| markov chain monte carlo | MCMC | 276 | 48 | 1.000648 | 1709.08635,1709.01578,etc |
| very high energy | VHE | 107 | 25 | 2.001534 | 1709.02570,1709.04630,etc |
| signal to noise | S/N | 192 | 21 | 1.001177 | 1709.08661,1709.06731,etc |
| monte carlo | MC | 153 | 19 | 1.001204 | 1709.02570,1709.00690,etc |
| two dimensional | 2D | 234 | 19 | 2.001018 | 1709.00746,1709.03673,etc |
| inverse compton | IC | 259 | 19 | 1.003831 | 1709.09397,1709.07653,etc |
| imaging atmospheric cherenkov telescope | IACT | 62 | 17 | 1.002205 | 1709.02570,1709.00280,etc |
| large area telescope | LAT | 256 | 17 | 2.002442 | 1709.00899,1709.04457,etc |
| data processing and analysis consortium | DPAC | 37 | 17 | 1.000185 | 1709.06471,1709.09378,etc |
| one dimensional | 1D | 155 | 16 | 1.000962 | 1709.00746,1709.06731,etc |
| square kilometre array | SKA | 161 | 16 | 1.001397 | 1709.01827,1709.05184,etc |
| star formation history | SFH | 295 | 15 | 2.002093 | 1709.00429,1709.00457,etc |
| european research council | ERC | 21 | 15 | 1.000182 | 1709.01453,1709.06649,etc |
| deutsche forschungsgemeinschaft | DFG | 19 | 14 | 1.000135 | 1709.09365,1709.02514,etc |
| full width half maximum | FWHM | 52 | 14 | 2.000338 | 1709.05184,1709.03510,etc |
| astrophysik potsdam | AIP | 15 | 14 | 1.00008 | 1709.06335,1709.06649,etc |
| wide field camera 3 | WFC3 | 101 | 13 | 1.001958 | 1709.08635,1709.03502,etc |
| synchrotron self compton | SSC | 83 | 13 | 2.00116 | 1709.09188,1709.09799,etc |
| navarro frenk white | NFW | 42 | 13 | 2.000326 | 1709.05756,1709.01551,etc |
| three dimensional | 3D | 97 | 12 | 1.001713 | 1709.03673,1709.03216,etc |
| region of interest | ROI | 50 | 12 | 1.00092 | 1709.00899,1709.04457,etc |
| kolmogorov smirnov | K-S | 85 | 12 | 1.001286 | 1709.06335,1709.09665,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 16 | 12 | 1.000077 | 1709.03651,1709.05689,etc |
| dark energy survey | DES | 34 | 11 | 2.001149 | 1709.08661,1709.01827,etc |
| friedmann robertson walker | FRW | 69 | 11 | 1.00119 | 1709.09671,1709.02678,etc |
| atacama large millimeter/submillimeter array | ALMA | 134 | 11 | 2.001438 | 1709.01463,1709.03510,etc |
| intra cluster medium | ICM | 85 | 11 | 1.000521 | 1709.01901,1709.02436,etc |
| ministry of economy and competitiveness | MINECO | 16 | 11 | 1.000194 | 1709.06649,1709.00457,etc |
| pan starrs1 surveys | PS1 | 67 | 10 | 2.001311 | 1709.08975,1709.05427,etc |
| particle in cell | PIC | 67 | 10 | 1.000956 | 1709.03673,1709.02961,etc |
| japan society for the promotion of science | JSPS | 17 | 10 | 1.000214 | 1709.03275,1709.06567,etc |
| very large telescope interferometer | VLTI | 48 | 10 | 1.00048 | 1709.01655,1709.01348,etc |
| friends of friends | FOF | 43 | 10 | 1.000423 | 1709.09665,1709.08647,etc |
| hertzsprung russell | HR | 79 | 10 | 2.000653 | 1709.06332,1709.01160,etc |
| colour magnitude diagram | CMD | 132 | 10 | 1.001728 | 1709.01736,1709.09064,etc |
| sunyaev zel'dovich | SZ | 260 | 10 | 2.003076 | 1709.06364,1709.02923,etc |
| monte carlo markov chain | MCMC | 30 | 9 | 1.000467 | 1709.06747,1709.09135,etc |
| helioseismic and magnetic imager | HMI | 114 | 9 | 2.002489 | 1709.03864,1709.01593,etc |
| equations of state | EOS | 113 | 9 | 2.0019 | 1709.02643,1709.07049,etc |
| power law | PL | 453 | 9 | 1.007246 | 1709.04689,1709.00280,etc |
| tolman oppenheimer volkoff | TOV | 59 | 9 | 1.001166 | 1709.07898,1709.03996,etc |
| super massive black hole | SMBH | 79 | 9 | 1.001516 | 1709.05566,1709.09863,etc |
| hyper suprime cam | HSC | 110 | 8 | 1.00179 | 1709.01576,1709.04474,etc |
| space telescope imaging spectrograph | STIS | 147 | 8 | 2.002316 | 1709.04686,1709.01563,etc |
| photodissociation region | PDR | 75 | 8 | 2.001039 | 1709.01463,1709.09232,etc |
| general relativistic | GR | 146 | 8 | 2.000953 | 1709.01598,1709.01660,etc |
| science and technology facilities council | STFC | 15 | 8 | 1.000104 | 1709.01329,1709.03095,etc |
| tycho gaia astrometric solution | TGAS | 115 | 8 | 2.003653 | 1709.06471,1709.03532,etc |
| test statistic | TS | 44 | 8 | 1.001321 | 1709.08319,1709.00131,etc |
| binary black hole | BBH | 265 | 8 | 2.005487 | 1709.03095,1709.01660,etc |
