| spectral energy distribution | SED | 1548 | 98 | 2.002009 | 1403.4089,1403.4250,etc |
| cosmic microwave background | CMB | 1184 | 95 | 2.002983 | 1403.3697,1403.4089,etc |
| interstellar medium | ISM | 917 | 87 | 2.001859 | 1403.6597,1403.0155,etc |
| active galactic nucleus | AGN | 2904 | 77 | 1.005408 | 1403.5308,1403.4961,etc |
| point spread function | PSF | 683 | 66 | 2.003206 | 1403.5372,1403.4250,etc |
| initial mass function | IMF | 413 | 56 | 1.002484 | 1403.3619,1403.3417,etc |
| sloan digital sky survey | SDSS | 987 | 55 | 1.00213 | 1403.5461,1403.1578,etc |
| star formation rate | SFR | 1897 | 55 | 2.004797 | 1403.1578,1403.0853,etc |
| signal to noise ratio | SNR | 400 | 45 | 2.001019 | 1403.5307,1403.4250,etc |
| near infrared | NIR | 525 | 44 | 1.001651 | 1403.3141,1403.3120,etc |
| dark matter | DM | 1806 | 43 | 2.006833 | 1403.3697,1403.8115,etc |
| supernova | SN | 2837 | 43 | 2.011493 | 1403.3141,1403.4250,etc |
| ultraviolet | UV | 964 | 35 | 1.004567 | 1403.6597,1403.0155,etc |
| markov chain monte carlo | MCMC | 180 | 35 | 2.000993 | 1403.1879,1403.1875,etc |
| full width at half maximum | FWHM | 192 | 33 | 1.000789 | 1403.5308,1403.5307,etc |
| asymptotic giant branch | AGB | 911 | 33 | 1.005578 | 1403.2892,1403.3087,etc |
| infrared | IR | 1717 | 31 | 2.004371 | 1403.4088,1403.4089,etc |
| field of view | FoV | 180 | 31 | 2.00123 | 1403.2586,1403.7925,etc |
| equation of state | EOS | 529 | 30 | 1.003577 | 1403.3096,1403.5301,etc |
| standard model | SM | 543 | 28 | 2.002296 | 1403.3697,1403.3219,etc |
| signal to noise | S/N | 201 | 28 | 1.000937 | 1403.4088,1403.3120,etc |
| cold dark matter | CDM | 465 | 28 | 2.002877 | 1403.1578,1403.1089,etc |
| general relativity | GR | 419 | 26 | 2.001443 | 1403.7251,1403.6115,etc |
| equivalent width | EW | 370 | 26 | 2.001372 | 1403.4088,1403.4250,etc |
| nasa/ipac extragalactic database | NED | 41 | 26 | 1.000131 | 1403.7555,1403.7089,etc |
| supernova remnant | SNR | 1011 | 26 | 2.010134 | 1403.6878,1403.5152,etc |
| polycyclic aromatic hydrocarbon | PAH | 328 | 23 | 2.004508 | 1403.5308,1403.5307,etc |
| very large array | VLA | 161 | 23 | 1.001173 | 1403.1907,1403.0882,etc |
| red giant branch | RGB | 166 | 23 | 1.001579 | 1403.3141,1403.2892,etc |
| main sequence | MS | 383 | 23 | 2.002165 | 1403.3141,1403.4764,etc |
| mid infrared | MIR | 207 | 22 | 1.002014 | 1403.1450,1403.4941,etc |
| gamma ray burst | GRB | 988 | 22 | 2.008019 | 1403.3825,1403.5661,etc |
| local thermodynamic equilibrium | LTE | 302 | 21 | 1.00405 | 1403.6245,1403.6461,etc |
| cosmic ray | CR | 721 | 21 | 2.005281 | 1403.2586,1403.4089,etc |
| white dwarf | WD | 601 | 21 | 1.00471 | 1403.4335,1403.4723,etc |
| intergalactic medium | IGM | 349 | 21 | 1.001668 | 1403.1261,1403.0325,etc |
| far infrared | FIR | 319 | 20 | 2.001687 | 1403.5308,1403.5307,etc |
| neutron star | NS | 662 | 20 | 2.006445 | 1403.5152,1403.5301,etc |
| line of sight | LOS | 255 | 19 | 1.001634 | 1403.7976,1403.0588,etc |
| black hole | BH | 605 | 19 | 1.006945 | 1403.5301,1403.7034,etc |
| planetary nebula | PN | 937 | 19 | 2.005835 | 1403.4723,1403.6715,etc |
| radial velocity | RV | 337 | 18 | 2.002869 | 1403.5564,1403.6841,etc |
| probability distribution function | PDF | 339 | 18 | 1.004824 | 1403.1578,1403.0454,etc |
| low mass x ray binary | LMXB | 153 | 18 | 2.000989 | 1403.4624,1403.7204,etc |
| big bang nucleosynthesis | BBN | 253 | 17 | 1.001757 | 1403.3697,1403.4909,etc |
| two micron all sky survey | 2MASS | 116 | 17 | 1.000957 | 1403.7925,1403.0813,etc |
| supermassive black hole | SMBH | 179 | 17 | 1.00127 | 1403.5555,1403.3933,etc |
| gravitational wave | GW | 479 | 16 | 2.004655 | 1403.5301,1403.6068,etc |
| hubble space telescope | HST | 139 | 16 | 1.001633 | 1403.1408,1403.6708,etc |
| lyman break galaxy | LBG | 319 | 16 | 1.002675 | 1403.3078,1403.4360,etc |
| magnetohydrodynamic | MHD | 197 | 15 | 2.002186 | 1403.6027,1403.0901,etc |
| large magellanic cloud | LMC | 287 | 15 | 2.002835 | 1403.3141,1403.4335,etc |
