| active galactic nucleus | AGN | 2625 | 84 | 1.005853 | 1001.0756,1001.5206,etc |
| cosmic microwave background | CMB | 1272 | 77 | 1.002759 | 1001.4707,1001.0334,etc |
| spectral energy distribution | SED | 682 | 70 | 2.002101 | 1001.4828,1001.3688,etc |
| nasa/ipac extragalactic database | NED | 76 | 43 | 1.00031 | 1001.0334,1001.3998,etc |
| point spread function | PSF | 352 | 42 | 1.002935 | 1001.2183,1001.5162,etc |
| sloan digital sky survey | SDSS | 541 | 38 | 1.002859 | 1001.4707,1001.4828,etc |
| signal to noise ratio | SNR | 157 | 37 | 1.000804 | 1001.3074,1001.4555,etc |
| interstellar medium | ISM | 403 | 36 | 1.002239 | 1001.4903,1001.2141,etc |
| initial mass function | IMF | 929 | 28 | 1.004956 | 1001.2009,1001.0145,etc |
| supernova | SN | 1654 | 26 | 2.01151 | 1001.0145,1001.2141,etc |
| star formation rate | SFR | 337 | 25 | 2.002004 | 1001.2009,1001.3672,etc |
| cold dark matter | CDM | 336 | 25 | 1.002255 | 1001.1656,1001.5088,etc |
| full width at half maximum | FWHM | 111 | 24 | 1.001016 | 1001.3688,1001.1973,etc |
| asymptotic giant branch | AGB | 390 | 24 | 1.002632 | 1001.0145,1001.3672,etc |
| black hole | BH | 1072 | 23 | 2.00879 | 1001.2771,1001.3074,etc |
| near infrared | near-IR | 284 | 23 | 2.001647 | 1001.3688,1001.2141,etc |
| dark matter | DM | 593 | 23 | 2.006544 | 1001.1656,1001.2737,etc |
| gamma ray burst | GRB | 879 | 22 | 1.01077 | 1001.3688,1001.0598,etc |
| equation of state | EOS | 561 | 22 | 2.005396 | 1001.0575,1001.3577,etc |
| field of view | FOV | 112 | 21 | 1.000821 | 1001.0258,1001.0501,etc |
| large area telescope | LAT | 265 | 20 | 1.003489 | 1001.0059,1001.2958,etc |
| max planck institute for astronomy | MPIA | 19 | 19 | 1.000075 | 1001.4479,1001.2015,etc |
| max planck institute for astrophysics | MPA | 21 | 19 | 1.000084 | 1001.4479,1001.2015,etc |
| infrared | IR | 936 | 18 | 2.006333 | 1001.1668,1001.4634,etc |
| supernova remnant | SNR | 511 | 18 | 1.004709 | 1001.2606,1001.5150,etc |
| equivalent width | EW | 102 | 17 | 2.000941 | 1001.3688,1001.2108,etc |
| very large array | VLA | 177 | 17 | 2.001757 | 1001.3998,1001.0173,etc |
| hubble space telescope | HST | 144 | 17 | 2.001356 | 1001.5070,1001.1737,etc |
| low frequency instrument | LFI | 601 | 15 | 2.002823 | 1001.4646,1001.4787,etc |
| wilkinson microwave anisotropy probe | WMAP | 311 | 15 | 1.008172 | 1001.1790,1001.4635,etc |
| ultraviolet | UV | 431 | 14 | 2.004662 | 1001.2141,1001.4634,etc |
| signal to noise | S/N | 44 | 14 | 1.00022 | 1001.2141,1001.3687,etc |
| kolmogorov smirnov | K-S | 46 | 14 | 1.0004 | 1001.4479,1001.3415,etc |
| intergalactic medium | IGM | 318 | 14 | 2.003905 | 1001.4127,1001.3415,etc |
| white dwarf | WD | 365 | 13 | 2.006966 | 1001.0145,1001.1668,etc |
| big bang nucleosynthesis | BBN | 169 | 13 | 1.003659 | 1001.5088,1001.1790,etc |
| magnetohydrodynamic | MHD | 124 | 13 | 2.001374 | 1001.1973,1001.2606,etc |
| globular cluster | GC | 906 | 13 | 2.011945 | 1001.1790,1001.0979,etc |
| star formation history | SFH | 99 | 12 | 1.001677 | 1001.2009,1001.2141,etc |
| smoothed particle hydrodynamics | SPH | 67 | 12 | 1.00041 | 1001.3417,1001.3612,etc |
| intracluster medium | ICM | 198 | 12 | 2.002664 | 1001.1443,1001.4127,etc |
| luminosity function | LF | 337 | 12 | 2.005086 | 1001.2168,1001.2015,etc |
| large magellanic cloud | LMC | 283 | 12 | 2.003464 | 1001.0983,1001.2169,etc |
| advanced camera for surveys | ACS | 65 | 11 | 2.000575 | 1001.2141,1001.1161,etc |
| adaptive mesh refinement | AMR | 57 | 11 | 2.000625 | 1001.0575,1001.0971,etc |
| markov chain monte carlo | MCMC | 103 | 11 | 1.001417 | 1001.4639,1001.0501,etc |
| planetary nebula | PN | 404 | 11 | 2.007719 | 1001.0876,1001.0799,etc |
| color magnitude diagram | CMD | 190 | 11 | 2.001694 | 1001.1161,1001.4442,etc |
| line of sight | LOS | 116 | 11 | 1.000643 | 1001.1924,1001.2434,etc |
| low mass x ray binary | LMXB | 114 | 10 | 1.001255 | 1001.3688,1001.5410,etc |
| synchrotron self compton | SSC | 97 | 10 | 1.001612 | 1001.1606,1001.2590,etc |
