Multi-wavelength calibration procedure for the pierre Auger Observatory Fluorescence Detectors

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 measur...

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Autor principal: Rovero, A.C
Otros Autores: Bauleo, P., Brack, J.T, Harton, J.L, Knapik, R.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2009
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100 1 |a Rovero, A.C. 
245 1 0 |a Multi-wavelength calibration procedure for the pierre Auger Observatory Fluorescence Detectors 
260 |c 2009 
270 1 0 |m Rovero, A.C.; Instituto de Astronomía y Física del Espacio (CONICET), CC 67 Suc 28, C1428ZAA Buenos Aires, Argentina; email: rovero@iafe.uba.ar 
506 |2 openaire  |e Política editorial 
504 |a Abraham, J., (2004) NIM A, 523, pp. 50-95. , Pierre Auger Collaboration 
504 |a Roth, M., Pierre Auger Collaboration (2007) Proceeding 30th ICRC, , Merida 
504 |a Abraham, J., (2008) Phys. Rev. Lett., 101, p. 061101. , Pierre Auger Collaboration 
504 |a Verzi, V., (2007) Nucl. Phys. B (Proc. Suppl.), 165, p. 37. , Pierre Auger Collaboration 
504 |a Knapik, R., Pierre Auger Collaboration (2007) Proceeding 30th ICRC, , Merida 
504 |a Aramo, C., Pierre Auger Collaboration (2005) Proceeding 29th ICRC, 8, p. 101. , Pune 
504 |a Brack, J.T., (2004) Astropart. Phys., 20, p. 653 
504 |a Bauleo, P., Pierre Auger Collaboration (2005) Proceeding 29th ICRC, 8, pp. 5-8. , Pune 
504 |a Matthews, J.A.J., Pierre Auger Collaboration (2003) Proceeding SPIE Astronomical Telescopes and Instrumentation, 4858, pp. 121-130. , Waikoloa, Hawaii 
504 |a Matthiae, G., Pierre Auger Collaboration (2001) Proceeding 27th ICRC, , Hamburg 
504 |a Nagano, M., (2003) Astropart. Phys., 20, p. 293 
504 |a Larson, T.C., Bruce, S.S., Parr, A.C., Spectroradiometric Detector Measurements, National Institute of Standards and Technology, Calibration Program, Gaithersburg, MD 20899-2330 (1998) Special Publication, 250 -41 
504 |a Corporation, chip, pp. ivc102. , http://www.burr-brown.com 
520 3 |a 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%. © 2009 Elsevier B.V. All rights reserved.  |l eng 
593 |a Instituto de Astronomía y Física del Espacio (CONICET), CC 67 Suc 28, C1428ZAA Buenos Aires, Argentina 
593 |a Colorado State University, Department of Physics, Fort Collins, CO 80523, United States 
690 1 0 |a AUGER OBSERVATORY 
690 1 0 |a CALIBRATION 
690 1 0 |a COSMIC RAY 
690 1 0 |a EXTENSIVE AIR SHOWER 
690 1 0 |a FLUORESCENCE DETECTORS 
690 1 0 |a AT WAVELENGTHS 
690 1 0 |a AUGER OBSERVATORY 
690 1 0 |a COSMIC RAY 
690 1 0 |a DETECTOR COMPONENTS 
690 1 0 |a EXTENSIVE AIR SHOWER 
690 1 0 |a FLUORESCENCE DETECTORS 
690 1 0 |a MULTI WAVELENGTHS 
690 1 0 |a PIERRE AUGER OBSERVATORIES 
690 1 0 |a RELATIVE SPECTRAL RESPONSE 
690 1 0 |a AUGERS 
690 1 0 |a BUILDINGS 
690 1 0 |a CALIBRATION 
690 1 0 |a COSMIC RAYS 
690 1 0 |a COSMOLOGY 
690 1 0 |a DETECTORS 
690 1 0 |a LIGHT 
690 1 0 |a LIGHT SOURCES 
690 1 0 |a NOTCH FILTERS 
690 1 0 |a OBSERVATORIES 
690 1 0 |a PARTICLE DETECTORS 
690 1 0 |a FLUORESCENCE 
650 1 7 |2 spines  |a XENON 
700 1 |a Bauleo, P. 
700 1 |a Brack, J.T. 
700 1 |a Harton, J.L. 
700 1 |a Knapik, R. 
773 0 |d 2009  |g v. 31  |h pp. 305-311  |k n. 4  |p Astropart. Phys.  |x 09276505  |w (AR-BaUEN)CENRE-3851  |t Astroparticle Physics 
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856 4 0 |u https://doi.org/10.1016/j.astropartphys.2009.02.009  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_09276505_v31_n4_p305_Rovero  |y Handle 
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