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.
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Permanent link for public information only:
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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.
I have read and understood the above.
Permanent link for public information only:
Permanent link for all public and protected information:
HAWC’s Eye es un prototipo de Telescopio Cherenkov Atmosférico (IACT) compacto y refractivo, diseñado para detectar las cascadas atmosféricas extensas (EAS) producidas por partículas con energías de 100 GeV hasta 100 TeV que entran en la atmósfera terrestre. Se realizaron simulaciones Monte Carlo para un arreglo de 55 telescopios HAWC’s Eye a 4100 m. s.n. m. para estimar el rendimiento
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Presented by Francisco GONZÁLEZ
on
28/3/2023
at
17:15
Las distintas técnicas de observación para la detección de rayos gamma presentan ventajas intrínsecas que, al ser combinadas, podrían mejorar significativamente las estimaciones de resolución angular, resolución de energía y separación gamma-hadrón. El telescopio HAWC's Eye es un prototipo de Telescopio Atmosférico Cherenkov (IACT) compacto, refractivo y ligero, diseñado con un arreglo
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Presented by Mr. José Erandi SERNA FRANCO
on
28/3/2023
at
17:00
En este trabajo presentamos el proceso de instalación del detector de agua cherenkov (WCD), al cual llamamos Jaguarito, este es parte de la colaboración internacional LAGO, por sus siglas en ingles Latin American Gigant Observatory, el ensamblado del tanque se realizó por estudiantes y profesores de la facultad de ciencias en Física y Matemáticas de la Universidad Autónoma de Chiapas, este p
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Presented by Ms. Emily FRANCO ESCUDERO
on
28/3/2023
at
17:30
Los rayos cósmicos se caracterizan por ser eventos de altas energías y con velocidades cercanas a la de la luz. Para estudiarlos se requiere de instrumentos que digitalicen la señal y que operen a la velocidad del tiempo de vida de los eventos de ∼ $10^{-9}$s. El presente trabajo pretende contribuir al estudio de los rayos cósmicos por medio del desarrollo de programas para digitalizar y alm
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Presented by Victor Manuel ACAMETITLA LÓPEZ
on
28/3/2023
at
18:00
En los experimentos de partículas y astro-partículas uno de los elementos principales para la detección de luz es un detector sensible en un amplio rango de longitudes de onda. En específico para detectores especializados para observar el efecto Cherenkov (250-500nm); es por ello importante que este tipo de sensores estén correctamente calibrados. El diseño e impresión 3D ha permitido dise�
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Presented by Mr. Enrique MARTÍNEZ VÁZQUEZ
on
28/3/2023
at
17:45
Llevamos a cabo la simulación de los componentes activos del Telescopio Centellador de Rayos Cósmicos (SciCRT). El SciCRT es un detector de rayos cósmicos de última generación y forma parte del Observatorio de Rayos Cósmicos de Sierra Negra (ORC-SN) que se encuentra en la cima del volcán de Sierra Negra en Puebla, México (19.0 N 97.3 O) a 4580 m s.n.m. (575 g/cm2). Debido a su posici
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Presented by Fernando MONTERDE ANDRADE
on
28/3/2023
at
18:15
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