| markov chain monte carlo | MCMC | 236 | 58 | 1.000679 | 1911.04497,1911.02051,etc |
| data processing and analysis consortium | DPAC | 100 | 50 | 1.000149 | 1911.04500,1911.05745,etc |
| european research council | ERC | 49 | 37 | 1.000103 | 1911.02051,1911.10817,etc |
| signal to noise | S/N | 127 | 28 | 2.000829 | 1911.01433,1911.12455,etc |
| science and technology facilities council | STFC | 65 | 26 | 1.000195 | 1911.06050,1911.08857,etc |
| kolmogorov smirnov | KS | 99 | 23 | 1.000935 | 1911.10212,1911.11877,etc |
| atacama large millimeter/submillimeter array | ALMA | 335 | 23 | 1.001654 | 1911.10756,1911.12999,etc |
| star formation history | SFH | 261 | 19 | 2.001744 | 1911.04095,1911.08857,etc |
| axion like particle | ALP | 850 | 19 | 2.008728 | 1911.12499,1911.07838,etc |
| large area telescope | LAT | 216 | 18 | 1.00174 | 1911.01558,1911.08961,etc |
| astrophysik potsdam | AIP | 18 | 17 | 1.000077 | 1911.04095,1911.10212,etc |
| inverse compton | IC | 207 | 17 | 1.001512 | 1911.06680,1911.08499,etc |
| navarro frenk white | NFW | 141 | 16 | 2.001172 | 1911.04095,1911.07853,etc |
| japan society for the promotion of science | JSPS | 34 | 16 | 1.000232 | 1911.04095,1911.04653,etc |
| synchrotron self compton | SSC | 145 | 16 | 2.001236 | 1911.01558,1911.08961,etc |
| very high energy | VHE | 231 | 15 | 2.003054 | 1911.01558,1911.08961,etc |
| colour magnitude diagram | CMD | 193 | 15 | 2.001569 | 1911.02075,1911.04714,etc |
| effective field theory | EFT | 191 | 15 | 1.002388 | 1911.03305,1911.00853,etc |
| max planck institut f"ur extraterrestrische physik | MPE | 14 | 14 | 1.000069 | 1911.04095,1911.10212,etc |
| dark energy survey | DES | 399 | 14 | 2.006709 | 1911.04507,1911.05717,etc |
| wide field camera 3 | WFC3 | 104 | 14 | 2.000816 | 1911.02051,1911.04496,etc |
| two dimensional | 2D | 121 | 14 | 1.001379 | 1911.00326,1911.00257,etc |
| intra cluster medium | ICM | 220 | 13 | 2.002082 | 1911.03145,1911.05717,etc |
| three dimensional | 3D | 209 | 13 | 2.001707 | 1911.00019,1911.00257,etc |
| square kilometre array | SKA | 301 | 13 | 1.008169 | 1911.07853,1911.03250,etc |
| integral field spectroscopy | IFS | 32 | 12 | 1.000404 | 1911.08857,1911.09367,etc |
| full width half maximum | FWHM | 31 | 12 | 1.000217 | 1911.08857,1911.05902,etc |
| sunyaev zel'dovich | SZ | 419 | 12 | 2.006163 | 1911.10778,1911.03145,etc |
| one dimensional | 1-D | 97 | 12 | 2.001026 | 1911.02983,1911.08596,etc |
| dark energy spectroscopic instrument | DESI | 36 | 12 | 1.001543 | 1911.05717,1911.06823,etc |
| monte carlo | MC | 66 | 11 | 1.000538 | 1911.08857,1911.04589,etc |
| hyper suprime cam | HSC | 218 | 11 | 2.003043 | 1911.11783,1911.12832,etc |
| deutsche forschungsgemeinschaft | DFG | 18 | 11 | 1.00015 | 1911.05092,1911.03479,etc |
| natural science foundation of china | NSFC | 21 | 11 | 1.000251 | 1911.00257,1911.02284,etc |
| super massive black hole | SMBH | 64 | 10 | 2.000476 | 1911.04095,1911.11959,etc |
| circum galactic medium | CGM | 180 | 10 | 2.002529 | 1911.08857,1911.09342,etc |
| atacama large millimeter array | ALMA | 87 | 10 | 2.001119 | 1911.12176,1911.00028,etc |
| swiss national science foundation | SNSF | 12 | 10 | 1.000045 | 1911.02051,1911.02814,etc |
| particle in cell | PIC | 86 | 10 | 2.001345 | 1911.00326,1911.00059,etc |
| friends of friends | FOF | 49 | 10 | 1.000659 | 1911.11959,1911.06768,etc |
| cosmic infrared background | CIB | 190 | 10 | 1.002929 | 1911.05717,1911.09466,etc |
| convolutional neural network | CNN | 162 | 9 | 2.003067 | 1911.09210,1911.06378,etc |
| pan starrs1 surveys | PS1 | 43 | 9 | 1.000705 | 1911.05068,1911.05745,etc |
| wolf rayet | WR | 61 | 9 | 2.000651 | 1911.02023,1911.10638,etc |
| atmospheric imaging assembly | AIA | 115 | 9 | 2.002196 | 1911.00257,1911.08357,etc |
| gaussian process | GP | 155 | 9 | 1.001254 | 1911.12628,1911.05179,etc |
| japan science and technology agency | JST | 8 | 8 | 1.000056 | 1911.04095,1911.04653,etc |
| all sky automated survey for supernovae | ASAS-SN | 91 | 8 | 2.001415 | 1911.08778,1911.13049,etc |
| general circulation model | GCM | 114 | 8 | 2.002361 | 1911.05577,1911.02983,etc |
| galaxy and mass assembly | GAMA | 79 | 8 | 2.001497 | 1911.01433,1911.12888,etc |
