U. Remmel

Publication List Details

Period

2000 - 2003

Number

63

Co-Authors

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...

Hybrid Performance of the Pierre Auger Observatory and Reconstruction of Hybrid Events (2003)

Kick, B., Altmann, E., Alvarez, P., Bauleo, P., Bonifazi, C., Etchegoyen, A., ...

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in...

The Lateral Distribution Function of Shower Signals in the Surface Detector of the Pierre Auger Observatory (2003)

Roth, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The surface detector (SD) array of the southern Pierre Auger Observatory will consist of a triangular grid of 1600 water Cherenkov tanks with 1.5 km spacing. For zenith angles less than 60deg the...

Processing of the Signals from the Surface Detectors of the Pierre - Auger Observatory (2003)

Suomijarvi, T., Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The signals from each tank are read out using three photomultipliers. The energy of the primary particle...

Calibration of the Pierre Auger fluorescence detector (2003)

Roberts, M., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The absolute calibration of an air fluorescence detector (FD) is an important element in correctly determining the energy of detected cosmic rays. The absolute calibration relates the flux of photons...

Performance of the Pierre Auger Fluorescence Detector and Analysis of well recontructed events (2003)

Argiro, S., Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of...

Shower Studies at around $10^{18}$ eV with the Surface Detector of the Pierre Auger Observatory (2003)

Ghia, P-L., Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., ...

Three months of data taken by the Engineering Array Surface Detector of the Pierre Auger Observatory have been analyzed with the aim of setting a procedure for the study of showers at E_0 ~ 10^18 eV....

Atmospheric Monitoring for the Pierre Auger Fluorescence Detector (2003)

Mostafa, M.A., Fick, B., Ave, M., Letessier, A., Bertou, X., Deligny, O., ...

Major uncertainties in the fluorescence energy measurement come from the precision of various atmospheric transmission, air Cerenkov subtraction, light multiple-scattering and cloud corrections. The...

The Anisotropy Search Program For the Pierre Auger Observatory (2003)

Clay, W., Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., ...

The Pierre Auger Southern Observatory in Argentina has begun taking data as it is being developed up to a final enclosed area of 3000 square kilometres. A key aspect of the project is to provide...

A Study Of Very Inclined Showers In The Pierre Auger Observatory (2003)

Ave, M., Letessier, A., Bertou, X., Deligny, O., Lachaud, C., Altmann, E., ...

The Engineering Array of the Auger Observatory has been running successfully since 2001 and inclined showers have been recorded from the start. We have analysed the events with zenith angle $>$...