| active galactic nucleus | AGN | 2664 | 89 | 1.005957 | 1305.6116,1305.5380,etc |
| spectral energy distribution | SED | 1066 | 86 | 2.001408 | 1305.2984,1305.3608,etc |
| point spread function | PSF | 606 | 75 | 2.001501 | 1305.1628,1305.7426,etc |
| cosmic microwave background | CMB | 699 | 72 | 1.002159 | 1305.1325,1305.0600,etc |
| interstellar medium | ISM | 538 | 54 | 2.001075 | 1305.7113,1305.5178,etc |
| dark matter | DM | 3083 | 49 | 2.010445 | 1305.7204,1305.5178,etc |
| sloan digital sky survey | SDSS | 775 | 44 | 2.003302 | 1305.6116,1305.2984,etc |
| nasa/ipac extragalactic database | NED | 78 | 43 | 1.00017 | 1305.7067,1305.7113,etc |
| signal to noise ratio | S/N | 321 | 43 | 1.001612 | 1305.6116,1305.2984,etc |
| star formation rate | SFR | 743 | 38 | 1.003209 | 1305.4791,1305.7113,etc |
| field of view | FOV | 161 | 36 | 2.000627 | 1305.2246,1305.1493,etc |
| initial mass function | IMF | 643 | 34 | 1.003968 | 1305.1325,1305.2273,etc |
| ultraviolet | UV | 780 | 32 | 1.003503 | 1305.0600,1305.0846,etc |
| hubble space telescope | HST | 252 | 30 | 1.000984 | 1305.7067,1305.1857,etc |
| full width at half maximum | FWHM | 136 | 30 | 1.000329 | 1305.0902,1305.5308,etc |
| signal to noise | S/N | 179 | 29 | 2.000695 | 1305.2273,1305.7113,etc |
| gamma ray burst | GRB | 1416 | 28 | 1.007356 | 1305.3194,1305.2530,etc |
| black hole | BH | 981 | 28 | 2.004313 | 1305.2199,1305.0565,etc |
| equivalent width | EW | 328 | 26 | 1.001514 | 1305.6116,1305.2984,etc |
| markov chain monte carlo | MCMC | 174 | 26 | 1.001204 | 1305.2130,1305.0055,etc |
| near infrared | near-IR | 323 | 26 | 2.001215 | 1305.6926,1305.6997,etc |
| supernova | SN | 1710 | 25 | 2.010039 | 1305.1325,1305.5178,etc |
| infrared | IR | 656 | 25 | 2.004164 | 1305.6926,1305.0846,etc |
| local thermodynamic equilibrium | LTE | 192 | 24 | 1.00293 | 1305.7067,1305.2371,etc |
| equation of state | EoS | 316 | 24 | 2.001836 | 1305.2530,1305.7101,etc |
| cold dark matter | CDM | 566 | 24 | 2.003727 | 1305.5178,1305.0823,etc |
| supermassive black hole | SBH | 268 | 22 | 1.001975 | 1305.1628,1305.4634,etc |
| red giant branch | RGB | 282 | 22 | 2.003196 | 1305.0846,1305.4837,etc |
| supernova remnant | SNR | 587 | 22 | 1.005858 | 1305.1845,1305.2354,etc |
| very large telescope | VLT | 85 | 21 | 1.000873 | 1305.0565,1305.1096,etc |
| standard model | SM | 454 | 20 | 2.002784 | 1305.0147,1305.0456,etc |
| very large array | VLA | 130 | 19 | 1.001755 | 1305.2941,1305.1509,etc |
| asymptotic giant branch | AGB | 213 | 19 | 2.003643 | 1305.1857,1305.5178,etc |
| polycyclic aromatic hydrocarbon | PAH | 340 | 18 | 2.003372 | 1305.6116,1305.5258,etc |
| intergalactic medium | IGM | 229 | 18 | 2.002718 | 1305.1325,1305.5178,etc |
| adaptive mesh refinement | AMR | 135 | 18 | 2.001541 | 1305.1325,1305.5178,etc |
| general relativity | GR | 158 | 18 | 2.001078 | 1305.0055,1305.7333,etc |
| magnetohydrodynamic | MHD | 263 | 17 | 2.002207 | 1305.5654,1305.2761,etc |
| color magnitude diagram | CMD | 234 | 17 | 2.001553 | 1305.1857,1305.7152,etc |
| kolmogorov smirnov | K-S | 67 | 17 | 2.000859 | 1305.6997,1305.6931,etc |
| milky way | MW | 272 | 17 | 2.001775 | 1305.7231,1305.0456,etc |
| broad line region | BLR | 226 | 17 | 2.001985 | 1305.3952,1305.2946,etc |
| large area telescope | LAT | 175 | 16 | 2.002817 | 1305.0302,1305.3217,etc |
| young stellar object | YSO | 224 | 16 | 1.002122 | 1305.2681,1305.1339,etc |
| coronal mass ejection | CME | 277 | 15 | 2.00315 | 1305.6980,1305.4039,etc |
| intracluster medium | ICM | 207 | 15 | 2.001808 | 1305.5654,1305.6617,etc |
| advanced camera for surveys | ACS | 171 | 15 | 1.002027 | 1305.0846,1305.0565,etc |
| large magellanic cloud | LMC | 331 | 15 | 2.003319 | 1305.7426,1305.4837,etc |
| burst alert telescope | BAT | 307 | 15 | 2.003798 | 1305.3165,1305.6611,etc |
| big bang nucleosynthesis | BBN | 76 | 15 | 2.001005 | 1305.0456,1305.5188,etc |
| star formation history | SFH | 223 | 14 | 1.003126 | 1305.4791,1305.2984,etc |
