| markov chain monte carlo | MCMC | 150 | 28 | 1.000654 | 1506.07517,1506.00644,etc |
| signal to noise | S/N | 160 | 23 | 1.000634 | 1506.08043,1506.00635,etc |
| large area telescope | LAT | 204 | 16 | 2.002144 | 1506.07373,1506.05119,etc |
| kolmogorov smirnov | K-S | 68 | 15 | 1.000707 | 1506.04144,1506.03891,etc |
| burst alert telescope | BAT | 215 | 14 | 1.002458 | 1506.06780,1506.06700,etc |
| dark energy survey | DES | 92 | 14 | 2.001372 | 1506.07366,1506.07640,etc |
| square kilometre array | SKA | 285 | 14 | 1.00575 | 1506.04473,1506.05807,etc |
| wolf rayet | WR | 400 | 14 | 2.005717 | 1506.01515,1506.04238,etc |
| monte carlo | MC | 167 | 13 | 2.002107 | 1506.05104,1506.05121,etc |
| innermost stable circular orbit | ISCO | 168 | 12 | 2.001507 | 1506.00560,1506.04056,etc |
| three dimensional | 3D | 254 | 12 | 2.003234 | 1506.01496,1506.07523,etc |
| two dimensional | 2D | 124 | 12 | 1.001294 | 1506.01496,1506.08492,etc |
| advanced camera for surveys | ACS | 109 | 11 | 1.001276 | 1506.01323,1506.04144,etc |
| max planck institute for astronomy | MPIA | 11 | 11 | 1.000071 | 1506.01378,1506.00902,etc |
| wide field camera 3 | WFC3 | 89 | 10 | 2.000986 | 1506.01323,1506.01400,etc |
| asi science data center | ASDC | 12 | 10 | 1.000057 | 1506.06780,1506.08043,etc |
| submillimeter array | SMA | 84 | 10 | 2.001528 | 1506.03244,1506.04160,etc |
| navarro frenk white | NFW | 136 | 10 | 2.002346 | 1506.01529,1506.08202,etc |
| friedmann robertson walker | FRW | 27 | 10 | 1.000485 | 1506.00644,1506.01011,etc |
| one dimensional | 1D | 89 | 10 | 1.001193 | 1506.05494,1506.04796,etc |
| star formation history | SFH | 160 | 10 | 1.001511 | 1506.04155,1506.01653,etc |
| national research foundation of korea | NRF | 19 | 9 | 1.000183 | 1506.05176,1506.08821,etc |
| atacama large millimeter/submillimeter array | ALMA | 105 | 9 | 2.001043 | 1506.00430,1506.07536,etc |
| japan society for the promotion of science | JSPS | 12 | 9 | 1.000225 | 1506.06164,1506.02358,etc |
| inverse compton | IC | 139 | 9 | 1.003253 | 1506.01107,1506.00636,etc |
| synchrotron self compton | SSC | 41 | 8 | 1.000874 | 1506.06780,1506.03947,etc |
| power law | PWRL | 95 | 8 | 1.001039 | 1506.05899,1506.00702,etc |
| proportional counter array | PCA | 24 | 8 | 1.000386 | 1506.06700,1506.02526,etc |
| particle in cell | PIC | 89 | 8 | 1.001623 | 1506.02034,1506.08492,etc |
| ministry of economy and competitiveness | MINECO | 14 | 8 | 1.000117 | 1506.05153,1506.03819,etc |
| space telescope imaging spectrograph | STIS | 114 | 8 | 2.00274 | 1506.07607,1506.03459,etc |
| line of sight velocity distribution | LOSVD | 49 | 7 | 1.000659 | 1506.05315,1506.01037,etc |
| windowed timing | WT | 17 | 7 | 1.000455 | 1506.03079,1506.03376,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 9 | 7 | 1.00008 | 1506.03900,1506.03725,etc |
| effective field theory | EFT | 105 | 7 | 1.002704 | 1506.05107,1506.03047,etc |
| european photon imaging camera | EPIC | 47 | 7 | 2.001351 | 1506.04206,1506.04634,etc |
| friends of friends | FOF | 27 | 6 | 1.000532 | 1506.05877,1506.08222,etc |
| palomar transient factory | PTF | 149 | 6 | 2.002996 | 1506.08719,1506.04829,etc |
| integral field spectroscopy | IFS | 19 | 6 | 1.000373 | 1506.04144,1506.01037,etc |
| integrated sachs wolfe | ISW | 21 | 6 | 1.000435 | 1506.04977,1506.07433,etc |
| post newtonian | PN | 50 | 6 | 1.00103 | 1506.00560,1506.07602,etc |
| super massive black hole | SMBH | 88 | 6 | 2.003297 | 1506.01765,1506.04750,etc |
| helioseismic and magnetic imager | HMI | 36 | 6 | 1.000927 | 1506.08490,1506.01424,etc |
| intra cluster medium | ICM | 46 | 6 | 2.001278 | 1506.00451,1506.06164,etc |
| hertzsprung russell | HR | 61 | 6 | 2.000655 | 1506.05126,1506.02956,etc |
| charge transfer efficiency | CTE | 20 | 6 | 1.000329 | 1506.05718,1506.03089,etc |
| deutsche forschungsgemeinschaft | DFG | 8 | 6 | 1.000105 | 1506.03235,1506.07981,etc |
| stellar population synthesis | SPS | 36 | 6 | 2.000452 | 1506.01653,1506.06762,etc |
| friedmann lema^{i}tre robertson walker | FLRW | 43 | 5 | 1.000615 | 1506.08575,1506.04543,etc |
| maximum likelihood | MLE | 40 | 5 | 2.001467 | 1506.02704,1506.05289,etc |
