| max planck institute for astronomy | MPIA | 191 | 191 | 1.000077 | 0801.1678,0801.3485,etc |
| advanced camera for surveys | ACS | 1746 | 144 | 1.563995 | 0801.1142,0801.2003,etc |
| inverse compton | IC | 1998 | 142 | 1.77 | 0801.2602,0801.2086,etc |
| kolmogorov smirnov | K-S | 511 | 130 | 1.092884 | 0801.4319,0801.4759,etc |
| signal to noise | S/N | 641 | 125 | 1.200621 | 0801.2375,0801.3959,etc |
| markov chain monte carlo | MCMC | 919 | 105 | 1.543844 | 0801.0006,0801.1685,etc |
| friedmann robertson walker | FRW | 634 | 99 | 1.32449 | 0801.2809,0801.2692,etc |
| wolf rayet | W-R | 3689 | 85 | 1.547372 | 0801.1678,0801.3267,etc |
| colour magnitude diagram | CMD | 918 | 81 | 1.582022 | 0801.2774,0801.4661,etc |
| very high energy | VHE | 1038 | 80 | 1.77799 | 0801.4029,0801.3555,etc |
| intra cluster medium | ICM | 1140 | 76 | 1.686272 | 0801.1032,0801.4729,etc |
| synchrotron self compton | SSC | 721 | 75 | 1.454916 | 0801.4029,0801.3599,etc |
| astrophysical research consortium | ARC | 88 | 74 | 1.10823 | 0801.2774,0801.1109,etc |
| star formation history | SFH | 1081 | 70 | 1.503054 | 0801.1184,0801.3297,etc |
| full width half maximum | FWHM | 279 | 68 | 1.08877 | 0801.0630,0801.1223,etc |
| infrared array camera | IRAC | 1332 | 64 | 1.502679 | 0801.2917,0801.2375,etc |
| monte carlo | MC | 523 | 63 | 1.477815 | 0801.3886,0801.1825,etc |
| infrared spectrograph | IRS | 836 | 61 | 1.673482 | 0801.1842,0801.4637,etc |
| friends of friends | FOF | 460 | 61 | 1.574883 | 0801.1127,0801.2771,etc |
| three dimensional | 3D | 595 | 58 | 1.415161 | 0801.2424,0801.4448,etc |
| integrated sachs wolfe | ISW | 858 | 55 | 1.530337 | 0801.2692,0801.0644,etc |
| submillimeter array | SMA | 781 | 52 | 1.522576 | 0801.1236,0801.4493,etc |
| basic calibrated data | BCD | 175 | 51 | 1.000351 | 0801.2917,0801.1842,etc |
| burst alert telescope | BAT | 722 | 51 | 1.513008 | 0801.4029,0801.1236,etc |
| advanced ccd imaging spectrometer | ACIS | 419 | 49 | 1.552087 | 0801.1052,0801.4552,etc |
| dwarf spheroidal | dSph | 1061 | 48 | 1.878067 | 0801.1442,0801.2172,etc |
| magneto rotational instability | MRI | 543 | 47 | 1.448265 | 0801.4004,0801.1637,etc |
| navarro frenk white | NFW | 301 | 47 | 1.490252 | 0801.2169,0801.0630,etc |
| science and technology facilities council | STFC | 59 | 46 | 1.000235 | 0801.0384,0801.4559,etc |
| proportional counter array | PCA | 295 | 45 | 1.20096 | 0801.3329,0801.1259,etc |
| nasa extragalactic database | NED | 155 | 43 | 1.209575 | 0801.4755,0801.0454,etc |
| science analysis system | SAS | 91 | 42 | 1.000214 | 0801.3752,0801.4226,etc |
| space telescope imaging spectrograph | STIS | 336 | 42 | 1.215072 | 0801.0064,0801.4286,etc |
| wide field camera | WFC | 186 | 41 | 1.245124 | 0801.4319,0801.2898,etc |
| power law | PL | 528 | 40 | 1.501783 | 0801.2602,0801.4319,etc |
| photodissociation region | PDR | 409 | 40 | 1.276765 | 0801.4649,0801.1625,etc |
| innermost stable circular orbit | ISCO | 338 | 39 | 1.565386 | 0801.2974,0801.1547,etc |
| two dimensional | 2D | 370 | 39 | 1.386312 | 0802.0327,0802.3220,etc |
| european photon imaging camera | EPIC | 258 | 38 | 1.685071 | 0801.1761,0801.1692,etc |
| ultra luminous infrared galaxy | ULIRG | 314 | 38 | 1.264734 | 0801.0447,0801.1494,etc |
| sunyaev zel'dovich | SZ | 877 | 38 | 1.686652 | 0801.3698,0801.2007,etc |
| orion nebula cluster | ONC | 398 | 37 | 1.596444 | 0801.1329,0801.2584,etc |
| all sky monitor | ASM | 311 | 37 | 1.082378 | 0801.1259,0801.3268,etc |
| super massive black hole | SMBH | 284 | 35 | 1.572771 | 0802.4119,0802.4004,etc |
| monte carlo markov chain | MCMC | 176 | 34 | 1.441826 | 0801.3928,0801.4233,etc |
| japan society for the promotion of science | JSPS | 48 | 34 | 1.000208 | 0801.4827,0801.3186,etc |
| large area telescope | LAT | 360 | 33 | 1.729243 | 0801.1487,0801.4546,etc |
| spitzer science center | SSC | 78 | 32 | 1.000293 | 0801.2917,0801.1223,etc |
| equations of state | EOSs | 451 | 31 | 1.711758 | 0801.3182,0801.0110,etc |
| period luminosity | P-L | 743 | 30 | 1.805168 | 0801.1501,0801.4465,etc |
