| markov chain monte carlo | MCMC | 133 | 25 | 2.000934 | 1404.1375,1404.2273,etc |
| kolmogorov smirnov | KS | 123 | 20 | 1.00098 | 1404.3556,1404.4358,etc |
| signal to noise | S/N | 86 | 18 | 1.000455 | 1404.6540,1404.2782,etc |
| max planck institute for astronomy | MPIA | 14 | 14 | 1.000063 | 1404.1697,1404.0012,etc |
| three dimensional | 3D | 100 | 14 | 2.001429 | 1404.7049,1404.0511,etc |
| star formation history | SFH | 557 | 13 | 2.005935 | 1404.1697,1404.4056,etc |
| large area telescope | LAT | 220 | 13 | 2.001998 | 1404.3556,1404.4059,etc |
| navarro frenk white | NFW | 107 | 10 | 1.001512 | 1404.1375,1404.2538,etc |
| particle in cell | PIC | 87 | 10 | 1.001935 | 1404.2913,1404.0499,etc |
| deutsche forschungsgemeinschaft | DFG | 15 | 9 | 1.000167 | 1404.1375,1404.5964,etc |
| dwarf spheroidal | dSph | 91 | 9 | 2.00123 | 1404.1697,1404.1211,etc |
| sunyaev zel'dovich | SZ | 68 | 8 | 1.002209 | 1404.7130,1404.7735,etc |
| friends of friends | FoF | 30 | 8 | 1.000383 | 1404.7579,1404.1644,etc |
| atacama large millimeter/submillimeter array | ALMA | 60 | 8 | 1.001517 | 1404.7668,1404.7393,etc |
| full width half maximum | FWHM | 31 | 8 | 1.000392 | 1404.6470,1404.6948,etc |
| inverse compton | IC | 91 | 8 | 2.001995 | 1404.3556,1404.6943,etc |
| the red giant branch | TRGB | 214 | 8 | 2.006473 | 1404.7222,1404.2987,etc |
| wide field camera 3 | WFC3 | 68 | 7 | 2.001212 | 1404.1375,1404.2595,etc |
| advanced camera for surveys | ACS | 44 | 7 | 2.000539 | 1404.1375,1404.2186,etc |
| photodissociation region | PDR | 96 | 7 | 2.002712 | 1404.2217,1404.7798,etc |
| monte carlo | MC | 62 | 7 | 1.00118 | 1404.5986,1404.5102,etc |
| imaging atmospheric cherenkov telescope | IACT | 42 | 7 | 1.001003 | 1404.5017,1404.2734,etc |
| position velocity | PV | 54 | 7 | 1.000677 | 1404.5298,1404.0728,etc |
| innermost stable circular orbit | ISCO | 50 | 7 | 2.000698 | 1404.1543,1404.0527,etc |
| two dimensional | 2D | 44 | 7 | 1.000832 | 1404.3961,1404.2646,etc |
| japan society for the promotion of science | JSPS | 11 | 6 | 1.000098 | 1404.7579,1404.6066,etc |
| intra cluster medium | ICM | 47 | 6 | 2.00062 | 1404.2782,1404.1384,etc |
| wolf rayet | WR | 176 | 6 | 1.004714 | 1404.2597,1404.5755,etc |
| post newtonian | PN | 72 | 6 | 2.002762 | 1404.0092,1404.1543,etc |
| colour magnitude diagram | CMD | 41 | 6 | 1.000563 | 1404.5807,1404.6952,etc |
| photon dominated region | PDR | 59 | 6 | 1.000995 | 1404.0121,1404.7143,etc |
| very high energy | VHE | 127 | 6 | 2.00283 | 1404.6943,1404.2193,etc |
| dark energy survey | DES | 11 | 5 | 1.000126 | 1404.2782,1404.1740,etc |
| metallicity distribution function | MDF | 77 | 5 | 2.001853 | 1404.7291,1404.2476,etc |
| ultra violet | UV | 20 | 5 | 2.000655 | 1404.5676,1404.5004,etc |
| hertzsprung russell | HR | 27 | 5 | 1.000625 | 1404.7384,1404.4358,etc |
| kernel density estimation | KDE | 38 | 5 | 1.00068 | 1404.5211,1404.5960,etc |
| wilson devinney | WD | 5 | 5 | 1.000065 | 1404.2808,1404.2790,etc |
| region of interest | ROI | 14 | 5 | 1.000309 | 1404.4059,1404.5004,etc |
| magneto hydrodynamic | MHD | 42 | 5 | 2.0017 | 1404.6889,1404.4651,etc |
| effective field theory | EFT | 14 | 5 | 1.000252 | 1404.3713,1404.7522,etc |
| charge transfer efficiency | CTE | 14 | 5 | 1.000274 | 1404.1037,1404.0213,etc |
| burst alert telescope | BAT | 30 | 5 | 1.001959 | 1404.0899,1404.7367,etc |
| leiden/argentine/bonn | LAB | 7 | 4 | 1.000123 | 1404.7130,1404.0152,etc |
| carbon enhanced metal poor | CEMP | 150 | 4 | 2.005703 | 1404.0385,1404.0234,etc |
| circumstellar medium | CSM | 55 | 4 | 2.001696 | 1404.4463,1404.2282,etc |
| infrared processing and analysis center | IRSA | 35 | 4 | 2.000493 | 1404.0234,1404.6505,etc |
| atacama pathfinder experiment | APEX | 69 | 4 | 1.002912 | 1404.7668,1404.7103,etc |
| astrophysik potsdam | AIP | 7 | 4 | 1.000471 | 1404.2217,1404.6354,etc |
| integral field spectroscopy | IFS | 46 | 4 | 2.000323 | 1404.2217,1404.1082,etc |
| false alarm probability | FAP | 28 | 4 | 2.000277 | 1404.3247,1404.1267,etc |
