| self-similar solution | 33 | 11 | 2.9 | 0.004728 | 0303519,0303156,etc |
| two-point correlation function | 54 | 16 | 3.533 | 0.003617 | 0303382,0303668,etc |
| internal shock | 46 | 11 | 4.4 | 0.003472 | 0303288,0303339,etc |
| black hole mass | 117 | 26 | 4.52 | 0.003308 | 0303387,0303227,etc |
| dust temperature | 83 | 21 | 4.1 | 0.002673 | 0303004,0303216,etc |
| star formation history | 102 | 37 | 2.694 | 0.002646 | 0303240,0303166,etc |
| one-dimensional spectrum | 26 | 11 | 2.5 | 0.002591 | 0303102,0303234,etc |
| red galaxy | 76 | 11 | 5.4 | 0.002395 | 0303166,0303163,etc |
| central black hole | 84 | 27 | 3.192 | 0.002289 | 0303151,0303382,etc |
| early-type galaxy | 181 | 36 | 4.886 | 0.002246 | 0303387,0303382,etc |
| N-body simulation | 43 | 16 | 2.533 | 0.002168 | 0303558,0303555,etc |
| SNe Ia | 59 | 16 | 3.867 | 0.002158 | 0303176,0303101,etc |
| Paper I | 300 | 36 | 8.457 | 0.002106 | 0303387,0303014,etc |
| X-ray emission | 194 | 65 | 3.016 | 0.001873 | 0303387,0303382,etc |
| central surface brightness | 30 | 12 | 2.636 | 0.001841 | 0303293,0303292,etc |
| quintessence model | 42 | 12 | 3.727 | 0.001808 | 0303353,0303564,etc |
| spectral slope | 38 | 19 | 2.056 | 0.001711 | 0303558,0303591,etc |
| type Ia supernova | 37 | 15 | 2.571 | 0.0017 | 0303428,0303501,etc |
| accretion rate | 194 | 45 | 4.136 | 0.001694 | 0303375,0303456,etc |
| galaxy luminosity function | 33 | 15 | 2.214 | 0.001669 | 0303558,0303668,etc |
| mass-loss rate | 54 | 12 | 4.818 | 0.001645 | 0303456,0303026,etc |
| high velocity | 32 | 13 | 2.5 | 0.001642 | 0303456,0303586,etc |
| magnetic field structure | 24 | 11 | 2.3 | 0.001636 | 0303644,0303157,etc |
| cold gas | 41 | 15 | 2.786 | 0.001588 | 0303257,0303525,etc |
| old population | 59 | 13 | 4.833 | 0.001574 | 0303325,0303487,etc |
| star-forming galaxy | 68 | 26 | 2.68 | 0.001558 | 0303302,0303166,etc |
| late-type galaxy | 42 | 15 | 2.714 | 0.001484 | 0303382,0303267,etc |
| mass accretion rate | 63 | 21 | 3.1 | 0.001477 | 0303375,0303456,etc |
| central source | 68 | 19 | 3.611 | 0.001476 | 0303597,0303479,etc |
| magnetic field strength | 82 | 32 | 2.581 | 0.001462 | 0303375,0303456,etc |
| matter power spectrum | 29 | 12 | 2.455 | 0.001452 | 0303555,0303353,etc |
| gas mass | 52 | 22 | 2.429 | 0.001441 | 0303240,0303558,etc |
| population synthesis model | 31 | 12 | 2.727 | 0.001397 | 0303325,0303257,etc |
| density field | 55 | 14 | 4.077 | 0.001376 | 0303249,0303519,etc |
| fitting result | 22 | 11 | 2.1 | 0.001373 | 0303091,0303024,etc |
| shock velocity | 56 | 17 | 3.375 | 0.001371 | 0303051,0303423,etc |
| redshift distribution | 45 | 18 | 2.529 | 0.001333 | 0303382,0303166,etc |
| electric field | 67 | 21 | 2.95 | 0.001333 | 0303157,0303194,etc |
| flat model | 29 | 12 | 2.455 | 0.001318 | 0303558,0303248,etc |
| massive cluster | 47 | 23 | 2.091 | 0.001294 | 0303293,0303519,etc |
| entire sample | 40 | 18 | 2.235 | 0.001294 | 0303221,0303493,etc |
| local density | 37 | 13 | 3.0 | 0.00127 | 0303532,0303071,etc |
| particle distribution | 56 | 14 | 4.231 | 0.001239 | 0303161,0303519,etc |
| X-ray source | 111 | 35 | 3.235 | 0.001193 | 0303387,0303382,etc |
| X-ray spectrum | 93 | 38 | 2.486 | 0.001186 | 0303387,0303110,etc |
| young stellar population | 40 | 17 | 2.375 | 0.001133 | 0303110,0303066,etc |
| inner radius | 56 | 25 | 2.292 | 0.001129 | 0303387,0303525,etc |
| semimajor axis | 30 | 14 | 2.231 | 0.001123 | 0303269,0303362,etc |
| power law | 192 | 88 | 2.184 | 0.001117 | 0303302,0303644,etc |
