |
| relic density | 81 | 17 | 5.0 | 0.001974 | 2103.02161,2103.06303,etc |
| thermal model | 68 | 11 | 2.2 | 0.001965 | 2103.01989,2103.02612,etc |
| external magnetic field | 50 | 15 | 3.5 | 0.001943 | 2103.00470,2103.00656,etc |
| event rate | 91 | 24 | 3.348 | 0.001936 | 2103.00943,2103.01175,etc |
| hard state | 84 | 11 | 8.3 | 0.00192 | 2103.02178,2103.04601,etc |
| effective mass | 55 | 24 | 2.304 | 0.001884 | 2103.00248,2103.00470,etc |
| gas fraction | 108 | 20 | 5.632 | 0.001883 | 2103.00012,2103.01295,etc |
| ray source | 39 | 15 | 2.714 | 0.001864 | 2103.00292,2103.01557,etc |
| explosion energy | 72 | 19 | 3.944 | 0.00186 | 2103.01336,2103.01814,etc |
| Fe K line | 55 | 14 | 4.077 | 0.001851 | 2103.00012,2103.02612,etc |
| planet candidate | 114 | 12 | 10.182 | 0.001828 | 2103.01016,2103.02709,etc |
| triple system | 59 | 18 | 3.412 | 0.001823 | 2103.00568,2103.01963,etc |
| correlated noise | 49 | 18 | 2.824 | 0.001796 | 2103.01016,2103.03644,etc |
| optical band | 110 | 42 | 2.634 | 0.001794 | 2103.00004,2103.00999,etc |
| magnetic structure | 70 | 23 | 2.591 | 0.001783 | 2103.00478,2103.01583,etc |
| external source | 34 | 11 | 3.3 | 0.00177 | 2103.02666,2103.03950,etc |
| stationary solution | 33 | 13 | 2.583 | 0.001753 | 2103.05119,2103.05279,etc |
| mass accretion rate | 183 | 59 | 3.138 | 0.001742 | 2103.00267,2103.00828,etc |
| galaxy number density | 24 | 11 | 2.3 | 0.001727 | 2103.01229,2103.01964,etc |
| transmission spectrum | 139 | 19 | 6.944 | 0.001713 | 2103.03822,2103.04342,etc |
| dust model | 58 | 16 | 3.8 | 0.001709 | 2103.00666,2103.01245,etc |
| synthetic image | 36 | 13 | 2.917 | 0.001693 | 2103.01753,2103.02665,etc |
| first peak | 33 | 13 | 2.667 | 0.001692 | 2103.01229,2103.01336,etc |
| key quantity | 47 | 13 | 3.833 | 0.001678 | 2103.00374,2103.01183,etc |
| outer disk | 193 | 41 | 3.4 | 0.001674 | 2103.00292,2103.01142,etc |
| Kerr solution | 24 | 11 | 2.3 | 0.001674 | 2103.03160,2103.07593,etc |
| black hole solution | 39 | 12 | 3.455 | 0.001657 | 2103.03160,2103.00108,etc |
| surface abundance | 49 | 11 | 4.8 | 0.001653 | 2103.01741,2103.02609,etc |
| lensed image | 37 | 11 | 3.6 | 0.001649 | 2103.01183,2103.03257,etc |
| geometric albedo | 40 | 12 | 2.909 | 0.001649 | 2103.02673,2103.06275,etc |
| control sample | 105 | 21 | 3.45 | 0.001638 | 2103.00666,2103.00999,etc |
| core mass | 66 | 23 | 2.864 | 0.001615 | 2103.01239,2103.01316,etc |
| spectral synthesis | 63 | 14 | 4.692 | 0.00161 | 2103.02041,2103.03880,etc |
| star particle | 77 | 18 | 4.294 | 0.001589 | 2103.01962,2103.02234,etc |
| Gaussian process | 65 | 23 | 2.818 | 0.001574 | 2103.00010,2103.00138,etc |
| mode frequency | 51 | 12 | 4.545 | 0.001573 | 2103.02499,2103.04713,etc |
| peak frequency | 58 | 16 | 3.667 | 0.00157 | 2103.00292,2103.03225,etc |
| integration constant | 38 | 18 | 2.118 | 0.001565 | 2103.01965,2103.07252,etc |
| massive particle | 41 | 14 | 3.077 | 0.001562 | 2103.01797,2103.08978,etc |
| bulk density | 42 | 16 | 2.733 | 0.00155 | 2103.01016,2103.01504,etc |
| gamma-ray emission | 49 | 14 | 3.538 | 0.001547 | 2103.01536,2103.01787,etc |
| line-of-sight velocity | 68 | 24 | 2.913 | 0.001536 | 2103.00211,2103.00248,etc |
| short GRBs | 85 | 21 | 4.2 | 0.001506 | 2103.00943,2103.01881,etc |
| boson star | 33 | 11 | 3.2 | 0.001498 | 2103.00818,2103.12342,etc |
| stellar rotation period | 53 | 13 | 2.5 | 0.001492 | 2103.01016,2103.01246,etc |
| gas temperature | 131 | 53 | 2.481 | 0.001475 | 2103.01042,2103.02234,etc |
| tensor-to-scalar ratio | 66 | 21 | 3.25 | 0.001473 | 2103.01183,2103.01797,etc |
| inner disc | 71 | 18 | 3.059 | 0.001471 | 2103.00017,2103.00211,etc |
| Eddington ratio | 126 | 31 | 4.133 | 0.001469 | 2103.00014,2103.00999,etc |
| hydrogen column density | 58 | 27 | 2.192 | 0.001461 | 2103.00017,2103.00332,etc |
| neutrino flux | 64 | 15 | 3.857 | 0.001449 | 2103.00789,2103.01274,etc |
| Gaussian model | 29 | 11 | 2.8 | 0.001438 | 2103.05371,2103.07204,etc |
| Paper I | 318 | 37 | 8.361 | 0.001434 | 2103.00036,2103.00666,etc |
| accretion rate | 469 | 128 | 3.685 | 0.001432 | 2103.00017,2103.00267,etc |
|