Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors

Autores
Rovero, Adrian Carlos; Bauleo, P.; Brack, J.; Harton, J.; Knapik, R.
Año de publicación
2009
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a method to measure the relative spectral response of the Pierre Auger Observatory Fluorescence Detector. The calibration was done at wavelengths of 320, 337, 355, 380 and 405 nm using an end-to-end technique in which the response of all detector components are combined in a single measurement. A xenon flasher and notch-filters were used as the light source for the calibration device. The overall uncertainty is 5%.
Fil: Rovero, Adrian Carlos. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Bauleo, P.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Brack, J.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Harton, J.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Knapik, R.. State University of Colorado - Fort Collins; Estados Unidos
Materia
Pierre Auger Observatory
Absolute Calibration
Fluorescence Telescopes
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/21215

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network_name_str CONICET Digital (CONICET)
spelling Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectorsRovero, Adrian CarlosBauleo, P.Brack, J.Harton, J.Knapik, R.Pierre Auger ObservatoryAbsolute CalibrationFluorescence Telescopeshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a method to measure the relative spectral response of the Pierre Auger Observatory Fluorescence Detector. The calibration was done at wavelengths of 320, 337, 355, 380 and 405 nm using an end-to-end technique in which the response of all detector components are combined in a single measurement. A xenon flasher and notch-filters were used as the light source for the calibration device. The overall uncertainty is 5%.Fil: Rovero, Adrian Carlos. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Bauleo, P.. State University of Colorado - Fort Collins; Estados UnidosFil: Brack, J.. State University of Colorado - Fort Collins; Estados UnidosFil: Harton, J.. State University of Colorado - Fort Collins; Estados UnidosFil: Knapik, R.. State University of Colorado - Fort Collins; Estados UnidosElsevier Science2009-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21215Rovero, Adrian Carlos; Bauleo, P.; Brack, J.; Harton, J.; Knapik, R.; Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors; Elsevier Science; Astroparticle Physics; 31; 4; 12-2009; 305-3110927-6505CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2009.02.009info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0927650509000371info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:51:59Zoai:ri.conicet.gov.ar:11336/21215instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:52:00.208CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
title Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
spellingShingle Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
Rovero, Adrian Carlos
Pierre Auger Observatory
Absolute Calibration
Fluorescence Telescopes
title_short Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
title_full Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
title_fullStr Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
title_full_unstemmed Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
title_sort Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors
dc.creator.none.fl_str_mv Rovero, Adrian Carlos
Bauleo, P.
Brack, J.
Harton, J.
Knapik, R.
author Rovero, Adrian Carlos
author_facet Rovero, Adrian Carlos
Bauleo, P.
Brack, J.
Harton, J.
Knapik, R.
author_role author
author2 Bauleo, P.
Brack, J.
Harton, J.
Knapik, R.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Pierre Auger Observatory
Absolute Calibration
Fluorescence Telescopes
topic Pierre Auger Observatory
Absolute Calibration
Fluorescence Telescopes
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present a method to measure the relative spectral response of the Pierre Auger Observatory Fluorescence Detector. The calibration was done at wavelengths of 320, 337, 355, 380 and 405 nm using an end-to-end technique in which the response of all detector components are combined in a single measurement. A xenon flasher and notch-filters were used as the light source for the calibration device. The overall uncertainty is 5%.
Fil: Rovero, Adrian Carlos. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Bauleo, P.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Brack, J.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Harton, J.. State University of Colorado - Fort Collins; Estados Unidos
Fil: Knapik, R.. State University of Colorado - Fort Collins; Estados Unidos
description We present a method to measure the relative spectral response of the Pierre Auger Observatory Fluorescence Detector. The calibration was done at wavelengths of 320, 337, 355, 380 and 405 nm using an end-to-end technique in which the response of all detector components are combined in a single measurement. A xenon flasher and notch-filters were used as the light source for the calibration device. The overall uncertainty is 5%.
publishDate 2009
dc.date.none.fl_str_mv 2009-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/21215
Rovero, Adrian Carlos; Bauleo, P.; Brack, J.; Harton, J.; Knapik, R.; Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors; Elsevier Science; Astroparticle Physics; 31; 4; 12-2009; 305-311
0927-6505
CONICET Digital
CONICET
url http://hdl.handle.net/11336/21215
identifier_str_mv Rovero, Adrian Carlos; Bauleo, P.; Brack, J.; Harton, J.; Knapik, R.; Multi-wavelength calibration procedure for the Pierre Auger Observatory fluorescence detectors; Elsevier Science; Astroparticle Physics; 31; 4; 12-2009; 305-311
0927-6505
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2009.02.009
info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0927650509000371
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier Science
publisher.none.fl_str_mv Elsevier Science
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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