| 1 | signal to noise | S/N | 88 | 18 | 1.000461 | 1003.6061,1003.3347,etc |
| 2 | kolmogorov smirnov | KS | 66 | 18 | 1.000408 | 1003.5163,1003.0351,etc |
| 3 | large area telescope | LAT | 273 | 16 | 2.004309 | 1003.3475,1003.5163,etc |
| 4 | max planck institute for astronomy | MPIA | 14 | 14 | 1.000083 | 1003.0673,1003.5425,etc |
| 5 | star formation history | SFH | 160 | 12 | 1.001397 | 1003.2565,1003.6061,etc |
| 6 | inverse compton | IC | 242 | 11 | 1.003957 | 1003.3475,1003.3104,etc |
| 7 | colour magnitude diagram | CMD | 101 | 11 | 2.001379 | 1003.0758,1003.6061,etc |
| 8 | intra cluster medium | ICM | 141 | 11 | 2.002858 | 1003.0003,1003.0578,etc |
| 9 | integrated sachs wolfe | ISW | 249 | 10 | 1.003638 | 1003.1259,1003.4468,etc |
| 10 | markov chain monte carlo | MCMC | 45 | 9 | 2.000512 | 1003.0003,1003.6084,etc |
| 11 | advanced camera for surveys | ACS | 50 | 9 | 2.000906 | 1003.6061,1003.1780,etc |
| 12 | friends of friends | FOF | 80 | 9 | 1.000846 | 1003.3021,1003.0939,etc |
| 13 | super massive black hole | SMBH | 239 | 9 | 2.0046 | 1003.4379,1003.1108,etc |
| 14 | ultra luminous infrared galaxy | ULIRG | 90 | 9 | 2.002406 | 1003.5773,1003.2647,etc |
| 15 | double degenerate | DD | 67 | 8 | 1.001404 | 1003.6029,1003.4113,etc |
| 16 | friedmann robertson walker | FRW | 55 | 8 | 1.00108 | 1003.4777,1003.2881,etc |
| 17 | submillimeter array | SMA | 40 | 8 | 1.001214 | 1003.5634,1003.1365,etc |
| 18 | science and technology facilities council | STFC | 12 | 8 | 1.000246 | 1003.0322,1003.2755,etc |
| 19 | science analysis system | SAS | 18 | 8 | 1.000224 | 1003.4128,1003.1789,etc |
| 20 | infrared spectrograph | IRS | 91 | 7 | 2.001106 | 1003.1252,1003.2904,etc |
| 21 | full width half maximum | FWHM | 19 | 7 | 2.000284 | 1003.3790,1003.4318,etc |
| 22 | infrared array camera | IRAC | 127 | 7 | 2.003274 | 1003.0938,1003.1663,etc |
| 23 | square kilometre array | SKA | 79 | 7 | 1.007846 | 1003.4519,1003.1436,etc |
| 24 | three dimensional | 3D | 61 | 7 | 1.001088 | 1003.3646,1003.2406,etc |
| 25 | cosmic infrared background | CIB | 63 | 7 | 2.000558 | 1003.5541,1003.2446,etc |
| 26 | wolf rayet | WR | 112 | 7 | 1.002365 | 1003.4125,1003.3856,etc |
| 27 | advanced ccd imaging spectrometer | ACIS | 126 | 7 | 1.003053 | 1003.2397,1003.5334,etc |
| 28 | astrophysical research consortium | ARC | 6 | 6 | 1.000078 | 1003.0673,1003.3239,etc |
| 29 | single degenerate | SD | 62 | 6 | 1.001505 | 1003.6029,1003.3031,etc |
| 30 | sunyaev zel'dovich | SZ | 155 | 6 | 2.002868 | 1003.0003,1003.0939,etc |
| 31 | basic calibrated data | BCD | 46 | 6 | 2.001272 | 1003.0866,1003.2446,etc |
| 32 | hard x ray | HXR | 131 | 6 | 2.002459 | 1003.0665,1003.2251,etc |
| 33 | monte carlo markov chain | MCMC | 39 | 6 | 2.000486 | 1003.6108,1003.1311,etc |
