| markov chain monte carlo | MCMC | 244 | 37 | 1.001216 | 1211.2585,1211.3862,etc |
| signal to noise | S/N | 188 | 22 | 1.001281 | 1211.3424,1211.5966,etc |
| three dimensional | 3D | 362 | 18 | 1.003157 | 1211.4870,1211.7313,etc |
| kolmogorov smirnov | KS | 60 | 18 | 2.00046 | 1211.6440,1211.3170,etc |
| advanced camera for surveys | ACS | 147 | 15 | 1.0011 | 1211.2069,1211.4353,etc |
| max planck institute for astronomy | MPIA | 15 | 15 | 1.00005 | 1211.6723,1211.5156,etc |
| monte carlo | MC | 115 | 12 | 2.003107 | 1211.1033,1211.3862,etc |
| large area telescope | LAT | 166 | 12 | 2.001968 | 1211.3726,1211.3165,etc |
| inverse compton | IC | 126 | 11 | 1.00302 | 1211.0679,1211.0774,etc |
| false alarm probability | FAP | 76 | 10 | 1.000587 | 1211.1389,1211.7263,etc |
| intra cluster medium | ICM | 209 | 10 | 2.001694 | 1211.6722,1211.3206,etc |
| wolf rayet | WR | 105 | 10 | 2.001299 | 1211.2761,1211.1889,etc |
| atacama large millimeter/submillimeter array | ALMA | 72 | 9 | 1.00408 | 1211.2807,1211.3790,etc |
| star formation history | SFH | 88 | 9 | 1.001285 | 1211.2208,1211.4746,etc |
| friedmann robertson walker | FRW | 29 | 9 | 1.000376 | 1211.4633,1211.3416,etc |
| ultra violet | UV | 185 | 9 | 1.002639 | 1211.5854,1211.3120,etc |
| wide field camera | WFC | 32 | 8 | 2.000535 | 1211.2069,1211.6153,etc |
| friends of friends | FoF | 25 | 8 | 2.000261 | 1211.3976,1211.0014,etc |
| national research council | NRC | 13 | 8 | 1.000086 | 1211.3245,1211.4630,etc |
| data release 7 | DR7 | 53 | 8 | 2.00104 | 1211.1421,1211.1397,etc |
| dark energy survey | DES | 52 | 8 | 2.001777 | 1211.4480,1211.5966,etc |
| photon dominated region | PDR | 114 | 7 | 2.001771 | 1211.3554,1211.7142,etc |
| helioseismic and magnetic imager | HMI | 64 | 7 | 1.004618 | 1211.6870,1211.5473,etc |
| advanced ccd imaging spectrometer | ACIS | 25 | 7 | 2.000674 | 1211.6722,1211.0347,etc |
| navarro frenk white | NFW | 53 | 7 | 1.001257 | 1211.1951,1211.1421,etc |
| two dimensional | 2D | 76 | 7 | 1.001441 | 1211.6345,1211.0554,etc |
| submillimeter array | SMA | 78 | 7 | 1.002384 | 1211.5206,1211.6605,etc |
| full width half maximum | FWHM | 44 | 7 | 1.000489 | 1211.0523,1211.2527,etc |
| burst alert telescope | BAT | 69 | 7 | 2.001178 | 1211.1117,1211.3537,etc |
| sunyaev zel'dovich | SZ | 166 | 7 | 1.005589 | 1211.5662,1211.6515,etc |
| low surface brightness | LSB | 298 | 7 | 1.008588 | 1211.6923,1211.4068,etc |
| one dimensional | 1D | 104 | 7 | 2.00249 | 1211.3157,1211.6450,etc |
| infrared array camera | IRAC | 146 | 7 | 2.002383 | 1211.6492,1211.3092,etc |
| monte carlo markov chain | MCMC | 41 | 7 | 1.001255 | 1211.2797,1211.6404,etc |
| integrated sachs wolfe | ISW | 153 | 6 | 2.004253 | 1211.4610,1211.1132,etc |
| double degenerate | DD | 121 | 6 | 1.010091 | 1211.6219,1211.2475,etc |
| atacama large millimeter array | ALMA | 29 | 6 | 1.002268 | 1211.3316,1211.3663,etc |
| cosmic infrared background | CIB | 46 | 6 | 1.001891 | 1211.3902,1211.6668,etc |
| synchrotron self compton | SSC | 20 | 6 | 1.000879 | 1211.1543,1211.5120,etc |
| flux limited diffusion | FLD | 16 | 6 | 1.000678 | 1211.6345,1211.3467,etc |
| science and technology facilities council | STFC | 6 | 6 | 1.000092 | 1211.2761,1211.5810,etc |
| colour magnitude diagram | CMD | 62 | 6 | 2.000937 | 1211.4746,1211.3541,etc |
| radio transient | RRAT | 83 | 6 | 1.006936 | 1211.2183,1211.4689,etc |
| nasa extragalactic database | NED | 17 | 6 | 2.000342 | 1211.3764,1211.6808,etc |
| japan society for the promotion of science | JSPS | 11 | 6 | 1.000321 | 1211.0151,1211.4712,etc |
| transit timing variation | TTV | 84 | 6 | 1.001514 | 1211.0218,1211.4028,etc |
| deutsche forschungsgemeinschaft | DFG | 6 | 6 | 1.000023 | 1211.4901,1211.1695,etc |
| direct numerical simulations | DNS | 23 | 6 | 1.000765 | 1211.6708,1211.0452,etc |
| very high energy | VHE | 63 | 6 | 1.003966 | 1211.5997,1211.3054,etc |
| infra red | IR | 83 | 5 | 1.002999 | 1211.3595,1211.3878,etc |
| infrared science archive | IRSA | 6 | 5 | 1.000112 | 1211.4612,1211.1341,etc |
