| spectral energy distribution | SED | 834 | 63 | 2.002137 | 0812.2951,0812.1500,etc |
| cosmic microwave background | CMB | 566 | 60 | 1.001782 | 0812.2023,0812.3421,etc |
| active galactic nucleus | AGN | 1713 | 53 | 2.007147 | 0812.3312,0812.0810,etc |
| interstellar medium | ISM | 553 | 47 | 2.002412 | 0812.2023,0812.3235,etc |
| sloan digital sky survey | SDSS | 606 | 40 | 2.00431 | 0812.3043,0812.2586,etc |
| supernova | SN | 1118 | 33 | 1.009018 | 0812.2150,0812.4016,etc |
| gamma ray burst | GRB | 1714 | 32 | 1.008538 | 0812.4677,0812.3913,etc |
| star formation rate | SFR | 532 | 29 | 2.003074 | 0812.3409,0812.2913,etc |
| point spread function | PSF | 245 | 28 | 1.001732 | 0812.3827,0812.2125,etc |
| dark matter | DM | 1198 | 26 | 2.008297 | 0812.4016,0812.0808,etc |
| signal to noise ratio | S/N | 150 | 24 | 2.000924 | 0812.1010,0812.2586,etc |
| initial mass function | IMF | 161 | 22 | 1.001461 | 0812.2915,0812.1417,etc |
| intergalactic medium | IGM | 172 | 21 | 2.001983 | 0812.2052,0812.4904,etc |
| equation of state | EoS | 502 | 19 | 2.005184 | 0812.5021,0812.1850,etc |
| field of view | FOV | 114 | 19 | 1.001 | 0812.2975,0812.2283,etc |
| cold dark matter | CDM | 275 | 19 | 2.002886 | 0812.4904,0812.3912,etc |
| asymptotic giant branch | AGB | 314 | 18 | 1.003005 | 0812.2060,0812.3265,etc |
| ultraviolet | UV | 367 | 18 | 2.004775 | 0812.2913,0812.2812,etc |
| supernova remnant | SNR | 379 | 16 | 2.005371 | 0812.2186,0812.1448,etc |
| black hole | BH | 680 | 16 | 2.006711 | 0812.3995,0812.2915,etc |
| magnetohydrodynamic | MHD | 217 | 15 | 2.002196 | 0812.2023,0812.2836,etc |
| inverse compton | IC | 296 | 15 | 2.002396 | 0812.1500,0812.3235,etc |
| big bang nucleosynthesis | BBN | 166 | 15 | 1.002804 | 0812.4016,0812.3745,etc |
| very large array | VLA | 94 | 15 | 2.001075 | 0812.3327,0812.0281,etc |
| nasa/ipac extragalactic database | NED | 48 | 15 | 1.000396 | 0812.2022,0812.2088,etc |
| full width at half maximum | FWHM | 52 | 15 | 1.000752 | 0812.1920,0812.4213,etc |
| near infrared | NIR | 79 | 14 | 2.000653 | 0812.0880,0812.2034,etc |
| max planck institute for astrophysics | MPA | 26 | 12 | 1.000913 | 0812.1220,0812.1224,etc |
| smoothed particle hydrodynamics | SPH | 200 | 12 | 2.002183 | 0812.2913,0812.0304,etc |
| polycyclic aromatic hydrocarbon | PAH | 275 | 12 | 2.005711 | 0812.0450,0812.3664,etc |
| very large telescope | VLT | 34 | 12 | 1.000385 | 0812.2815,0812.3402,etc |
| hubble space telescope | HST | 59 | 12 | 2.000516 | 0812.2360,0812.1844,etc |
| far infrared | FIR | 137 | 11 | 2.001513 | 0812.2023,0812.1417,etc |
| signal to noise | S/N | 48 | 11 | 1.000601 | 0812.1960,0812.0281,etc |
| max planck institute for astronomy | MPIA | 11 | 11 | 1.000084 | 0812.1220,0812.1224,etc |
| supermassive black hole | SMBH | 222 | 11 | 2.004861 | 0812.4473,0812.2756,etc |
| quasi periodic oscillation | QPO | 157 | 10 | 2.005119 | 0812.2417,0812.4751,etc |
| equivalent width | EW | 105 | 10 | 1.001407 | 0812.2626,0812.2510,etc |
| cosmic ray | CR | 478 | 10 | 2.004129 | 0812.2150,0812.3576,etc |
| line of sight | LOS | 55 | 10 | 1.001344 | 0812.2150,0812.1920,etc |
| standard model | SM | 162 | 10 | 1.001613 | 0812.4624,0812.2196,etc |
| weakly interacting massive particle | WIMP | 197 | 10 | 2.003101 | 0812.1150,0812.3598,etc |
| main sequence | MS | 114 | 10 | 1.004996 | 0812.0285,0812.1027,etc |
| markov chain monte carlo | MCMC | 92 | 10 | 1.001755 | 0812.4016,0812.0632,etc |
| probability distribution function | PDF | 113 | 10 | 1.002618 | 0812.2125,0812.3662,etc |
| friedmann robertson walker | FRW | 73 | 10 | 2.001327 | 0812.4904,0812.5108,etc |
| advanced camera for surveys | ACS | 107 | 10 | 2.001074 | 0812.2283,0812.1668,etc |
| star formation | SF | 253 | 10 | 2.007437 | 0812.0427,0812.1226,etc |
| pre main sequence | PMS | 124 | 9 | 2.003042 | 0812.1960,0812.3664,etc |
| young stellar object | YSO | 86 | 9 | 2.001272 | 0812.3849,0812.2360,etc |
| large scale structure | LSS | 58 | 9 | 2.001536 | 0812.4016,0812.0013,etc |
