| max planck institute for astronomy | MPIA | 22 | 22 | 1.00005 | 0810.4144,0810.0780,etc |
| kolmogorov smirnov | KS | 58 | 16 | 1.000251 | 0810.4923,0810.1015,etc |
| very high energy | VHE | 143 | 16 | 2.003089 | 0810.0988,0810.4864,etc |
| synchrotron self compton | SSC | 78 | 15 | 1.000874 | 0810.4864,0810.2522,etc |
| signal to noise | S/N | 75 | 14 | 2.000459 | 0810.3648,0810.5311,etc |
| inverse compton | IC | 133 | 13 | 2.002895 | 0810.2784,0810.0988,etc |
| advanced camera for surveys | ACS | 228 | 13 | 2.002336 | 0810.0969,0810.3945,etc |
| astrophysical research consortium | ARC | 11 | 11 | 1.000051 | 0810.0780,0810.3651,etc |
| all sky monitor | ASM | 108 | 10 | 1.001786 | 0810.0951,0810.2202,etc |
| markov chain monte carlo | MCMC | 73 | 10 | 1.000679 | 0810.5123,0810.1015,etc |
| magneto rotational instability | MRI | 94 | 10 | 1.00299 | 0810.1393,0810.3192,etc |
| monte carlo | MC | 111 | 10 | 2.001522 | 0810.3757,0810.3561,etc |
| nasa extragalactic database | NED | 35 | 10 | 1.000248 | 0810.3129,0810.5132,etc |
| infrared array camera | IRAC | 104 | 10 | 1.001836 | 0810.0021,0810.3852,etc |
| science and technology facilities council | STFC | 11 | 9 | 1.000294 | 0810.5131,0810.2689,etc |
| hardness ratio | HR | 38 | 8 | 1.000417 | 0810.3945,0810.3556,etc |
| proportional counter array | PCA | 47 | 7 | 1.001375 | 0810.1685,0810.4864,etc |
| european photon imaging camera | EPIC | 51 | 7 | 2.00088 | 0810.4804,0810.2023,etc |
| science analysis system | SAS | 15 | 7 | 1.000142 | 0810.5188,0810.5319,etc |
| intra cluster medium | ICM | 133 | 7 | 1.003575 | 0810.2223,0810.0408,etc |
| wolf rayet | WR | 195 | 7 | 2.007767 | 0810.0652,0810.4361,etc |
| star formation history | SFH | 178 | 7 | 2.002654 | 0810.5132,0810.0266,etc |
| square kilometre array | SKA | 75 | 6 | 2.003822 | 0810.0951,0810.2923,etc |
| friedmann robertson walker | FRW | 24 | 6 | 1.000799 | 0810.4939,0810.0270,etc |
| national research council | NRC | 10 | 6 | 1.000085 | 0810.4863,0810.1709,etc |
| infrared spectrograph | IRS | 58 | 6 | 2.000705 | 0810.0473,0810.2803,etc |
| non equilibrium ionization | NEI | 41 | 6 | 1.001264 | 0810.4704,0810.5209,etc |
| colour magnitude diagram | CMD | 110 | 6 | 2.001558 | 0810.1409,0810.5110,etc |
| super massive black hole | SMBH | 64 | 6 | 2.002732 | 0810.2802,0810.0177,etc |
| dwarf spheroidal | dSph | 100 | 5 | 2.005094 | 0810.1511,0810.0710,etc |
| deutsche forschungsgemeinschaft | DFG | 5 | 5 | 1.000112 | 0810.2556,0810.3140,etc |
| innermost stable circular orbit | ISCO | 43 | 5 | 2.00045 | 0810.4947,0810.0237,etc |
| front illuminated | FI | 24 | 5 | 1.000976 | 0810.0873,0810.5188,etc |
| friends of friends | FoF | 14 | 5 | 1.000149 | 0810.0024,0810.3650,etc |
| main sequence turn off | MSTO | 136 | 5 | 2.003009 | 0810.0843,0810.4353,etc |
| collisional ionization equilibrium | CIE | 22 | 5 | 2.000384 | 0810.4687,0810.5209,etc |
| time of flight | TOF | 55 | 5 | 2.003139 | 0810.3830,0810.0132,etc |
| full width half maximum | FWHM | 21 | 5 | 1.000384 | 0810.3563,0810.3944,etc |
| low surface brightness | LSB | 133 | 5 | 1.004656 | 0810.1326,0810.2119,etc |
| large velocity gradient | LVG | 27 | 5 | 1.000941 | 0810.2796,0810.2698,etc |
| large area survey | LAS | 64 | 5 | 1.002085 | 0810.4011,0810.2300,etc |
| ancillary response file | ARF | 11 | 5 | 1.000285 | 0810.4704,0810.5209,etc |
| orion nebula cluster | ONC | 77 | 5 | 2.000555 | 0810.3584,0810.1836,etc |
| poynting robertson | P-R | 30 | 5 | 2.000647 | 0810.5087,0810.3701,etc |
| long wavelength array | LWA | 7 | 4 | 1.00033 | 0810.0951,0810.2923,etc |
| the hi nearby galaxy survey | THINGS | 55 | 4 | 2.000814 | 0810.2556,0810.2825,etc |
| theoretical institute for advanced research in astrophysics | TIARA | 5 | 4 | 1.000133 | 0810.0489,0810.0865,etc |
| herbig haro | HH | 65 | 4 | 1.001926 | 0810.1712,0810.3944,etc |
| canada france hawaii telescope legacy survey | CFHTLS | 17 | 4 | 1.000515 | 0810.4170,0810.4863,etc |
| galactic globular cluster | GGC | 69 | 4 | 1.008953 | 0810.3902,0810.1897,etc |
