| 1 | inverse compton | IC | 35 | 6 | 2.002204 | 0302039,0302524,etc |
| 2 | kolmogorov smirnov | KS | 35 | 6 | 1.000579 | 0302369,0302211,etc |
| 3 | low surface brightness | LSB | 62 | 6 | 2.002157 | 0302440,0302147,etc |
| 4 | time ordered data | TOD | 26 | 5 | 1.000912 | 0302276,0302224,etc |
| 5 | space telescope imaging spectrograph | STIS | 45 | 5 | 2.001098 | 0302534,0302369,etc |
| 6 | charge transfer efficiency | CTE | 12 | 5 | 1.000245 | 0302434,0302526,etc |
| 7 | nasa extragalactic database | NED | 10 | 5 | 1.000197 | 0302251,0302572,etc |
| 8 | max planck institute for astronomy | MPIA | 4 | 4 | 1.000081 | 0302405,0302287,etc |
| 9 | high electron mobility transistor | HEMT | 10 | 4 | 1.000422 | 0302224,0302207,etc |
| 10 | pulsar wind bubble | PWB | 57 | 4 | 2.003781 | 0302524,0302110,etc |
| 11 | proportional counter array | PCA | 36 | 4 | 1.00063 | 0302611,0302417,etc |
| 12 | signal to noise | S/N | 16 | 4 | 1.000441 | 0302369,0302149,etc |
| 13 | faint object spectrograph | FOS | 33 | 4 | 2.00052 | 0302369,0302394,etc |
| 14 | intra cluster medium | ICM | 109 | 4 | 2.002655 | 0302322,0302185,etc |
| 15 | deutsche forschungsgemeinschaft | DFG | 4 | 4 | 1.000338 | 0302606,0302052,etc |
| 16 | inter stellar medium | ISM | 33 | 4 | 1.002017 | 0302069,0302101,etc |
| 17 | science analysis system | SAS | 8 | 4 | 1.000097 | 0302288,0302570,etc |
| 18 | low resolution | LRS | 27 | 4 | 1.000996 | 0302244,0302251,etc |
| 19 | sunyaev zel'dovich | SZ | 99 | 4 | 1.005357 | 0302471,0302567,etc |
| 20 | colour magnitude diagram | CMD | 68 | 4 | 2.000832 | 0302119,0302428,etc |
| 21 | one dimensional | 1-D | 57 | 4 | 2.001154 | 0302041,0302260,etc |
| 22 | integrated sachs wolfe | ISW | 9 | 4 | 1.000284 | 0302167,0302138,etc |
| 23 | astrophysical research consortium | ARC | 7 | 3 | 1.000637 | 0302405,0302287,etc |
| 24 | synchrotron self compton | SSC | 22 | 3 | 2.001391 | 0302524,0302270,etc |
| 25 | blue compact dwarf | BCD | 111 | 3 | 1.002036 | 0302032,0302221,etc |
| 26 | high surface brightness | HSB | 21 | 3 | 1.002366 | 0302440,0302445,etc |
| 27 | maximum likelihood | ML | 7 | 3 | 1.000204 | 0302553,0302354,etc |
| 28 | differencing assembly | DA | 18 | 3 | 2.000517 | 0302496,0302213,etc |
| 29 | virginia tech spectral line survey | VTSS | 6 | 3 | 1.00007 | 0302024,0302208,etc |
| 30 | southern h alpha sky survey atlas | SHASSA | 19 | 3 | 1.000626 | 0302024,0302208,etc |
| 31 | hot bottom burning | HBB | 22 | 3 | 2.002156 | 0302083,0302090,etc |
| 32 | period luminosity | P-L | 31 | 3 | 1.000802 | 0302083,0302246,etc |
| 33 | wolf rayet | WR | 31 | 3 | 2.00179 | 0302515,0302579,etc |
| 34 | reflection grating spectrometer | RGS | 37 | 3 | 2.002194 | 0302391,0302288,etc |
| 35 | wisconsin h alpha mapper | WHAM | 7 | 3 | 1.000681 | 0302208,0302207,etc |
| 36 | sunyaev zeldovich | SZ | 96 | 3 | 1.00418 | 0302208,0302087,etc |
| 37 | color magnitude | CM | 80 | 3 | 2.004605 | 0302537,0302169,etc |
| 38 | temperature polarization | TE | 46 | 3 | 2.000798 | 0302207,0302213,etc |
| 39 | legacy archive for microwave background data analysis | LAMBDA | 5 | 3 | 1.000153 | 0302207,0302222,etc |
| 40 | san diego supercomputer center | SDSC | 4 | 3 | 1.000139 | 0302293,0302600,etc |
| 41 | compact symmetric object | CSO | 26 | 3 | 2.001291 | 0302211,0302356,etc |
| 42 | 2 micron all sky survey | 2MASS | 56 | 3 | 1.004201 | 0302331,0302572,etc |
| 43 | point source catalog | PSC | 13 | 3 | 2.000149 | 0302164,0302481,etc |
| 44 | full width half maximum | FWHM | 34 | 3 | 2.001194 | 0302091,0302243,etc |
| 45 | ultra violet | UV | 54 | 3 | 2.001649 | 0302491,0302572,etc |
| 46 | advanced camera for surveys | ACS | 56 | 3 | 2.002006 | 0302587,0302402,etc |
| 47 | press schechter | PS | 18 | 3 | 2.001783 | 0302339,0302446,etc |
| 48 | markov chain monte carlo | MCMC | 40 | 3 | 1.001099 | 0302225,0302218,etc |
| 49 | compact steep spectrum | CSS | 33 | 3 | 2.001273 | 0302281,0302356,etc |
| 50 | wide field camera | WFC | 12 | 3 | 2.000299 | 0302205,0302402,etc |
| 51 | dwarf spheroidal | dSph | 56 | 3 | 2.001129 | 0302480,0302287,etc |
| 52 | power law | POWL | 21 | 3 | 2.002172 | 0302546,0302209,etc |
| 53 | national radio astronomy observatory's | NRAO | 6 | 3 | 1.000051 | 0302289,0302066,etc |