| markov chain monte carlo | MCMC | 108 | 21 | 1.000668 | 1105.6274,1105.3211,etc |
| advanced camera for surveys | ACS | 348 | 20 | 1.00162 | 1105.5405,1105.0444,etc |
| max planck institute for astronomy | MPIA | 16 | 16 | 1.000059 | 1105.1632,1105.3034,etc |
| kolmogorov smirnov | KS | 101 | 14 | 1.001738 | 1105.4676,1105.3125,etc |
| wolf rayet | WR | 538 | 14 | 2.007781 | 1105.1477,1105.5133,etc |
| signal to noise | S/N | 97 | 13 | 2.000785 | 1105.3455,1105.4747,etc |
| inverse compton | IC | 200 | 13 | 2.001407 | 1105.4877,1105.3900,etc |
| large area telescope | LAT | 73 | 12 | 2.001529 | 1105.0572,1105.0772,etc |
| star formation history | SFH | 134 | 12 | 2.001484 | 1105.1882,1105.5265,etc |
| three dimensional | 3D | 69 | 11 | 2.000823 | 1105.5864,1105.5323,etc |
| colour magnitude diagram | CMD | 167 | 11 | 2.00136 | 1105.5682,1105.3455,etc |
| science and technology facilities council | STFC | 14 | 11 | 1.000168 | 1105.1076,1105.3596,etc |
| deutsche forschungsgemeinschaft | DFG | 11 | 10 | 1.000108 | 1105.2326,1105.5405,etc |
| navarro frenk white | NFW | 81 | 10 | 1.001546 | 1105.5189,1105.0444,etc |
| infrared dark cloud | IRDC | 135 | 8 | 2.004616 | 1105.4481,1105.5884,etc |
| infra red | IR | 124 | 8 | 2.002433 | 1105.3455,1105.4539,etc |
| submillimeter array | SMA | 161 | 8 | 2.005627 | 1105.0427,1105.2410,etc |
| two dimensional | 2D | 64 | 8 | 1.002113 | 1105.5323,1105.2487,etc |
| dwarf spheroidal | dSph | 166 | 8 | 1.003242 | 1105.3218,1105.4102,etc |
| proportional counter array | PCA | 97 | 7 | 2.001394 | 1105.5617,1105.2025,etc |
| sunyaev zel'dovich | SZ | 275 | 7 | 2.011034 | 1105.4271,1105.2826,etc |
| very high energy | VHE | 44 | 6 | 2.001956 | 1105.3482,1105.3900,etc |
| synchrotron self compton | SSC | 22 | 6 | 2.000629 | 1105.3482,1105.3900,etc |
| wide field camera 3 | WFC3 | 173 | 6 | 2.002485 | 1105.0472,1105.2522,etc |
| friedmann robertson walker | FRW | 20 | 6 | 1.00024 | 1105.3606,1105.3165,etc |
| imaging atmospheric cherenkov telescope | IACT | 29 | 6 | 2.000592 | 1105.5113,1105.0449,etc |
| burst alert telescope | BAT | 17 | 6 | 1.000282 | 1105.4875,1105.0422,etc |
| wide field camera | WFC | 83 | 6 | 1.00422 | 1105.2837,1105.0606,etc |
| super massive black hole | SMBH | 36 | 6 | 1.000792 | 1105.2778,1105.1677,etc |
| low surface brightness | LSB | 47 | 5 | 2.001053 | 1105.5654,1105.3034,etc |
| ultra high energy | UHE | 85 | 5 | 2.002078 | 1105.5113,1105.3900,etc |
| monte carlo | MC | 22 | 5 | 1.000718 | 1105.5884,1105.5571,etc |
| hertzsprung russell | H-R | 35 | 5 | 1.000641 | 1105.1045,1105.2645,etc |
| innermost stable circular orbit | ISCO | 60 | 5 | 2.001343 | 1105.5617,1105.3586,etc |
| proportional counter unit | PCU | 15 | 5 | 1.000239 | 1105.5617,1105.4717,etc |
| cosmic origins spectrograph | COS | 72 | 5 | 1.002488 | 1105.5381,1105.2323,etc |
| lyman werner | LW | 127 | 5 | 2.002583 | 1105.5158,1105.2395,etc |
| large velocity gradient | LVG | 23 | 5 | 2.000643 | 1105.3787,1105.4199,etc |
| dark energy survey | DES | 27 | 5 | 2.000685 | 1105.2320,1105.1933,etc |
| photodissociation region | PDR | 25 | 5 | 1.001133 | 1105.2055,1105.1107,etc |
| potential field source surface | PFSS | 8 | 5 | 1.000186 | 1105.3119,1105.2191,etc |
| optical monitor | OM | 83 | 5 | 2.001713 | 1105.2717,1105.0590,etc |
| narrow line seyfert 1 | NLS1 | 24 | 5 | 1.001282 | 1105.2218,1105.4391,etc |
| magneto hydrodynamic | MHD | 57 | 5 | 2.000792 | 1105.0387,1105.5491,etc |
| wide field planetary camera 2 | WF/PC2 | 40 | 5 | 1.000859 | 1105.3381,1105.2329,etc |
| lomb scargle | L-S | 7 | 4 | 1.000081 | 1105.5599,1105.6131,etc |
| one dimensional | 1D | 37 | 4 | 2.001787 | 1105.4481,1105.4052,etc |
| ultra deep field | UDF | 48 | 4 | 1.00102 | 1105.2522,1105.3186,etc |
| contact discontinuity | CD | 37 | 4 | 2.000311 | 1105.5966,1105.6342,etc |
| single degenerate | SD | 39 | 4 | 2.001346 | 1105.0754,1105.6188,etc |
| double degenerate | DD | 17 | 4 | 2.000385 | 1105.0754,1105.6188,etc |
