| max planck institute for astronomy | MPIA | 22 | 22 | 1.000063 | 0805.3580,0805.0001,etc |
| inverse compton | IC | 303 | 15 | 2.003794 | 0805.1898,0805.2085,etc |
| kolmogorov smirnov | KS | 51 | 12 | 2.001998 | 0805.4541,0805.2851,etc |
| advanced camera for surveys | ACS | 225 | 10 | 2.002848 | 0805.1522,0805.0376,etc |
| wolf rayet | WR | 1850 | 9 | 1.011354 | 0805.1914,0805.4529,etc |
| three dimensional | 3-D | 73 | 9 | 2.00128 | 0805.1794,0805.3356,etc |
| markov chain monte carlo | MCMC | 103 | 9 | 2.001613 | 0805.2946,0805.2399,etc |
| astrophysical research consortium | ARC | 19 | 8 | 2.000434 | 0805.3580,0805.4746,etc |
| two dimensional | 2D | 155 | 8 | 1.004691 | 0805.1098,0805.0928,etc |
| intra cluster medium | ICM | 55 | 7 | 1.002293 | 0805.4159,0805.2771,etc |
| equations of state | EOSs | 49 | 7 | 1.001837 | 0805.1820,0805.3356,etc |
| signal to noise | S/N | 71 | 7 | 1.001053 | 0805.1227,0805.3257,etc |
| infrared array camera | IRAC | 66 | 6 | 2.001625 | 0805.2594,0805.1732,etc |
| star formation history | SFH | 95 | 6 | 2.001847 | 0805.1512,0805.1930,etc |
| friedmann robertson walker | FRW | 19 | 6 | 1.000673 | 0805.3570,0805.0413,etc |
| extended press schechter | ePS | 144 | 5 | 2.003188 | 0805.3580,0805.2174,etc |
| natural sciences and engineering research council of canada | NSERC | 5 | 5 | 1.000101 | 0805.4607,0805.1249,etc |
| orion nebula cluster | ONC | 36 | 5 | 1.000842 | 0805.0569,0805.0714,etc |
| full width half maximum | FWHM | 13 | 5 | 1.000455 | 0805.1137,0805.2155,etc |
| front illuminated | FI | 29 | 5 | 2.000915 | 0805.2771,0805.2079,etc |
| dwarf spheroidal | dSph | 157 | 5 | 2.003531 | 0805.0795,0805.1054,etc |
| interactive data language | IDL | 7 | 5 | 1.000091 | 0805.0791,0805.3503,etc |
| very high energy | VHE | 66 | 5 | 2.002266 | 0805.0417,0805.2221,etc |
| integrated sachs wolfe | ISW | 99 | 5 | 2.003274 | 0805.3645,0805.3710,etc |
| monte carlo | MC | 43 | 5 | 1.000891 | 0805.1754,0805.2251,etc |
| colour magnitude diagram | CMD | 89 | 5 | 2.000974 | 0805.1189,0805.3459,etc |
| ultra luminous infrared galaxy | ULIRG | 8 | 4 | 1.000286 | 0805.1420,0805.1732,etc |
| hertzsprung russell | H-R | 20 | 4 | 1.001316 | 0805.0062,0805.4360,etc |
| michelson doppler imager | MDI | 22 | 4 | 1.000673 | 0805.1055,0805.0472,etc |
| nasa extragalactic database | NED | 14 | 4 | 1.000339 | 0805.2594,0805.1260,etc |
| supergiant fast x ray transient | SFXT | 69 | 4 | 1.002724 | 0805.1808,0805.0496,etc |
| particle in cell | PIC | 21 | 4 | 1.00056 | 0805.1098,0805.0928,etc |
| one dimensional | 1D | 151 | 4 | 2.003188 | 0805.1098,0805.3356,etc |
| all sky monitor | ASM | 17 | 4 | 1.000342 | 0805.2577,0805.0422,etc |
| double degenerate | DD | 91 | 4 | 1.004896 | 0805.1512,0805.4360,etc |
| kaluza klein | KK | 178 | 4 | 2.00454 | 0805.1905,0805.3818,etc |
| period luminosity | P-L | 106 | 4 | 1.009562 | 0805.4624,0805.2655,etc |
| dvali gabadadze porrati | DGP | 123 | 4 | 2.003549 | 0805.4113,0805.4466,etc |
| monte carlo markov chain | MCMC | 29 | 4 | 2.000805 | 0805.1267,0805.3915,etc |
| back illuminated | BI | 15 | 4 | 1.000487 | 0805.2771,0805.2079,etc |
| non x ray background | NXB | 49 | 4 | 2.000979 | 0805.2771,0805.0500,etc |
| gigahertz peaked spectrum | GPS | 28 | 4 | 1.000776 | 0805.4746,0805.3413,etc |
| sunyaev zel'dovich | SZ | 77 | 4 | 2.003443 | 0805.2155,0805.4361,etc |
| navarro frenk white | NFW | 12 | 4 | 1.000226 | 0805.2155,0805.1054,etc |
