| markov chain monte carlo | MCMC | 186 | 20 | 1.001393 | 1112.2683,1112.3165,etc |
| large area telescope | LAT | 142 | 15 | 1.002232 | 1112.2505,1112.5541,etc |
| synchrotron self compton | SSC | 63 | 15 | 2.001845 | 1112.3933,1112.2253,etc |
| inverse compton | IC | 73 | 14 | 1.000561 | 1112.3933,1112.6247,etc |
| very high energy | VHE | 159 | 14 | 1.003939 | 1112.0786,1112.5940,etc |
| signal to noise | S/N | 217 | 14 | 1.004367 | 1112.0322,1112.2165,etc |
| max planck institute for astronomy | MPIA | 12 | 12 | 1.00007 | 1112.1411,1112.3300,etc |
| kolmogorov smirnov | KS | 47 | 10 | 1.000688 | 1112.1402,1112.2260,etc |
| full width half maximum | FWHM | 34 | 10 | 1.000525 | 1112.3736,1112.0606,etc |
| wolf rayet | WR | 116 | 9 | 2.002575 | 1112.3933,1112.0952,etc |
| japan society for the promotion of science | JSPS | 13 | 9 | 1.000195 | 1112.5955,1112.3030,etc |
| three dimensional | 3D | 84 | 9 | 2.001621 | 1112.3736,1112.4175,etc |
| friedmann robertson walker | FRW | 30 | 8 | 1.000615 | 1112.5178,1112.1830,etc |
| monte carlo markov chain | MCMC | 78 | 8 | 1.002008 | 1112.2350,1112.0326,etc |
| intra cluster medium | ICM | 87 | 8 | 1.00164 | 1112.1599,1112.4848,etc |
| innermost stable circular orbit | ISCO | 71 | 8 | 2.001245 | 1112.0569,1112.4640,etc |
| super massive black hole | SMBH | 120 | 8 | 1.002748 | 1112.1417,1112.2701,etc |
| ultra luminous infrared galaxy | ULIRG | 34 | 8 | 2.000414 | 1112.1195,1112.3358,etc |
| submillimeter array | SMA | 72 | 7 | 2.002803 | 1112.0566,1112.0108,etc |
| sunyaev zel'dovich | S-Z | 352 | 7 | 1.010681 | 1112.2911,1112.6252,etc |
| science and technology facilities council | STFC | 9 | 7 | 1.000197 | 1112.1415,1112.3809,etc |
| star formation history | SFH | 39 | 7 | 1.000418 | 1112.6270,1112.0431,etc |
| dwarf spheroidal | dSph | 266 | 7 | 2.004249 | 1112.0431,1112.4493,etc |
| field programmable gate array | FPGA | 34 | 6 | 2.000981 | 1112.1463,1112.4215,etc |
| interactive data language | IDL | 8 | 6 | 1.000138 | 1112.0656,1112.1062,etc |
| orion nebula cluster | ONC | 141 | 6 | 1.001991 | 1112.2711,1112.3107,etc |
| spin independent | SI | 31 | 6 | 1.000585 | 1112.4387,1112.3123,etc |
| burst alert telescope | BAT | 67 | 6 | 1.000714 | 1112.5940,1112.2029,etc |
| region of interest | ROI | 18 | 6 | 1.000466 | 1112.1476,1112.3312,etc |
| astrophysical research consortium | ARC | 10 | 6 | 1.000136 | 1112.3300,1112.2740,etc |
| data release 7 | DR7 | 30 | 5 | 2.00087 | 1112.2214,1112.0313,etc |
| infrared array camera | IRAC | 19 | 5 | 2.000795 | 1112.5898,1112.1426,etc |
| advanced camera for surveys | ACS | 83 | 5 | 1.001493 | 1112.0313,1112.1426,etc |
| navarro frenk white | NFW | 50 | 5 | 2.000916 | 1112.1703,1112.3447,etc |
| graphics processing unit | GPU | 127 | 5 | 2.004771 | 1112.0065,1112.1701,etc |
| monte carlo | MC | 24 | 5 | 1.00134 | 1112.5162,1112.2600,etc |
| equations of state | EOS | 63 | 5 | 2.003662 | 1112.2878,1112.4154,etc |
| wide field camera 3 | WFC3 | 131 | 5 | 2.002078 | 1112.1426,1112.2657,etc |
| deutsche forschungsgemeinschaft | DFG | 7 | 5 | 1.000054 | 1112.3807,1112.5816,etc |
| legacy archive for microwave background data analysis | LAMBDA | 17 | 5 | 1.000404 | 1112.0924,1112.5435,etc |
| cosmic infrared background | CIB | 45 | 5 | 1.004419 | 1112.6267,1112.1820,etc |
| national research foundation of korea | NRF | 7 | 5 | 1.000136 | 1112.6267,1112.6241,etc |
| luminous red galaxies | LRG | 6 | 4 | 1.000326 | 1112.0170,1112.5447,etc |
| anti de sitter | AdS | 15 | 4 | 1.000602 | 1112.4488,1112.5178,etc |
| supergiant fast x ray transient | SFXT | 18 | 4 | 1.002503 | 1112.3965,1112.5341,etc |
| texas advanced computing center | TACC | 5 | 4 | 1.000107 | 1112.0319,1112.5207,etc |
| effective field theory | EFT | 15 | 4 | 1.000419 | 1112.2683,1112.5185,etc |
| space telescope imaging spectrograph | STIS | 79 | 4 | 2.00148 | 1112.1402,1112.4338,etc |
| two dimensional | 2D | 13 | 4 | 1.000423 | 1112.3736,1112.4175,etc |
| inter stellar medium | ISM | 31 | 4 | 1.001511 | 1112.1703,1112.5221,etc |
