| markov chain monte carlo | MCMC | 95 | 18 | 2.000693 | 1006.2096,1006.3552,etc |
| kolmogorov smirnov | K-S | 62 | 16 | 2.00034 | 1006.3381,1006.2179,etc |
| max planck institute for astronomy | MPIA | 16 | 16 | 1.000084 | 1006.3255,1006.3975,etc |
| advanced camera for surveys | ACS | 206 | 12 | 2.001482 | 1006.1016,1006.3558,etc |
| friedmann robertson walker | FRW | 46 | 12 | 2.001008 | 1006.1738,1006.1299,etc |
| large area telescope | LAT | 199 | 12 | 2.0027 | 1006.3986,1006.1628,etc |
| sunyaev zel'dovich | SZ | 652 | 11 | 2.007135 | 1006.3068,1006.5599,etc |
| signal to noise | S/N | 76 | 11 | 2.000986 | 1006.0504,1006.5243,etc |
| inverse compton | IC | 153 | 11 | 2.002271 | 1006.3986,1006.2507,etc |
| very high energy | VHE | 166 | 9 | 2.006506 | 1006.4401,1006.5289,etc |
| friends of friends | FoF | 94 | 8 | 2.000971 | 1006.2828,1006.3761,etc |
| metallicity distribution function | MDF | 113 | 8 | 1.00416 | 1006.3594,1006.4885,etc |
| burst alert telescope | BAT | 65 | 8 | 2.00098 | 1006.0286,1006.5463,etc |
| super massive black hole | SMBH | 69 | 7 | 2.001276 | 1006.1016,1006.3536,etc |
| wolf rayet | WR | 201 | 7 | 2.007428 | 1006.0504,1006.0625,etc |
| infrared spectrograph | IRS | 78 | 7 | 1.000828 | 1006.0120,1006.1130,etc |
| navarro frenk white | NFW | 34 | 7 | 1.000719 | 1006.3484,1006.5325,etc |
| colour magnitude diagram | CMD | 50 | 7 | 1.001868 | 1006.5867,1006.0246,etc |
| magneto hydrodynamic | MHD | 73 | 6 | 2.001603 | 1006.3811,1006.4398,etc |
| integrated sachs wolfe | ISW | 30 | 6 | 1.001154 | 1006.5694,1006.0911,etc |
| binary stellar population | BSP | 64 | 6 | 2.005682 | 1006.3590,1006.3975,etc |
| evolutionary population synthesis | EPS | 34 | 6 | 2.002585 | 1006.3590,1006.3975,etc |
| magneto rotational instability | MRI | 43 | 6 | 1.001191 | 1006.5250,1006.4309,etc |
| science and technology facilities council | STFC | 8 | 6 | 1.000058 | 1006.1504,1006.0925,etc |
| synchrotron self compton | SSC | 30 | 6 | 2.00077 | 1006.1649,1006.5289,etc |
| data release 7 | DR7 | 39 | 6 | 2.000528 | 1006.2825,1006.5178,etc |
| ordinary differential equation | ODE | 37 | 6 | 1.000444 | 1006.1355,1006.0299,etc |
| star formation history | SFH | 92 | 6 | 2.001322 | 1006.3831,1006.5555,etc |
| low surface brightness | LSB | 62 | 5 | 2.002542 | 1006.5446,1006.3273,etc |
| three dimensional | 3D | 33 | 5 | 2.001305 | 1006.3239,1006.3579,etc |
| transit timing variation | TTV | 159 | 5 | 2.002195 | 1006.3026,1006.3580,etc |
| ministry of science and innovation | MICINN | 7 | 5 | 1.000053 | 1006.2770,1006.5573,etc |
| wide field camera 3 | WFC3 | 46 | 5 | 1.001973 | 1006.5456,1006.1364,etc |
| spin independent | SI | 86 | 5 | 2.001531 | 1006.0972,1006.5588,etc |
| lick observatory supernova search | LOSS | 93 | 5 | 2.001018 | 1006.3899,1006.4612,etc |
| rosat all sky survey | RASS | 20 | 5 | 1.001211 | 1006.0572,1006.3556,etc |
| dvali gabadadze porrati | DGP | 114 | 5 | 2.008049 | 1006.4889,1006.4630,etc |
| delay time distribution | DTD | 208 | 5 | 1.004149 | 1006.1147,1006.5751,etc |
| dwarf spheroidal | dSph | 117 | 5 | 2.002491 | 1006.5037,1006.3538,etc |
| warm neutral medium | WNM | 21 | 5 | 1.001533 | 1006.1364,1006.5450,etc |
| submillimeter array | SMA | 86 | 5 | 1.002316 | 1006.4058,1006.3084,etc |
| science analysis system | SAS | 10 | 5 | 1.000087 | 1006.1035,1006.2918,etc |
| infrared array camera | IRAC | 61 | 4 | 2.00171 | 1006.1016,1006.2640,etc |
| charge transfer inefficiency | CTI | 7 | 4 | 1.000317 | 1006.3381,1006.2605,etc |
| ultra luminous infrared galaxy | ULIRG | 128 | 4 | 2.00378 | 1006.2408,1006.2336,etc |
| quantum field theory | QFT | 25 | 4 | 2.000278 | 1006.2483,1006.4615,etc |
| false alarm probability | FAP | 26 | 4 | 1.000614 | 1006.4244,1006.5476,etc |
| subdwarf b | sdB | 88 | 4 | 2.003968 | 1006.3170,1006.1756,etc |
| low mass x ray binaries | LMXB | 23 | 4 | 2.000554 | 1006.0485,1006.3106,etc |
| legacy archive for microwave background data analysis | LAMBDA | 11 | 4 | 1.00023 | 1006.1979,1006.5573,etc |
