Calibration of the Whipple atmospheric Čerenkov telescope
Čerenkov ring images from single muons have been used to calibrate the Whipple Observatory 10 m imaging telescope. This approach tests the total throughput of the telescope and uses a known atmospheric Cerenkov light signal that closely matches the spectrum of the atmospheric Čerenkov signal from an...
Guardado en:
| Publicado: |
1996
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09276505_v5_n1_p27_Rovero http://hdl.handle.net/20.500.12110/paper_09276505_v5_n1_p27_Rovero |
| Aporte de: |
| Sumario: | Čerenkov ring images from single muons have been used to calibrate the Whipple Observatory 10 m imaging telescope. This approach tests the total throughput of the telescope and uses a known atmospheric Cerenkov light signal that closely matches the spectrum of the atmospheric Čerenkov signal from an air-shower. The absolute calibration is derived by matching the observed ring images with those predicted by a simple geometrical and physical model; a value of 1.25 ± 0.13 photoelectrons equivalent to 1 digital count was found. Using this value simulations indicate that the telescope had an energy threshold of 300 GeV when this calibration was made. |
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