| cosmic microwave background | CMB | 1473 | 102 | 2.00375 | 1405.7399,1405.5360,etc |
| spectral energy distribution | SED | 1024 | 84 | 2.002082 | 1405.5416,1405.0927,etc |
| interstellar medium | ISM | 651 | 77 | 2.001557 | 1405.5487,1405.0062,etc |
| active galactic nucleus | AGN | 2056 | 74 | 1.006836 | 1405.5487,1405.5360,etc |
| point spread function | PSF | 429 | 60 | 1.001587 | 1405.4285,1405.1529,etc |
| star formation rate | SFR | 2113 | 57 | 2.004747 | 1405.5487,1405.0927,etc |
| initial mass function | IMF | 818 | 51 | 1.003609 | 1405.2338,1405.0927,etc |
| sloan digital sky survey | SDSS | 924 | 51 | 1.002248 | 1405.7410,1405.2934,etc |
| dark matter | DM | 2326 | 49 | 1.00705 | 1405.5738,1405.5181,etc |
| full width at half maximum | FWHM | 159 | 40 | 1.000476 | 1405.2160,1405.2934,etc |
| field of view | FoV | 202 | 40 | 2.000843 | 1405.0451,1405.4517,etc |
| nasa/ipac extragalactic database | NED | 120 | 39 | 1.000497 | 1405.4344,1405.5360,etc |
| supernova | SN | 1691 | 39 | 2.005492 | 1405.0062,1405.1417,etc |
| near infrared | NIR | 502 | 37 | 1.002134 | 1405.1456,1405.5284,etc |
| gamma ray burst | GRB | 2062 | 36 | 2.00754 | 1405.5487,1405.4331,etc |
| signal to noise ratio | SNR | 363 | 34 | 1.001407 | 1405.1529,1405.2338,etc |
| markov chain monte carlo | MCMC | 207 | 34 | 1.000766 | 1405.1417,1405.1072,etc |
| magnetohydrodynamic | MHD | 342 | 32 | 2.001978 | 1405.6382,1405.0942,etc |
| cold dark matter | CDM | 322 | 28 | 2.002644 | 1405.3178,1405.1039,etc |
| radial velocity | RV | 792 | 27 | 2.004218 | 1405.2887,1405.2929,etc |
| black hole | BH | 948 | 27 | 2.008759 | 1405.3696,1405.0249,etc |
| asymptotic giant branch | AGB | 619 | 26 | 1.002556 | 1405.0062,1405.0927,etc |
| milky way | MW | 674 | 25 | 2.004352 | 1405.7700,1405.5487,etc |
| ultraviolet | UV | 1091 | 25 | 2.008473 | 1405.4344,1405.2085,etc |
| equivalent width | EW | 328 | 24 | 1.001351 | 1405.1072,1405.2645,etc |
| hubble space telescope | HST | 170 | 23 | 2.001062 | 1405.7823,1405.1529,etc |
| supermassive black hole | SMBH | 598 | 23 | 1.006765 | 1405.5360,1405.0474,etc |
| globular cluster | GC | 1683 | 22 | 2.0082 | 1405.7823,1405.4344,etc |
| signal to noise | S/N | 209 | 22 | 2.000706 | 1405.4344,1405.3552,etc |
| general relativity | GR | 309 | 22 | 2.002179 | 1405.2896,1405.5476,etc |
| white dwarf | WD | 540 | 22 | 2.003785 | 1405.0062,1405.1426,etc |
| standard model | SM | 457 | 22 | 1.002592 | 1405.5738,1405.7679,etc |
| neutron star | NS | 550 | 22 | 2.005283 | 1405.2663,1405.0249,etc |
| main sequence | MS | 714 | 21 | 2.002078 | 1405.0739,1405.0639,etc |
| infrared | IR | 956 | 21 | 2.006585 | 1405.4517,1405.5387,etc |
| supernova remnant | SNR | 521 | 20 | 1.004727 | 1405.2835,1405.0557,etc |
| line of sight | LOS | 264 | 20 | 2.001056 | 1405.0871,1405.1751,etc |
| very large telescope | VLT | 67 | 20 | 1.000534 | 1405.6966,1405.1936,etc |
| local thermodynamic equilibrium | LTE | 279 | 19 | 2.001675 | 1405.0236,1405.6966,etc |
| kolmogorov smirnov | KS | 88 | 18 | 1.000918 | 1405.7823,1405.0763,etc |
| intergalactic medium | IGM | 306 | 18 | 1.002149 | 1405.5487,1405.2085,etc |
| smoothed particle hydrodynamics | SPH | 101 | 18 | 1.001072 | 1405.3178,1405.3984,etc |
| large magellanic cloud | LMC | 222 | 17 | 1.003307 | 1405.1035,1405.1274,etc |
| very large array | VLA | 199 | 17 | 1.002377 | 1405.3308,1405.6986,etc |
| red giant branch | RGB | 287 | 17 | 1.001445 | 1405.0062,1405.6729,etc |
| large area telescope | LAT | 123 | 17 | 2.001065 | 1405.4168,1405.6074,etc |
| adaptive optics | AO | 214 | 17 | 1.004017 | 1405.2932,1405.1493,etc |
| three dimensional | 3-D | 153 | 17 | 2.00216 | 1405.2790,1405.0951,etc |
| cosmic ray | CR | 483 | 16 | 1.007099 | 1405.5487,1405.0557,etc |
| equation of state | EoS | 192 | 16 | 2.002187 | 1405.7834,1405.2663,etc |
| young stellar object | YSO | 173 | 16 | 2.001904 | 1405.4494,1405.7492,etc |
| probability distribution function | PDF | 242 | 15 | 1.001863 | 1405.7700,1405.0871,etc |