| baryon acoustic oscillation | BAO | 109 | 9 | 2.005401 | 0812.3500,0812.0521,etc |
| giant molecular cloud | GMC | 213 | 9 | 1.005138 | 0812.3733,0812.3080,etc |
| infrared | IR | 226 | 9 | 2.006639 | 0812.2601,0812.1964,etc |
| luminous red galaxy | LRG | 233 | 8 | 1.005635 | 0812.3831,0812.1406,etc |
| large area telescope | LAT | 97 | 8 | 2.002838 | 0812.2908,0812.3598,etc |
| low mass x ray binary | LMXB | 33 | 8 | 1.000616 | 0812.4751,0812.2815,etc |
| white dwarf | WD | 311 | 8 | 2.005538 | 0812.0791,0812.3995,etc |
| very long baseline array | VLBA | 37 | 8 | 1.001248 | 0812.3327,0812.1156,etc |
| local thermodynamic equilibrium | LTE | 29 | 8 | 1.000417 | 0812.2125,0812.0450,etc |
| neutron star | NS | 282 | 8 | 2.004389 | 0812.3995,0812.2815,etc |
| general relativity | GR | 96 | 8 | 2.00238 | 0812.0013,0812.2244,etc |
| wilkinson microwave anisotropy probe | WMAP | 71 | 8 | 1.001373 | 0812.2244,0812.1253,etc |
| kolmogorov smirnov | KS | 70 | 8 | 1.000896 | 0812.4780,0812.3733,etc |
| canada france hawaii telescope | CFHT | 47 | 8 | 2.00149 | 0812.0521,0812.2788,etc |
| magneto rotational instability | MRI | 45 | 8 | 2.000503 | 0812.2068,0812.4925,etc |
| color magnitude diagram | CMD | 119 | 8 | 2.002526 | 0812.1668,0812.0911,etc |
| x ray telescope | XRT | 133 | 7 | 2.001408 | 0812.1500,0812.4677,etc |
| advanced ccd imaging spectrometer | ACIS | 31 | 7 | 1.000496 | 0812.2186,0812.3598,etc |
| proportional counter array | PCA | 47 | 7 | 1.000996 | 0812.4519,0812.0810,etc |
| fast fourier transform | FFT | 33 | 7 | 1.000732 | 0812.2975,0812.1052,etc |
| horizontal branch | HB | 115 | 7 | 2.001536 | 0812.4411,0812.1974,etc |
| red giant branch | RGB | 32 | 7 | 1.000477 | 0812.4541,0812.1027,etc |
| small magellanic cloud | SMC | 110 | 7 | 2.001742 | 0812.1448,0812.3080,etc |
| gravitational wave | GW | 139 | 7 | 2.004919 | 0812.3656,0812.2721,etc |
| luminosity function | LF | 228 | 7 | 2.006001 | 0812.1668,0812.0427,etc |
| synchrotron self compton | SSC | 39 | 7 | 2.001404 | 0812.1217,0812.0021,etc |
| large magellanic cloud | LMC | 190 | 7 | 2.002569 | 0812.4925,0812.1226,etc |
| dark energy | DE | 252 | 7 | 2.002758 | 0812.0002,0812.3901,etc |
| probability density function | PDF | 48 | 6 | 2.002088 | 0812.2023,0812.3260,etc |
| position angle | PA | 54 | 6 | 1.001192 | 0812.3444,0812.1417,etc |
| integrated sachs wolfe | ISW | 117 | 6 | 1.004148 | 0812.4016,0812.2244,etc |
| lightest supersymmetric particle | LSP | 254 | 6 | 1.003682 | 0812.4016,0812.2196,etc |
| three dimensional | 3-D | 113 | 6 | 2.002754 | 0812.2949,0812.4400,etc |
| william herschel telescope | WHT | 39 | 6 | 1.000725 | 0812.2022,0812.2034,etc |
| two micron all sky survey | 2MASS | 217 | 6 | 1.004137 | 0812.0880,0812.2034,etc |
| lyman break galaxy | LBG | 245 | 6 | 1.005411 | 0812.0991,0812.5111,etc |
| galactic center | GC | 88 | 6 | 2.00307 | 0812.3576,0812.0865,etc |
| innermost stable circular orbit | ISCO | 54 | 6 | 2.000592 | 0812.2325,0812.0365,etc |
| intra cluster medium | ICM | 56 | 5 | 2.001552 | 0812.2052,0812.3598,etc |
| full width half maximum | FWHM | 18 | 5 | 1.000193 | 0812.2052,0812.3444,etc |
| collisional ionization equilibrium | CIE | 31 | 5 | 2.000808 | 0812.2186,0812.2020,etc |
| submillimeter array | SMA | 30 | 5 | 1.000453 | 0812.3444,0812.0991,etc |
| high mass x ray binary | HMXB | 113 | 5 | 2.002251 | 0812.2975,0812.4189,etc |
| korea science and engineering foundation | KOSEF | 5 | 5 | 1.000111 | 0812.1406,0812.2088,etc |
| kelvin helmholtz | KH | 26 | 5 | 2.000244 | 0812.2239,0812.1060,etc |
| cosmic microwave background radiation | CMBR | 10 | 5 | 1.000328 | 0812.0788,0812.1920,etc |
| x ray binary | XRB | 157 | 5 | 2.005321 | 0812.2815,0812.2788,etc |
| broad line region | BLR | 78 | 5 | 2.001049 | 0812.2283,0812.0251,etc |
| intermediate mass black hole | IMBH | 140 | 5 | 2.009757 | 0812.1402,0812.0984,etc |
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