| globular cluster | GC | 639 | 14 | 2.005252 | 1305.5975,1305.3275,etc |
| weakly interacting massive particle | WIMP | 208 | 14 | 2.003065 | 1305.5178,1305.0302,etc |
| wilkinson microwave anisotropy probe | WMAP | 56 | 14 | 1.001184 | 1305.0055,1305.4464,etc |
| friedmann robertson walker | FRW | 89 | 13 | 1.002182 | 1305.0600,1305.0761,etc |
| far infrared | FIR | 242 | 13 | 2.002656 | 1305.7113,1305.2681,etc |
| position angle | PA | 144 | 13 | 2.005523 | 1305.6062,1305.4968,etc |
| smoothed particle hydrodynamics | SPH | 93 | 13 | 1.001021 | 1305.5178,1305.2913,etc |
| very high energy | VHE | 103 | 13 | 2.00152 | 1305.2761,1305.0312,etc |
| white dwarf | WD | 340 | 13 | 2.008931 | 1305.5245,1305.6925,etc |
| brightest cluster galaxy | BCG | 372 | 13 | 1.005125 | 1305.5254,1305.2420,etc |
| two micron all sky survey | 2MASS | 92 | 13 | 1.000744 | 1305.5035,1305.3679,etc |
| full width half maximum | FWHM | 60 | 12 | 1.000443 | 1305.7067,1305.6509,etc |
| line of sight | LOS | 167 | 12 | 2.002024 | 1305.6980,1305.1687,etc |
| main sequence | MS | 120 | 12 | 1.003934 | 1305.5975,1305.5178,etc |
| cosmic ray | CR | 298 | 12 | 1.005404 | 1305.5178,1305.1242,etc |
| cherenkov telescope array | CTA | 122 | 12 | 1.003421 | 1305.2761,1305.0264,etc |
| inverse compton | IC | 89 | 12 | 2.0015 | 1305.0286,1305.4032,etc |
| probability distribution function | PDF | 526 | 12 | 1.003673 | 1305.2345,1305.7486,etc |
| large scale structure | LSS | 52 | 11 | 2.000762 | 1305.4642,1305.0055,etc |
| mid infrared | MIR | 189 | 11 | 2.001594 | 1305.6116,1305.5258,etc |
| luminosity function | LF | 445 | 11 | 2.004518 | 1305.1630,1305.5308,etc |
| red supergiant | RSG | 220 | 11 | 2.002899 | 1305.3386,1305.6179,etc |
| radial velocity | RV | 272 | 11 | 2.002144 | 1305.1951,1305.5107,etc |
| cosmic microwave background radiation | CMBR | 129 | 10 | 2.005189 | 1305.6676,1305.1964,etc |
| active region | AR | 154 | 10 | 2.002943 | 1305.6980,1305.1687,etc |
| wide field camera 3 | WFC3 | 101 | 10 | 2.00132 | 1305.1628,1305.0565,etc |
| wolf rayet | WR | 128 | 10 | 1.001981 | 1305.5178,1305.2290,etc |
| synchrotron self compton | SSC | 99 | 10 | 2.002014 | 1305.5920,1305.2535,etc |
| deutsche forschungsgemeinschaft | DFG | 13 | 10 | 1.000088 | 1305.6982,1305.3909,etc |
| south pole telescope | SPT | 94 | 10 | 1.004105 | 1305.0055,1305.3921,etc |
| association of universities for research in astronomy | AURA | 11 | 10 | 1.000129 | 1305.0277,1305.5158,etc |
| small magellanic cloud | SMC | 255 | 10 | 2.0025 | 1305.7237,1305.2628,etc |
| max planck institute for astronomy | MPIA | 10 | 10 | 1.000044 | 1305.5308,1305.6154,etc |
| imaging atmospheric cherenkov telescope | IACT | 55 | 10 | 2.001028 | 1305.0312,1305.0022,etc |
| adaptive optics | AO | 91 | 10 | 2.001125 | 1305.0421,1305.0280,etc |
| extragalactic background light | EBL | 195 | 10 | 2.004983 | 1305.3217,1305.2162,etc |
| cosmic x ray background | CXB | 50 | 10 | 1.001776 | 1305.4901,1305.7452,etc |
| wide field infrared survey explorer | WISE | 169 | 9 | 1.003161 | 1305.6116,1305.5254,etc |
| canada france hawaii telescope | CFHT | 61 | 9 | 1.001138 | 1305.3608,1305.0268,etc |
| ultra high energy cosmic ray | UHECR | 112 | 9 | 2.001219 | 1305.2331,1305.2761,etc |
| probability density function | PDF | 79 | 9 | 2.001495 | 1305.5178,1305.2433,etc |
| one dimensional | 1-D | 98 | 9 | 1.002137 | 1305.6926,1305.2085,etc |
| three dimensional | 3-D | 146 | 9 | 1.003995 | 1305.6926,1305.5256,etc |
| colour magnitude diagram | CMD | 130 | 9 | 1.001066 | 1305.7426,1305.4837,etc |
| very long baseline array | VLBA | 132 | 9 | 2.001327 | 1305.2761,1305.4865,etc |
| galactic center | GC | 187 | 9 | 2.004479 | 1305.6921,1305.0302,etc |
| narrow line seyfert 1 | NLSy1 | 70 | 9 | 1.004059 | 1305.3273,1305.1096,etc |
| x ray telescope | XRT | 69 | 9 | 2.000985 | 1305.3165,1305.3217,etc |
| photon counting | PC | 38 | 9 | 1.000964 | 1305.3165,1305.5065,etc |
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