Design and development of the SOXS calibration unit
Autor: | Anna Brucalassi, Sergio Campana, P. Schipani, Maximilian Stritzinger, Seppo Mattila, José Antonio Araiza-Duran, Andrea Baruffolo, Jari Kotilainen, Stephen Smartt, Fabrizio Vitali, Rosario Di Benedetto, Hanindyo Kuncarayakti, Massimo Della Valle, Rachel Bruch, Marco Landoni, Hector Ventura, Ricardo Zanmar Sanchez, O. Hershko, J. Achrén, D. R. Young, Rosario Cosentino, Matteo Aliverti, Salvatore Scuderi, Riccardo Claudi, Giuliano Pignata, Kalyan Radhakrishnan, Michael Rappaport, Matteo Munari, Sergio D'Orsi, Francesco D'Alessio, Mirko Colapietro, Matteo Genoni, Marco Riva, Davide Ricci, Avishay Gal-Yam, Bernardo Salasnich, Enrico Cappellaro, Adam Rubin, Marco De Pascale, P. D'Avanzo, Giulio Capasso, Federico Biondi, Gianluca Li Causi, Iair Arcavi, Marcos Hernandez, Sagi Ben-Ami |
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Přispěvatelé: | Evans, Christopher J., Bryant, Julia J., Motohara, Kentaro |
Jazyk: | angličtina |
Rok vydání: | 2020 |
Předmět: |
Physics
Point source business.industry FOS: Physical sciences Linear stage 01 natural sciences law.invention 010309 optics Telescope Transients Integrating sphere Optics law 0103 physical sciences Calibration Pinhole (optics) Transient (oscillation) business Astrophysics - Instrumentation and Methods for Astrophysics 010303 astronomy & astrophysics Spectrograph Instrumentation and Methods for Astrophysics (astro-ph.IM) Spectroscopy |
Zdroj: | Kuncarayakti, H, Achrén, J, Campana, S, Claudi, R, Schipani, P, Aliverti, M, Baruffolo, A, Ben-Ami, S, Biondi, F, Capasso, G, Cosentino, R, D'Alessio, F, D'Avanzo, P, Hershko, O, Landoni, M, Munari, M, Pignata, G, Rubin, A, Scuderi, S, Vitali, F, Young, D, Araiza-Duran, J A, Arcavi, I, Brucalassi, A, Bruch, R, Cappellaro, E, Colapietro, M, della Valle, M, de Pascale, M, Di Benedetto, R, D'Orsi, S, Gal-Yam, A, Genoni, M, Hernandez, M, Kotilainen, J, Li Causi, G, Mattila, S, Radhakrishnan, K, Rappaport, M, Ricci, D, Riva, M, Salasnich, B, Smartt, S, Sanchez, R Z, Stritzinger, M & Ventura, H 2020, Design and development of the SOXS calibration unit . in C J Evans, J J Bryant & K Motohara (eds), Ground-Based and Airborne Instrumentation for Astronomy VIII ., 1144766, SPIE-International Society for Optical Engineering, Proceedings of SPIE-The International Society for Optical Engineering, vol. 11447, Ground-Based and Airborne Instrumentation for Astronomy VIII 2020, Virtual, Online, United States, 14/12/2020 . https://doi.org/10.1117/12.2560951 |
DOI: | 10.1117/12.2560951 |
Popis: | SOXS is a new spectrograph for the New Technology Telescope (NTT), optimized for transient and variable objects, covering a wide wavelength range from 350 to 2000 nm. SOXS is equipped with a calibration unit that will be used to remove the instrument signatures and to provide wavelength calibration to the data. The calibration unit will employ seven calibration lamps: a quartz-tungsten-halogen and a deuterium lamp for the flat-field correction, a ThAr lamp and four pencil-style rare-gas lamps for the wavelength calibration. The light from the calibration lamps is injected into the spectrograph mimicking the f/11 input beam of the NTT, by using an integrating sphere and a custom doublet. The oversized illumination patch covers the length of the spectrograph slit homogeneously, with $< 1\%$ variation. The optics also supports the second mode of the unit, the star-simulator mode that emulates a point source by utilizing a pinhole mask. Switching between the direct illumination and pinhole modes is performed by a linear stage. A safety interlock switches off the main power when the lamp box cover is removed, preventing accidental UV exposure to the service personnel. All power supplies and control modules are located in an electronic rack at a distance from the telescope platform. In this presentation we describe the optical, mechanical, and electrical designs of the SOXS calibration unit, and report the status of development in which the unit is currently in the test and verification stage. 7 pages, 7 figures |
Databáze: | OpenAIRE |
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