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In order to enable an iCal export link, your account needs to have a key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
I have read and understood the above.
In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.
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D1-Talks
Date:
27 Mar 09:15 - 10:00
Conveners
Cosmic Rays
Dr. Martínez-Huerta, Humberto (Departamento de Física y Matemáticas, UDEM)
The number of muons in extensive air showers (EAS) is a useful quantity to investigate the composition of high-energy cosmic rays by indirect detection techniques. It is also a sensitive probe for tests of high-energy hadronic interaction models at laboratory energies that are several orders of magnitude larger than those achieved at current particle physics facilities. For these reasons, it is i
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Presented by Dr. Juan Carlos ARTEAGA VELAZQUEZ
on
27/3/2023
at
15:45
Simulations with CORSIKA and EXPACS Software were performed to complete calculations based on Dorman’s general theory of atmospheric electric field effects on secondary cosmic rays. The calculations were done for the particles detected at the Sierra Negra Cosmic Ray Observatory, located at a height of 4580 m a.s.l. Variations of 1.15-3.47% on the intensity of the charged component were estimated
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Presented by Mrs. Jania NEWTON
on
27/3/2023
at
15:30
In the quest for particle dark matter and physics beyond the Standard Model, the possibility of the existence of neutral long-lived particles (LLPs) has been proposed. The MATHUSLA project is designed as a surface experiment to detect possible LLPs produced in collisions at the CERN High-Luminosity Large Hadron Collider (HL-LHC). The MATHUSLA detector will cover a 10^4 m^2 surface and will have 9
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Presented by Prof. Paolo CAMARRI
on
27/3/2023
at
15:15
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