| markov chain monte carlo | MCMC | 106 | 20 | 1.000987 | 1402.4298,1402.0053,etc |
| signal to noise | S/N | 73 | 14 | 1.000317 | 1402.3599,1402.4154,etc |
| kolmogorov smirnov | KS | 49 | 14 | 1.000405 | 1402.5778,1402.6333,etc |
| wolf rayet | W-R | 301 | 12 | 2.004819 | 1402.5150,1402.4477,etc |
| large area telescope | LAT | 85 | 11 | 1.002198 | 1402.4558,1402.4804,etc |
| advanced camera for surveys | ACS | 171 | 11 | 1.008015 | 1402.7174,1402.3723,etc |
| effective field theory | EFT | 81 | 10 | 1.000933 | 1402.0959,1402.1576,etc |
| friedmann robertson walker | FRW | 42 | 10 | 1.001035 | 1402.5104,1402.6661,etc |
| wide field camera 3 | WFC3 | 92 | 9 | 2.000787 | 1402.5752,1402.4129,etc |
| one dimensional | 1D | 45 | 9 | 1.000947 | 1402.3915,1402.4777,etc |
| infrared spectrograph | IRS | 96 | 8 | 2.000805 | 1402.2686,1402.3509,etc |
| large velocity gradient | LVG | 28 | 8 | 1.000305 | 1402.2686,1402.2329,etc |
| deutsche forschungsgemeinschaft | DFG | 14 | 8 | 1.000146 | 1402.2686,1402.4650,etc |
| friends of friends | FOF | 94 | 8 | 2.001101 | 1402.5986,1402.1350,etc |
| monte carlo | MC | 34 | 8 | 1.000274 | 1402.5227,1402.3267,etc |
| magneto rotational instability | MRI | 68 | 8 | 1.001794 | 1402.2891,1402.2979,etc |
| inverse compton | IC | 145 | 8 | 1.003421 | 1402.6344,1402.0853,etc |
| star formation history | SFH | 59 | 8 | 2.000944 | 1402.3597,1402.5145,etc |
| asi science data center | ASDC | 7 | 7 | 1.000074 | 1402.4804,1402.6755,etc |
| three dimensional | 3D | 29 | 7 | 1.000726 | 1402.4527,1402.2644,etc |
| cold neutral medium | CNM | 52 | 7 | 2.001165 | 1402.5465,1402.2858,etc |
| square kilometre array | SKA | 34 | 7 | 1.000638 | 1402.1548,1402.7180,etc |
| tolman oppenheimer volkoff | TOV | 28 | 7 | 1.000742 | 1402.5412,1402.0251,etc |
| science and technology facilities council | STFC | 8 | 7 | 1.000105 | 1402.3701,1402.1849,etc |
| circumstellar medium | CSM | 65 | 6 | 1.001509 | 1402.1633,1402.5150,etc |
| japan society for the promotion of science | JSPS | 6 | 6 | 1.000056 | 1402.1633,1402.2770,etc |
| hertzsprung russell | HR | 18 | 6 | 2.000134 | 1402.0824,1402.3323,etc |
| burst alert telescope | BAT | 43 | 6 | 2.000477 | 1402.4804,1402.0766,etc |
| national research foundation of korea | NRF | 6 | 6 | 1.000366 | 1402.1549,1402.2443,etc |
| friedmann lema^itre robertson walker | FLRW | 27 | 6 | 1.000303 | 1402.5719,1402.3121,etc |
| warm neutral medium | WNM | 42 | 6 | 1.000568 | 1402.5465,1402.2858,etc |
| specific sfr | sSFR | 120 | 6 | 1.001724 | 1402.3394,1402.4139,etc |
| very high energy | VHE | 38 | 6 | 1.001714 | 1402.2332,1402.0383,etc |
| full width half maximum | FWHM | 31 | 6 | 1.000509 | 1402.5101,1402.6684,etc |
| maximum likelihood | ML | 41 | 6 | 1.000483 | 1402.3723,1402.1373,etc |
| atacama large millimeter/submillimeter array | ALMA | 53 | 6 | 2.001974 | 1402.0832,1402.6619,etc |
| submillimeter array | SMA | 46 | 6 | 2.001876 | 1402.7103,1402.3518,etc |
| california institute of technology | Caltech | 8 | 6 | 1.000253 | 1402.4811,1402.2992,etc |
| infrared array camera | IRAC | 74 | 6 | 1.001705 | 1402.2631,1402.2983,etc |
| super massive black hole | SMBH | 14 | 5 | 1.000207 | 1402.3509,1402.2980,etc |
| kennicutt schmidt | KS | 37 | 5 | 2.000503 | 1402.7208,1402.1039,etc |
| position velocity | P-V | 40 | 5 | 1.000259 | 1402.7208,1402.0999,etc |
| max planck institute for astronomy | MPIA | 5 | 5 | 1.000018 | 1402.7208,1402.4814,etc |
| national research council | NRC | 7 | 5 | 1.000094 | 1402.3599,1402.2670,etc |
| stellar population synthesis | SPS | 25 | 5 | 2.000816 | 1402.3599,1402.0888,etc |
| innermost stable circular orbit | ISCO | 18 | 5 | 1.000366 | 1402.0148,1402.5809,etc |
| two dimensional | 2D | 47 | 5 | 2.000907 | 1402.2769,1402.6337,etc |
| atmospheric imaging assembly | AIA | 62 | 5 | 2.002148 | 1402.7016,1402.6554,etc |
| galactic globular cluster | GGC | 59 | 5 | 2.003483 | 1402.3938,1402.0691,etc |
| navarro frenk white | NFW | 49 | 5 | 2.001023 | 1402.0695,1402.6259,etc |