| spin dependent | SD | 22 | 4 | 2.000908 | 1112.4387,1112.3123,etc |
| tolman oppenheimer volkoff | TOV | 20 | 4 | 1.000989 | 1112.2878,1112.4154,etc |
| external inverse compton | EIC | 54 | 4 | 2.003605 | 1112.2253,1112.5940,etc |
| science foundation | SNF | 7 | 4 | 1.000822 | 1112.5684,1112.1035,etc |
| damped lyman system | DLA | 242 | 4 | 2.00545 | 1112.0745,1112.1438,etc |
| proto neutron star | PNS | 135 | 4 | 2.006589 | 1112.3342,1112.0335,etc |
| gamma ray burst monitor | GBM | 148 | 4 | 2.005836 | 1112.5190,1112.5940,etc |
| high energy grating | HEG | 33 | 4 | 1.002737 | 1112.1569,1112.1066,etc |
| friedmann lema^itre robertson walker | FLRW | 14 | 4 | 2.000212 | 1112.4798,1112.4837,etc |
| advanced ccd imaging spectrometer | ACIS | 7 | 4 | 1.000086 | 1112.2707,1112.3300,etc |
| natural sciences and engineering research council | NSERC | 4 | 4 | 1.000018 | 1112.4229,1112.4517,etc |
| soft gamma ray repeater | SGR | 5 | 4 | 1.000041 | 1112.1123,1112.1542,etc |
| polarity inversion line | PIL | 87 | 4 | 2.001413 | 1112.3389,1112.3948,etc |
| extreme horizontal branch | EHB | 9 | 4 | 1.000378 | 1112.2925,1112.4269,etc |
| external compton | EC | 8 | 4 | 1.000266 | 1112.3126,1112.3042,etc |
| structure function | SF | 108 | 4 | 1.003756 | 1112.3126,1112.4614,etc |
| post newtonian | pN | 93 | 4 | 2.001843 | 1112.1404,1112.6040,etc |
| integrated sachs wolfe | ISW | 22 | 4 | 1.000853 | 1112.4837,1112.3701,etc |
| infrared spectrograph | IRS | 14 | 4 | 1.00465 | 1112.1461,1112.3386,etc |
| magnetohydrodynamical | MHD | 59 | 4 | 2.000345 | 1112.4390,1112.3801,etc |
| infrared dark cloud | IRDC | 49 | 4 | 2.001905 | 1112.1885,1112.0928,etc |
| cosmic origins spectrograph | COS | 19 | 4 | 1.000389 | 1112.4527,1112.2706,etc |
| sunyaev zeldovich | SZ | 155 | 4 | 2.004429 | 1112.0327,1112.3260,etc |
| friends of friends | FOF | 12 | 4 | 1.000408 | 1112.1031,1112.5479,etc |
| null energy condition | NEC | 30 | 4 | 2.001834 | 1112.4255,1112.2057,etc |
| period luminosity | P-L | 36 | 3 | 1.001228 | 1112.0170,1112.1406,etc |
| high mass x ray binaries | HMXB | 9 | 3 | 2.000387 | 1112.3965,1112.5190,etc |
| infra red | IR | 22 | 3 | 1.000198 | 1112.1087,1112.3895,etc |
| metallicity distribution function | MDF | 26 | 3 | 2.000416 | 1112.2214,1112.5240,etc |
| inamori magellan areal camera and spectrograph | IMACS | 94 | 3 | 2.002119 | 1112.0312,1112.5435,etc |
| ultrahigh energy cosmic ray | UHECR | 38 | 3 | 2.003643 | 1112.4188,1112.5940,etc |
| line of sight velocity distribution | LOSVD | 27 | 3 | 2.001521 | 1112.0319,1112.4497,etc |
| natural science foundation of china | NSFC | 3 | 3 | 1.000124 | 1112.1921,1112.1578,etc |
| particle in cell | PIC | 10 | 3 | 1.000398 | 1112.3933,1112.3114,etc |
| rosat all sky survey | RASS | 12 | 3 | 1.000507 | 1112.5049,1112.1409,etc |
| calibration database | CALDB | 5 | 3 | 1.000137 | 1112.4933,1112.5955,etc |
| newfirm medium band survey | NMBS | 11 | 3 | 1.000583 | 1112.0313,1112.1077,etc |
| ultra luminous x ray source | ULX | 10 | 3 | 1.000345 | 1112.0530,1112.1949,etc |
| hypervelocity star | HVS | 183 | 3 | 2.01243 | 1112.2088,1112.1955,etc |
| supersymmetric | SUSY | 5 | 3 | 1.000178 | 1112.4995,1112.5559,etc |
| star formation rate density | SFR | 20 | 3 | 2.001 | 1112.6270,1112.2260,etc |
| ancillary response file | ARF | 12 | 3 | 2.000114 | 1112.3030,1112.0314,etc |
| gemini multi object spectrograph | GMOS | 35 | 3 | 2.001348 | 1112.2882,1112.4848,etc |
| ministry of science and innovation | MICINN | 5 | 3 | 1.000671 | 1112.1830,1112.1839,etc |
| data processing and analysis consortium | DPAC | 10 | 3 | 2.000307 | 1112.4165,1112.0187,etc |
| angular differential imaging | ADI | 9 | 3 | 1.000304 | 1112.3191,1112.1725,etc |
| infrared science archive | IRSA | 6 | 3 | 1.000138 | 1112.1705,1112.1955,etc |
| submillimeter galaxy | SMG | 37 | 3 | 2.009524 | 1112.1949,1112.6241,etc |
| time of arrival | TOA | 20 | 3 | 1.000773 | 1112.2158,1112.2151,etc |
| one dimensional | 1D | 43 | 3 | 1.002064 | 1112.4175,1112.0745,etc |
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