| magnetohydrodynamical | MHD | 47 | 5 | 2.000518 | 1506.07170,1506.06398,etc |
| colour magnitude diagram | CMD | 152 | 5 | 1.005385 | 1506.01400,1506.03145,etc |
| on the fly | OTF | 7 | 5 | 1.000053 | 1506.01860,1506.08034,etc |
| science analysis software | SAS | 11 | 5 | 1.000422 | 1506.01515,1506.01493,etc |
| gamma ray burst monitor | GBM | 17 | 5 | 1.000465 | 1506.06700,1506.08604,etc |
| ultra violet | UV | 31 | 5 | 2.00078 | 1506.01380,1506.04156,etc |
| spin independent | SI | 82 | 5 | 2.001583 | 1506.01529,1506.06767,etc |
| nasa extragalactic database | NED | 15 | 5 | 1.000117 | 1506.04587,1506.05612,etc |
| photodissociation region | PDR | 99 | 5 | 2.003171 | 1506.06782,1506.03712,etc |
| full width half maximum | FWHM | 30 | 5 | 1.000972 | 1506.01276,1506.04790,etc |
| supersymmetric | SUSY | 37 | 5 | 1.000704 | 1506.02513,1506.08202,etc |
| science and technology facilities council | STFC | 9 | 5 | 1.00014 | 1506.04748,1506.04015,etc |
| cold neutral medium | CNM | 21 | 5 | 1.000465 | 1506.02426,1506.04156,etc |
| self interacting dark matter | SIDM | 45 | 5 | 1.002856 | 1506.00214,1506.08713,etc |
| relativistic mean field | RMF | 20 | 5 | 1.000343 | 1506.05552,1506.00375,etc |
| tolman oppenheimer volkoff | TOV | 11 | 5 | 1.000725 | 1506.05552,1506.01868,etc |
| sunyaev zel'dovich | SZ | 83 | 5 | 1.001723 | 1506.01907,1506.08835,etc |
| national research foundation | NRF | 6 | 5 | 1.000192 | 1506.05153,1506.00730,etc |
| collisional ionization equilibrium | CIE | 38 | 5 | 2.000736 | 1506.07926,1506.07127,etc |
| uksa | UK | 21 | 5 | 2.000422 | 1506.01962,1506.07135,etc |
| photon dominated region | PDR | 108 | 5 | 2.00189 | 1506.03235,1506.01991,etc |
| dwarf spheroidal | dSph | 96 | 5 | 1.002442 | 1506.04155,1506.02041,etc |
| infrared array camera | IRAC | 22 | 4 | 1.000603 | 1506.07037,1506.05153,etc |
| natural science foundation of china | NSFC | 6 | 4 | 1.000171 | 1506.02097,1506.01681,etc |
| basic calibrated data | BCD | 14 | 4 | 1.000366 | 1506.08719,1506.07610,etc |
| total infrared | TIR | 45 | 4 | 1.002085 | 1506.08821,1506.06782,etc |
| carbon enhanced metal poor | CEMP | 357 | 4 | 2.003747 | 1506.04508,1506.05684,etc |
| data release | DR | 23 | 4 | 1.001074 | 1506.05931,1506.04748,etc |
| intermediate frequency | IF | 12 | 4 | 1.000182 | 1506.05931,1506.04827,etc |
| binary black hole | BBH | 121 | 4 | 2.002916 | 1506.00560,1506.03492,etc |
| compact array broadband backend | CABB | 10 | 4 | 1.000313 | 1506.07498,1506.02892,etc |
| calibration database | CALDB | 5 | 4 | 1.000081 | 1506.08604,1506.05736,etc |
| monte carlo markov chain | MCMC | 31 | 4 | 1.000538 | 1506.08089,1506.05298,etc |
| time of arrival | TOA | 18 | 4 | 1.000571 | 1506.02104,1506.00182,etc |
| optical monitor | OM | 33 | 4 | 2.000486 | 1506.05289,1506.08572,etc |
| brightest cluster galaxies | BCG | 15 | 4 | 2.000464 | 1506.00451,1506.06762,etc |
| international centre for radio astronomy research | ICRAR | 4 | 4 | 1.000062 | 1506.00451,1506.01026,etc |
| region of interest | ROI | 36 | 4 | 1.000797 | 1506.05104,1506.05124,etc |
| short gamma ray burst | sGRB | 102 | 4 | 1.003705 | 1506.05048,1506.02359,etc |
| rossiter mclaughlin | RM | 102 | 4 | 2.007729 | 1506.04829,1506.02471,etc |
| proto neutron star | PNS | 7 | 4 | 1.000257 | 1506.00106,1506.02358,etc |
| direct numerical simulations | DNS | 15 | 4 | 1.000922 | 1506.03450,1506.05999,etc |
| national research council | NRC | 5 | 4 | 1.000039 | 1506.03817,1506.01962,etc |
| star forming | SFR | 301 | 4 | 2.003581 | 1506.07791,1506.02670,etc |
| beyond the standard model | BSM | 15 | 4 | 1.000401 | 1506.04057,1506.08195,etc |
| interactive data language | IDL | 9 | 4 | 1.000158 | 1506.07712,1506.08255,etc |
| swiss national science foundation | SNSF | 4 | 4 | 1.000023 | 1506.07981,1506.08309,etc |
| jansky very large array | JVLA | 27 | 4 | 2.000754 | 1506.03679,1506.03075,etc |
| atmospheric imaging assembly | AIA | 56 | 4 | 2.000921 | 1506.07716,1506.08035,etc |
| broken power law | BPL | 25 | 4 | 2.000487 | 1506.05463,1506.02359,etc |
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