Development status of the UV-VIS detector system of SOXS for the ESO-NTT telescope

Rosario Cosentino, Marcos Hernandez, Hector Ventura, Sergio Campana, Riccardo Claudi, Pietro Schipani, Matteo Aliverti, Andrea Baruffolo, Sagi Ben-Ami, Federico Biondi, Giulio Capasso, Francesco D'Alessio, Paolo D'Avanzo, Ofir Hershko, Hanindyo Kuncarayakti, Marco Landoni, Matteo Munari, Giuliano Pignata, Adam Rubin, Salvatore ScuderiFabrizio Vitali, David Young, Jani Achrén, José Antonio Araiza-Duran, Iair Arcavi, Anna Brucalassi, Rachel Bruch, Enrico Cappellaro, Mirko Colapietro, Massimo della Valle, Marco de Pascale, Rosario Di Benedetto, Sergio D'Orsi, Avishay Gal-Yam, Matteo Genoni, Jari Kotilainen, Gianluca Li Causi, Seppo Mattila, Michael Rappaport, Kalyan Radhakrishnan, Davide Ricci, Marco Riva, Bernardo Salasnich, Stephen Smartt, Ricardo Zanmar Sanchez, Maximilian Stritzinger, Matteo Accardo, Leander H. Mehrgan, Derek Ives, Josh Hopgood

Resultado de la investigación: Contribución a los tipos de informe/libroContribución a la conferenciarevisión exhaustiva

2 Citas (Scopus)

Resumen

SOXS will be the new spectroscopic facility for the ESO NTT telescope able to cover the optical and NIR bands by using two different arms: the UV-VIS (350-850 nm), and the NIR (800-2000 nm). In this article, we describe the development status of the visible camera cryostat, the architecture of the acquisition system and the progress in the electronic design. The UV-VIS detector system is based on a CCD detector 44-82 from e2v, a custom detector head, coupled with the ESO continuous flow cryostats (CFC), a custom cooling system, based on a Programmable Logic Controller (PLC), and the New General Controller (NGC) developed by ESO. This paper outlines the development status of the system, describes the design of the different parts that make up the UV-VIS arm and is accompanied by a series of information describing the SOXS design solutions in the mechanics and in the electronics parts. The first tests of the detector system with the UV-VIS camera will be shown.

Idioma originalInglés
Título de la publicación alojadaGround-Based and Airborne Instrumentation for Astronomy VIII
EditoresChristopher J. Evans, Julia J. Bryant, Kentaro Motohara
EditorialSPIE
ISBN (versión digital)9781510636811
DOI
EstadoPublicada - 2020
EventoGround-Based and Airborne Instrumentation for Astronomy VIII 2020 - Virtual, Online, Estados Unidos
Duración: 14 dic 202022 dic 2020

Serie de la publicación

NombreProceedings of SPIE - The International Society for Optical Engineering
Volumen11447
ISSN (versión impresa)0277-786X
ISSN (versión digital)1996-756X

Conferencia

ConferenciaGround-Based and Airborne Instrumentation for Astronomy VIII 2020
País/TerritorioEstados Unidos
CiudadVirtual, Online
Período14/12/2022/12/20

Áreas temáticas de ASJC Scopus

  • Materiales electrónicos, ópticos y magnéticos
  • Física de la materia condensada
  • Informática aplicada
  • Matemáticas aplicadas
  • Ingeniería eléctrica y electrónica

Huella

Profundice en los temas de investigación de 'Development status of the UV-VIS detector system of SOXS for the ESO-NTT telescope'. En conjunto forman una huella única.

Citar esto