| kolmogorov smirnov | KS | 92 | 24 | 1.000567 | 1306.3503,1306.6496,etc |
| markov chain monte carlo | MCMC | 85 | 23 | 1.000449 | 1306.3536,1306.6423,etc |
| signal to noise | S/N | 103 | 19 | 2.00081 | 1306.2317,1306.5946,etc |
| three dimensional | 3D | 161 | 16 | 1.001388 | 1306.1397,1306.3742,etc |
| star formation history | SFH | 168 | 15 | 1.001142 | 1306.1722,1306.3559,etc |
| friedmann robertson walker | FRW | 83 | 14 | 1.000827 | 1306.1364,1306.1637,etc |
| max planck institute for astronomy | MPIA | 14 | 12 | 1.000044 | 1306.0891,1306.5798,etc |
| large area telescope | LAT | 105 | 11 | 2.001685 | 1306.1699,1306.0827,etc |
| colour magnitude diagram | CMD | 103 | 10 | 2.000998 | 1306.0777,1306.1722,etc |
| wolf rayet | WR | 28 | 9 | 1.000318 | 1306.0547,1306.5490,etc |
| deutsche forschungsgemeinschaft | DFG | 12 | 9 | 1.000069 | 1306.3233,1306.5714,etc |
| monte carlo | MC | 372 | 9 | 1.009156 | 1306.3742,1306.5700,etc |
| two dimensional | 2D | 56 | 8 | 1.001727 | 1306.4315,1306.1090,etc |
| chandra x ray center | CXC | 13 | 8 | 1.000142 | 1306.5579,1306.1570,etc |
| ultra violet | UV | 347 | 8 | 1.006121 | 1306.6426,1306.1405,etc |
| full width half maximum | FWHM | 28 | 8 | 1.000171 | 1306.1842,1306.0904,etc |
| inverse compton | IC | 86 | 8 | 1.00339 | 1306.1090,1306.0734,etc |
| galaxy and mass assembly | GAMA | 166 | 8 | 2.002505 | 1306.3990,1306.2424,etc |
| japan society for the promotion of science | JSPS | 14 | 8 | 1.000207 | 1306.5131,1306.4406,etc |
| synchrotron self compton | SSC | 44 | 7 | 1.001974 | 1306.1355,1306.1792,etc |
| photodissociation region | PDR | 114 | 7 | 2.001648 | 1306.1831,1306.5485,etc |
| one dimensional | 1D | 30 | 7 | 1.000752 | 1306.6426,1306.5178,etc |
| friends of friends | FoF | 41 | 7 | 2.000744 | 1306.3990,1306.6496,etc |
| science and technology facilities council | STFC | 9 | 7 | 1.000125 | 1306.6496,1306.3237,etc |
| wide field camera | WFC | 24 | 7 | 1.000217 | 1306.3237,1306.4971,etc |
| advanced camera for surveys | ACS | 79 | 7 | 1.001977 | 1306.0268,1306.2496,etc |
| navarro frenk white | NFW | 54 | 7 | 1.000799 | 1306.6096,1306.6632,etc |
| dark energy survey | DES | 147 | 7 | 1.003457 | 1306.1821,1306.2634,etc |
| ultra luminous infrared galaxy | ULIRG | 75 | 6 | 2.001768 | 1306.1831,1306.3136,etc |
| uksa | UK | 27 | 6 | 1.000187 | 1306.5485,1306.5946,etc |
| advanced ccd imaging spectrometer | ACIS | 13 | 6 | 1.000364 | 1306.1570,1306.1680,etc |
| polarity inversion line | PIL | 121 | 6 | 2.002087 | 1306.1122,1306.1009,etc |
| region of interest | ROI | 39 | 6 | 1.001978 | 1306.2303,1306.0088,etc |
| baryonic acoustic oscillation | BAO | 40 | 6 | 1.00183 | 1306.1527,1306.5932,etc |
| national research foundation of korea | NRF | 10 | 6 | 1.000228 | 1306.0666,1306.1642,etc |
| innermost stable circular orbit | ISCO | 26 | 6 | 1.000924 | 1306.1040,1306.0900,etc |
| axion like particle | ALP | 252 | 6 | 2.005563 | 1306.0443,1306.1425,etc |
| atacama large millimeter array | ALMA | 38 | 5 | 1.00162 | 1306.1831,1306.3572,etc |
| spin independent | SI | 74 | 5 | 1.003373 | 1306.1858,1306.2349,etc |
| spectral and photometric imaging receiver | SPIRE | 97 | 5 | 2.001642 | 1306.5485,1306.3981,etc |
| maximum likelihood | ML | 23 | 5 | 1.000575 | 1306.5485,1306.5581,etc |
| hertzsprung russell | H-R | 21 | 5 | 1.000507 | 1306.3237,1306.6339,etc |
| low luminosity agn | LLAGN | 20 | 5 | 1.00063 | 1306.1570,1306.2639,etc |
| submillimeter array | SMA | 56 | 5 | 2.001397 | 1306.6475,1306.5276,etc |
| magneto rotational instability | MRI | 35 | 5 | 2.001187 | 1306.5243,1306.1871,etc |
| message passing interface | MPI | 11 | 5 | 1.00046 | 1306.1122,1306.0355,etc |
| proportional counter array | PCA | 49 | 5 | 1.00154 | 1306.2475,1306.6237,etc |
| burst alert telescope | BAT | 29 | 5 | 1.000853 | 1306.4096,1306.3949,etc |
| wide field camera 3 | WFC3 | 36 | 5 | 2.000388 | 1306.2496,1306.2940,etc |
| stellar population synthesis | SPS | 31 | 5 | 2.001006 | 1306.5581,1306.6076,etc |
| carbon oxygen | CO | 35 | 5 | 2.001152 | 1306.4024,1306.6007,etc |