| distant cluster | 35 | 17 | 2.125 | 0.001085 | 0303066,0303416,etc |
| systemic velocity | 74 | 26 | 2.64 | 0.001075 | 0303052,0303423,etc |
| thermal pressure | 56 | 19 | 3.056 | 0.001072 | 0303240,0303532,etc |
| X-ray binary | 59 | 15 | 4.143 | 0.001061 | 0303387,0303110,etc |
| inner boundary | 39 | 13 | 3.167 | 0.00103 | 0303171,0303525,etc |
| diffuse emission | 76 | 22 | 3.571 | 0.001006 | 0303387,0303609,etc |
| small radius | 50 | 14 | 3.615 | 0.000985 | 0303519,0303052,etc |
| source size | 43 | 12 | 3.636 | 0.000979 | 0303387,0303317,etc |
| density contrast | 55 | 24 | 2.348 | 0.000954 | 0303161,0303071,etc |
| hot gas | 96 | 38 | 2.486 | 0.000941 | 0303004,0303532,etc |
| equal mass | 25 | 12 | 2.182 | 0.000928 | 0303558,0303227,etc |
| power-law index | 43 | 16 | 2.467 | 0.000923 | 0303240,0303597,etc |
| disk model | 34 | 16 | 2.133 | 0.00091 | 0303241,0303546,etc |
| non-linear regime | 31 | 12 | 2.727 | 0.000897 | 0303555,0303519,etc |
| magnetic field line | 64 | 24 | 2.522 | 0.000891 | 0303214,0303199,etc |
| semi-major axis | 73 | 28 | 2.63 | 0.000866 | 0303456,0303398,etc |
| boundary condition | 101 | 42 | 2.439 | 0.00084 | 0303202,0303214,etc |
| central engine | 39 | 19 | 2.056 | 0.00084 | 0303611,0303546,etc |
| galaxy spectrum | 54 | 13 | 4.333 | 0.000837 | 0303668,0303581,etc |
| semi-analytic model | 28 | 13 | 2.25 | 0.000824 | 0303249,0303481,etc |
| peak flux | 44 | 19 | 2.389 | 0.000803 | 0303508,0303106,etc |
| band image | 60 | 27 | 2.269 | 0.000785 | 0303387,0303066,etc |
| energy-momentum tensor | 35 | 15 | 2.071 | 0.000779 | 0303248,0303241,etc |
| Monte Carlo simulation | 40 | 18 | 2.235 | 0.000771 | 0303387,0303252,etc |
| photon index | 50 | 23 | 2.136 | 0.00074 | 0303387,0303494,etc |
| Hubble type | 46 | 11 | 4.5 | 0.00073 | 0303190,0303257,etc |
| numerical calculation | 37 | 17 | 2.25 | 0.000723 | 0303257,0303006,etc |
| gamma-ray burst | 55 | 27 | 2.038 | 0.000717 | 0303110,0303161,etc |
| outer boundary | 43 | 16 | 2.467 | 0.000709 | 0303449,0303525,etc |
| nuclear region | 46 | 21 | 2.25 | 0.000707 | 0303216,0303184,etc |
| ambient gas | 41 | 19 | 2.167 | 0.000701 | 0303004,0303257,etc |
| mass flux | 25 | 11 | 2.4 | 0.0007 | 0303241,0303362,etc |
| mass star | 41 | 17 | 2.438 | 0.000692 | 0303325,0303221,etc |
| present day | 33 | 16 | 2.133 | 0.000691 | 0303519,0303127,etc |
| spectral indices | 58 | 19 | 3.167 | 0.000688 | 0303014,0303644,etc |
| radial dependence | 30 | 14 | 2.231 | 0.00068 | 0303532,0303416,etc |
| count rate | 98 | 37 | 2.667 | 0.000675 | 0303387,0303508,etc |
| hardness ratio | 35 | 13 | 2.833 | 0.00066 | 0303387,0303508,etc |
| linear theory | 24 | 12 | 2.091 | 0.000658 | 0303382,0303519,etc |
| initial energy | 29 | 14 | 2.077 | 0.000645 | 0303202,0303233,etc |
| late-type star | 37 | 15 | 2.571 | 0.000638 | 0303151,0303106,etc |
| power-law model | 28 | 13 | 2.167 | 0.000637 | 0303387,0303508,etc |
| outer disk | 29 | 14 | 2.154 | 0.000621 | 0303532,0303130,etc |
| strong shock | 32 | 16 | 2.067 | 0.00061 | 0303007,0303593,etc |
| bright end | 43 | 17 | 2.562 | 0.000609 | 0303302,0303066,etc |
| radiative loss | 43 | 19 | 2.333 | 0.000609 | 0303456,0303558,etc |
| calibration uncertainty | 33 | 15 | 2.286 | 0.000608 | 0303551,0303051,etc |
| cluster core | 60 | 27 | 2.192 | 0.000606 | 0303293,0303214,etc |
| inflationary model | 29 | 12 | 2.455 | 0.000602 | 0303475,0303591,etc |
| matter distribution | 23 | 11 | 2.2 | 0.000591 | 0303240,0303382,etc |
| Stokes parameter | 28 | 12 | 2.364 | 0.000571 | 0303644,0303652,etc |