| active galactic nucleus | AGN | 2090 | 96 | 2.004118 | 1406.5898,1406.7420,etc |
| spectral energy distribution | SED | 843 | 84 | 1.00131 | 1406.4120,1406.0868,etc |
| point spread function | PSF | 811 | 77 | 1.004181 | 1406.5508,1406.0507,etc |
| interstellar medium | ISM | 661 | 64 | 1.001061 | 1406.0310,1406.4127,etc |
| cosmic microwave background | CMB | 810 | 63 | 2.003551 | 1406.4120,1406.5918,etc |
| sloan digital sky survey | SDSS | 1036 | 62 | 1.002763 | 1406.5508,1406.4908,etc |
| initial mass function | IMF | 535 | 53 | 2.002275 | 1406.4120,1406.6069,etc |
| field of view | FOV | 288 | 50 | 1.001125 | 1406.4343,1406.6436,etc |
| signal to noise ratio | S/N | 378 | 50 | 2.001178 | 1406.2747,1406.0359,etc |
| full width at half maximum | FWHM | 249 | 41 | 1.000876 | 1406.3093,1406.3574,etc |
| nasa/ipac extragalactic database | NED | 102 | 39 | 1.000336 | 1406.0868,1406.2747,etc |
| ultraviolet | UV | 810 | 39 | 1.004508 | 1406.1456,1406.0425,etc |
| near infrared | NIR | 537 | 38 | 2.002467 | 1406.4887,1406.6069,etc |
| star formation rate | SFR | 883 | 36 | 1.005416 | 1406.0310,1406.6069,etc |
| supernova | SN | 1869 | 35 | 2.007907 | 1406.2287,1406.5220,etc |
| dark matter | DM | 1672 | 34 | 2.007675 | 1406.3413,1406.6027,etc |
| supermassive black hole | SMBH | 822 | 33 | 1.005622 | 1406.5898,1406.7420,etc |
| equivalent width | EW | 475 | 32 | 2.002284 | 1406.5220,1406.5968,etc |
| black hole | BH | 1437 | 28 | 2.007905 | 1406.4120,1406.2181,etc |
| radial velocity | RV | 474 | 28 | 2.002665 | 1406.2605,1406.0521,etc |
| infrared | IR | 1577 | 27 | 2.004364 | 1406.1456,1406.7034,etc |
| markov chain monte carlo | MCMC | 144 | 26 | 2.000679 | 1406.6063,1406.3354,etc |
| magnetohydrodynamic | MHD | 358 | 26 | 1.002511 | 1406.6112,1406.2377,etc |
| main sequence | MS | 673 | 26 | 2.003264 | 1406.5513,1406.3090,etc |
| supernova remnant | SNR | 604 | 25 | 1.004724 | 1406.2287,1406.5190,etc |
| equation of state | EOS | 296 | 24 | 2.002561 | 1406.3388,1406.7661,etc |
| milky way | MW | 650 | 24 | 2.004656 | 1406.1799,1406.4018,etc |
| gamma ray burst | GRB | 1447 | 24 | 1.010601 | 1406.4568,1406.4836,etc |
| asymptotic giant branch | AGB | 334 | 23 | 1.003895 | 1406.5220,1406.1048,etc |
| color magnitude diagram | CMD | 305 | 23 | 2.001098 | 1406.4375,1406.6451,etc |
| gravitational wave | GW | 777 | 22 | 2.00777 | 1406.2151,1406.7154,etc |
| globular cluster | GC | 2011 | 22 | 2.00902 | 1406.2384,1406.6091,etc |
| cold dark matter | CDM | 229 | 22 | 2.003544 | 1406.3413,1406.0388,etc |
| red giant branch | RGB | 359 | 20 | 2.003094 | 1406.5220,1406.4375,etc |
| coronal mass ejection | CME | 1205 | 20 | 1.01169 | 1406.6112,1406.2377,etc |
| general relativity | GR | 331 | 20 | 2.001528 | 1406.2790,1406.6187,etc |
| intergalactic medium | IGM | 466 | 19 | 2.003504 | 1406.4120,1406.2314,etc |
| polycyclic aromatic hydrocarbon | PAH | 479 | 19 | 1.002379 | 1406.7034,1406.0425,etc |
| young stellar object | YSO | 335 | 19 | 1.003013 | 1406.2604,1406.0068,etc |
| line of sight | LOS | 107 | 19 | 2.000907 | 1406.3871,1406.3574,etc |
| standard model | SM | 347 | 19 | 1.002932 | 1406.5558,1406.5192,etc |
| white dwarf | WD | 775 | 19 | 2.007589 | 1406.1707,1406.4514,etc |
| neutron star | NS | 667 | 18 | 2.004473 | 1406.7661,1406.6091,etc |
| two micron all sky survey | 2MASS | 164 | 18 | 2.001301 | 1406.4778,1406.7353,etc |
| far infrared | FIR | 117 | 18 | 1.000743 | 1406.3951,1406.4132,etc |
| three dimensional | 3D | 206 | 18 | 1.001673 | 1406.2377,1406.6069,etc |
| kolmogorov smirnov | KS | 63 | 17 | 2.000492 | 1406.2314,1406.5164,etc |
| probability distribution function | PDF | 144 | 17 | 2.001643 | 1406.6048,1406.3871,etc |
| pre main sequence | PMS | 392 | 17 | 2.003171 | 1406.3979,1406.3090,etc |
| signal to noise | S/N | 96 | 16 | 1.000426 | 1406.5508,1406.2002,etc |
| zero age main sequence | ZAMS | 141 | 16 | 1.00111 | 1406.5078,1406.4836,etc |
