Observation of M87 with the Whipple 10m telescope

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dc.creatorLeBohec, S.
dc.date2003-05-29
dc.date.accessioned2026-07-07T02:08:38Z
dc.date.available2026-07-07T02:08:38Z
dc.descriptionThe Whipple 10-m telescope was used to observe M87 since 2000. No significant gamma-ray signal was found and upper limits compared to the HEGRA detection suggest the source may be variable. We found weak evidence for a correlation with the X-ray activity in 2000-2001 but this tendency did not persist in 2002-2003.
dc.description4 pages to be published in the Proceedings of the 28th International Cosmic Ray Conference (Tsukuba, Japan 2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0305582
dc.identifierhttp://arxiv.org/abs/astro-ph/0305582
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6131
dc.subjectAstrophysics
dc.titleObservation of M87 with the Whipple 10m telescope
dc.typetext

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