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Characterisation and assessment of the SOXS Spectrograph UV-VIS Detector System

Fuente: arXiv

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Bibliographische Detailangaben
Hauptverfasser:	Cosentino, R., Hernandez, M., Ventura, H., Campana, S., Claudi, R., Schipani, P., Aliverti, M., Asquini, L., Baruffolo, A., Battaini, F., Ben-Ami, Sagi, Bichkovsky, A., Capasso, G., D'Alessio, F., D'Avanzo, P., Hershko, O., Kuncarayakti, H., Landoni, M., Munari, M., Pignata, G., Rubin, A., Scuderi, S., Vitali, F., Young, D., Achren, J., Araiza-Duran, J. A., Arcavi, I., Brucalassi, A., Bruch, R., Cappellaro, E., Colapietro, M., Della Valle, M., Di Benedetto, R., Di Filippo, S., D'Orsi, S., Gal-Yam, A., Genoni, M., Kotilainen, J., Causi, G. Li, Marty, L., Mattila, S., Rappaport, M., Radhakrishnan, K., Ricci, D., Riva, M., Salasnich, B., Savarese, S., Smartt, S., Sanchez, R. Zanmar, Stritzinger, M., Accardo, M., Mehrgan, L. H., Ives, D.
Format:	Preprint
Veröffentlicht:	2024
Schlagworte:	Instrumentation and Methods for Astrophysics
Online-Zugang:	Acceder al recurso
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_version_	1866929435341488128
author	Cosentino, R. Hernandez, M. Ventura, H. Campana, S. Claudi, R. Schipani, P. Aliverti, M. Asquini, L. Baruffolo, A. Battaini, F. Ben-Ami, Sagi Bichkovsky, A. Capasso, G. D'Alessio, F. D'Avanzo, P. Hershko, O. Kuncarayakti, H. Landoni, M. Munari, M. Pignata, G. Rubin, A. Scuderi, S. Vitali, F. Young, D. Achren, J. Araiza-Duran, J. A. Arcavi, I. Brucalassi, A. Bruch, R. Cappellaro, E. Colapietro, M. Della Valle, M. Di Benedetto, R. Di Filippo, S. D'Orsi, S. Gal-Yam, A. Genoni, M. Kotilainen, J. Causi, G. Li Marty, L. Mattila, S. Rappaport, M. Radhakrishnan, K. Ricci, D. Riva, M. Salasnich, B. Savarese, S. Smartt, S. Sanchez, R. Zanmar Stritzinger, M. Accardo, M. Mehrgan, L. H. Ives, D.
author_facet	Cosentino, R. Hernandez, M. Ventura, H. Campana, S. Claudi, R. Schipani, P. Aliverti, M. Asquini, L. Baruffolo, A. Battaini, F. Ben-Ami, Sagi Bichkovsky, A. Capasso, G. D'Alessio, F. D'Avanzo, P. Hershko, O. Kuncarayakti, H. Landoni, M. Munari, M. Pignata, G. Rubin, A. Scuderi, S. Vitali, F. Young, D. Achren, J. Araiza-Duran, J. A. Arcavi, I. Brucalassi, A. Bruch, R. Cappellaro, E. Colapietro, M. Della Valle, M. Di Benedetto, R. Di Filippo, S. D'Orsi, S. Gal-Yam, A. Genoni, M. Kotilainen, J. Causi, G. Li Marty, L. Mattila, S. Rappaport, M. Radhakrishnan, K. Ricci, D. Riva, M. Salasnich, B. Savarese, S. Smartt, S. Sanchez, R. Zanmar Stritzinger, M. Accardo, M. Mehrgan, L. H. Ives, D.
contents	The SOXS spectrograph, designed for the ESO NTT telescope, operates in both the optical (UV-VIS: 350-850 nm) and NIR (800-2000 nm) bands. This article provides an overview of the final tests conducted on the UV-VIS camera system using a telescope simulator. It details the system's performance evaluation, including key metrics such as gain, readout noise, and linearity, and highlights the advancements made in the upgraded acquisition system. The testing process, conducted in the Padua laboratory, involved comprehensive simulations of the telescope environment to ensure the results closely resemble those expected at the ESO-NTT telescope. The successful completion of these tests confirms the system's readiness for deployment to Chile, where it will be installed on the NTT telescope, marking a significant milestone in the SOXS project.
format	Preprint
id	arxiv_https___arxiv_org_abs_2407_17245
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Characterisation and assessment of the SOXS Spectrograph UV-VIS Detector System Cosentino, R. Hernandez, M. Ventura, H. Campana, S. Claudi, R. Schipani, P. Aliverti, M. Asquini, L. Baruffolo, A. Battaini, F. Ben-Ami, Sagi Bichkovsky, A. Capasso, G. D'Alessio, F. D'Avanzo, P. Hershko, O. Kuncarayakti, H. Landoni, M. Munari, M. Pignata, G. Rubin, A. Scuderi, S. Vitali, F. Young, D. Achren, J. Araiza-Duran, J. A. Arcavi, I. Brucalassi, A. Bruch, R. Cappellaro, E. Colapietro, M. Della Valle, M. Di Benedetto, R. Di Filippo, S. D'Orsi, S. Gal-Yam, A. Genoni, M. Kotilainen, J. Causi, G. Li Marty, L. Mattila, S. Rappaport, M. Radhakrishnan, K. Ricci, D. Riva, M. Salasnich, B. Savarese, S. Smartt, S. Sanchez, R. Zanmar Stritzinger, M. Accardo, M. Mehrgan, L. H. Ives, D. Instrumentation and Methods for Astrophysics The SOXS spectrograph, designed for the ESO NTT telescope, operates in both the optical (UV-VIS: 350-850 nm) and NIR (800-2000 nm) bands. This article provides an overview of the final tests conducted on the UV-VIS camera system using a telescope simulator. It details the system's performance evaluation, including key metrics such as gain, readout noise, and linearity, and highlights the advancements made in the upgraded acquisition system. The testing process, conducted in the Padua laboratory, involved comprehensive simulations of the telescope environment to ensure the results closely resemble those expected at the ESO-NTT telescope. The successful completion of these tests confirms the system's readiness for deployment to Chile, where it will be installed on the NTT telescope, marking a significant milestone in the SOXS project.
title	Characterisation and assessment of the SOXS Spectrograph UV-VIS Detector System
topic	Instrumentation and Methods for Astrophysics
url	https://arxiv.org/abs/2407.17245