Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Guada, C."'
Autor:
Camacho, R., Chacon, R., Diaz, G., Guada, C., Hamar, V., Hoeger, H., Melfo, A., Nunez, L. A., Perez, Y., Quintero, C., Rosales, M., Torrens, R., Collaboration, the LAGO
We present the LAGOVirtual Project: an ongoing project to develop platform to collaborate in the Large Aperture GRB Observatory (LAGO). This continental-wide observatory is devised to detect high energy (around 100 GeV) component of Gamma Ray Bursts,
Externí odkaz:
http://arxiv.org/abs/0912.2381
Autor:
Allard, D., Alvarez, C., Asorey, H., Barros, H., Bertou, X., Castillo, M., Chirinos, J. M., De Castro, A., Flores, S., Gonzalez, J., Berisso, M. Gomez, Grajales, J., Guada, C., Day, W. R. Guevara, Ishitsuka, J., Lopez, J. A., Martinez, O., Melfo, A., Meza, E., Loza, P. Miranda, Barbosa, E. Moreno, Murrugarra, C., Nunez, L. A., Ormachea, L. J. Otiniano, Perez, G., Perez, Y., Ponce, E., Quispe, J., Quintero, C., Rivera, H., Rosales, M., Rovero, A. C., Saavedra, O., Salazar, H., Tello, J. C., Peralda, R. Ticona, Varela, E., Velarde, A., Villasenor, L., Wahl, D., Zamalloa, M. A.
In order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of 1 GeV - 1 TeV background photons from a Gamma Ray Burst (GRB), simulations were conducted and compared to data acquired by the WCD of the Large Apert
Externí odkaz:
http://arxiv.org/abs/0906.0820
Autor:
Allard, D., Alvarez, C., Asorey, H., Barros, H., Bertou, X., Castillo, M., Chirinos, J. M., De Castro, A., Flores, S., Gonzalez, J., Berisso, M. Gomez, Grajales, J., Guada, C., Day, W. R. Guevara, Ishitsuka, J., Lopez, J. A., Martinez, O., Melfo, A., Meza, E., Loza, P. Miranda, Barbosa, E. Moreno, Murrugarra, C., Nunez, L. A., Ormachea, L. J. Otiniano, Perez, G., Perez, Y., Ponce, E., Quispe, J., Quintero, C., Rivera, H., Rosales, M., Rovero, A. C., Saavedra, O., Salazar, H., Tello, J. C., Peralda, R. Ticona, Varela, E., Velarde, A., Villasenor, L., Wahl, D., Zamalloa, M. A.
The Large Aperture GRB Observatory (LAGO) is aiming at the detection of the high energy (around 100 GeV) component of Gamma Ray Bursts, using the single particle technique in arrays of Water Cherenkov Detectors (WCD) in high mountain sites (Chacaltay
Externí odkaz:
http://arxiv.org/abs/0906.0816
Autor:
Allard, D., Alvarez, C., Asorey, H., Barros, H., Bertou, X., Castillo, M., Chirinos, J. M., De Castro, A., Flores, S., Gonzalez, J., Berisso, M. Gomez, Grajales, J., Guada, C., Day, W. R. Guevara, Ishitsuka, J., Lopez, J. A., Martinez, O., Melfo, A., Meza, E., Loza, P. Miranda, Barbosa, E. Moreno, Murrugarra, C., Nunez, L. A., Ormachea, L. J. Otiniano, Perez, G., Perez, Y., Ponce, E., Quispe, J., Quintero, C., Rivera, H., Rosales, M., Rovero, A. C., Saavedra, O., Salazar, H., Tello, J. C., Peralda, R. Ticona, Varela, E., Velarde, A., Villasenor, L., Wahl, D., Zamalloa, M. A.
Water Cherenkov Detectors (WCD) are efficient detectors for detecting GRBs in the 10 GeV - 1 TeV energy range using the single particle technique, given their sensitivity to low energy secondary photons produced by high energy photons when cascading
Externí odkaz:
http://arxiv.org/abs/0906.0814
Akademický článek
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Autor:
GUADA, C.
Publikováno v:
Uncertainty Modelling in Knowledge Engineering & Decision Making - Proceedings of the 12th International Flins Conference (Flins 2016); 2016, p1149-1154, 6p
Akademický článek
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Akademický článek
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K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Camacho, R., Chacon, R., Diaz, G., Guada, C., Hamar, V., Hoeger, H., Melfo, A., Luis Nunez, Perez, Y., Quintero, C., Rosales, M., Torrens, R., Lago, The Collaboration
Publikováno v:
NASA Astrophysics Data System
We present the LAGOVirtual Project: an ongoing project to develop platform to collaborate in the Large Aperture GRB Observatory (LAGO). This continental-wide observatory is devised to detect high energy (around 100 GeV) component of Gamma Ray Bursts,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9380fe4aef86d5bb7dd3580a84d05622
https://ui.adsabs.harvard.edu/#abs/2009arXiv0912.2381C
https://ui.adsabs.harvard.edu/#abs/2009arXiv0912.2381C
Autor:
Allard, D., Alvarez, C., Asorey, H., Barros, H., Bertou, Xavier, Castillo, M., Chirinos, J. M., Castro, A., Flores, S., Gonzalez, J., Berisso, M. Gomez, Grajales, J., Guada, C., Day, W. R. Guevara, Ishitsuka, J., Lopez, J. A., Martinez, O., Melfo, A., Meza, E., Loza, P. Miranda, Barbosa, E. Moreno, Cecilia Murrugarra, Nunez, L. A., Ormachea, L. J. Otiniano, Perez, G., Perez, Y., Ponce, E., Quispe, J., Quintero, C., Rivera, H., Rosales, M., Rovero, Adrian C., Saavedra, O., Salazar, H., Tello, J. C., Peralda, R. Ticona, Varela, E., Velarde, A., Villasenor, L., Wahl, D., Zamalloa, M. A.
Publikováno v:
NASA Astrophysics Data System
INSPIRE-HEP
INSPIRE-HEP
In order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of 1 GeV - 1 TeV background photons from a Gamma Ray Burst (GRB), simulations were conducted and compared to data acquired by the WCD of the Large Apert
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd941fd6d0e2bec39f7775847db131b1
https://ui.adsabs.harvard.edu/#abs/2009arXiv0906.0820A
https://ui.adsabs.harvard.edu/#abs/2009arXiv0906.0820A