| bundesministerium f"ur bildung und forschung | BMBF | 5 | 5 | 1.000088 | 1402.3677,1402.1600,etc |
| central molecular zone | CMZ | 88 | 5 | 2.00125 | 1402.6110,1402.6196,etc |
| monte carlo markov chain | MCMC | 40 | 5 | 2.001685 | 1402.6842,1402.6546,etc |
| infrared dark cloud | IRDC | 196 | 5 | 2.004213 | 1402.0919,1402.2983,etc |
| synchrotron self compton | SSC | 20 | 4 | 2.000722 | 1402.4558,1402.0853,etc |
| front illuminated | FI | 19 | 4 | 1.000568 | 1402.1633,1402.3700,etc |
| non x ray background | NXB | 12 | 4 | 1.000225 | 1402.1633,1402.1852,etc |
| optical monitor | OM | 15 | 4 | 2.000239 | 1402.6790,1402.0765,etc |
| charged current | CC | 33 | 4 | 1.000411 | 1402.0959,1402.3861,etc |
| spin independent | SI | 57 | 4 | 2.001542 | 1402.5870,1402.4650,etc |
| particle in cell | PIC | 25 | 4 | 1.000738 | 1402.0014,1402.3915,etc |
| axion like particle | ALP | 119 | 4 | 2.008302 | 1402.2533,1402.2161,etc |
| nasa extragalactic database | NED | 5 | 4 | 1.000026 | 1402.0766,1402.5465,etc |
| interactive data language | IDL | 5 | 4 | 1.000052 | 1402.3599,1402.2975,etc |
| polarity inversion line | PIL | 19 | 4 | 2.000341 | 1402.6558,1402.2010,etc |
| warm ionized medium | WIM | 41 | 4 | 2.002423 | 1402.5465,1402.6110,etc |
| semi analytic model | SAM | 28 | 4 | 2.000471 | 1402.0075,1402.1172,etc |
| photodissociation region | PDR | 12 | 4 | 1.000103 | 1402.5041,1402.5614,etc |
| charge transfer efficiency | CTE | 10 | 4 | 1.000241 | 1402.3723,1402.0691,etc |
| metallicity distribution function | MDF | 82 | 4 | 2.001776 | 1402.0446,1402.3874,etc |
| main sequence turn off | MSTO | 30 | 4 | 2.000516 | 1402.0446,1402.0981,etc |
| baryonic acoustic oscillation | BAO | 29 | 4 | 2.00044 | 1402.4269,1402.5145,etc |
| rosat all sky survey | RASS | 5 | 4 | 1.000063 | 1402.0868,1402.2670,etc |
| ultra violet | UV | 96 | 4 | 2.000653 | 1402.2443,1402.0003,etc |
| nederlandse organisatie voor wetenschappelijk onderzoek | NWO | 4 | 4 | 1.000091 | 1402.3677,1402.1600,etc |
| fundamenteel onderzoek der materie | FOM | 4 | 4 | 1.000091 | 1402.3677,1402.1600,etc |
| ministerio de ciencia e innovaci'on | MICINN | 4 | 4 | 1.000096 | 1402.1600,1402.0083,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 6 | 4 | 1.000155 | 1402.6842,1402.0765,etc |
| extreme mass ratio inspiral | EMRI | 13 | 4 | 1.000348 | 1402.4737,1402.0005,etc |
| imaging atmospheric cherenkov telescope | IACT | 70 | 4 | 2.001572 | 1402.6884,1402.5081,etc |
| basic calibrated data | BCD | 14 | 4 | 1.00053 | 1402.3750,1402.5850,etc |
| dwarf spheroidal | dSph | 151 | 4 | 2.006663 | 1402.6328,1402.4480,etc |
| michelson doppler imager | MDI | 22 | 4 | 1.001131 | 1402.5934,1402.2881,etc |
| back illuminated | BI | 13 | 3 | 1.000782 | 1402.1633,1402.2350,etc |
| ancillary response file | ARF | 13 | 3 | 1.000236 | 1402.1633,1402.2301,etc |
| all sky monitor | ASM | 13 | 3 | 1.000152 | 1402.3940,1402.0085,etc |
| minimum mass solar nebula | MMSN | 13 | 3 | 1.000261 | 1402.7086,1402.7075,etc |
| time projection chamber | TPC | 39 | 3 | 2.002411 | 1402.0043,1402.1078,etc |
| median absolute deviation | MAD | 5 | 3 | 1.000083 | 1402.5752,1402.6343,etc |
| soft x ray | SXR | 12 | 3 | 1.000187 | 1402.1676,1402.4794,etc |
| natural science foundation of china | NSFC | 4 | 3 | 1.000347 | 1402.7135,1402.6470,etc |
| fluorescence detector | FD | 32 | 3 | 1.005172 | 1402.6186,1402.3677,etc |
| surface detector | SD | 33 | 3 | 1.001854 | 1402.6186,1402.3677,etc |
| 2 dimensional | 2D | 17 | 3 | 1.000368 | 1402.2842,1402.5340,etc |
| rayleigh taylor | RT | 36 | 3 | 1.000234 | 1402.4527,1402.4134,etc |
| kelvin helmholtz | KH | 11 | 3 | 1.000133 | 1402.4527,1402.1788,etc |
| friend of friend | FoF | 36 | 3 | 2.001106 | 1402.1350,1402.1172,etc |
| local correlation tracking | LCT | 46 | 3 | 1.001918 | 1402.6558,1402.2293,etc |
| intermediate frequency | IF | 7 | 3 | 1.000421 | 1402.7174,1402.1548,etc |
| ordinary differential equation | ODE | 9 | 3 | 1.000198 | 1402.2769,1402.0005,etc |
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