| max planck institute for astronomy | MPIA | 20 | 20 | 1.000093 | 0903.3695,0903.3601,etc |
| kolmogorov smirnov | KS | 91 | 19 | 2.000449 | 0903.3258,0903.3057,etc |
| signal to noise | S/N | 82 | 15 | 1.00037 | 0903.4635,0903.2280,etc |
| integrated sachs wolfe | ISW | 111 | 12 | 2.004427 | 0903.1541,0903.4920,etc |
| markov chain monte carlo | MCMC | 142 | 12 | 1.002058 | 0903.2687,0903.4920,etc |
| wolf rayet | WR | 230 | 12 | 2.004617 | 0903.0775,0903.1858,etc |
| very high energy | VHE | 128 | 12 | 2.003907 | 0903.2924,0903.1784,etc |
| star formation history | SFH | 105 | 11 | 1.000892 | 0903.3695,0903.3035,etc |
| sunyaev zel'dovich | SZ | 274 | 11 | 2.003722 | 0903.0401,0903.4410,etc |
| advanced camera for surveys | ACS | 142 | 10 | 2.000953 | 0903.2478,0903.2839,etc |
| full width half maximum | FWHM | 77 | 9 | 1.002483 | 0903.3546,0903.4116,etc |
| burst alert telescope | BAT | 237 | 9 | 2.004734 | 0903.3195,0903.5363,etc |
| intra cluster medium | ICM | 41 | 8 | 1.001188 | 0903.3067,0903.3818,etc |
| synchrotron self compton | SSC | 174 | 8 | 2.003091 | 0903.3655,0903.2924,etc |
| inverse compton | IC | 139 | 8 | 2.002125 | 0903.3649,0903.1824,etc |
| basic calibrated data | BCD | 17 | 7 | 1.000094 | 0903.4063,0903.3405,etc |
| colour magnitude diagram | CMD | 82 | 7 | 2.001179 | 0903.4787,0903.3258,etc |
| infrared array camera | IRAC | 72 | 7 | 2.004362 | 0903.3405,0903.1289,etc |
| navarro frenk white | NFW | 23 | 7 | 1.000307 | 0903.2562,0903.3625,etc |
| science and technology facilities council | STFC | 8 | 7 | 1.000354 | 0903.3967,0903.2924,etc |
| hard x ray | HX | 109 | 7 | 2.002843 | 0903.4175,0903.2271,etc |
| friedmann robertson walker | FRW | 21 | 6 | 1.000641 | 0903.1541,0903.0574,etc |
| astrophysical research consortium | ARC | 6 | 6 | 1.00014 | 0903.3695,0903.5377,etc |
| spitzer science center | SSC | 16 | 6 | 1.000106 | 0903.4063,0903.1661,etc |
| space telescope imaging spectrograph | STIS | 120 | 6 | 2.002114 | 0903.5310,0903.4787,etc |
| infrared spectrograph | IRS | 72 | 6 | 2.000759 | 0903.1289,0903.1495,etc |
| dwarf spheroidal | dSph | 81 | 6 | 1.001472 | 0903.4635,0903.4393,etc |
| all sky monitor | ASM | 147 | 6 | 2.003413 | 0903.3195,0903.2606,etc |
| parameterized post newtonian | PPN | 21 | 6 | 1.000276 | 0903.3602,0903.0866,etc |
| ultra high energy | UHE | 32 | 6 | 1.000839 | 0903.3385,0903.0624,etc |
| magneto hydrodynamic | MHD | 73 | 5 | 2.001218 | 0903.5315,0903.0556,etc |
| submillimeter common user bolometer array | SCUBA | 50 | 5 | 1.000621 | 0903.4063,0903.1354,etc |
| monte carlo | MC | 21 | 5 | 1.000416 | 0903.4557,0903.2350,etc |
| front illuminated | FI | 50 | 5 | 2.001272 | 0903.2878,0903.3307,etc |
| low surface brightness | LSB | 145 | 5 | 2.005138 | 0903.0793,0903.5331,etc |
| dwarf irregular | dIrr | 79 | 5 | 2.001591 | 0903.4635,0903.4364,etc |
| submillimeter array | SMA | 80 | 5 | 2.00124 | 0903.0159,0903.4455,etc |
| period luminosity | PL | 50 | 5 | 1.001565 | 0903.4088,0903.4186,etc |
| windowed timing | WT | 12 | 5 | 1.000263 | 0903.2924,0903.2958,etc |
| turn off | TO | 31 | 5 | 1.000663 | 0903.2839,0903.0896,etc |
| general relativistic | GR | 55 | 5 | 1.00092 | 0903.3582,0903.3047,etc |
| legacy archive for microwave background data analysis | LAMBDA | 8 | 5 | 1.00021 | 0903.4446,0903.2806,etc |
| friends of friends | FOF | 118 | 5 | 2.002414 | 0903.3041,0903.4682,etc |
| spin dependent | SD | 30 | 4 | 2.001645 | 0903.3895,0903.4320,etc |
| three dimensional | 3D | 41 | 4 | 2.002039 | 0903.3885,0903.1872,etc |
| wide field channel | WFC | 28 | 4 | 2.000414 | 0903.1731,0903.2839,etc |
| back illuminated | BI | 37 | 4 | 2.001216 | 0903.2878,0903.3307,etc |
| x ray imaging spectrometer | XIS | 97 | 4 | 2.000601 | 0903.2878,0903.3307,etc |
| non x ray background | NXB | 30 | 4 | 2.000505 | 0903.2878,0903.3307,etc |
| line of sight velocity distribution | LOSVD | 23 | 4 | 1.001707 | 0903.3064,0903.5331,etc |
| rosat all sky survey | RASS | 19 | 4 | 1.000881 | 0903.3067,0903.2981,etc |
