| markov chain monte carlo | MCMC | 163 | 25 | 1.000945 | 1010.4106,1010.5298,etc |
| max planck institute for astronomy | MPIA | 25 | 25 | 1.000244 | 1010.0415,1010.2749,etc |
| wolf rayet | W-R | 262 | 17 | 2.005508 | 1010.2689,1010.1063,etc |
| kolmogorov smirnov | KS | 105 | 16 | 2.000658 | 1010.4697,1010.4804,etc |
| intra cluster medium | ICM | 254 | 14 | 1.003007 | 1010.4697,1010.6213,etc |
| large area telescope | LAT | 340 | 14 | 2.006197 | 1010.1588,1010.2752,etc |
| very high energy | VHE | 144 | 13 | 2.002919 | 1010.2397,1010.3730,etc |
| signal to noise | S/N | 73 | 13 | 2.000352 | 1010.3199,1010.1806,etc |
| colour magnitude diagram | CMD | 127 | 12 | 2.001258 | 1010.0687,1010.0247,etc |
| three dimensional | 3D | 113 | 12 | 1.001768 | 1010.0167,1010.4489,etc |
| submillimeter array | SMA | 127 | 11 | 2.001266 | 1010.3016,1010.3428,etc |
| basic calibrated data | BCD | 32 | 11 | 1.000336 | 1010.0007,1010.4323,etc |
| friedmann robertson walker | FRW | 30 | 10 | 1.000622 | 1010.1307,1010.2215,etc |
| innermost stable circular orbit | ISCO | 229 | 10 | 2.005214 | 1010.0651,1010.3865,etc |
| monte carlo | MC | 42 | 9 | 2.001371 | 1010.3980,1010.5354,etc |
| deutsche forschungsgemeinschaft | DFG | 12 | 9 | 1.000266 | 1010.3980,1010.5932,etc |
| sunyaev zel'dovich | SZ | 268 | 9 | 1.003796 | 1010.1065,1010.6011,etc |
| inverse compton | IC | 171 | 9 | 2.001633 | 1010.5354,1010.4306,etc |
| infrared array camera | IRAC | 124 | 9 | 2.001604 | 1010.3868,1010.2497,etc |
| ultra high energy | UHE | 145 | 8 | 2.003129 | 1010.3019,1010.2788,etc |
| integrated sachs wolfe | ISW | 182 | 8 | 2.004519 | 1010.0578,1010.2291,etc |
| astrophysical research consortium | ARC | 9 | 8 | 1.000052 | 1010.5386,1010.2495,etc |
| advanced camera for surveys | ACS | 33 | 7 | 2.000427 | 1010.5273,1010.3715,etc |
| science and technology facilities council | STFC | 9 | 7 | 1.000228 | 1010.5604,1010.0677,etc |
| friends of friends | FOF | 23 | 7 | 1.000388 | 1010.6128,1010.3378,etc |
| synchrotron self compton | SSC | 26 | 7 | 1.000533 | 1010.5354,1010.5399,etc |
| two dimensional | 2D | 23 | 7 | 1.000618 | 1010.5284,1010.0167,etc |
| infrared spectrograph | IRS | 94 | 7 | 2.001249 | 1010.1783,1010.2323,etc |
| star formation history | SFH | 225 | 7 | 1.00526 | 1010.1325,1010.1966,etc |
| photodissociation region | PDR | 62 | 6 | 1.002384 | 1010.0007,1010.2290,etc |
| proportional counter array | PCA | 27 | 6 | 1.00056 | 1010.4793,1010.5621,etc |
| science demonstration phase | SDP | 65 | 6 | 1.001059 | 1010.0673,1010.5782,etc |
| hertzsprung russell | H-R | 22 | 6 | 1.000356 | 1010.5369,1010.5643,etc |
| kelvin helmholtz | KH | 23 | 6 | 2.000333 | 1010.0997,1010.4899,etc |
| navarro frenk white | NFW | 15 | 5 | 1.000519 | 1010.5236,1010.6128,etc |
| ultra violet | UV | 64 | 5 | 1.001245 | 1010.1407,1010.0119,etc |
| japan society for promotion of science | JSPS | 6 | 5 | 1.000254 | 1010.3980,1010.2025,etc |
| swiss national science foundation | SNSF | 6 | 5 | 1.000079 | 1010.3980,1010.2025,etc |
| star formation rate density | SFRD | 23 | 5 | 2.00053 | 1010.2260,1010.1150,etc |
| maximum likelihood | ML | 16 | 5 | 1.000143 | 1010.1065,1010.1266,etc |
| supersymmetric | SUSY | 135 | 5 | 1.003083 | 1010.0245,1010.5507,etc |
| tolman oppenheimer volkoff | TOV | 29 | 5 | 2.001046 | 1010.3759,1010.3041,etc |
| short low | SL | 10 | 5 | 1.000135 | 1010.2170,1010.1783,etc |
| natural sciences and engineering research council | NSERC | 5 | 5 | 1.0003 | 1010.6109,1010.4605,etc |
| nasa extragalactic database | NED | 40 | 5 | 1.000597 | 1010.0677,1010.5942,etc |
| narrow line seyfert 1 | NLS1 | 33 | 5 | 2.001929 | 1010.3744,1010.3771,etc |
| magellanic cloud | MC | 307 | 5 | 2.01205 | 1010.4797,1010.1327,etc |
| space interferometry mission | SIM | 16 | 5 | 1.000313 | 1010.4044,1010.4041,etc |
| false alarm probability | FAP | 74 | 5 | 1.002119 | 1010.4044,1010.2616,etc |
| european photon imaging camera | EPIC | 25 | 5 | 1.000828 | 1010.0783,1010.2781,etc |
| extreme mass ratio inspiral | EMRI | 80 | 5 | 1.003745 | 1010.5255,1010.1721,etc |
