A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Technical Design

Fuente: arXiv
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Main Authors: Ballester, Otger, Blanch, Oscar, Boix, Joan, Calisse, Paolo G., Campoy-Ordaz, Anna, Çolak, Sidika Merve, Da Deppo, Vania, Doro, Michele, Font, Lluís, Font-Pladevall, Eudald, Garcia, Rafael, Gaug, Markus, Grau, Roger, Kolar, Darko, López-Oramas, Alicia, Maggio, Camilla, Martinez, Manel, Martínez, Òscar, Riu-Molinero, Victor, Roman, David, Stanič, Samo, Tartera-Barberà, Júlia, Ubach, Santiago, Zavrtanik, Marko, Živec, Miha
Format: Preprint
Published: 2025
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author Ballester, Otger
Blanch, Oscar
Boix, Joan
Calisse, Paolo G.
Campoy-Ordaz, Anna
Çolak, Sidika Merve
Da Deppo, Vania
Doro, Michele
Font, Lluís
Font-Pladevall, Eudald
Garcia, Rafael
Gaug, Markus
Grau, Roger
Kolar, Darko
López-Oramas, Alicia
Maggio, Camilla
Martinez, Manel
Martínez, Òscar
Riu-Molinero, Victor
Roman, David
Stanič, Samo
Tartera-Barberà, Júlia
Ubach, Santiago
Zavrtanik, Marko
Živec, Miha
author_facet Ballester, Otger
Blanch, Oscar
Boix, Joan
Calisse, Paolo G.
Campoy-Ordaz, Anna
Çolak, Sidika Merve
Da Deppo, Vania
Doro, Michele
Font, Lluís
Font-Pladevall, Eudald
Garcia, Rafael
Gaug, Markus
Grau, Roger
Kolar, Darko
López-Oramas, Alicia
Maggio, Camilla
Martinez, Manel
Martínez, Òscar
Riu-Molinero, Victor
Roman, David
Stanič, Samo
Tartera-Barberà, Júlia
Ubach, Santiago
Zavrtanik, Marko
Živec, Miha
contents This paper presents the technical design of the pathfinder Barcelona Raman LIDAR (pBRL) for the northern site of the Cherenkov Telescope Array Observatory (CTAO-N) located at the Roque de los Muchachos Observatory (ORM). The pBRL is developed for continuous atmospheric characterization, essential for correcting high-energy gamma-ray observations captured by Imaging Atmospheric Cherenkov Telescopes (IACTs). The LIDAR consists of a steerable telescope with a 1.8 m parabolic mirror and a pulsed Nd:YAG laser with frequency doubling and tripling. It emits at wavelengths of 355 nm and 532 nm to measure aerosol scattering and extinction through two elastic and Raman channels. Built upon a former Cherenkov Light Ultraviolet Experiment (CLUE) telescope, the pBRL's design includes a Newtonian mirror configuration, a coaxial laser beam, a near-range system, a liquid light guide and a custom-made polychromator. During a one-year test at the ORM, the stability of the LIDAR and semi-remote-controlled operations were tested. This pathfinder leads the way to designing a final version of a CTAO Raman LIDAR which will provide real-time atmospheric monitoring and, as such, ensure the necessary accuracy of scientific data collected by the CTAO-N telescope array.
format Preprint
id arxiv_https___arxiv_org_abs_2503_13349
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Technical Design
Ballester, Otger
Blanch, Oscar
Boix, Joan
Calisse, Paolo G.
Campoy-Ordaz, Anna
Çolak, Sidika Merve
Da Deppo, Vania
Doro, Michele
Font, Lluís
Font-Pladevall, Eudald
Garcia, Rafael
Gaug, Markus
Grau, Roger
Kolar, Darko
López-Oramas, Alicia
Maggio, Camilla
Martinez, Manel
Martínez, Òscar
Riu-Molinero, Victor
Roman, David
Stanič, Samo
Tartera-Barberà, Júlia
Ubach, Santiago
Zavrtanik, Marko
Živec, Miha
Instrumentation and Methods for Astrophysics
This paper presents the technical design of the pathfinder Barcelona Raman LIDAR (pBRL) for the northern site of the Cherenkov Telescope Array Observatory (CTAO-N) located at the Roque de los Muchachos Observatory (ORM). The pBRL is developed for continuous atmospheric characterization, essential for correcting high-energy gamma-ray observations captured by Imaging Atmospheric Cherenkov Telescopes (IACTs). The LIDAR consists of a steerable telescope with a 1.8 m parabolic mirror and a pulsed Nd:YAG laser with frequency doubling and tripling. It emits at wavelengths of 355 nm and 532 nm to measure aerosol scattering and extinction through two elastic and Raman channels. Built upon a former Cherenkov Light Ultraviolet Experiment (CLUE) telescope, the pBRL's design includes a Newtonian mirror configuration, a coaxial laser beam, a near-range system, a liquid light guide and a custom-made polychromator. During a one-year test at the ORM, the stability of the LIDAR and semi-remote-controlled operations were tested. This pathfinder leads the way to designing a final version of a CTAO Raman LIDAR which will provide real-time atmospheric monitoring and, as such, ensure the necessary accuracy of scientific data collected by the CTAO-N telescope array.
title A 1.8 m class pathfinder Raman LIDAR for the Northern Site of the Cherenkov Telescope Array Observatory -- Technical Design
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2503.13349