| spin independent | SI | 61 | 4 | 2.001796 | 0903.4320,0903.3300,etc |
| chemically peculiar | CP | 48 | 4 | 2.000441 | 0903.3474,0903.5182,etc |
| ordinary differential equation | ODE | 19 | 4 | 2.000225 | 0903.0505,0903.4103,etc |
| position velocity | P-V | 17 | 4 | 1.000206 | 0903.2280,0903.5331,etc |
| spring observatory | SSO | 15 | 4 | 2.001073 | 0903.1123,0903.5121,etc |
| friedmann lemaitre robertson walker | FLRW | 14 | 4 | 1.00016 | 0903.3602,0903.0270,etc |
| the red giant branch | TRGB | 54 | 4 | 1.001697 | 0903.4088,0903.0215,etc |
| compact steep spectrum | CSS | 47 | 4 | 2.004377 | 0903.3846,0903.1899,etc |
| gigahertz peaked spectrum | GPS | 13 | 4 | 2.001352 | 0903.3846,0903.5119,etc |
| smooth particle hydrodynamics | SPH | 112 | 4 | 2.00223 | 0903.3409,0903.4559,etc |
| narrow line seyfert 1 | NLSy1 | 38 | 4 | 1.002503 | 0903.3582,0903.4411,etc |
| dvali gabadadze porrati | DGP | 80 | 4 | 2.002666 | 0903.3738,0903.0528,etc |
| point source catalog | PSC | 6 | 4 | 1.000045 | 0903.2496,0903.0946,etc |
| surface detector | SD | 36 | 3 | 2.000714 | 0903.1755,0903.4716,etc |
| proportional counter array | PCA | 11 | 3 | 1.000198 | 0903.5166,0903.4118,etc |
| orion nebula cluster | ONC | 60 | 3 | 1.00215 | 0903.3242,0903.3893,etc |
| one dimensional | 1D | 29 | 3 | 1.000541 | 0903.3885,0903.4904,etc |
| wide field x ray telescope | WFXT | 50 | 3 | 2.005494 | 0903.1107,0903.5320,etc |
| magneto rotational instability | MRI | 44 | 3 | 1.002073 | 0903.5315,0903.0183,etc |
| herbig haro | HH | 30 | 3 | 2.000057 | 0903.4063,0903.0268,etc |
| cosmic origins spectrograph | COS | 8 | 3 | 1.000029 | 0903.5310,0903.3963,etc |
| thermally pulsing asymptotic giant branch | TP-AGB | 17 | 3 | 1.000592 | 0903.1731,0903.2324,etc |
| ultra deep field | UDF | 13 | 3 | 2.001206 | 0903.1731,0903.3035,etc |
| guaranteed time observations | GTO | 11 | 3 | 1.000132 | 0903.1731,0903.4892,etc |
| atacama large millimeter array | ALMA | 10 | 3 | 2.000289 | 0903.1354,0903.3046,etc |
| wide field and planetary camera 2 | WFPC2 | 43 | 3 | 1.002047 | 0903.4787,0903.2839,etc |
| inter galactic medium | IGM | 13 | 3 | 2.000366 | 0903.2669,0903.0165,etc |
| extended press schechter | EPS | 34 | 3 | 2.0014 | 0903.4492,0903.4681,etc |
| ultra luminous infrared galaxy | ULIRG | 65 | 3 | 2.001289 | 0903.1858,0903.1495,etc |
| super massive black hole | SMBH | 9 | 3 | 1.001865 | 0903.2878,0903.1784,etc |
| hard x ray detector | HXD | 16 | 3 | 1.000234 | 0903.2878,0903.3583,etc |
| metallicity distribution function | MDF | 57 | 3 | 2.002451 | 0903.3258,0903.4211,etc |
| blue compact dwarf | BCD | 39 | 3 | 1.000452 | 0903.0793,0903.2280,etc |
| integral field spectroscopy | IFS | 8 | 3 | 1.000419 | 0903.3064,0903.2280,etc |
| first look survey | FLS | 18 | 3 | 2.00107 | 0903.0299,0903.3035,etc |
| lower centaurus crux | LCC | 43 | 3 | 1.004012 | 0903.3801,0903.0368,etc |
| minimum mass solar nebula | MMSN | 25 | 3 | 2.000914 | 0903.3801,0903.2660,etc |
| semi analytic model | SAM | 72 | 3 | 2.001829 | 0903.4681,0903.3700,etc |
| radio galaxies | RG | 84 | 3 | 1.004767 | 0903.0978,0903.0755,etc |
| navarro, frenk and white | NFW | 17 | 3 | 1.000548 | 0903.4410,0903.2829,etc |
| cassegrain teleskop kamera | CTK | 83 | 3 | 2.009435 | 0903.0822,0903.4116,etc |
| helio and asteroseismology network | HELAS | 3 | 3 | 1.00002 | 0903.3967,0903.0616,etc |
| optical path difference | OPD | 30 | 3 | 2.000424 | 0903.5001,0903.4892,etc |
| far infrared surveyor | FIS | 14 | 3 | 2.000323 | 0903.3350,0903.1333,etc |
| astroparticule et cosmologie | APC | 3 | 3 | 1.000065 | 0903.2924,0903.1582,etc |
| institute of high energy physics | IHEP | 3 | 3 | 1.00002 | 0903.2065,0903.0631,etc |
| gauss bonnet | GB | 32 | 3 | 2.002122 | 0903.4214,0903.0270,etc |
| charge transfer efficiency | CTE | 16 | 3 | 1.000424 | 0903.4325,0903.4511,etc |
| collisional ionization equilibrium | CIE | 34 | 3 | 2.000393 | 0903.4175,0903.1678,etc |
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