| 34 | infrared dark cloud | IRDC | 207 | 6 | 2.00258 | 1003.1365,1003.5102,etc |
| 35 | burst alert telescope | BAT | 24 | 6 | 1.003041 | 1003.3573,1003.4404,etc |
| 36 | synchrotron self compton | SSC | 30 | 6 | 1.000814 | 1003.3104,1003.4351,etc |
| 37 | legacy archive for microwave background data analysis | LAMBDA | 9 | 5 | 1.000089 | 1003.0003,1003.6108,etc |
| 38 | dwarf spheroidal | dSph | 25 | 5 | 2.000577 | 1003.5164,1003.4268,etc |
| 39 | photodissociation region | PDR | 61 | 5 | 1.003527 | 1003.2638,1003.3141,etc |
| 40 | very high energy | VHE | 49 | 5 | 1.001906 | 1003.4615,1003.1734,etc |
| 41 | deutsche forschungsgemeinschaft | DFG | 6 | 5 | 1.000324 | 1003.0825,1003.2320,etc |
| 42 | false alarm probability | FAP | 26 | 5 | 1.000293 | 1003.3488,1003.3445,etc |
| 43 | two dimensional | 2D | 37 | 5 | 2.001058 | 1003.3646,1003.5244,etc |
| 44 | innermost stable circular orbit | ISCO | 21 | 5 | 2.000672 | 1003.1430,1003.3417,etc |
| 45 | michelson doppler imager | MDI | 47 | 5 | 1.001381 | 1003.4262,1003.3773,etc |
| 46 | monte carlo | MC | 172 | 5 | 2.005005 | 1003.5759,1003.1521,etc |
| 47 | point source catalog | PSC | 69 | 5 | 1.001765 | 1003.4426,1003.1130,etc |
| 48 | national research council | NRC | 9 | 5 | 1.000217 | 1003.4264,1003.5119,etc |
| 49 | dark energy survey | DES | 19 | 5 | 1.000511 | 1003.0896,1003.2416,etc |
| 50 | dark energy task force | DETF | 38 | 5 | 1.002053 | 1003.2416,1003.5959,etc |
| 51 | infra red | IR | 27 | 4 | 1.000259 | 1003.2835,1003.5119,etc |
| 52 | navarro frenk white | NFW | 89 | 4 | 2.001952 | 1003.1875,1003.0409,etc |
| 53 | galactic centre | GC | 22 | 4 | 2.000307 | 1003.0758,1003.0440,etc |
| 54 | interactive data language | IDL | 9 | 4 | 1.000063 | 1003.3447,1003.1780,etc |
| 55 | one dimensional | 1D | 28 | 4 | 2.000462 | 1003.3646,1003.3697,etc |
| 56 | standard big bang nucleosynthesis | SBBN | 11 | 4 | 1.000317 | 1003.2935,1003.1144,etc |
| 57 | baryonic acoustic oscillations | BAO | 19 | 4 | 2.000606 | 1003.5754,1003.2422,etc |
| 58 | association of variable star observers | AAVSO | 22 | 4 | 1.001087 | 1003.2901,1003.3694,etc |
| 59 | helio and asteroseismology network | HELAS | 4 | 4 | 1.000204 | 1003.4354,1003.0052,etc |
| 60 | optical monitor | OM | 15 | 4 | 1.000097 | 1003.2336,1003.0800,etc |
| 61 | submillimeter galaxy | SMG | 24 | 4 | 1.000437 | 1003.0827,1003.2174,etc |
| 62 | period luminosity | PL | 47 | 4 | 1.001383 | 1003.4518,1003.4135,etc |
| 63 | leiden/argentine/bonn | LAB | 14 | 4 | 2.000466 | 1003.3955,1003.5334,etc |
| 64 | wide field camera | WFC | 24 | 4 | 1.000842 | 1003.5942,1003.5183,etc |
| 65 | murchison wide field array | MWA | 7 | 4 | 1.000131 | 1003.1750,1003.2497,etc |
| 66 | dirac born infeld | DBI | 62 | 4 | 1.00223 | 1003.2881,1003.4094,etc |
| 67 | hard x ray detector | HXD | 25 | 4 | 2.000574 | 1003.3417,1003.1989,etc |