| position velocity | PV | 23 | 4 | 2.000403 | 1006.3273,1006.5873,etc |
| ancillary response file | ARF | 9 | 4 | 1.000179 | 1006.3255,1006.1318,etc |
| innermost stable circular orbit | ISCO | 11 | 4 | 1.000234 | 1006.5394,1006.5168,etc |
| front illuminated | FI | 13 | 4 | 2.000578 | 1006.0335,1006.4486,etc |
| back illuminated | BI | 13 | 4 | 2.000421 | 1006.0335,1006.4486,etc |
| long low | LL | 38 | 4 | 2.001219 | 1006.2153,1006.5470,etc |
| monte carlo | MC | 31 | 4 | 2.000239 | 1006.0978,1006.3536,etc |
| two dimensional | 2-D | 30 | 4 | 1.001518 | 1006.2015,1006.3540,etc |
| hertzsprung russell | H-R | 13 | 4 | 2.00053 | 1006.5695,1006.5481,etc |
| star formation rate density | SFRD | 53 | 4 | 2.000879 | 1006.2336,1006.5712,etc |
| period luminosity | PL | 133 | 4 | 1.01003 | 1006.1821,1006.1553,etc |
| imaging atmospheric cherenkov telescope | IACT | 19 | 4 | 1.00148 | 1006.4835,1006.5955,etc |
| cold neutral medium | CNM | 10 | 4 | 1.000455 | 1006.0793,1006.1364,etc |
| x ray imaging spectrometer | XIS | 86 | 4 | 2.001223 | 1006.3536,1006.5463,etc |
| photodissociation region | PDR | 66 | 4 | 2.001051 | 1006.1964,1006.5470,etc |
| intra cluster medium | ICM | 38 | 4 | 2.000503 | 1006.1648,1006.4486,etc |
| texas advanced computing center | TACC | 6 | 4 | 1.000119 | 1006.3559,1006.2016,etc |
| baryonic acoustic oscillation | BAO | 49 | 4 | 2.002486 | 1006.1105,1006.4845,etc |
| spherical overdensity | SO | 110 | 4 | 2.002399 | 1006.3205,1006.5793,etc |
| all wavelength extended groth strip international survey | AEGIS | 9 | 3 | 1.000113 | 1006.1016,1006.3558,etc |
| blanco cosmology survey | BCS | 12 | 3 | 1.000324 | 1006.3068,1006.5639,etc |
| sydney university molonglo sky survey | SUMSS | 17 | 3 | 1.000756 | 1006.3068,1006.4282,etc |
| lemaitre tolman bondi | LTB | 20 | 3 | 1.001957 | 1006.5694,1006.4735,etc |
| advanced ccd imaging spectrometer | ACIS | 6 | 3 | 1.000533 | 1006.3381,1006.1649,etc |
| circumstellar medium | CSM | 30 | 3 | 1.000783 | 1006.0504,1006.2537,etc |
| space telescope imaging spectrograph | STIS | 55 | 3 | 1.002416 | 1006.1995,1006.5450,etc |
| center for computational astrophysics | CfCA | 3 | 3 | 1.000063 | 1006.5250,1006.3399,etc |
| transneptunian object | TNO | 115 | 3 | 2.001392 | 1006.2220,1006.5949,etc |
| galactic chemical evolution | GCE | 35 | 3 | 1.000428 | 1006.5863,1006.0243,etc |
| galactic ridge x ray emission | GRXE | 28 | 3 | 2.000252 | 1006.2463,1006.5932,etc |
| compact steep spectrum | CSS | 11 | 3 | 1.000648 | 1006.2049,1006.2507,etc |
| chandra x ray center | CXC | 5 | 3 | 1.000078 | 1006.1649,1006.4486,etc |
| universidad de la laguna | ULL | 3 | 3 | 1.000152 | 1006.0120,1006.0231,etc |
| semi analytic model | SAM | 18 | 3 | 1.001111 | 1006.3558,1006.1147,etc |
| region of interest | ROI | 8 | 3 | 1.000066 | 1006.1628,1006.3528,etc |
| vienna atomic line database | VALD | 5 | 3 | 1.000062 | 1006.3710,1006.1627,etc |
| very small grain | VSG | 13 | 3 | 1.000621 | 1006.2770,1006.0206,etc |
| warm ionized medium | WIM | 26 | 3 | 2.001803 | 1006.2770,1006.2187,etc |
| magneto hydrodynamical | MHD | 10 | 3 | 1.000634 | 1006.1305,1006.1967,etc |
| power density spectrum | PDS | 37 | 3 | 2.000585 | 1006.0925,1006.4773,etc |
| noao deep wide field survey | NDWFS | 18 | 3 | 2.000195 | 1006.3071,1006.4162,etc |
| photon dominated region | PDR | 7 | 3 | 1.000241 | 1006.0833,1006.3438,etc |
| wide field infrared camera | WIRC | 14 | 3 | 1.000688 | 1006.5456,1006.0737,etc |
| data release 3 | DR3 | 12 | 3 | 2.000235 | 1006.2166,1006.2043,etc |
| on the fly | OTF | 6 | 3 | 1.000416 | 1006.4631,1006.5764,etc |
| berkeley illinois maryland association | BIMA | 6 | 3 | 1.000408 | 1006.2828,1006.5764,etc |
| infrared science archive | IRSA | 5 | 3 | 1.000341 | 1006.4956,1006.2336,etc |
| rayleigh taylor | RT | 15 | 3 | 2.00184 | 1006.3072,1006.2385,etc |
| fine guidance sensor | FGS | 6 | 3 | 1.000065 | 1006.5243,1006.5932,etc |
| palomar transient factory | PTF | 6 | 3 | 1.000092 | 1006.3899,1006.4612,etc |
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