selected results from the argo-ybj experiment

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Selected results from the ARGO-YBJ experiment P. Camarri [email protected] INFN Roma Tor Vergata On behalf of the ARGO-YBJ Collaboration 36 th ICHEP – Melbourne, Australia – July 4-11, 2012

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Selected results from the ARGO-YBJ experiment. P. Camarri [email protected] INFN Roma Tor Vergata. On behalf of the ARGO-YBJ Collaboration. 36 th ICHEP – Melbourne, Australia – July 4-11, 2012. Detector layout. Mrk421 long-term monitoring. - PowerPoint PPT Presentation

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Page 1: Selected results  from the ARGO-YBJ experiment

Selected results from the ARGO-YBJ experiment

P. [email protected]

INFN Roma Tor Vergata

On behalf of the ARGO-YBJ Collaboration

36th ICHEP – Melbourne, Australia – July 4-11, 2012

Page 2: Selected results  from the ARGO-YBJ experiment

36th ICHEP - Melbourne, Australia - July 4-11, 2012

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36th ICHEP - Melbourne, Australia - July 4-11, 2012

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Detector layout

36th ICHEP - Melbourne, Australia - July 4-11, 2012

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36th ICHEP - Melbourne, Australia - July 4-11, 2012

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36th ICHEP - Melbourne, Australia - July 4-11, 2012

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36th ICHEP - Melbourne, Australia - July 4-11, 2012

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36th ICHEP - Melbourne, Australia - July 4-11, 2012

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ARGO-YBJ coll., ApJ 734 (2011) 110

RXTE/ASM 2-12 keVSwift/BAT 15-50 keV ARGO-YBJ TeV

ARGO-YBJ cumulative light curve (>TeV) compared with Swift and Rossi/RXTE data.

Good correlation between TeV/X-ray data. No other continuous observation at TeV energies

Mrk421 long-term monitoring

36th ICHEP - Melbourne, Australia - July 4-11, 2012

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Mrk501

36th ICHEP - Melbourne, Australia - July 4-11, 2012

A strong X-ray flare in 1997 followed by a long “quiet” period

New strong X-ray flare 14 years later: Oct 2011

Flare associated to a strong TeV emission detected by ARGO-YBJ

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SPARE SLIDES

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36th ICHEP - Melbourne, Australia - July 4-11, 2012