| 68 | general relativistic | GR | 39 | 4 | 1.00171 | 1003.3518,1003.0633,etc |
| 69 | post newtonian | PN | 65 | 4 | 1.001344 | 1003.3865,1003.1860,etc |
| 70 | maximum likelihood | ML | 16 | 4 | 1.000691 | 1003.2307,1003.0632,etc |
| 71 | large velocity gradient | LVG | 34 | 4 | 2.000891 | 1003.0012,1003.5889,etc |
| 72 | external compton | EC | 27 | 4 | 2.000423 | 1003.4293,1003.4676,etc |
| 73 | baryonic acoustic oscillation | BAO | 32 | 4 | 2.000441 | 1003.0008,1003.5722,etc |
| 74 | photon dominated region | PDR | 23 | 4 | 1.00101 | 1003.4219,1003.1375,etc |
| 75 | compact steep spectrum | CSS | 7 | 3 | 1.000031 | 1003.2835,1003.0129,etc |
| 76 | intermediate frequency | IF | 38 | 3 | 2.001973 | 1003.2835,1003.3347,etc |
| 77 | particle in cell | PIC | 15 | 3 | 1.000388 | 1003.1217,1003.1140,etc |
| 78 | balloon borne large aperture submillimeter telescope | BLAST | 245 | 3 | 2.002189 | 1003.0866,1003.0833,etc |
| 79 | supersymmetric | SUSY | 65 | 3 | 2.001389 | 1003.5164,1003.2691,etc |
| 80 | minimal supergravity | mSUGRA | 39 | 3 | 2.00219 | 1003.5164,1003.3677,etc |
| 81 | sunyaev zeldovich | SZ | 60 | 3 | 1.002526 | 1003.3718,1003.0827,etc |
| 82 | spin independent | SI | 41 | 3 | 2.002249 | 1003.5277,1003.2987,etc |
| 83 | spin dependent | SD | 41 | 3 | 2.003327 | 1003.5277,1003.2987,etc |
| 84 | scottish universities physics alliance | SUPA | 3 | 3 | 1.000006 | 1003.5003,1003.3238,etc |
| 85 | kaluza klein | KK | 21 | 3 | 2.001079 | 1003.2691,1003.0904,etc |
| 86 | warm ionized medium | WIM | 58 | 3 | 1.001264 | 1003.2638,1003.4519,etc |
| 87 | hi parkes all sky survey | HIPASS | 9 | 3 | 1.00013 | 1003.3109,1003.3110,etc |
| 88 | automatic photometric telescope | APT | 24 | 3 | 1.000671 | 1003.3488,1003.3444,etc |
| 89 | charge transfer efficiency | CTE | 18 | 3 | 2.000602 | 1003.4626,1003.0786,etc |
| 90 | extended press schechter | EPS | 6 | 3 | 1.000191 | 1003.3021,1003.3442,etc |
| 91 | dual imaging spectrograph | DIS | 9 | 3 | 1.001054 | 1003.3467,1003.3057,etc |
| 92 | cherenkov detector | CD | 42 | 3 | 2.001869 | 1003.5757,1003.5759,etc |
| 93 | silicon charge detector | SCD | 18 | 3 | 1.001269 | 1003.5757,1003.5759,etc |
| 94 | fourier transformation | FFT | 4 | 3 | 1.000388 | 1003.5013,1003.2420,etc |
| 95 | luminous red galaxies | LRG | 10 | 3 | 2.00037 | 1003.3214,1003.2422,etc |
| 96 | magneto hydrodynamic | MHD | 45 | 3 | 1.001235 | 1003.0725,1003.4471,etc |
| 97 | dwarf irregular | dI | 43 | 3 | 2.002765 | 1003.6026,1003.3110,etc |
| 98 | blue compact dwarf | BCD | 9 | 3 | 1.000341 | 1003.6026,1003.0875,etc |
| 99 | ukirt infrared deep sky survey | UKIDSS | 7 | 3 | 1.00061 | 1003.0835,1003.1663,etc |
| 100 | polarity inversion line | PIL | 40 | 3 | 2.001404 | 1003.2333,1003.4653,etc |
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