End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES

We present our numerical simulation approach for the End-to-End (E2E) model applied to various astronomical spectrographs, such as SOXS (ESO-NTT), CUBES (ESO-VLT), and ANDES (ESO-ELT), covering multiple wavelength regions. The E2E model aim at simulating the expected astronomical observations starting from the radiation of the scientific sources (or calibration sources) up to the raw-frame data produced by the detectors. The comprehensive description includes E2E architecture, computational models, and tools for rendering the simulated frames. Collaboration with Data Reduction Software (DRS) teams is discussed, along with efforts to meet instrument requirements. The contribution to the cross-correlation algorithm for the Active Flexure Compensation (AFC) system of CUBES is detailed.

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Published
2024-08-23
DOI
https://doi.org/10.1117/12.3019941
Citations
1
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
0.51

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End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES

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End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES

N. Sanna, Héctor Pérez Ventura, Marco De Pascale, Matteo Genoni, P. D’Avanzo, Matteo Aliverti, Giulio Capasso, Marco Landoni, Matteo Porru, Isabelle Boisse, Andrea Scaudo, Federico Battaini, Laurent Marty, R. Bruch, Allan de Meideros Martins, R. Sordo, F. Vitali, M. Della Valle, E. Mason, S. Mattila, P. Di Marcantonio, Sergio D’Orsi, Andrea Baruffolo, M. Stritzinger, Lorenzo Cabona, Marcos Hernandez, Marco Riva, A. Balestra, E. Cappellaro, Alessio Zanutta, Bernardo Salasnich, A. Marconi, Giorgio Calderone, Sérgio Sousa, S. Covino, R. Cosentino, H. Kuncarayakti, Mirko Colapietro, Salvatore Scuderi, T. Marquart, G. Cupani, M. Franchini, Anna Brucalassi, I. C. Leão, Gianluca Li Causi, R. Cirami, S. Campana, Johannes Puschnig, A. Rubin, Pietro Schipani, Federico Biondi, Kalyan Radhakrishnan, David Young, R. Smiljanić, D. Ricci, Ricardo Sánchez, D. Sosnowska, Sylvain Rousseau, Manuel Monteiro, Rosario Di Benedetto, Nikolai Piskunov, Giuliano Pignata, Ofir Hershko, Michael Rappaport, Iair Arcavi, José Antonio Araiza-Durán, Sagi Ben-Ami, Riccardo Claudi, Matteo Munari, Jari Kotilainen, Stephen Smartt, Francesco D'Alessio, Jani Achrén, Avishay Gal-Yam, Bruno C. Martins, Jonay G. Hernandez
article en
1 citations

Abstract

We present our numerical simulation approach for the End-to-End (E2E) model applied to various astronomical spectrographs, such as SOXS (ESO-NTT), CUBES (ESO-VLT), and ANDES (ESO-ELT), covering multiple wavelength regions. The E2E model aim at simulating the expected astronomical observations starting from the radiation of the scientific sources (or calibration sources) up to the raw-frame data produced by the detectors. The comprehensive description includes E2E architecture, computational models, and tools for rendering the simulated frames. Collaboration with Data Reduction Software (DRS) teams is discussed, along with efforts to meet instrument requirements. The contribution to the cross-correlation algorithm for the Active Flexure Compensation (AFC) system of CUBES is detailed.

Vol. 12184-24
University of Turku (FI), Astronomical Observatory of Rome (IT), Astronomical Observatory of Capodimonte (IT), Brera Astronomical Observatory (IT), Institute for Space Astrophysics and Planetology (IT), Osservatorio Astronomico di Cagliari (IT), Osservatorio Astronomico di Padova (IT), Telescopio Nazionale Galileo (ES), Weizmann Institute of Science (IL), National Institute for Astrophysics (IT)
Science and Technology Facilities Council
Openalex Percentile: Top 27%
Astronomy and Astrophysical Research
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