| neutron star | NS | 172 | 10 | 1.00295 | 1001.3074,1001.2583,etc |
| red giant branch | RGB | 147 | 10 | 2.002135 | 1001.5412,1001.1395,etc |
| supermassive black hole | SMBH | 216 | 10 | 2.003093 | 1001.1680,1001.2480,etc |
| principal component analysis | PCA | 83 | 10 | 1.002901 | 1001.2480,1001.4551,etc |
| pre main sequence | PMS | 148 | 10 | 2.002452 | 1001.5141,1001.4825,etc |
| adaptive optics | AO | 69 | 10 | 2.001205 | 1001.3577,1001.4825,etc |
| main sequence | MS | 268 | 10 | 1.005813 | 1001.1161,1001.2624,etc |
| weakly interacting massive particle | WIMP | 182 | 10 | 1.003111 | 1001.5408,1001.1381,etc |
| local thermodynamic equilibrium | LTE | 42 | 9 | 1.000598 | 1001.0334,1001.2775,etc |
| flat spectrum radio quasar | FSRQ | 129 | 9 | 2.00211 | 1001.5206,1001.1606,etc |
| inverse compton | IC | 212 | 9 | 1.004095 | 1001.5206,1001.5150,etc |
| far infrared | FIR | 93 | 9 | 2.001142 | 1001.0896,1001.1419,etc |
| baryon acoustic oscillations | BAO | 146 | 9 | 2.003347 | 1001.5088,1001.2015,etc |
| brightest cluster galaxy | BCG | 449 | 9 | 1.006945 | 1001.3115,1001.2168,etc |
| star formation | SF | 247 | 9 | 2.002998 | 1001.1871,1001.0799,etc |
| very large telescope | VLT | 36 | 9 | 1.000738 | 1001.4825,1001.4080,etc |
| large scale structure | LSS | 63 | 8 | 2.001295 | 1001.4707,1001.5088,etc |
| japan society for the promotion of science | JSPS | 12 | 8 | 1.00137 | 1001.0145,1001.0005,etc |
| position angle | PA | 98 | 8 | 1.00247 | 1001.3998,1001.0698,etc |
| magnetohydrodynamics | MHD | 195 | 8 | 1.002448 | 1001.2857,1001.4046,etc |
| x ray telescope | XRT | 82 | 8 | 1.001843 | 1001.2989,1001.1296,etc |
| high frequency instrument | HFI | 65 | 8 | 2.001657 | 1001.4787,1001.4644,etc |
| data acquisition electronics | DAE | 47 | 8 | 2.000659 | 1001.4787,1001.4644,etc |
| friends of friends | FOF | 55 | 8 | 2.000778 | 1001.3115,1001.3447,etc |
| cross correlation function | CCF | 40 | 8 | 1.000474 | 1001.0356,1001.1426,etc |
| cosmic ray | CR | 359 | 8 | 2.005222 | 1001.5150,1001.1419,etc |
| radial velocity | RV | 403 | 8 | 2.006603 | 1001.3892,1001.0043,etc |
| large synoptic survey telescope | LSST | 39 | 8 | 1.000776 | 1001.2772,1001.2991,etc |
| probability density function | PDF | 93 | 7 | 2.00147 | 1001.4707,1001.2183,etc |
| friedmann robertson walker | FRW | 21 | 7 | 1.00032 | 1001.3125,1001.1155,etc |
| probability distribution function | PDF | 47 | 7 | 1.001187 | 1001.2009,1001.2141,etc |
| cosmic microwave background radiation | CMBR | 27 | 7 | 1.00054 | 1001.3998,1001.5110,etc |
| intra cluster medium | ICM | 119 | 7 | 2.003976 | 1001.1656,1001.1356,etc |
| extragalactic background light | EBL | 146 | 7 | 2.004801 | 1001.0896,1001.0770,etc |
| very high energy | VHE | 92 | 7 | 2.002058 | 1001.1606,1001.2590,etc |
| gravitational wave | GW | 285 | 7 | 1.004305 | 1001.3951,1001.2583,etc |
| nordic optical telescope | NOT | 27 | 7 | 1.000971 | 1001.0501,1001.0913,etc |
| general relativity | GR | 102 | 7 | 2.001661 | 1001.4704,1001.4733,etc |
| monte carlo | MC | 52 | 7 | 2.000949 | 1001.2590,1001.2105,etc |
| radiometer chain assembly | RCA | 69 | 7 | 2.002193 | 1001.4787,1001.4644,etc |
| simple stellar population | SSP | 45 | 7 | 1.001819 | 1001.0979,1001.2624,etc |
| magnetorotational instability | MRI | 119 | 7 | 2.003728 | 1001.3571,1001.1895,etc |
| cataclysmic variable | CV | 101 | 7 | 2.001 | 1001.1161,1001.1520,etc |
| three dimensional | 3D | 125 | 7 | 1.004874 | 1001.1046,1001.2043,etc |
| small magellanic cloud | SMC | 87 | 7 | 1.003645 | 1001.2169,1001.4442,etc |
| innermost stable circular orbit | ISCO | 62 | 7 | 2.001315 | 1001.0588,1001.1642,etc |
| association of universities for research in astronomy | AURA | 9 | 7 | 1.000155 | 1001.4442,1001.2991,etc |
| standard model | SM | 108 | 7 | 2.001346 | 1001.4936,1001.0969,etc |
| young stellar object | YSO | 119 | 7 | 2.000944 | 1001.4487,1001.5107,etc |
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