| near infrared camera and multi object spectrometer | NICMOS | 19 | 4 | 2.001586 | 0805.0791,0805.3503,etc |
| spitzer science center | SSC | 6 | 4 | 1.000107 | 0805.4818,0805.0573,etc |
| magneto hydrodynamic | MHD | 4 | 4 | 1.000094 | 0805.0250,0805.2514,etc |
| advanced ccd imaging spectrometer | ACIS | 44 | 4 | 2.000827 | 0805.2320,0805.1232,etc |
| power law | PL | 153 | 4 | 2.002751 | 0805.0201,0805.0500,etc |
| wide field camera | WFCAM | 19 | 4 | 1.00021 | 0805.2861,0805.1143,etc |
| the red giant branch | TRGB | 17 | 4 | 2.000325 | 0805.1250,0805.1074,etc |
| radio luminosity function | RLF | 113 | 3 | 2.001227 | 0805.1750,0805.4541,etc |
| galactic centre | GC | 22 | 3 | 1.00176 | 0805.0185,0805.1050,etc |
| data release 6 | DR6 | 10 | 3 | 1.000132 | 0805.3580,0805.2612,etc |
| national research council | NRC | 6 | 3 | 1.000164 | 0805.0001,0805.3983,etc |
| time of arrival | ToA | 34 | 3 | 2.002619 | 0805.1519,0805.4610,etc |
| inter galactic medium | IGM | 8 | 3 | 1.000216 | 0805.4159,0805.4184,etc |
| blue compact dwarf | BCD | 209 | 3 | 2.007295 | 0805.3298,0805.1250,etc |
| synchrotron self compton | SSC | 22 | 3 | 2.002276 | 0805.2577,0805.1707,etc |
| burst alert telescope | BAT | 30 | 3 | 2.000222 | 0805.2577,0805.1094,etc |
| hardness ratio | HR | 11 | 3 | 1.00014 | 0805.2577,0805.1232,etc |
| single degenerate | SD | 71 | 3 | 2.00125 | 0805.1512,0805.4360,etc |
| particle mesh | PM | 7 | 3 | 1.000149 | 0805.0276,0805.0117,etc |
| uk infrared telescope | UKIRT | 6 | 3 | 1.000085 | 0805.4184,0805.1732,etc |
| soft x ray | SXR | 18 | 3 | 1.000949 | 0805.4474,0805.4468,etc |
| luminous red galaxies | LRG | 5 | 3 | 1.000243 | 0805.1267,0805.3645,etc |
| magneto rotational instability | MRI | 8 | 3 | 1.000195 | 0805.1681,0805.3996,etc |
| super massive black hole | SMBH | 23 | 3 | 2.001185 | 0805.1919,0805.1050,etc |
| gemini deep deep survey | GDDS | 3 | 3 | 1.000129 | 0805.1409,0805.1713,etc |
| kinetic sunyaev zel'dovich | kSZ | 66 | 3 | 2.005014 | 0805.2155,0805.0596,etc |
| fokker planck | FP | 59 | 3 | 1.003856 | 0805.0054,0805.0058,etc |
| science research center | SRC | 3 | 3 | 1.000061 | 0805.0054,0805.1103,etc |
| x ray imaging spectrometer | XIS | 150 | 3 | 2.003256 | 0805.2079,0805.3582,etc |
| basic calibrated data | BCD | 8 | 3 | 1.000212 | 0805.4818,0805.0573,etc |
| cosmic infrared background | CIB | 11 | 3 | 1.00037 | 0805.2487,0805.1732,etc |
| nobeyama millimeter array | NMA | 9 | 3 | 1.001742 | 0805.1801,0805.3648,etc |
| submillimeter array | SMA | 18 | 3 | 1.000429 | 0805.1801,0805.3503,etc |
| good time interval | GTI | 3 | 3 | 1.000059 | 0805.3582,0805.1369,etc |
| legacy archive for microwave background data analysis | LAMBDA | 6 | 3 | 1.000353 | 0805.0594,0805.0269,etc |
| infrared spectrograph | IRS | 45 | 3 | 2.000739 | 0805.3257,0805.0573,etc |
| singular isothermal ellipsoid | SIE | 25 | 3 | 2.000517 | 0805.2897,0805.2381,etc |
| friedmann lemaitre robertson walker | FLRW | 37 | 3 | 2.001539 | 0805.4157,0805.2197,etc |
| inter stellar medium | ISM | 13 | 3 | 1.000362 | 0805.1732,0805.0600,etc |
| deutsche forschungsgemeinschaft | DFG | 4 | 3 | 1.000108 | 0805.3459,0805.1998,etc |
| soft gamma ray repeater | SGR | 34 | 3 | 1.000872 | 0805.3919,0805.3807,etc |
| large velocity gradient | LVG | 10 | 3 | 1.000461 | 0805.1205,0805.4297,etc |
| bose einstein condensate | BEC | 30 | 3 | 2.003082 | 0805.2877,0805.4188,etc |
| maximum likelihood | ML | 42 | 3 | 1.001532 | 0805.2945,0805.4417,etc |
| ultra high energy | UHE | 69 | 3 | 2.004226 | 0805.4304,0805.1498,etc |