| color magnitude diagram | CMD | 131 | 15 | 1.001795 | 1405.5750,1405.2929,etc |
| one dimensional | 1D | 160 | 15 | 2.001242 | 1405.0236,1405.3450,etc |
| adaptive mesh refinement | AMR | 35 | 14 | 1.000409 | 1405.2085,1405.4873,etc |
| star formation | SF | 532 | 14 | 1.0057 | 1405.0927,1405.3178,etc |
| broad line region | BLR | 135 | 14 | 2.001181 | 1405.1869,1405.4168,etc |
| two dimensional | 2-D | 101 | 14 | 2.001754 | 1405.2790,1405.0331,etc |
| low mass x ray binary | LMXB | 93 | 13 | 2.000753 | 1405.2663,1405.3495,etc |
| inverse compton | IC | 192 | 13 | 2.002778 | 1405.5647,1405.6074,etc |
| two micron all sky survey | 2MASS | 95 | 13 | 2.001285 | 1405.4168,1405.4517,etc |
| mikulski archive for space telescopes | MAST | 37 | 13 | 1.000253 | 1405.1493,1405.0222,etc |
| weakly interacting massive particle | WIMP | 172 | 13 | 1.002918 | 1405.1030,1405.5999,etc |
| galactic center | GC | 314 | 13 | 2.001733 | 1405.7691,1405.7710,etc |
| large scale structure | LSS | 70 | 12 | 1.001458 | 1405.1844,1405.1039,etc |
| zero age main sequence | ZAMS | 25 | 12 | 1.000253 | 1405.0062,1405.0236,etc |
| star formation history | SFH | 304 | 12 | 2.005265 | 1405.0927,1405.1049,etc |
| gravitational wave | GW | 357 | 12 | 2.007471 | 1405.0249,1405.2072,etc |
| small magellanic cloud | SMC | 287 | 12 | 1.002946 | 1405.7788,1405.1274,etc |
| giant molecular cloud | GMC | 174 | 11 | 2.002618 | 1405.5487,1405.5884,etc |
| friedmann robertson walker | FRW | 67 | 11 | 1.000796 | 1405.7834,1405.6301,etc |
| max planck institute for astronomy | MPIA | 11 | 11 | 1.000058 | 1405.2160,1405.1072,etc |
| max planck institute for astrophysics | MPA | 14 | 11 | 1.000076 | 1405.2160,1405.5573,etc |
| australia telescope compact array | ATCA | 43 | 11 | 1.000398 | 1405.3495,1405.7788,etc |
| coronal mass ejection | CME | 418 | 11 | 2.008846 | 1405.3450,1405.6088,etc |
| infrared array camera | IRAC | 58 | 11 | 1.000319 | 1405.5284,1405.5387,etc |
| innermost stable circular orbit | ISCO | 158 | 11 | 1.001876 | 1405.2072,1405.6750,etc |
| navarro frenk white | NFW | 43 | 11 | 1.001404 | 1405.2072,1405.5013,etc |
| european southern observatory | ESO | 54 | 11 | 2.000371 | 1405.0299,1405.0511,etc |
| local standard of rest | LSR | 26 | 11 | 1.000252 | 1405.0639,1405.7266,etc |
| dwarf spheroidal | dSph | 177 | 10 | 2.002371 | 1405.7823,1405.1443,etc |
| wide field camera 3 | WFC3 | 127 | 10 | 2.00148 | 1405.1056,1405.5387,etc |
| submillimeter array | SMA | 137 | 10 | 2.001354 | 1405.4331,1405.0821,etc |
| planetary nebula | PN | 374 | 10 | 2.007751 | 1405.0062,1405.1274,etc |
| roche lobe overflow | RLOF | 56 | 10 | 1.001314 | 1405.0062,1405.2374,etc |
| cosmic infrared background | CIB | 246 | 10 | 2.007333 | 1405.0871,1405.0872,etc |
| polycyclic aromatic hydrocarbon | PAH | 259 | 10 | 1.002323 | 1405.4872,1405.1274,etc |
| baryon acoustic oscillation | BAO | 98 | 10 | 2.001685 | 1405.1072,1405.1432,etc |
| far infrared | FIR | 173 | 10 | 1.003676 | 1405.5387,1405.6074,etc |
| brightest cluster galaxy | BCG | 333 | 10 | 2.007455 | 1405.2072,1405.3412,etc |
| probability density function | PDF | 119 | 10 | 1.002209 | 1405.5383,1405.2638,etc |
| full width half maximum | FWHM | 45 | 10 | 1.000665 | 1405.0160,1405.6542,etc |
| wolf rayet | WR | 256 | 10 | 2.004429 | 1405.1423,1405.1205,etc |
| wide field infrared survey explorer | WISE | 341 | 10 | 1.005621 | 1405.7350,1405.0511,etc |
| dark energy survey | DES | 90 | 9 | 1.001091 | 1405.4285,1405.1035,etc |
| luminosity function | LF | 156 | 9 | 1.005812 | 1405.0062,1405.0802,etc |
| advanced camera for surveys | ACS | 327 | 9 | 2.007308 | 1405.7410,1405.7055,etc |
| high mass x ray binary | HMXB | 67 | 9 | 2.001353 | 1405.3495,1405.4833,etc |
| intracluster medium | ICM | 80 | 9 | 1.001317 | 1405.0557,1405.3412,etc |
| confidence level | CL | 36 | 9 | 1.002057 | 1405.1390,1405.1030,etc |
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