| astrophysical research consortium | ARC | 5 | 4 | 1.000062 | 1105.3034,1105.4469,etc |
| semi analytic model | SAM | 124 | 4 | 1.004362 | 1105.6043,1105.0674,etc |
| particle in cell | PIC | 34 | 4 | 1.000274 | 1105.3221,1105.3593,etc |
| main sequence turn off | MSTO | 186 | 4 | 2.003079 | 1105.5388,1105.1317,etc |
| association of variable star observers | AAVSO | 13 | 4 | 2.000143 | 1105.2025,1105.3273,etc |
| magneto rotational instability | MRI | 11 | 4 | 1.000328 | 1105.2821,1105.4459,etc |
| klein nishina | KN | 16 | 4 | 1.000217 | 1105.3900,1105.1591,etc |
| interactive data language | IDL | 6 | 4 | 1.00016 | 1105.2175,1105.2681,etc |
| infrared array camera | IRAC | 26 | 4 | 1.000578 | 1105.4373,1105.2598,etc |
| bose einstein condensate | BEC | 91 | 4 | 2.002665 | 1105.5189,1105.4325,etc |
| intermediate frequency | IF | 41 | 4 | 1.000656 | 1105.0715,1105.4663,etc |
| ultra luminous infrared galaxy | ULIRG | 7 | 4 | 1.000251 | 1105.0602,1105.4177,etc |
| data release 7 | DR7 | 5 | 4 | 1.000144 | 1105.6011,1105.1933,etc |
| turn off | TO | 75 | 4 | 1.002008 | 1105.3691,1105.2022,etc |
| standard perturbation theory | SPT | 78 | 4 | 1.00246 | 1105.1491,1105.1194,etc |
| warm neutral medium | WNM | 22 | 4 | 2.000253 | 1105.2376,1105.4777,etc |
| wide field channel | WFC | 31 | 4 | 2.001005 | 1105.4178,1105.3970,etc |
| legacy archive for microwave background data analysis | LAMBDA | 8 | 4 | 1.000138 | 1105.5885,1105.4426,etc |
| friends of friends | FoF | 25 | 4 | 2.000736 | 1105.3683,1105.1397,etc |
| uniform disk | UD | 38 | 4 | 2.000621 | 1105.3273,1105.0082,etc |
| square kilometre array | SKA | 232 | 4 | 2.01229 | 1105.6333,1105.5953,etc |
| full width half maximum | FWHM | 12 | 4 | 1.000119 | 1105.4559,1105.2172,etc |
| gigahertz peaked spectrum | GPS | 86 | 3 | 2.004106 | 1105.4676,1105.2371,etc |
| metallicity distribution function | MDF | 60 | 3 | 2.001101 | 1105.5864,1105.6037,etc |
| gemini deep deep survey | GDDS | 3 | 3 | 1.000092 | 1105.6274,1105.1868,etc |
| large binocular camera | LBC | 21 | 3 | 2.000258 | 1105.5682,1105.5381,etc |
| kelvin helmholtz | KH | 40 | 3 | 1.00127 | 1105.1344,1105.6236,etc |
| rayleigh taylor | RT | 8 | 3 | 1.00008 | 1105.1344,1105.5966,etc |
| dwarf irregular | dIrr | 15 | 3 | 1.000447 | 1105.5654,1105.4117,etc |
| national research council | NRC | 5 | 3 | 1.000159 | 1105.5654,1105.2047,etc |
| minimal supergravity | mSUGRA | 5 | 3 | 1.000228 | 1105.5136,1105.5162,etc |
| on the fly | OTF | 4 | 3 | 1.000083 | 1105.4481,1105.5207,etc |
| herbig haro | HH | 53 | 3 | 1.001835 | 1105.1663,1105.2702,etc |
| extragalactic ray background | EGRB | 101 | 3 | 2.005235 | 1105.5113,1105.4230,etc |
| monte carlo markov chain | MCMC | 28 | 3 | 2.000973 | 1105.2037,1105.3186,etc |
| advanced ccd imaging spectrometer | ACIS | 18 | 3 | 2.000088 | 1105.3515,1105.0601,etc |
| friedmann lema^itre robertson walker | FLRW | 23 | 3 | 2.000574 | 1105.6088,1105.6366,etc |
| non x ray background | NXB | 22 | 3 | 2.000696 | 1105.5984,1105.3586,etc |
| ultra violet | UV | 13 | 3 | 1.001052 | 1105.4539,1105.3240,etc |
| very large telescope interferometer | VLTI | 11 | 3 | 2.001684 | 1105.4875,1105.0082,etc |
| south east | SE | 20 | 3 | 1.00057 | 1105.1978,1105.5405,etc |
| helioseismic and magnetic imager | HMI | 13 | 3 | 1.001761 | 1105.0953,1105.3119,etc |
| post newtonian | PN | 44 | 3 | 2.002958 | 1105.1845,1105.3184,etc |
| optical path difference | OPD | 38 | 3 | 1.001399 | 1105.3924,1105.0989,etc |
| black hole x ray binary | BHXB | 36 | 3 | 2.000843 | 1105.5617,1105.4694,etc |
| position velocity | PV | 30 | 3 | 2.001057 | 1105.2410,1105.4117,etc |
| national optical astronomy observatories | NOAO | 5 | 3 | 1.000102 | 1105.2025,1105.1164,etc |
| liquid argon | LAr | 59 | 3 | 2.003384 | 1105.5156,1105.4524,etc |
| photon dominated region | PDR | 13 | 3 | 1.002143 | 1105.5158,1105.5219,etc |
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