| markov chain monte carlo | MCMC | 353 | 86 | 1.000967 | 1910.04793,1910.02928,etc |
| european research council | ERC | 94 | 59 | 1.000196 | 1910.02928,1910.00591,etc |
| data processing and analysis consortium | DPAC | 108 | 56 | 1.000142 | 1910.09558,1910.06256,etc |
| dark energy survey | DES | 211 | 24 | 1.002111 | 1910.11327,1910.13548,etc |
| atacama large millimeter/submillimeter array | ALMA | 890 | 24 | 1.006453 | 1910.06980,1910.03863,etc |
| three dimensional | 3-D | 256 | 21 | 1.002049 | 1910.08110,1910.01106,etc |
| kolmogorov smirnov | KS | 98 | 19 | 1.000421 | 1910.13628,1910.00952,etc |
| science and technology facilities council | STFC | 42 | 19 | 1.000471 | 1910.14042,1910.10177,etc |
| star formation history | SFH | 289 | 19 | 2.003615 | 1910.12754,1910.03443,etc |
| one dimensional | 1D | 195 | 17 | 2.001906 | 1910.08110,1910.04929,etc |
| binary neutron star | BNS | 135 | 17 | 1.001694 | 1910.08971,1910.12973,etc |
| binary black hole | BBH | 325 | 17 | 1.003404 | 1910.08971,1910.13409,etc |
| signal to noise | S/N | 128 | 16 | 2.001352 | 1910.02928,1910.13154,etc |
| square kilometre array | SKA | 143 | 16 | 2.001125 | 1910.05377,1910.09634,etc |
| wolf rayet | W-R | 312 | 16 | 2.003689 | 1910.09730,1910.14049,etc |
| chinese academy of sciences | CAS | 39 | 16 | 1.000293 | 1910.06822,1910.03357,etc |
| astrophysik potsdam | AIP | 16 | 16 | 1.000059 | 1910.03076,1910.02962,etc |
| natural science foundation of china | NSFC | 23 | 15 | 1.000361 | 1910.13628,1910.13154,etc |
| innermost stable circular orbit | ISCO | 105 | 15 | 1.002229 | 1910.01148,1910.07804,etc |
| atacama large millimeter array | ALMA | 168 | 15 | 1.002192 | 1910.05830,1910.03130,etc |
| deutsche forschungsgemeinschaft | DFG | 20 | 15 | 1.000157 | 1910.03076,1910.06945,etc |
| two dimensional | 2D | 125 | 14 | 1.002438 | 1910.05386,1910.08560,etc |
| convolutional neural network | CNN | 148 | 14 | 2.002169 | 1910.01148,1910.06617,etc |
| data release 2 | DR2 | 89 | 12 | 2.000934 | 1910.09558,1910.05856,etc |
| navarro frenk white | NFW | 112 | 12 | 2.000659 | 1910.11257,1910.07397,etc |
| effective field theory | EFT | 90 | 12 | 1.001431 | 1910.08837,1910.11569,etc |
| large area telescope | LAT | 208 | 12 | 2.001395 | 1910.00952,1910.14049,etc |
| monte carlo | MC | 113 | 12 | 1.002975 | 1910.09321,1910.10450,etc |
| pan starrs1 surveys | PS1 | 79 | 12 | 1.001726 | 1910.03076,1910.12089,etc |
| hyper suprime cam | HSC | 186 | 12 | 1.00391 | 1910.14672,1910.10927,etc |
| japan society for the promotion of science | JSPS | 26 | 12 | 1.000285 | 1910.13235,1910.11343,etc |
| super massive black hole | SMBH | 225 | 11 | 1.003754 | 1910.05049,1910.10156,etc |
| friends of friends | FoF | 82 | 11 | 1.000774 | 1910.05345,1910.08066,etc |
| wide field camera 3 | WFC3 | 148 | 11 | 2.001105 | 1910.08117,1910.01093,etc |
| event horizon telescope | EHT | 70 | 11 | 1.001144 | 1910.04929,1910.02957,etc |
| max planck institut f"ur extraterrestrische physik | MPE | 17 | 11 | 1.000204 | 1910.02962,1910.07031,etc |
| ultra luminous infrared galaxy | ULIRG | 43 | 10 | 2.000304 | 1910.05049,1910.01661,etc |
| national research foundation of korea | NRF | 23 | 10 | 1.000352 | 1910.11569,1910.02429,etc |
| swiss national science foundation | SNSF | 12 | 10 | 1.000274 | 1910.13350,1910.04627,etc |
| national research council | NRC | 13 | 10 | 1.000084 | 1910.10719,1910.03076,etc |
| einstein telescope | ET | 109 | 10 | 2.002371 | 1910.05631,1910.12357,etc |
| hertzsprung russell | H-R | 28 | 9 | 1.000615 | 1910.09558,1910.09730,etc |
| atmospheric imaging assembly | AIA | 127 | 9 | 2.002288 | 1910.13279,1910.08620,etc |
| ministry of economy and competitiveness | MINECO | 14 | 9 | 1.000367 | 1910.13947,1910.03512,etc |
| advanced camera for surveys | ACS | 108 | 9 | 2.000926 | 1910.08117,1910.10240,etc |
| very high energy | VHE | 55 | 9 | 1.001778 | 1910.00952,1910.14414,etc |
| nexus for exoplanet system science | NExSS | 9 | 9 | 1.00008 | 1910.00609,1910.08659,etc |
| particle in cell | PIC | 47 | 9 | 1.001616 | 1910.02429,1910.13370,etc |
| full width half maximum | FWHM | 71 | 9 | 2.002074 | 1910.03512,1910.06175,etc |
| machine learning | ML | 205 | 9 | 2.005292 | 1910.01529,1910.06330,etc |
