| active galactic nucleus | AGN | 3990 | 113 | 1.005584 | 1707.00176,1707.06147,etc |
| cosmic microwave background | CMB | 1830 | 91 | 2.00368 | 1707.01300,1707.06147,etc |
| spectral energy distribution | SED | 839 | 89 | 1.001757 | 1707.01094,1707.00591,etc |
| interstellar medium | ISM | 828 | 84 | 1.001581 | 1707.06147,1707.03416,etc |
| point spread function | PSF | 514 | 65 | 2.001236 | 1707.01094,1707.03416,etc |
| signal to noise ratio | S/N | 377 | 64 | 1.001191 | 1707.03570,1707.06236,etc |
| dark matter | DM | 2658 | 63 | 2.007642 | 1707.06147,1707.05318,etc |
| star formation rate | SFR | 1206 | 56 | 2.003286 | 1707.02454,1707.05293,etc |
| markov chain monte carlo | MCMC | 273 | 45 | 2.000637 | 1707.04262,1707.00062,etc |
| full width at half maximum | FWHM | 310 | 45 | 2.001236 | 1707.02454,1707.08806,etc |
| initial mass function | IMF | 246 | 44 | 1.000777 | 1707.01094,1707.04554,etc |
| black hole | BH | 1688 | 44 | 2.007714 | 1707.08822,1707.01527,etc |
| sloan digital sky survey | SDSS | 507 | 44 | 2.001515 | 1707.01411,1707.00611,etc |
| supernova | SN | 3888 | 41 | 2.013003 | 1707.06147,1707.04253,etc |
| near infrared | NIR | 458 | 39 | 1.002151 | 1707.04992,1707.00611,etc |
| nasa/ipac extragalactic database | NED | 82 | 35 | 1.000203 | 1707.01542,1707.01411,etc |
| field of view | FOV | 127 | 34 | 1.000668 | 1707.03570,1707.05293,etc |
| infrared | IR | 1135 | 34 | 1.00409 | 1707.04399,1707.04037,etc |
| supermassive black hole | SMBH | 385 | 33 | 1.003919 | 1707.04671,1707.04001,etc |
| supernova remnant | SNR | 914 | 32 | 2.004762 | 1707.06147,1707.00054,etc |
| hubble space telescope | HST | 179 | 29 | 1.00099 | 1707.08328,1707.00696,etc |
| cold dark matter | CDM | 355 | 28 | 1.003023 | 1707.06277,1707.00588,etc |
| general relativity | GR | 216 | 28 | 1.001236 | 1707.06460,1707.01802,etc |
| equation of state | EOS | 629 | 27 | 1.004692 | 1707.09475,1707.08142,etc |
| cosmic ray | CR | 1195 | 27 | 2.005444 | 1707.06147,1707.01412,etc |
| magnetohydrodynamic | MHD | 352 | 26 | 2.001968 | 1707.03827,1707.06619,etc |
| signal to noise | S/N | 172 | 26 | 1.000562 | 1707.04102,1707.07991,etc |
| asymptotic giant branch | AGB | 398 | 26 | 2.003108 | 1707.05318,1707.00054,etc |
| gamma ray burst | GRB | 815 | 25 | 2.006015 | 1707.04253,1707.07684,etc |
| gravitational wave | GW | 1197 | 25 | 2.006804 | 1707.01480,1707.02299,etc |
| atacama large millimeter/submillimeter array | ALMA | 370 | 24 | 2.002276 | 1707.03827,1707.08697,etc |
| radial velocity | RV | 489 | 24 | 2.005039 | 1707.00591,1707.06192,etc |
| milky way | MW | 317 | 24 | 2.002549 | 1707.01108,1707.03456,etc |
| ultraviolet | UV | 414 | 24 | 1.00178 | 1707.08328,1707.00611,etc |
| very large array | VLA | 187 | 22 | 2.00145 | 1707.03827,1707.08697,etc |
| neutron star | NS | 571 | 22 | 2.003287 | 1707.06147,1707.09479,etc |
| large magellanic cloud | LMC | 435 | 22 | 1.004404 | 1707.00696,1707.03828,etc |
| far infrared | FIR | 170 | 22 | 2.001774 | 1707.04259,1707.01097,etc |
| european space agency | ESA | 41 | 21 | 2.000278 | 1707.04554,1707.01405,etc |
| three dimensional | 3D | 173 | 21 | 1.001084 | 1707.04992,1707.01863,etc |
| polycyclic aromatic hydrocarbon | PAH | 416 | 21 | 1.004006 | 1707.00568,1707.09230,etc |
| standard model | SM | 264 | 21 | 1.002123 | 1707.08571,1707.09980,etc |
| intergalactic medium | IGM | 202 | 20 | 1.001624 | 1707.02302,1707.01906,etc |
| data processing and analysis consortium | DPAC | 40 | 19 | 1.000503 | 1707.04554,1707.04006,etc |
| line of sight | LOS | 121 | 19 | 1.000661 | 1707.04421,1707.06734,etc |
| broad line region | BLR | 197 | 18 | 1.001481 | 1707.01411,1707.04671,etc |
| main sequence | MS | 496 | 18 | 2.003924 | 1707.04037,1707.05329,etc |
| adaptive optics | AO | 120 | 17 | 1.001166 | 1707.01573,1707.00591,etc |
| probability distribution function | PDF | 431 | 17 | 2.007025 | 1707.03416,1707.07691,etc |
| science and technology facilities council | STFC | 24 | 17 | 1.00017 | 1707.05268,1707.03658,etc |
| local thermodynamic equilibrium | LTE | 212 | 17 | 1.004233 | 1707.08697,1707.03745,etc |