| burst alert telescope | BAT | 23 | 8 | 2.00017 | 1911.08961,1911.10028,etc |
| advanced camera for surveys | ACS | 73 | 8 | 2.000843 | 1911.04496,1911.08357,etc |
| stellar population synthesis | SPS | 129 | 8 | 1.004857 | 1911.11877,1911.03479,etc |
| binary neutron star | BNS | 131 | 8 | 1.002182 | 1911.04495,1911.08107,etc |
| transit timing variation | TTV | 76 | 8 | 2.001055 | 1911.07903,1911.07355,etc |
| region of interest | ROI | 26 | 8 | 1.000222 | 1911.08550,1911.09707,etc |
| national research foundation of korea | NRF | 17 | 8 | 1.000119 | 1911.00654,1911.01852,etc |
| position velocity | PV | 77 | 7 | 2.001821 | 1911.11194,1911.10756,etc |
| artificial neural network | ANN | 163 | 7 | 2.001899 | 1911.08857,1911.11767,etc |
| friedmann robertson walker | FRW | 31 | 7 | 1.000495 | 1911.06827,1911.07371,etc |
| innermost stable circular orbit | ISCO | 61 | 7 | 1.003138 | 1911.04305,1911.07645,etc |
| data release 2 | DR2 | 40 | 7 | 2.000701 | 1911.05068,1911.10638,etc |
| binary black hole | BBH | 109 | 7 | 2.002876 | 1911.00903,1911.02588,etc |
| high end computing | HEC | 7 | 7 | 1.000085 | 1911.05150,1911.07872,etc |
| astrophysics in taiwan | ASIAA | 14 | 7 | 1.0001 | 1911.12832,1911.08497,etc |
| imaging atmospheric cherenkov telescope | IACT | 62 | 7 | 2.001797 | 1911.06134,1911.09862,etc |
| galactic chemical evolution | GCE | 98 | 7 | 1.001468 | 1911.02598,1911.01457,etc |
| mean squared error | MSE | 34 | 7 | 1.00132 | 1911.12398,1911.01486,etc |
| photodissociation region | PDR | 41 | 6 | 2.000562 | 1911.04095,1911.00654,etc |
| european photon imaging camera | EPIC | 72 | 6 | 2.000622 | 1911.06560,1911.09568,etc |
| self interacting dark matter | SIDM | 145 | 6 | 1.004528 | 1911.04497,1911.09167,etc |
| space telescope imaging spectrograph | STIS | 49 | 6 | 2.000955 | 1911.02051,1911.12628,etc |
| polarity inversion line | PIL | 61 | 6 | 2.002045 | 1911.10817,1911.00257,etc |
| monte carlo markov chain | MCMC | 33 | 6 | 2.000496 | 1911.08228,1911.09466,etc |
| gamma ray burst monitor | GBM | 31 | 6 | 2.000875 | 1911.08961,1911.04642,etc |
| thermal sunyaev zel'dovich | tSZ | 193 | 6 | 2.003488 | 1911.05717,1911.11841,etc |
| nexus for exoplanet system science | NExSS | 7 | 6 | 1.000052 | 1911.11814,1911.05150,etc |
| natural sciences and engineering research council of canada | NSERC | 6 | 6 | 1.000065 | 1911.08536,1911.03479,etc |
| minimum mass solar nebula | MMSN | 27 | 6 | 1.000344 | 1911.01530,1911.12999,etc |
| northern extended millimeter array | NOEMA | 46 | 6 | 1.005417 | 1911.03479,1911.00028,etc |
| lomb scargle | L-S | 57 | 6 | 1.000835 | 1911.03543,1911.00832,etc |
| kennicutt schmidt | KS | 22 | 6 | 1.000186 | 1911.05252,1911.02041,etc |
| infrared array camera | IRAC | 44 | 6 | 1.001766 | 1911.12628,1911.00560,etc |
| median absolute deviation | MAD | 16 | 6 | 1.000257 | 1911.08390,1911.04370,etc |
| equations of state | EOS | 76 | 6 | 2.002673 | 1911.01983,1911.04182,etc |
| hertzsprung russell | HR | 19 | 5 | 1.000643 | 1911.00018,1911.09972,etc |
| random forest | RF | 136 | 5 | 2.001757 | 1911.08857,1911.11767,etc |
| max planck institute for astronomy | MPIA | 6 | 5 | 1.000048 | 1911.08857,1911.11140,etc |
| reflection grating spectrometer | RGS | 92 | 5 | 1.001956 | 1911.09568,1911.13108,etc |
| support vector machine | SVM | 54 | 5 | 2.002442 | 1911.10778,1911.04572,etc |
| high frequency instrument | HFI | 60 | 5 | 2.001261 | 1911.10778,1911.05717,etc |
| bose einstein condensate | BEC | 40 | 5 | 2.000437 | 1911.00486,1911.07371,etc |
| basic calibrated data | BCD | 10 | 5 | 1.000045 | 1911.02051,1911.01390,etc |
| cold neutral medium | CNM | 18 | 5 | 1.000903 | 1911.09396,1911.03480,etc |
| department of energy | DOE | 7 | 5 | 1.000171 | 1911.03867,1911.06344,etc |
| peccei quinn | PQ | 45 | 5 | 1.003452 | 1911.07838,1911.08550,etc |
| zwicky transient facility | ZTF | 40 | 5 | 1.005826 | 1911.05068,1911.05902,etc |
| inner working angle | IWA | 58 | 5 | 2.001097 | 1911.09808,1911.11814,etc |
| beyond the standard model | BSM | 15 | 5 | 1.000418 | 1911.09169,1911.00532,etc |
| low surface brightness | LSB | 179 | 5 | 2.005222 | 1911.11877,1911.08497,etc |
|