| data release 7 | DR7 | 37 | 5 | 1.000595 | 1010.2906,1010.2655,etc |
| faulkes telescope north | FTN | 9 | 5 | 1.000174 | 1010.2203,1010.1742,etc |
| kaluza klein | KK | 90 | 4 | 1.005062 | 1010.5236,1010.5354,etc |
| louisiana optical network initiative | LONI | 4 | 4 | 1.000087 | 1010.3980,1010.2025,etc |
| swedish national infrastructure for computing | SNIC | 4 | 4 | 1.000087 | 1010.3980,1010.2025,etc |
| belgian federal science policy office | Belspo | 4 | 4 | 1.000087 | 1010.3980,1010.2025,etc |
| burst alert telescope | BAT | 22 | 4 | 1.001632 | 1010.0911,1010.2206,etc |
| wide field x ray telescope | WFXT | 156 | 4 | 2.002059 | 1010.6213,1010.6252,etc |
| extremely metal poor | EMP | 232 | 4 | 2.003497 | 1010.0415,1010.4360,etc |
| full width half maximum | FWHM | 35 | 4 | 1.001636 | 1010.5243,1010.5387,etc |
| data release | DR | 18 | 4 | 2.000526 | 1010.1307,1010.0289,etc |
| inter stellar medium | ISM | 25 | 4 | 1.000838 | 1010.0119,1010.5056,etc |
| the red giant branch | TRGB | 10 | 4 | 1.000533 | 1010.3788,1010.1806,etc |
| main sequence turn off | MSTO | 83 | 4 | 1.005044 | 1010.0247,1010.2973,etc |
| wide field camera 3 | WFC3 | 34 | 4 | 2.001025 | 1010.1002,1010.2261,etc |
| gamma ray burst monitor | GBM | 57 | 4 | 1.00477 | 1010.1588,1010.2679,etc |
| orion nebula cluster | ONC | 99 | 4 | 2.003227 | 1010.1677,1010.1962,etc |
| good time interval | GTI | 6 | 4 | 1.000176 | 1010.5703,1010.4907,etc |
| international max planck research school | IMPRS | 5 | 4 | 1.000272 | 1010.1566,1010.0655,etc |
| dwarf spheroidal | dSph | 66 | 4 | 2.002515 | 1010.1261,1010.3023,etc |
| long low | LL | 21 | 4 | 2.000529 | 1010.2170,1010.1783,etc |
| space telescope imaging spectrograph | STIS | 24 | 4 | 2.001446 | 1010.2211,1010.2261,etc |
| atacama pathfinder experiment | APEX | 22 | 4 | 1.000916 | 1010.3868,1010.0788,etc |
| palomar green | PG | 148 | 4 | 2.003679 | 1010.3846,1010.5591,etc |
| position velocity | PV | 39 | 4 | 1.001359 | 1010.1996,1010.1393,etc |
| national research foundation of korea | NRF | 5 | 4 | 1.00007 | 1010.1996,1010.1995,etc |
| x ray luminosity function | XLF | 64 | 4 | 2.00128 | 1010.5675,1010.6024,etc |
| infra red | IR | 82 | 4 | 1.001151 | 1010.4176,1010.1079,etc |
| collisional ionization equilibrium | CIE | 38 | 4 | 1.002265 | 1010.5654,1010.0783,etc |
| palomar high precision astrometric search for exoplanet systems | PHASES | 161 | 4 | 2.002426 | 1010.4044,1010.4041,etc |
| magneto rotational instability | MRI | 4 | 4 | 1.000039 | 1010.0997,1010.6189,etc |
| dark energy survey | DES | 24 | 4 | 1.000992 | 1010.0744,1010.1005,etc |
| solar terrestrial relations observatory | STEREO | 70 | 4 | 2.001292 | 1010.5927,1010.0192,etc |
| partial differential equation | PDE | 18 | 4 | 1.000141 | 1010.4492,1010.3631,etc |
| power law | PL | 43 | 4 | 2.002923 | 1010.4027,1010.1003,etc |
| effective one body | EOB | 58 | 4 | 2.001178 | 1010.5255,1010.1721,etc |
| california institute of technology | Caltech | 9 | 4 | 1.000172 | 1010.4028,1010.5618,etc |
| monte carlo markov chain | MCMC | 14 | 4 | 1.000351 | 1010.1150,1010.1461,etc |
| ultra luminous infrared galaxy | ULIRG | 19 | 4 | 1.000405 | 1010.0788,1010.1704,etc |
| spitzer science center | SSC | 13 | 4 | 1.000227 | 1010.1227,1010.1704,etc |
| japan society for the promotion of science | JSPS | 8 | 4 | 1.000074 | 1010.4964,1010.1267,etc |
| time of arrival | TOA | 132 | 3 | 2.002594 | 1010.3785,1010.4337,etc |
| grid laboratory of wisconsin | GLOW | 3 | 3 | 1.000089 | 1010.3980,1010.2025,etc |
| open science grid | OSG | 3 | 3 | 1.000089 | 1010.3980,1010.2025,etc |
| auto correlation function | ACF | 27 | 3 | 2.001031 | 1010.5770,1010.4176,etc |
| analog to digital converter | ADC | 7 | 3 | 1.000433 | 1010.5893,1010.2734,etc |
| inter galactic medium | IGM | 17 | 3 | 1.00094 | 1010.6213,1010.1806,etc |
| field programmable gate array | FPGA | 46 | 3 | 2.003322 | 1010.2734,1010.5224,etc |
| atacama large millimeter array | ALMA | 8 | 3 | 2.000532 | 1010.3016,1010.0843,etc |
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