| national research council | NRC | 5 | 4 | 1.000041 | 1404.5807,1404.0125,etc |
| inter galactic medium | IGM | 31 | 4 | 2.000822 | 1404.5301,1404.6524,etc |
| spectral line energy distribution | SLED | 128 | 4 | 1.002871 | 1404.6470,1404.6090,etc |
| chandra x ray center | CXC | 5 | 4 | 1.000056 | 1404.5211,1404.5315,etc |
| natural sciences and engineering research council | NSERC | 6 | 4 | 1.000159 | 1404.7142,1404.6236,etc |
| synchrotron self compton | SSC | 17 | 4 | 1.000415 | 1404.3556,1404.6943,etc |
| test statistic | TS | 19 | 4 | 1.000972 | 1404.3556,1404.4059,etc |
| friedmann robertson walker | FRW | 22 | 4 | 1.001103 | 1404.7825,1404.3713,etc |
| submillimeter array | SMA | 53 | 4 | 2.00129 | 1404.1954,1404.2024,etc |
| soft x ray | SXR | 13 | 4 | 1.000647 | 1404.7223,1404.6117,etc |
| loop quantum cosmology | LQC | 86 | 4 | 2.00176 | 1404.4364,1404.2944,etc |
| atacama large millimeter array | ALMA | 52 | 4 | 1.002919 | 1404.7128,1404.5849,etc |
| time of arrival | TOA | 52 | 4 | 1.001842 | 1404.4682,1404.1267,etc |
| general relativistic magnetohydrodynamic | GRMHD | 10 | 4 | 1.00037 | 1404.6889,1404.5495,etc |
| sub mm galaxy | SMG | 21 | 4 | 1.000649 | 1404.2578,1404.2297,etc |
| super massive black hole | SMBH | 164 | 4 | 2.006151 | 1404.0379,1404.5183,etc |
| transit timing variation | TTV | 43 | 4 | 2.001264 | 1404.5617,1404.6354,etc |
| california institute of technology | Caltech | 6 | 4 | 1.000077 | 1404.5620,1404.5614,etc |
| star forming | SF | 211 | 4 | 2.001726 | 1404.0881,1404.1082,etc |
| national research foundation of korea | NRF | 5 | 4 | 1.000149 | 1404.7855,1404.1630,etc |
| extreme mass ratio inspiral | EMRI | 50 | 4 | 2.001041 | 1404.1543,1404.3848,etc |
| centre of excellence for all sky astrophysics | CAASTRO | 5 | 4 | 1.000048 | 1404.1002,1404.3799,etc |
| charge transfer inefficiency | CTI | 15 | 4 | 1.000649 | 1404.3587,1404.3561,etc |
| science and technology facilities council | STFC | 4 | 4 | 1.000104 | 1404.2206,1404.2611,etc |
| spin independent | SI | 28 | 4 | 1.001031 | 1404.6705,1404.5257,etc |
| near infrared integral field spectrograph | NIFS | 60 | 4 | 2.001285 | 1404.0728,1404.7539,etc |
| kelvin helmholtz | KH | 31 | 4 | 2.000157 | 1404.0728,1404.0521,etc |
| european photon imaging camera | EPIC | 7 | 4 | 1.000064 | 1404.3823,1404.1532,etc |
| angular differential imaging | ADI | 80 | 4 | 1.003141 | 1404.1574,1404.4635,etc |
| cosmic origins spectrograph | COS | 44 | 3 | 2.001668 | 1404.6540,1404.2933,etc |
| apparent optical depth | AOD | 6 | 3 | 1.000107 | 1404.6540,1404.2639,etc |
| ultra luminous infrared galaxy | ULIRG | 9 | 3 | 1.000382 | 1404.4875,1404.4371,etc |
| advanced ccd imaging spectrometer | ACIS | 7 | 3 | 1.00006 | 1404.4875,1404.1532,etc |
| probability to exceed | PTE | 12 | 3 | 2.000338 | 1404.1375,1404.6530,etc |
| supersymmetric | SUSY | 38 | 3 | 2.003334 | 1404.4976,1404.1373,etc |
| thermal sunyaev zeldovich | tSZ | 88 | 3 | 1.002428 | 1404.2782,1404.4808,etc |
| luminous red galaxies | LRG | 12 | 3 | 1.001363 | 1404.1933,1404.0238,etc |
| inter stellar medium | ISM | 7 | 3 | 1.000266 | 1404.4463,1404.6066,etc |
| adaptive refinement tree | ART | 3 | 3 | 1.000073 | 1404.4634,1404.4636,etc |
| low mass x ray binaries | LMXB | 63 | 3 | 2.00062 | 1404.0134,1404.2578,etc |
| non x ray background | NXB | 6 | 3 | 1.000068 | 1404.0134,1404.7486,etc |
| response matrix file | RMF | 3 | 3 | 1.000027 | 1404.0134,1404.2631,etc |
| binary population synthesis | BPS | 22 | 3 | 2.001072 | 1404.0219,1404.3848,etc |
| pan starrs1 surveys | PS1 | 101 | 3 | 2.000872 | 1404.4823,1404.2004,etc |
| infrared science archive | IRSA | 32 | 3 | 1.000541 | 1404.4371,1404.1953,etc |
| infra red | IR | 36 | 3 | 2.000812 | 1404.4811,1404.3644,etc |
| wide field camera | WFC | 38 | 3 | 2.001291 | 1404.5807,1404.2539,etc |
| circum galactic medium | CGM | 14 | 3 | 1.000618 | 1404.5301,1404.7656,etc |
| all sky imaging survey | AIS | 14 | 3 | 1.000858 | 1404.5301,1404.4882,etc |
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