Extensive multi-frequency monitoring of the classical TeV blazars Mrk 421 and Mr
收藏ESA Earth Online2026-06-22 收录
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Owing to their brightness and proximity, Mrk421 and Mrk501 are among the blazarsthat can be studied with the greatest level of detail, and thus excellentastrophysical laboratories to study the underlying physics of blazars. Werequest MAGIC observations to provide sensitive VHE coverage for themultiinstrument campaigns in 2023/2024. These MAGIC observations are needed tocharacterise with accuracy the highenergy bump and its temporal evolution withsimultaneous coverage for the lowenergy bump.