| color magnitude diagram | CMD | 192 | 15 | 2.002723 | 1403.3141,1403.6325,etc |
| globular cluster | GC | 874 | 15 | 2.005767 | 1403.3141,1403.4624,etc |
| large scale structure | LSS | 107 | 15 | 2.001281 | 1403.5555,1403.7958,etc |
| luminosity function | LF | 577 | 15 | 2.004621 | 1403.3938,1403.5563,etc |
| root mean square | RMS | 72 | 15 | 1.000643 | 1403.2621,1403.0644,etc |
| smoothed particle hydrodynamics | SPH | 63 | 14 | 1.000723 | 1403.1907,1403.1589,etc |
| three dimensional | 3D | 168 | 14 | 2.002776 | 1403.1907,1403.6245,etc |
| kolmogorov smirnov | KS | 83 | 14 | 1.000352 | 1403.3141,1403.5886,etc |
| broad line region | BLR | 217 | 14 | 1.002801 | 1403.3078,1403.7534,etc |
| probability density function | PDF | 275 | 13 | 2.003361 | 1403.5307,1403.1368,etc |
| young stellar object | YSO | 638 | 13 | 2.005437 | 1403.4088,1403.4663,etc |
| zero age main sequence | ZAMS | 42 | 13 | 2.000517 | 1403.7925,1403.2731,etc |
| very large telescope | VLT | 59 | 13 | 1.000294 | 1403.0813,1403.4046,etc |
| interstellar radiation field | ISRF | 53 | 13 | 2.000363 | 1403.1987,1403.4915,etc |
| star formation history | SFH | 453 | 13 | 2.003749 | 1403.1408,1403.2185,etc |
| integral field unit | IFU | 86 | 13 | 2.000642 | 1403.0040,1403.6840,etc |
| adaptive mesh refinement | AMR | 33 | 12 | 1.000245 | 1403.1907,1403.5152,etc |
| brightest cluster galaxy | BCG | 485 | 12 | 2.004975 | 1403.3063,1403.4249,etc |
| coronal mass ejection | CME | 315 | 12 | 1.00662 | 1403.4088,1403.6964,etc |
| very high energy | VHE | 71 | 12 | 2.000742 | 1403.2586,1403.4915,etc |
| two dimensional | 2D | 120 | 12 | 2.002186 | 1403.6115,1403.7555,etc |
| adaptive optics | AO | 148 | 12 | 1.004928 | 1403.4250,1403.6708,etc |
| weakly interacting massive particle | WIMP | 672 | 12 | 2.004715 | 1403.8115,1403.5421,etc |
| south pole telescope | SPT | 39 | 12 | 1.00037 | 1403.5886,1403.3402,etc |
| canada france hawaii telescope | CFHT | 179 | 12 | 2.002154 | 1403.1879,1403.3692,etc |
| max planck institute for astronomy | MPIA | 13 | 12 | 1.000047 | 1403.3166,1403.7836,etc |
| max planck institute for astrophysics | MPA | 17 | 12 | 1.000076 | 1403.3166,1403.7836,etc |
| giant molecular cloud | GMC | 122 | 12 | 1.001152 | 1403.7098,1403.2576,etc |
| large area telescope | LAT | 210 | 11 | 1.00188 | 1403.4961,1403.6878,etc |
| horizontal branch | HB | 271 | 11 | 2.002713 | 1403.3141,1403.1536,etc |
| full width half maximum | FWHM | 35 | 11 | 2.000178 | 1403.2892,1403.1432,etc |
| specific star formation rate | sSFR | 278 | 11 | 2.00311 | 1403.1578,1403.3856,etc |
| monte carlo | MC | 127 | 11 | 1.002912 | 1403.1089,1403.0588,etc |
| orion nebula cluster | ONC | 115 | 11 | 1.001639 | 1403.8099,1403.7047,etc |
| position angle | PA | 113 | 11 | 1.000791 | 1403.1463,1403.4723,etc |
| milky way | MW | 146 | 11 | 2.001926 | 1403.6708,1403.4335,etc |
| star formation | SF | 156 | 10 | 2.002686 | 1403.5308,1403.5265,etc |
| national research council | NRC | 17 | 10 | 1.000144 | 1403.0882,1403.1879,etc |
| centre national de la recherche scientifique | CNRS | 27 | 10 | 1.000637 | 1403.0882,1403.4945,etc |
| one dimensional | 1D | 27 | 10 | 1.000385 | 1403.6245,1403.7555,etc |
| baryon acoustic oscillation | BAO | 192 | 10 | 2.002139 | 1403.4599,1403.2571,etc |
| japan society for the promotion of science | JSPS | 15 | 10 | 1.000245 | 1403.4599,1403.0040,etc |
| inverse compton | IC | 206 | 10 | 2.002985 | 1403.1987,1403.7534,etc |
| atacama large millimeter/submillimeter array | ALMA | 196 | 10 | 2.00228 | 1403.3436,1403.5853,etc |
| principal component analysis | PCA | 149 | 10 | 2.002777 | 1403.6964,1403.4141,etc |
| wolf rayet | WR | 156 | 10 | 2.00448 | 1403.6708,1403.2731,etc |
| wide field infrared survey explorer | WISE | 238 | 10 | 2.003956 | 1403.7047,1403.2561,etc |
| atacama cosmology telescope | ACT | 117 | 10 | 1.006972 | 1403.3361,1403.5277,etc |
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