| general circulation model | GCM | 106 | 9 | 2.001839 | 1910.07523,1910.02355,etc |
| tolman oppenheimer volkoff | TOV | 57 | 9 | 1.001646 | 1910.10856,1910.12971,etc |
| good time interval | GTI | 16 | 9 | 1.000163 | 1910.02956,1910.04174,etc |
| post newtonian | PN | 158 | 8 | 2.003934 | 1910.05202,1910.08971,etc |
| gaussian process | GP | 54 | 8 | 2.001105 | 1910.01040,1910.03518,etc |
| integral field spectroscopy | IFS | 23 | 8 | 1.00009 | 1910.05377,1910.10759,etc |
| colour magnitude diagram | CMD | 129 | 8 | 2.002455 | 1910.00591,1910.07940,etc |
| galaxy and mass assembly | GAMA | 38 | 8 | 2.000858 | 1910.05255,1910.11539,etc |
| monte carlo markov chain | MCMC | 22 | 8 | 1.000192 | 1910.05416,1910.00459,etc |
| zwicky transient facility | ZTF | 318 | 8 | 2.011847 | 1910.04548,1910.12973,etc |
| dwarf spheroidal | dSph | 85 | 8 | 1.002579 | 1910.03076,1910.10038,etc |
| single degenerate | SD | 119 | 8 | 2.002306 | 1910.02089,1910.01093,etc |
| canadian hydrogen intensity mapping experiment | CHIME | 75 | 8 | 2.0022 | 1910.08120,1910.03652,etc |
| receiver operating characteristic | ROC | 36 | 8 | 1.000431 | 1910.06982,1910.13236,etc |
| natural sciences and engineering research council of canada | NSERC | 11 | 8 | 1.000102 | 1910.01123,1910.10520,etc |
| transit timing variation | TTV | 134 | 8 | 2.00201 | 1910.08522,1910.06794,etc |
| the red giant branch | TRGB | 60 | 8 | 1.003125 | 1910.08748,1910.02788,etc |
| inverse compton | iC | 24 | 7 | 1.000218 | 1910.08231,1910.06578,etc |
| semi analytic model | SAM | 22 | 7 | 1.000409 | 1910.10947,1910.11345,etc |
| world premier international research center initiative | WPI | 8 | 7 | 1.00022 | 1910.02608,1910.13235,etc |
| complex organic molecule | COM | 147 | 7 | 2.003308 | 1910.05830,1910.04652,etc |
| gaussian mixture model | GMM | 36 | 7 | 2.000456 | 1910.08117,1910.05255,etc |
| ultra violet | UV | 199 | 7 | 2.004834 | 1910.14291,1910.13379,etc |
| magneto rotational instability | MRI | 21 | 7 | 1.000201 | 1910.14058,1910.04413,etc |
| infrared array camera | IRAC | 40 | 7 | 1.000951 | 1910.05416,1910.14042,etc |
| double degenerate | DD | 35 | 7 | 2.000439 | 1910.02089,1910.01093,etc |
| power law | PL | 215 | 7 | 2.006435 | 1910.09456,1910.11317,etc |
| ordinary differential equation | ODE | 20 | 7 | 1.000475 | 1910.11929,1910.06586,etc |
| munich institute for astro and particle physics | MIAPP | 6 | 6 | 1.000031 | 1910.08560,1910.02914,etc |
| star forming | SF | 379 | 6 | 2.008559 | 1910.05377,1910.09634,etc |
| diffuse ionized gas | DIG | 90 | 6 | 2.002221 | 1910.09730,1910.13594,etc |
| photodissociation region | PDR | 118 | 6 | 1.001752 | 1910.05830,1910.05416,etc |
| trans planckian censorship conjecture | TCC | 163 | 6 | 2.002241 | 1910.08837,1910.09460,etc |
| atacama compact array | ACA | 30 | 6 | 2.00038 | 1910.13070,1910.11622,etc |
| submillimeter array | SMA | 23 | 6 | 1.000416 | 1910.13070,1910.14082,etc |
| position velocity | PV | 32 | 6 | 2.000355 | 1910.14314,1910.13665,etc |
| telescope access program | TAP | 7 | 6 | 1.000066 | 1910.10719,1910.05068,etc |
| quantum field theory | QFT | 14 | 6 | 1.000065 | 1910.09460,1910.02186,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 6 | 6 | 1.000118 | 1910.04435,1910.05856,etc |
| proto neutron star | PNS | 178 | 6 | 1.00429 | 1910.04288,1910.01679,etc |
| ministry of science, innovation and universities | MCIUN | 12 | 6 | 1.000162 | 1910.10240,1910.06340,etc |
| nasa extragalactic database | NED | 22 | 6 | 1.000141 | 1910.12973,1910.11793,etc |
| dark energy spectroscopic instrument | DESI | 36 | 6 | 1.001437 | 1910.12973,1910.10983,etc |
| artificial neural network | ANN | 101 | 6 | 1.004673 | 1910.07291,1910.06982,etc |
| rectified linear unit | ReLU | 11 | 6 | 1.00022 | 1910.07291,1910.04255,etc |
| stellar population synthesis | SPS | 49 | 6 | 1.001157 | 1910.11345,1910.11884,etc |
| dark energy camera | DECam | 105 | 6 | 2.001068 | 1910.13409,1910.06982,etc |
| cosmic infrared background | CIB | 26 | 6 | 2.0007 | 1910.08353,1910.09881,etc |
| baryonic acoustic oscillation | BAO | 95 | 6 | 1.002962 | 1910.02694,1910.09975,etc |
| equations of state | EOS | 212 | 6 | 2.006345 | 1910.01049,1910.11929,etc |
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