| markov chain monte carlo | MCMC | 179 | 25 | 1.007545 | 1206.6056,1206.1056,etc |
| star formation history | SFH | 515 | 23 | 2.003745 | 1206.0665,1206.2732,etc |
| max planck institute for astronomy | MPIA | 20 | 17 | 1.000041 | 1206.1791,1206.3797,etc |
| kolmogorov smirnov | K-S | 97 | 17 | 2.000752 | 1206.3579,1206.6889,etc |
| large area telescope | LAT | 249 | 16 | 2.002143 | 1206.6515,1206.3530,etc |
| signal to noise | S/N | 76 | 16 | 1.000676 | 1206.6515,1206.0665,etc |
| full width half maximum | FWHM | 59 | 13 | 2.000485 | 1206.4305,1206.1662,etc |
| inverse compton | IC | 266 | 12 | 2.003364 | 1206.3530,1206.6715,etc |
| friedmann robertson walker | FRW | 56 | 11 | 1.001535 | 1206.1642,1206.6192,etc |
| advanced camera for surveys | ACS | 140 | 11 | 2.002906 | 1206.3797,1206.6274,etc |
| three dimensional | 3D | 145 | 11 | 1.00103 | 1206.3132,1206.5982,etc |
| synchrotron self compton | SSC | 128 | 9 | 1.002645 | 1206.3769,1206.3946,etc |
| monte carlo | MC | 93 | 9 | 1.026514 | 1206.4048,1206.5878,etc |
| two dimensional | 2D | 117 | 9 | 2.001813 | 1206.0291,1206.2087,etc |
| friends of friends | FoF | 52 | 8 | 2.000464 | 1206.0644,1206.3571,etc |
| atacama large millimeter array | ALMA | 119 | 8 | 2.00271 | 1206.0403,1206.4693,etc |
| wide field camera 3 | WFC3 | 79 | 8 | 1.001296 | 1206.3797,1206.1057,etc |
| wide field camera | WFCAM | 124 | 8 | 2.000999 | 1206.3886,1206.0759,etc |
| equations of state | EOS | 262 | 7 | 1.007378 | 1206.1642,1206.4108,etc |
| palomar transient factory | PTF | 148 | 7 | 2.003398 | 1206.0665,1206.4035,etc |
| jansky very large array | JVLA | 53 | 7 | 2.001596 | 1206.4693,1206.4046,etc |
| very high energy | VHE | 100 | 7 | 2.006181 | 1206.0745,1206.6147,etc |
| square kilometre array | SKA | 40 | 7 | 2.002745 | 1206.1602,1206.4437,etc |
| science and technology facilities council | STFC | 10 | 7 | 1.000141 | 1206.2361,1206.4322,etc |
| wolf rayet | WR | 69 | 7 | 1.001224 | 1206.2275,1206.1656,etc |
| atacama large millimeter/submillimeter array | ALMA | 54 | 6 | 1.002346 | 1206.3600,1206.4536,etc |
| submillimeter array | SMA | 187 | 6 | 2.004338 | 1206.3600,1206.5008,etc |
| ultra violet | UV | 157 | 6 | 2.003431 | 1206.6374,1206.4396,etc |
| core mass function | CMF | 122 | 6 | 1.002555 | 1206.2115,1206.1045,etc |
| dwarf spheroidal | dSph | 114 | 6 | 1.003362 | 1206.6691,1206.4999,etc |
| national research council | NRC | 10 | 6 | 1.000081 | 1206.0665,1206.6533,etc |
| infrared array camera | IRAC | 83 | 6 | 2.001146 | 1206.4060,1206.1907,etc |
| basic calibrated data | BCD | 21 | 6 | 1.000202 | 1206.4060,1206.4005,etc |
| position velocity | PV | 24 | 6 | 2.000465 | 1206.5708,1206.1249,etc |
| data release 7 | DR7 | 73 | 6 | 1.001018 | 1206.6496,1206.3566,etc |
| navarro frenk white | NFW | 52 | 6 | 1.000576 | 1206.5412,1206.7056,etc |
| proportional counter array | PCA | 40 | 6 | 1.000264 | 1206.0745,1206.4878,etc |
| particle in cell | PIC | 29 | 6 | 1.000523 | 1206.1360,1206.2087,etc |
| effective field theory | EFT | 63 | 6 | 1.001357 | 1206.0025,1206.3906,etc |
| texas advanced computing center | TACC | 8 | 6 | 1.000147 | 1206.4724,1206.6923,etc |
| national research foundation of korea | NRF | 6 | 5 | 1.000147 | 1206.1384,1206.0336,etc |
| dark energy survey | DES | 34 | 5 | 2.001459 | 1206.0665,1206.5801,etc |
| infrared spectrograph | IRS | 53 | 5 | 1.001008 | 1206.4047,1206.5830,etc |
| region of interest | ROI | 33 | 5 | 2.001036 | 1206.0796,1206.0745,etc |
| uksa | UK | 31 | 5 | 1.000788 | 1206.2319,1206.5982,etc |
| sunyaev zel'dovich | SZ | 21 | 5 | 1.000476 | 1206.1049,1206.4550,etc |
| innermost stable circular orbit | ISCO | 22 | 5 | 1.000592 | 1206.6130,1206.2727,etc |
| metallicity distribution function | MDF | 61 | 5 | 1.000994 | 1206.0015,1206.6968,etc |
| monte carlo markov chain | MCMC | 38 | 5 | 2.000852 | 1206.0015,1206.2569,etc |
| burst alert telescope | BAT | 17 | 5 | 1.000729 | 1206.3946,1206.1782,etc |
| colour magnitude diagram | CMD | 93 | 5 | 2.00157 | 1206.6968,1206.2361,etc |
