Presentation + Paper
23 August 2024 End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES
A. Scaudo, M. Genoni, G. Li Causi, L. Cabona, M. Landoni, S. Campana, P. Schipani, R. Claudi, M. Aliverti, A. Baruffolo, S. Ben-Ami, F. Biondi, G. Capasso, R. Cosentino, F. D'Alessio, P. D'Avanzo, O. Hershko, H. Kuncarayakti, M. Munari, K. Radhakrishnan Santhakumari, G. Pignata, A. Rubin, S. Scuderi, F. Vitali, D. Young, J. Achrén, J. A. Araiza-Duran, I. Arcavi, F. Battaini, A. Brucalassi, R. Bruch, E. Cappellaro, M. Colapietro, M. Della Valle, M. De Pascale, R. Di Benedetto, S. D'Orsi, A. Gal-Yam, M. Hernandez, J. Kotilainen, L. Marty, S. Mattila, M. Rappaport, D. Ricci, M. Riva, B. Salasnich, S. Smartt, R. Zanmar Sanchez, M. Stritzinger, H. Ventura, G. Cupani, M. Porru, M. Franchini, R. Cirami, G. Calderone, S. Covino, R. Smiljanic, M. Monteiro, A. Balestra, R. Sordo, E. Mason, S. Rousseau, I. de Castro Leão, A. Zanutta, A. de Meideros Martins, D. Sosnowska, T. Marquart, I. Boisse, S. Sousa, J. Hernandez, N. Piskunov, J. Puschnig, N. Sanna, B. Martins, P. Di Marcantonio, A. Marconi
Author Affiliations +
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.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
A. Scaudo, M. Genoni, G. Li Causi, L. Cabona, M. Landoni, S. Campana, P. Schipani, R. Claudi, M. Aliverti, A. Baruffolo, S. Ben-Ami, F. Biondi, G. Capasso, R. Cosentino, F. D'Alessio, P. D'Avanzo, O. Hershko, H. Kuncarayakti, M. Munari, K. Radhakrishnan Santhakumari, G. Pignata, A. Rubin, S. Scuderi, F. Vitali, D. Young, J. Achrén, J. A. Araiza-Duran, I. Arcavi, F. Battaini, A. Brucalassi, R. Bruch, E. Cappellaro, M. Colapietro, M. Della Valle, M. De Pascale, R. Di Benedetto, S. D'Orsi, A. Gal-Yam, M. Hernandez, J. Kotilainen, L. Marty, S. Mattila, M. Rappaport, D. Ricci, M. Riva, B. Salasnich, S. Smartt, R. Zanmar Sanchez, M. Stritzinger, H. Ventura, G. Cupani, M. Porru, M. Franchini, R. Cirami, G. Calderone, S. Covino, R. Smiljanic, M. Monteiro, A. Balestra, R. Sordo, E. Mason, S. Rousseau, I. de Castro Leão, A. Zanutta, A. de Meideros Martins, D. Sosnowska, T. Marquart, I. Boisse, S. Sousa, J. Hernandez, N. Piskunov, J. Puschnig, N. Sanna, B. Martins, P. Di Marcantonio, and A. Marconi "End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES", Proc. SPIE 13099, Modeling, Systems Engineering, and Project Management for Astronomy XI, 1309905 (23 August 2024); https://doi.org/10.1117/12.3019941
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KEYWORDS
Calibration

Spectrographs

Device simulation

Astronomy

Lamps

Point spread functions

Design

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