| hubble space telescope | HST | 85 | 16 | 2.001574 | 1406.6492,1406.3611,etc |
| adaptive optics | AO | 255 | 16 | 2.003577 | 1406.0202,1406.3611,etc |
| full width half maximum | FWHM | 92 | 15 | 2.000508 | 1406.5898,1406.5078,etc |
| colour magnitude diagram | CMD | 169 | 15 | 2.001918 | 1406.3090,1406.6116,etc |
| inverse compton | IC | 255 | 15 | 2.003246 | 1406.2179,1406.2706,etc |
| intracluster medium | ICM | 170 | 14 | 2.001506 | 1406.5190,1406.6831,etc |
| root mean square | RMS | 51 | 14 | 1.000379 | 1406.5496,1406.6062,etc |
| navarro frenk white | NFW | 136 | 13 | 2.002428 | 1406.4908,1406.6063,etc |
| max planck institute for astrophysics | MPA | 19 | 13 | 1.000199 | 1406.4908,1406.4179,etc |
| star formation history | SFH | 115 | 13 | 2.001935 | 1406.6069,1406.0838,etc |
| very large array | VLA | 95 | 13 | 2.002985 | 1406.0068,1406.3574,etc |
| large magellanic cloud | LMC | 302 | 13 | 1.002205 | 1406.3979,1406.4836,etc |
| big bang nucleosynthesis | BBN | 110 | 13 | 2.002432 | 1406.2790,1406.7482,etc |
| smoothed particle hydrodynamics | SPH | 427 | 13 | 1.002799 | 1406.4668,1406.5515,etc |
| mid infrared | mid-IR | 230 | 13 | 2.001746 | 1406.1707,1406.4514,etc |
| brightest cluster galaxy | BCG | 453 | 12 | 2.006624 | 1406.4908,1406.4179,etc |
| max planck institute for astronomy | MPIA | 12 | 12 | 1.000048 | 1406.4908,1406.4179,etc |
| weakly interacting massive particle | WIMP | 199 | 12 | 2.003619 | 1406.0388,1406.4683,etc |
| infrared array camera | IRAC | 53 | 12 | 1.000458 | 1406.6116,1406.2860,etc |
| cross correlation function | CCF | 149 | 11 | 1.002165 | 1406.5898,1406.5587,etc |
| very large telescope | VLT | 45 | 11 | 1.00025 | 1406.2868,1406.6069,etc |
| deutsche forschungsgemeinschaft | DFG | 16 | 11 | 1.00015 | 1406.5078,1406.0293,etc |
| hertzsprung russell | HR | 71 | 11 | 2.000823 | 1406.4836,1406.6750,etc |
| specific star formation rate | sSFR | 277 | 11 | 1.002645 | 1406.2327,1406.5219,etc |
| wolf rayet | WR | 194 | 11 | 1.003242 | 1406.5357,1406.5219,etc |
| wilkinson microwave anisotropy probe | WMAP | 43 | 11 | 1.001743 | 1406.0283,1406.0527,etc |
| giant molecular cloud | GMC | 78 | 10 | 2.002424 | 1406.0310,1406.5206,etc |
| broad line region | BLR | 131 | 10 | 1.00157 | 1406.5898,1406.7129,etc |
| far ultraviolet | FUV | 60 | 10 | 2.002149 | 1406.4343,1406.5058,etc |
| particle in cell | PIC | 40 | 10 | 1.000317 | 1406.7834,1406.5190,etc |
| small magellanic cloud | SMC | 194 | 10 | 1.002423 | 1406.7034,1406.4778,etc |
| galactic center | GC | 170 | 10 | 2.002702 | 1406.6027,1406.4375,etc |
| japan society for the promotion of science | JSPS | 17 | 10 | 1.000178 | 1406.3507,1406.3871,etc |
| local thermodynamic equilibrium | LTE | 111 | 10 | 2.004972 | 1406.4228,1406.0068,etc |
| horizontal branch | HB | 113 | 10 | 1.002982 | 1406.5513,1406.6053,etc |
| large scale structure | LSS | 72 | 10 | 2.001191 | 1406.1448,1406.6480,etc |
| luminous blue variable | LBV | 529 | 10 | 1.006061 | 1406.4836,1406.2120,etc |
| james webb space telescope | JWST | 99 | 10 | 2.002898 | 1406.1707,1406.3611,etc |
| very long baseline interferometry | VLBI | 135 | 10 | 1.002384 | 1406.6365,1406.2086,etc |
| national research foundation of korea | NRF | 20 | 10 | 1.000298 | 1406.0228,1406.6868,etc |
| monte carlo | MC | 70 | 10 | 1.000726 | 1406.6709,1406.2706,etc |
| probability density function | PDF | 52 | 10 | 1.000622 | 1406.4716,1406.4503,etc |
| one dimensional | 1D | 53 | 9 | 1.001109 | 1406.5190,1406.4145,etc |
| quasi periodic oscillation | QPO | 165 | 9 | 2.004373 | 1406.4688,1406.5512,etc |
| radio frequency interference | RFI | 89 | 9 | 1.001552 | 1406.6874,1406.0991,etc |
| cosmic ray | CR | 257 | 9 | 1.004969 | 1406.2322,1406.1117,etc |
| red clump | RC | 193 | 9 | 2.003738 | 1406.5183,1406.4390,etc |
| advanced camera for surveys | ACS | 75 | 9 | 2.001637 | 1406.1707,1406.7531,etc |
| dwarf spheroidal | dSph | 75 | 9 | 2.000768 | 1406.2120,1406.0527,etc |
|