| inverse compton | IC | 131 | 7 | 2.00362 | 9906272,9906212,etc |
| very high energy | VHE | 156 | 7 | 2.002871 | 9906405,9906137,etc |
| all sky monitor | ASM | 51 | 6 | 1.002916 | 9906087,9906150,etc |
| signal to noise | S/N | 45 | 5 | 2.000446 | 9906468,9906189,etc |
| intermediate frequency | IF | 16 | 4 | 1.000478 | 9906504,9906321,etc |
| optical transient | OT | 44 | 4 | 2.002154 | 9906395,9906096,etc |
| burst and transient source experiment | BATSE | 35 | 4 | 2.001 | 9906394,9906096,etc |
| wide field planetary camera 2 | WFPC2 | 69 | 4 | 2.000727 | 9906484,9906206,etc |
| landau pomeranchuk migdal | LPM | 23 | 3 | 2.003092 | 9906504,9906347,etc |
| phoswich detector system | PDS | 48 | 3 | 1.001613 | 9906476,9906162,etc |
| wide field and planetary camera 2 | WFPC2 | 13 | 3 | 1.000229 | 9906335,9906462,etc |
| gas imaging spectrometer | GIS | 42 | 3 | 2.001686 | 9906294,9906364,etc |
| particle mesh | PM | 22 | 3 | 2.00007 | 9906413,9906155,etc |
| kolmogorov smirnov | KS | 8 | 3 | 1.000186 | 9906466,9906163,etc |
| standard cold dark matter | SCDM | 60 | 3 | 2.001529 | 9906032,9906169,etc |
| intra cluster medium | ICM | 19 | 3 | 1.00316 | 9906169,9906329,etc |
| proportional counter array | PCA | 9 | 3 | 1.000224 | 9906178,9906122,etc |
| san diego supercomputer center | SDSC | 3 | 3 | 1.000016 | 9906016,9906238,etc |
| space interferometry mission | SIM | 26 | 3 | 1.00299 | 9906472,9906126,etc |
| ultra luminous infrared galaxy | ULIRG | 43 | 3 | 2.002352 | 9906493,9906332,etc |
| rosat all sky survey | RASS | 13 | 3 | 2.002019 | 9906163,9906316,etc |
| press schechter | PS | 30 | 3 | 1.001654 | 9906204,9906093,etc |
| cerro tololo interamerican observatory | CTIO | 40 | 3 | 1.002465 | 9906173,9906316,etc |
| synchrotron self compton | SSC | 10 | 3 | 1.00071 | 9906202,9906242,etc |
| national center for supercomputing applications | NCSA | 4 | 3 | 1.000018 | 9906160,9906238,etc |