| gemini multi object spectrograph | GMOS | 29 | 5 | 2.000347 | 1306.5237,1306.6339,etc |
| quantum field theory | QFT | 71 | 5 | 1.00081 | 1306.0591,1306.1527,etc |
| soft gamma ray repeater | SGR | 21 | 5 | 1.000675 | 1306.4503,1306.5936,etc |
| kelvin helmholtz | KH | 12 | 5 | 1.000464 | 1306.4258,1306.2282,etc |
| super massive black hole | SMBH | 44 | 4 | 1.001806 | 1306.6407,1306.2488,etc |
| particle in cell | PIC | 26 | 4 | 2.000806 | 1306.1355,1306.4380,etc |
| false alarm probability | FAP | 26 | 4 | 2.000411 | 1306.0687,1306.4024,etc |
| arnowitt deser misner | ADM | 12 | 4 | 1.000234 | 1306.4126,1306.4065,etc |
| submillimeter galaxy | SMG | 101 | 4 | 1.002921 | 1306.1831,1306.2288,etc |
| helioseismic and magnetic imager | HMI | 41 | 4 | 1.00062 | 1306.2273,1306.2661,etc |
| spin dependent | SD | 79 | 4 | 1.004382 | 1306.1858,1306.2349,etc |
| semi analytic model | SAM | 54 | 4 | 1.001538 | 1306.1722,1306.6496,etc |
| metallicity distribution function | MDF | 42 | 4 | 1.000777 | 1306.1722,1306.3559,etc |
| international space science institute | ISSI | 4 | 4 | 1.000052 | 1306.1722,1306.3306,etc |
| infrared array camera | IRAC | 27 | 4 | 2.000701 | 1306.5575,1306.0328,etc |
| european pulsar timing array | EPTA | 4 | 4 | 1.000172 | 1306.6719,1306.6911,etc |
| california institute of technology | Caltech | 6 | 4 | 1.000074 | 1306.5243,1306.3500,etc |
| chandra interactive analysis of observations | CIAO | 10 | 4 | 1.000117 | 1306.3500,1306.3387,etc |
| cosmic infrared background | CIB | 13 | 4 | 1.000167 | 1306.2288,1306.3470,etc |
| atacama large millimeter/submillimeter array | ALMA | 19 | 4 | 1.000731 | 1306.2288,1306.0902,etc |
| power law | PL | 39 | 4 | 1.001806 | 1306.6861,1306.3467,etc |
| national research council | NRC | 5 | 4 | 1.000076 | 1306.5271,1306.6626,etc |
| intra cluster medium | ICM | 82 | 4 | 2.002082 | 1306.3102,1306.3101,etc |
| friedmann lema^tre robertson walker | FLRW | 24 | 4 | 2.001058 | 1306.0004,1306.3164,etc |
| x ray luminosity function | XLF | 18 | 4 | 1.000356 | 1306.4316,1306.1227,etc |
| supergiant fast x ray transient | SFXT | 46 | 4 | 1.003465 | 1306.6443,1306.4597,etc |
| very high energy | VHE | 52 | 4 | 2.000808 | 1306.1792,1306.3186,etc |
| atacama pathfinder experiment | APEX | 10 | 4 | 1.000198 | 1306.3470,1306.0042,etc |
| ukirt infrared deep sky survey | UKIDSS | 29 | 4 | 2.000836 | 1306.3156,1306.1369,etc |
| space telescope imaging spectrograph | STIS | 10 | 4 | 1.000095 | 1306.6561,1306.3521,etc |
| hardness ratio | HR | 52 | 4 | 2.000488 | 1306.5752,1306.0640,etc |
| circumstellar medium | CSM | 24 | 4 | 2.000216 | 1306.2337,1306.2638,etc |
| photon dominated region | PDR | 36 | 3 | 1.001968 | 1306.0547,1306.5485,etc |
| hyper suprime cam | HSC | 24 | 3 | 2.000444 | 1306.6407,1306.4684,etc |
| half power beamwidth | HPBW | 4 | 3 | 1.000045 | 1306.3290,1306.4028,etc |
| acousto optical spectrometer | AOS | 3 | 3 | 1.000029 | 1306.3290,1306.0042,etc |
| local interstellar spectra | LIS | 54 | 3 | 2.00465 | 1306.6885,1306.4421,etc |
| lyman werner | LW | 75 | 3 | 2.002329 | 1306.2354,1306.4984,etc |
| compact steep spectrum | CSS | 65 | 3 | 2.001101 | 1306.5579,1306.5237,etc |
| low excitation galaxy | LEG | 32 | 3 | 2.001321 | 1306.5579,1306.4177,etc |
| atmospheric imaging assembly | AIA | 55 | 3 | 1.002324 | 1306.2273,1306.3354,etc |
| monte carlo markov chain | MCMC | 20 | 3 | 1.000285 | 1306.5240,1306.5544,etc |
| instituto de astrof'sica de canarias | IAC | 4 | 3 | 1.000041 | 1306.2680,1306.6093,etc |
| extremely metal poor | EMP | 14 | 3 | 2.00054 | 1306.6426,1306.1834,etc |
| spectral line energy distribution | SLED | 20 | 3 | 1.000704 | 1306.5485,1306.3981,etc |
| transverse traceless | TT | 23 | 3 | 1.00034 | 1306.6719,1306.6911,etc |
| low surface brightness | LSB | 77 | 3 | 2.00451 | 1306.3227,1306.1411,etc |
| national research foundation | NRF | 3 | 3 | 1.000391 | 1306.3227,1306.5191,etc |
| collisional ionization equilibrium | CIE | 16 | 3 | 1.000325 | 1306.4860,1306.4186,etc |
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