| magneto rotational instability | MRI | 88 | 8 | 2.001593 | 1709.01734,1709.01924,etc |
| swiss national science foundation | SNSF | 9 | 8 | 1.000109 | 1709.01274,1709.05695,etc |
| chinese academy of sciences | CAMS | 17 | 8 | 1.000144 | 1709.01065,1709.01689,etc |
| advanced camera for surveys | ACS | 111 | 8 | 2.001154 | 1709.01093,1709.00406,etc |
| instrument response function | IRF | 25 | 7 | 1.000703 | 1709.02570,1709.00131,etc |
| atmospheric imaging assembly | AIA | 107 | 7 | 1.002164 | 1709.03864,1709.03160,etc |
| cosmic infrared background | CIB | 62 | 7 | 2.002131 | 1709.10271,1709.07897,etc |
| wolf rayet | WR | 283 | 7 | 1.005657 | 1709.01023,1709.08727,etc |
| star formation rate density | SFRD | 59 | 7 | 1.000627 | 1709.00942,1709.07596,etc |
| central molecular zone | CMZ | 56 | 7 | 1.001051 | 1709.00974,1709.02464,etc |
| on the fly | OTF | 16 | 7 | 1.00017 | 1709.00974,1709.08391,etc |
| atacama large millimeter array | ALMA | 163 | 7 | 2.001954 | 1709.02001,1709.07704,etc |
| natural science foundation of china | NSFC | 13 | 7 | 1.000389 | 1709.03500,1709.01689,etc |
| national research foundation | NRF | 14 | 7 | 1.000305 | 1709.06903,1709.08220,etc |
| max planck institut f"ur extraterrestrische physik | MPE | 8 | 7 | 1.000098 | 1709.07003,1709.05438,etc |
| post newtonian | PN | 82 | 6 | 2.001216 | 1709.01598,1709.02816,etc |
| national research foundation of korea | NRF | 19 | 6 | 1.000281 | 1709.06292,1709.02052,etc |
| specific sfr | sSFR | 78 | 6 | 1.000679 | 1709.00429,1709.04601,etc |
| star forming | SF | 117 | 6 | 1.002149 | 1709.01827,1709.09912,etc |
| time of arrival | ToA | 68 | 6 | 1.001405 | 1709.00899,1709.07562,etc |
| european photon imaging camera | EPIC | 9 | 6 | 1.000065 | 1709.07562,1709.08574,etc |
| wide field camera | WFC | 19 | 6 | 1.000193 | 1709.01453,1709.00250,etc |
| ultra luminous infrared galaxy | ULIRG | 22 | 6 | 1.000414 | 1709.06335,1709.00942,etc |
| gaussian process | GP | 65 | 6 | 2.001499 | 1709.03532,1709.00865,etc |
| southern astrophysical research | SOAR | 60 | 6 | 1.001603 | 1709.05689,1709.05044,etc |
| effective field theory | EFT | 125 | 6 | 2.004018 | 1709.03243,1709.10076,etc |
| friedmann lema^itre robertson walker | FLRW | 31 | 6 | 1.001128 | 1709.03243,1709.09192,etc |
| california institute of technology | Caltech | 9 | 6 | 1.000116 | 1709.08679,1709.01957,etc |
| galaxy and mass assembly | GAMA | 131 | 6 | 1.002131 | 1709.08316,1709.07651,etc |
| system equivalent flux density | SEFD | 14 | 5 | 1.0003 | 1709.03491,1709.06752,etc |
| maximum likelihood | ML | 49 | 5 | 2.001064 | 1709.06752,1709.09729,etc |
| false alarm probability | FAP | 27 | 5 | 1.000395 | 1709.01650,1709.08361,etc |
| national research council | NRC | 7 | 5 | 1.000093 | 1709.01650,1709.00011,etc |
| polarity inversion line | PIL | 46 | 5 | 2.00144 | 1709.03864,1709.03216,etc |
| imaging atmospheric cherenkov technique | IACT | 32 | 5 | 1.001422 | 1709.00239,1709.06324,etc |
| silicon photomultiplier | SiPM | 76 | 5 | 2.004636 | 1709.00239,1709.03914,etc |
| millennium institute of astrophysics | MAS | 5 | 5 | 1.000057 | 1709.06605,1709.08656,etc |
| ultra violet | UV | 28 | 5 | 1.001205 | 1709.09232,1709.04867,etc |
| integral field spectroscopy | IFS | 26 | 5 | 2.000269 | 1709.03510,1709.03522,etc |
| burst alert telescope | BAT | 232 | 5 | 2.003439 | 1709.04689,1709.09145,etc |
| high end computing | HEC | 5 | 5 | 1.000119 | 1709.01468,1709.01277,etc |
| jansky very large array | JVLA | 16 | 5 | 1.000353 | 1709.00183,1709.08307,etc |
| auto correlation function | ACF | 17 | 5 | 2.000236 | 1709.09086,1709.05044,etc |
| wide field channel | WFC | 21 | 5 | 1.000214 | 1709.09172,1709.00406,etc |
| magneto hydrodynamic | MHD | 19 | 5 | 2.000408 | 1709.01446,1709.09037,etc |
| michigan state university | MSU | 5 | 5 | 1.000055 | 1709.05689,1709.06087,etc |
| innermost stable circular orbit | ISCO | 16 | 5 | 1.000708 | 1709.09799,1709.03500,etc |
| baryonic acoustic oscillations | BAO | 24 | 5 | 1.000561 | 1709.01074,1709.04141,etc |
| dark energy spectroscopic instrument | DESI | 15 | 5 | 1.000554 | 1709.05024,1709.08709,etc |
| laboratory directed research and development | LDRD | 5 | 5 | 1.000166 | 1709.04043,1709.03751,etc |
|