| coronal mass ejection | CME | 553 | 17 | 1.007461 | 1707.03579,1707.02107,etc |
| integral field unit | IFU | 370 | 17 | 2.003474 | 1707.02302,1707.07991,etc |
| radio frequency interference | RFI | 54 | 16 | 1.000428 | 1707.01542,1707.08581,etc |
| kolmogorov smirnov | KS | 64 | 16 | 2.000509 | 1707.01108,1707.01411,etc |
| principal component analysis | PCA | 181 | 16 | 2.001052 | 1707.01411,1707.08129,etc |
| equivalent width | EW | 251 | 16 | 2.002321 | 1707.02840,1707.04270,etc |
| dark energy survey | DES | 207 | 16 | 2.003376 | 1707.06640,1707.03954,etc |
| weakly interacting massive particle | WIMP | 279 | 15 | 1.002246 | 1707.08042,1707.06277,etc |
| young stellar object | YSO | 168 | 15 | 1.001703 | 1707.09243,1707.08594,etc |
| very large telescope | VLT | 56 | 15 | 1.000346 | 1707.04270,1707.01906,etc |
| ministry of economy and competitiveness | MINECO | 20 | 14 | 1.000245 | 1707.03456,1707.02454,etc |
| baryon acoustic oscillation | BAO | 321 | 14 | 2.005272 | 1707.00588,1707.08531,etc |
| white dwarf | WD | 238 | 14 | 2.003573 | 1707.04270,1707.09395,etc |
| probability density function | PDF | 148 | 13 | 2.001638 | 1707.02879,1707.01108,etc |
| diffusive shock acceleration | DSA | 156 | 13 | 1.001465 | 1707.06147,1707.00485,etc |
| inverse compton | IC | 229 | 13 | 2.002277 | 1707.08263,1707.02085,etc |
| adaptive mesh refinement | AMR | 61 | 13 | 2.000553 | 1707.04259,1707.06619,etc |
| wolf rayet | WR | 180 | 13 | 2.003648 | 1707.04644,1707.03828,etc |
| intra cluster medium | ICM | 258 | 12 | 1.002001 | 1707.05318,1707.02085,etc |
| european research council | ERC | 17 | 12 | 1.000109 | 1707.07684,1707.08596,etc |
| magnetohydrodynamics | MHD | 184 | 12 | 1.001407 | 1707.09419,1707.01863,etc |
| large area telescope | LAT | 131 | 12 | 1.001787 | 1707.08263,1707.02085,etc |
| color magnitude diagram | CMD | 172 | 12 | 2.001974 | 1707.05293,1707.03954,etc |
| large synoptic survey telescope | LSST | 239 | 12 | 2.002817 | 1707.06529,1707.06640,etc |
| low mass x ray binary | LMXB | 93 | 12 | 1.001252 | 1707.03161,1707.02349,etc |
| small magellanic cloud | SMC | 368 | 12 | 2.005823 | 1707.01571,1707.03130,etc |
| two dimensional | 2D | 74 | 12 | 2.00057 | 1707.01863,1707.07044,etc |
| pulsar wind nebula | PWN | 237 | 11 | 2.005561 | 1707.06147,1707.00054,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 14 | 11 | 1.00009 | 1707.01542,1707.02302,etc |
| national science foundation | NSF | 35 | 11 | 2.000235 | 1707.05268,1707.00611,etc |
| bayesian information criterion | BIC | 71 | 11 | 2.000897 | 1707.08328,1707.09932,etc |
| monte carlo | MC | 118 | 11 | 2.001854 | 1707.01412,1707.08571,etc |
| big bang nucleosynthesis | BBN | 122 | 11 | 2.003023 | 1707.06277,1707.03852,etc |
| large scale structure | LSS | 214 | 11 | 2.002926 | 1707.00588,1707.08471,etc |
| very high energy | VHE | 140 | 11 | 1.001287 | 1707.03658,1707.08599,etc |
| position angle | PA | 115 | 11 | 1.000828 | 1707.02302,1707.07614,etc |
| interstellar radiation field | ISRF | 99 | 11 | 2.002621 | 1707.04259,1707.03808,etc |
| colour magnitude diagram | CMD | 110 | 11 | 2.001715 | 1707.09932,1707.09153,etc |
| monte carlo markov chain | MCMC | 58 | 11 | 1.000504 | 1707.00779,1707.02298,etc |
| canada france hawaii telescope | CFHT | 83 | 11 | 1.001367 | 1707.03169,1707.03009,etc |
| square kilometre array | SKA | 51 | 10 | 1.001199 | 1707.00176,1707.09787,etc |
| star formation rates | SFR | 103 | 10 | 1.002804 | 1707.02879,1707.01108,etc |
| james clerk maxwell telescope | JCMT | 52 | 10 | 1.000521 | 1707.03827,1707.08697,etc |
| very long baseline interferometry | VLBI | 148 | 10 | 1.001484 | 1707.01542,1707.06596,etc |
| smoothed particle hydrodynamics | SPH | 127 | 10 | 1.003055 | 1707.01108,1707.03824,etc |
| cross correlation function | CCF | 245 | 10 | 1.003273 | 1707.04262,1707.07093,etc |
| narrow line region | NLR | 68 | 10 | 1.001154 | 1707.01411,1707.08123,etc |
| baryon oscillation spectroscopic survey | BOSS | 89 | 10 | 1.000739 | 1707.01411,1707.03388,etc |
| star formation history | SFH | 66 | 10 | 1.001361 | 1707.07691,1707.01840,etc |
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