| ultra violet | UV | 70 | 4 | 2.00171 | 0810.3918,0810.1052,etc |
| submillimeter galaxy | SMG | 122 | 4 | 2.0033 | 0810.3405,0810.2788,etc |
| navarro frenk white | NFW | 22 | 4 | 2.000934 | 0810.0491,0810.4329,etc |
| non x ray background | NXB | 22 | 4 | 1.000373 | 0810.1594,0810.3820,etc |
| basic calibrated data | BCD | 7 | 4 | 1.000124 | 0810.3577,0810.1052,etc |
| whole earth blazar telescope | WEBT | 28 | 4 | 2.000744 | 0810.4864,0810.2424,etc |
| soft gamma ray repeater | SGR | 149 | 4 | 2.007941 | 0810.4801,0810.3804,etc |
| optical monitor | OM | 35 | 4 | 1.000655 | 0810.2424,0810.1249,etc |
| gamma ray imaging detector | GRID | 52 | 4 | 2.000928 | 0810.1676,0810.1516,etc |
| one dimensional | 1-D | 37 | 4 | 2.000645 | 0810.2779,0810.1838,etc |
| period luminosity | P-L | 127 | 4 | 2.00437 | 0810.1780,0810.1210,etc |
| cerro tololo interamerican observatory | CTIO | 16 | 4 | 1.000488 | 0810.5110,0810.0027,etc |
| japan society for the promotion of science | JSPS | 6 | 4 | 1.000266 | 0810.1141,0810.0317,etc |
| equations of state | EOS | 39 | 4 | 2.002804 | 0810.1838,0810.2368,etc |
| two dimensional | 2D | 41 | 4 | 1.001302 | 0810.1838,0810.4145,etc |
| square kilometere array | SKA | 12 | 3 | 1.002366 | 0810.0951,0810.0321,etc |
| maximum likelihood | ML | 16 | 3 | 1.00033 | 0810.4144,0810.2023,etc |
| anti de sitter | AdS | 9 | 3 | 1.000062 | 0810.4251,0810.1517,etc |
| rosat all sky survey | RASS | 18 | 3 | 1.000696 | 0810.1578,0810.1272,etc |
| wide field camera | WFC | 3 | 3 | 1.000036 | 0810.4042,0810.0709,etc |
| baryonic acoustic oscillations | BAO | 13 | 3 | 2.001746 | 0810.1229,0810.5129,etc |
| mid ir | MIR | 129 | 3 | 2.004199 | 0810.2923,0810.3943,etc |
| chemically peculiar | CP | 17 | 3 | 1.001756 | 0810.2228,0810.0864,etc |
| charge transfer inefficiency | CTI | 48 | 3 | 1.006333 | 0810.0873,0810.0432,etc |
| spaced row charge injection | SCI | 29 | 3 | 1.003492 | 0810.0873,0810.4704,etc |
| back illuminated ccd | BI | 15 | 3 | 1.001398 | 0810.0873,0810.0317,etc |
| broad line agn | BLAGN | 38 | 3 | 2.000888 | 0810.3945,0810.1709,etc |
| three dimensional | 3D | 18 | 3 | 1.000363 | 0810.2547,0810.1271,etc |
| nederlandse organisatie voor wetenschappelijk onderzoek | NWO | 3 | 3 | 1.000188 | 0810.3426,0810.3459,etc |
| chandra x ray center | CXC | 3 | 3 | 1.000043 | 0810.5188,0810.1709,etc |
| imaging air cherenkov telescope | IACT | 18 | 3 | 1.000449 | 0810.3757,0810.1318,etc |
| high resolution echelle spectrograph | HIRES | 17 | 3 | 1.00014 | 0810.5131,0810.1356,etc |
| photon dominated region | PDR | 32 | 3 | 1.001183 | 0810.0832,0810.4375,etc |
| back illuminated | BI | 9 | 3 | 1.000272 | 0810.1594,0810.3077,etc |
| photodissociation region | PDR | 17 | 3 | 1.000459 | 0810.3685,0810.5069,etc |
| artificial neural network | ANN | 43 | 3 | 2.002649 | 0810.4527,0810.0867,etc |
| external compton | EC | 18 | 3 | 2.000553 | 0810.4864,0810.5243,etc |
| dwarf elliptical | dE | 33 | 3 | 2.006062 | 0810.3971,0810.2785,etc |
| maximum detectable rigidity | MDR | 4 | 3 | 1.000222 | 0810.3508,0810.4994,etc |
| hertzsprung russell | H-R | 8 | 3 | 1.000509 | 0810.5228,0810.0829,etc |
| monte carlo markov chain | MCMC | 23 | 3 | 1.000741 | 0810.4863,0810.2548,etc |
| galactic cosmic ray | GCR | 28 | 3 | 1.000338 | 0810.3972,0810.2034,etc |
| metallicity distribution function | MDF | 42 | 3 | 1.001472 | 0810.4102,0810.3648,etc |
| intermediate frequency | IF | 30 | 3 | 2.000615 | 0810.0321,0810.0077,etc |
| vimos vlt deep survey | VVDS | 71 | 3 | 2.00152 | 0810.4769,0810.2172,etc |
| imaging atmospheric cherenkov telescope | IACT | 26 | 3 | 2.001413 | 0810.3561,0810.3568,etc |
| hi parkes all sky survey | HIPASS | 87 | 3 | 1.006326 | 0810.5132,0810.1326,etc |
| burst alert telescope | BAT | 35 | 3 | 2.000445 | 0810.2481,0810.1249,etc |
| core mass function | CMF | 14 | 3 | 2.000389 | 0810.3852,0810.0299,etc |
| narrow line seyfert 1 | NLS1 | 18 | 3 | 1.001457 | 0810.2272,0810.0513,etc |
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