| soft gamma ray repeater | SGR | 86 | 5 | 1.005097 | 1211.4721,1211.6078,etc |
| atacama pathfinder experiment | APEX | 26 | 5 | 2.001132 | 1211.7142,1211.0455,etc |
| jansky very large array | JVLA | 75 | 5 | 1.003714 | 1211.3316,1211.3115,etc |
| main sequence turn off | MSTO | 86 | 5 | 2.002143 | 1211.2817,1211.2866,etc |
| atmospheric imaging assembly | AIA | 57 | 5 | 2.001708 | 1211.5473,1211.6569,etc |
| infrared spectrograph | IRS | 58 | 5 | 1.000932 | 1211.7252,1211.4510,etc |
| proportional counter array | PCA | 63 | 5 | 2.001239 | 1211.1600,1211.3537,etc |
| ultra luminous infrared galaxy | ULIRG | 30 | 5 | 2.000389 | 1211.1223,1211.0841,etc |
| dwarf spheroidal | dSph | 104 | 5 | 2.001514 | 1211.3764,1211.3170,etc |
| spin independent | SI | 132 | 5 | 1.002066 | 1211.4573,1211.7063,etc |
| potential field source surface | PFSS | 83 | 5 | 2.000522 | 1211.4684,1211.6171,etc |
| graphics processing unit | GPU | 100 | 5 | 2.003166 | 1211.4406,1211.3138,etc |
| sunyaev zeldovich | SZ | 454 | 5 | 2.006648 | 1211.3206,1211.7096,etc |
| square kilometre array | SKA | 30 | 5 | 1.000912 | 1211.5589,1211.4932,etc |
| agenzia spaziale italiana | ASI | 15 | 5 | 2.000233 | 1211.1524,1211.4997,etc |
| kinetic sunyaev zel'dovich | kSZ | 150 | 5 | 1.00732 | 1211.2832,1211.3743,etc |
| magneto hydrodynamic | MHD | 26 | 5 | 2.00111 | 1211.4836,1211.0347,etc |
| test statistic | TS | 64 | 5 | 1.002086 | 1211.6457,1211.3073,etc |
| infrared dark cloud | IRDC | 42 | 4 | 1.001434 | 1211.3554,1211.0198,etc |
| space telescope imaging spectrograph | STIS | 23 | 4 | 1.00072 | 1211.4612,1211.2907,etc |
| metropolis hastings | MH | 17 | 4 | 1.000614 | 1211.3862,1211.4876,etc |
| baryonic acoustic oscillation | BAO | 78 | 4 | 1.003405 | 1211.6213,1211.2154,etc |
| radiative transfer equation | RTE | 47 | 4 | 2.000822 | 1211.4870,1211.1502,etc |
| hardness ratio | HR | 20 | 4 | 1.000635 | 1211.2804,1211.1600,etc |
| chandra x ray center | CXC | 4 | 4 | 1.000171 | 1211.2761,1211.0017,etc |
| carbon oxygen | CO | 48 | 4 | 1.001592 | 1211.0624,1211.4794,etc |
| proportional counter unit | PCU | 16 | 4 | 1.000398 | 1211.1600,1211.6298,etc |
| non x ray background | NXB | 19 | 4 | 1.000626 | 1211.5810,1211.6782,etc |
| rossiter mclaughlin | RM | 23 | 4 | 2.000662 | 1211.7065,1211.0218,etc |
| galactic legacy infrared mid plane survey extraordinaire | GLIMPSE | 19 | 4 | 2.000182 | 1211.0455,1211.1620,etc |
| ordinary differential equation | ODE | 43 | 4 | 2.002096 | 1211.4633,1211.0837,etc |
| magneto rotational instability | MRI | 13 | 4 | 1.000254 | 1211.4969,1211.5135,etc |
| orion nebula cluster | ONC | 22 | 4 | 1.000399 | 1211.2935,1211.0198,etc |
| metallicity distribution function | MDF | 155 | 4 | 2.002344 | 1211.3170,1211.7073,etc |
| magellanic cloud | MC | 46 | 4 | 1.003674 | 1211.1978,1211.4583,etc |
| surface detector | SD | 75 | 4 | 2.003741 | 1211.4901,1211.6992,etc |
| least squares deconvolution | LSD | 148 | 4 | 1.00153 | 1211.2907,1211.2054,etc |
| multi gaussian expansion | MGE | 58 | 4 | 2.002228 | 1211.4399,1211.2317,etc |
| natural science foundation of china | NSFC | 4 | 4 | 1.000048 | 1211.3662,1211.0549,etc |
| innermost stable circular orbit | ISCO | 10 | 4 | 1.000297 | 1211.2513,1211.2273,etc |
| wide field camera 3 | WFC3 | 16 | 4 | 1.00047 | 1211.6153,1211.0278,etc |
| hard x ray | HXR | 34 | 4 | 1.002799 | 1211.3474,1211.6015,etc |
| interactive data language | IDL | 26 | 4 | 1.003581 | 1211.2382,1211.4055,etc |
| legacy archive for microwave background data analysis | LAMBDA | 7 | 4 | 1.000243 | 1211.2382,1211.6756,etc |
| cambridge astronomical survey unit | CASU | 5 | 4 | 1.000084 | 1211.3092,1211.6108,etc |
| photodissociation region | PDR | 27 | 4 | 2.000561 | 1211.5064,1211.1430,etc |
| compact steep spectrum | CSS | 53 | 4 | 1.002382 | 1211.4837,1211.6852,etc |
| star formation rate density | SFRD | 22 | 4 | 1.000437 | 1211.1397,1211.4579,etc |
| region of interest | ROI | 13 | 4 | 1.000391 | 1211.1671,1211.3073,etc |
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