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Table 1
Participating instruments in the campaign on Mrk 421 during 2010 March.
| Instrument/Observatory | Energy range covered |
|
|
|
| MAGIC | 0.08–5.0 TeV |
| VERITAS | 0.2–5.0 TeV |
| Whipple 10-m | 0.4–2.0 TeV |
| Fermi-LAT | 0.1–400 GeV |
| Swift/BAT | 14–195 keV |
| RXTE-PCA | 3–32 keV |
| Swift-XRT | 0.3–10 keV |
| RXTE-ASM | 2–10 keV |
| MAXI | 2–10 keV |
| Swift-UVOT | UVW1, UVM2, UVW2 |
| Abastumani† | R band |
| Lulin† | R band |
| Roque de los Muchachos (KVA)† | R band |
| St. Petersburg† | R band polarization |
| Sabadell† | R band |
| Goddard Robotic Telescope (GRT) | R band |
| The Remote Observatory for Variable Object Research (ROVOR) | B, R, V bands |
| New Mexico Skies (NMS) | R, V bands |
| Bradford Robotic Telescope (BRT) | B, R, V bands |
| Perkins | R band polarization |
| Steward | R band polarization |
| Crimean | R band polarization |
| Submillimeter Array (SMA) | 225 GHz |
| Metsähovi Radio Observatory† | 37 GHz |
| University of Michigan Radio Astronomy Observatory (UMRAO)† | 8.0, 14.5 GHz |
| Owens Valley Radio Observatory (OVRO) | 15 GHz |
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