| charge transfer inefficiency | CTI | 223 | 29 | 1.002602 | 0801.4418,0801.1825,etc |
| square kilometre array | SKA | 301 | 29 | 1.382193 | 0801.2864,0801.3304,etc |
| deutsche forschungsgemeinschaft | DFG | 31 | 28 | 1.000098 | 0801.4004,0801.1986,etc |
| ultra high energy | UHE | 702 | 28 | 1.610416 | 0801.3304,0801.3342,etc |
| wide field planetary camera 2 | WFPC2 | 241 | 28 | 1.679396 | 0802.4446,0802.1210,etc |
| legacy archive for microwave background data analysis | LAMBDA | 56 | 28 | 1.000234 | 0802.4005,0802.1525,etc |
| one dimensional | 1-D | 307 | 28 | 1.572603 | 0803.0805,0803.0990,etc |
| atacama large millimeter array | ALMA | 230 | 27 | 1.445806 | 0801.3848,0801.1272,etc |
| line of sight velocity distribution | LOSVD | 242 | 27 | 1.334396 | 0801.4912,0801.0871,etc |
| low surface brightness | LSB | 589 | 27 | 1.152208 | 0801.2342,0801.2467,etc |
| magneto hydrodynamic | MHD | 105 | 26 | 1.000682 | 0801.0995,0801.3848,etc |
| korea science and engineering foundation | KOSEF | 30 | 26 | 1.000112 | 0801.1558,0801.3186,etc |
| intermediate frequency | IF | 155 | 26 | 1.423544 | 0801.4755,0801.3219,etc |
| large velocity gradient | LVG | 122 | 26 | 1.077433 | 0801.0348,0801.1494,etc |
| non x ray background | NXB | 447 | 26 | 1.501704 | 0801.4029,0801.3315,etc |
| supersymmetric | SUSY | 283 | 26 | 1.616628 | 0801.3334,0801.1645,etc |
| hertzsprung russell | HR | 142 | 26 | 1.539465 | 0801.4010,0801.2155,etc |
| herbig haro | HH | 530 | 26 | 1.617661 | 0802.0518,0802.1424,etc |
| front illuminated | FI | 132 | 26 | 1.308287 | 0803.3858,0803.1528,etc |
| kaluza klein | KK | 583 | 25 | 1.762758 | 0801.0630,0801.3080,etc |
| soft gamma ray repeater | SGR | 455 | 25 | 1.602858 | 0804.1641,0804.1640,etc |
| rosat all sky survey | RASS | 190 | 24 | 1.417664 | 0801.1143,0801.4567,etc |
| particle in cell | PIC | 139 | 24 | 1.20886 | 0801.0995,0801.4583,etc |
| data release 6 | DR6 | 132 | 24 | 1.167136 | 0801.4863,0801.2400,etc |
| wide field channel | WFC | 96 | 24 | 1.208644 | 0801.0832,0801.1111,etc |
| ancillary response file | ARF | 62 | 24 | 1.000234 | 0801.4418,0801.4779,etc |
| galactic centre | GC | 273 | 24 | 1.501478 | 0801.4456,0801.2652,etc |
| smooth particle hydrodynamics | SPH | 208 | 24 | 1.292898 | 0802.0167,0802.0490,etc |
| inter galactic medium | IGM | 217 | 23 | 1.653556 | 0801.1062,0801.2551,etc |
| magellanic cloud | MC | 1976 | 23 | 1.74848 | 0802.3813,0802.0493,etc |
| collisional ionization equilibrium | CIE | 106 | 23 | 1.609229 | 0803.0172,0803.2020,etc |
| metallicity distribution function | MDF | 302 | 22 | 1.682956 | 0801.2124,0801.2159,etc |
| supergiant fast x ray transient | SFXT | 383 | 22 | 1.728959 | 0801.3863,0801.3803,etc |
| post newtonian | PN | 750 | 22 | 1.912378 | 0801.0900,0801.2911,etc |
| kelvin helmholtz | KH | 125 | 21 | 1.715074 | 0801.1825,0801.1048,etc |
| position velocity | PV | 147 | 21 | 1.381515 | 0801.0348,0801.2971,etc |
| michelson doppler imager | MDI | 207 | 21 | 1.667449 | 0801.0898,0801.4448,etc |
| data release 5 | DR5 | 118 | 21 | 1.143337 | 0801.1995,0801.1816,etc |
| optical monitor | OM | 253 | 21 | 1.477365 | 0801.3752,0801.3649,etc |
| dirac born infeld | DBI | 379 | 21 | 1.811477 | 0801.1854,0801.3375,etc |
| circumstellar medium | CSM | 221 | 21 | 1.572618 | 0801.2277,0801.2278,etc |
| photon dominated region | PDR | 177 | 21 | 1.858259 | 0806.3084,0806.0083,etc |
| cosmic infrared background | CIB | 259 | 20 | 1.502359 | 0801.4299,0801.2124,etc |
| narrow line seyfert 1 | NLS1 | 211 | 20 | 1.551334 | 0801.1488,0801.1494,etc |
| short high | SH | 96 | 20 | 1.20035 | 0802.0037,0802.3156,etc |
| back illuminated | BI | 72 | 20 | 1.200324 | 0803.3858,0803.1528,etc |
| luminous red galaxies | LRG | 302 | 19 | 1.422819 | 0801.3928,0801.4380,etc |
| national research council | NRC | 31 | 19 | 1.000098 | 0801.2969,0801.0002,etc |
| ordinary differential equation | ODE | 99 | 19 | 1.474234 | 0801.1023,0801.3303,etc |
| the red giant branch | TRGB | 244 | 19 | 1.633951 | 0803.3728,0803.0551,etc |
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