| transit timing variation | TTV | 43 | 5 | 1.000956 | 1206.5579,1206.5798,etc |
| rossiter mclaughlin | RM | 104 | 5 | 2.001397 | 1206.5579,1206.6105,etc |
| infrared processing and analysis center | IPAC | 11 | 5 | 1.000317 | 1206.0269,1206.6352,etc |
| japan society for the promotion of science | JSPS | 7 | 5 | 1.000057 | 1206.2011,1206.4702,etc |
| least squares deconvolution | LSD | 88 | 5 | 2.001031 | 1206.5692,1206.1770,etc |
| chandra x ray center | CXC | 5 | 4 | 1.000031 | 1206.7071,1206.4033,etc |
| semi analytic model | SAM | 35 | 4 | 2.000683 | 1206.2950,1206.3571,etc |
| on the fly | OTF | 7 | 4 | 1.000059 | 1206.2115,1206.1249,etc |
| space telescope imaging spectrograph | STIS | 31 | 4 | 2.000512 | 1206.1353,1206.3797,etc |
| helioseismic and magnetic imager | HMI | 118 | 4 | 2.004876 | 1206.1141,1206.5917,etc |
| hertzsprung russell | HR | 54 | 4 | 2.001161 | 1206.5238,1206.2922,etc |
| kelvin helmholtz | KH | 49 | 4 | 1.000925 | 1206.5006,1206.6516,etc |
| 2 dimensional | 2D | 6 | 4 | 1.000075 | 1206.4047,1206.5803,etc |
| precipitable water vapor | PWV | 20 | 4 | 1.000614 | 1206.4715,1206.0039,etc |
| maximum a posteriori | MAP | 15 | 4 | 1.000321 | 1206.4715,1206.3312,etc |
| right handed | RH | 138 | 4 | 2.002717 | 1206.4944,1206.5537,etc |
| ukirt infrared deep sky survey | UKIDSS | 38 | 4 | 2.000757 | 1206.4060,1206.2919,etc |
| stellar population synthesis | SPS | 62 | 4 | 2.000736 | 1206.2732,1206.4310,etc |
| particle mesh | PM | 13 | 4 | 1.000235 | 1206.5813,1206.5302,etc |
| deutsche forschungsgemeinschaft | DFG | 6 | 4 | 1.000272 | 1206.5803,1206.5133,etc |
| power law | PO | 45 | 4 | 1.001159 | 1206.5304,1206.1444,etc |
| astrophysical research consortium | ARC | 4 | 4 | 1.000019 | 1206.3797,1206.1827,etc |
| infrared dark cloud | IRDC | 213 | 4 | 2.003075 | 1206.1907,1206.6500,etc |
| association of variable star observers | AAVSO | 8 | 4 | 1.00025 | 1206.4035,1206.5133,etc |
| photon dominated region | PDR | 126 | 4 | 2.00242 | 1206.4098,1206.1249,etc |
| test statistic | TS | 24 | 4 | 2.001039 | 1206.3530,1206.1782,etc |
| relativistic mean field | RMF | 50 | 4 | 2.001367 | 1206.0139,1206.2156,etc |
| one dimensional | 1D | 35 | 4 | 1.001825 | 1206.3132,1206.2787,etc |
| post newtonian | PN | 149 | 4 | 2.00701 | 1206.6130,1206.5786,etc |
| lyman werner | LW | 156 | 4 | 2.00449 | 1206.1861,1206.5824,etc |
| spin independent | SI | 25 | 4 | 2.001198 | 1206.6809,1206.2279,etc |
| 2 micron all sky survey | 2MASS | 16 | 4 | 1.001253 | 1206.3873,1206.3569,etc |
| very low mass | VLM | 50 | 4 | 2.00071 | 1206.1045,1206.1021,etc |
| guo shou jing telescope | GSJT | 13 | 4 | 1.000312 | 1206.3577,1206.3378,etc |
| collision induced absorption | CIA | 26 | 4 | 2.001021 | 1206.1021,1206.5519,etc |
| high resolution echelle spectrometer | HIRES | 24 | 4 | 2.001164 | 1206.5579,1206.6533,etc |
| science demonstration phase | SDP | 37 | 4 | 1.002191 | 1206.4550,1206.4919,etc |
| magnetohydrodynamical | MHD | 71 | 4 | 1.001378 | 1206.7096,1206.4173,etc |
| convection dominated accretion flow | CDAF | 29 | 4 | 1.000364 | 1206.4157,1206.4173,etc |
| super massive black hole | SMBH | 32 | 4 | 2.001984 | 1206.0578,1206.3976,etc |
| vienna atomic line database | VALD | 4 | 4 | 1.000076 | 1206.4938,1206.5692,etc |
| intra cluster medium | ICM | 100 | 4 | 2.001062 | 1206.6067,1206.2355,etc |
| infra red | IR | 6 | 3 | 1.000226 | 1206.6374,1206.5021,etc |
| national optical astronomy observatories | NOAO | 5 | 3 | 1.000093 | 1206.1791,1206.6104,etc |
| legacy archive for microwave background data analysis | LAMBDA | 5 | 3 | 1.000166 | 1206.6981,1206.5309,etc |
| white light | WL | 7 | 3 | 1.000534 | 1206.3997,1206.0497,etc |
| supernovae type ia | SNeIa | 38 | 3 | 2.000562 | 1206.5309,1206.6700,etc |
| delay time distribution | DTD | 266 | 3 | 2.005677 | 1206.0665,1206.6897,etc |
| smooth particle hydrodynamics | SPH | 83 | 3 | 1.003534 | 1206.5006,1206.4028,etc |
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