Authors

The Pierre Auger Collaboration
A. Aab, Radboud Universiteit
P. Abreu, Instituto Superior Técnico
M. Aglietta, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
J. M. Albury, The University of Adelaide
I. Allekotte, Instituto Balseiro
A. Almela, Comision Nacional de Energia Atomica Argentina
J. Alvarez-Muniz, Universidad de Santiago de Compostela
R. Alves Batista, Radboud Universiteit
G. A. Anastasi, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
L. Anchordoqui, Lehman College
B. Andrada, Comision Nacional de Energia Atomica Argentina
S. Andringa, Instituto Superior Técnico
C. Aramo, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
P. R. Araújo Ferreira, Rheinisch-Westfälische Technische Hochschule Aachen
J. C. Arteaga Velázquez, Universidad Michoacana de San Nicolás de Hidalgo
H. Asorey, Comision Nacional de Energia Atomica Argentina
P. Assis, Instituto Superior Técnico
G. Avila, Comision Nacional de Energia Atomica Argentina
A. M. Badescu, University Politehnica of Bucharest
A. Bakalova, Institute of Physics of the Czech Academy of Sciences
A. Balaceanu, Horia Hulubei National Institute of Physics and Nuclear Engineering
F. Barbato, Gran Sasso Science Institute
R. J. Barreira Luz, Instituto Superior Técnico
K. H. Becker, Bergische Universität Wuppertal
J. A. Bellido, The University of Adelaide
C. Berat, Universite Grenoble Alpes
M. E. Bertaina, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
X. Bertou, Instituto Balseiro
P. L. Biermann, Max Planck Institute for Radio Astronomy
T. Bister, Rheinisch-Westfälische Technische Hochschule Aachen
J. Biteau, Universite Paris-Saclay
J. Blazek, Institute of Physics of the Czech Academy of Sciences

Document Type

Article

Publication Date

6-1-2021

Abstract

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system.

Publication Source (Journal or Book title)

Journal of Instrumentation

Share

COinS