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




TekijätScaudo, A.; Genoni, M.; Li Causi, G.; Cabona, L.; Landoni, M.; Campana, S.; Schipani, P.; Claudi, R.; Aliverti, M.; Baruffolo, A.; Ben-Ami, S.; Biondi, F.; Capasso, G.; Cosentino, R.; D'Alessio, F.; D'Avanzo, P.; Hershko, O.; Kuncarayakti, H.; Munari, M.; Santhakumari, K. Radhakrishnan; Pignata, G.; Rubin, A.; Scuderi, S.; Vitali, F.; Young, D.; Achren, J.; Araiza-Duran, J. A.; Arcavi, I; Battaini, F.; Brucalassi, A.; Bruch, R.; Cappellaro, E.; Colapietro, M.; Della Valle, M.; De Pascale, M.; Di Benedetto, R.; D'Orsi, S.; Gal-Yam, A.; Hernandez, M.; Kotilainen, J.; Marty, L.; Mattila, S.; Rappaport, M.; Ricci, D.; Riva, M.; Salasnich, B.; Smartt, S.; Sanchez, R. Zanmar; Stritzinger, M.; Ventura, H.; Cupani, G.; Porru, M.; Franchini, M.; Cirami, R.; Calderone, G.; Covino, S.; Smiljanic, R.; Monteiro, M.; Balestra, A.; Sordo, R.; Mason, E.; Rousseu, S.; Leao, I. de Castro; Zanutta, A.; Martins, A. de Meideros; Sosnowska, D.; Marquart, T.; Boisse, I; Sousa, S.; Hernandez, J.; Piskunov, N.; Puschnig, J.; Senna, N.; Martins, B.; Di Marcantonio, P.; Marconi, A.

ToimittajaEgner, Sébastien Elias; Roberts, Scott

Konferenssin vakiintunut nimiSPIE Astronomical Telescopes + Instrumentation

KustantajaSPIE-INT SOC OPTICAL ENGINEERING

KustannuspaikkaBELLINGHAM

Julkaisuvuosi2024

JournalProceedings of SPIE : the International Society for Optical Engineering

Kokoomateoksen nimiModeling, Systems Engineering, and Project Management for Astronomy XI

Lehden akronyymiPROC SPIE

Artikkelin numero 1309905

Sarjan nimiProceedings of SPIE

Vuosikerta13099

Sivujen määrä19

ISBN978-1-5106-7521-6

eISBN978-1-5106-7522-3

ISSN0277-786X

eISSN1996-756X

DOIhttps://doi.org/10.1117/12.3019941

Verkko-osoitehttps://doi.org/10.1117/12.3019941

Preprintin osoitehttp://arxiv.org/pdf/2407.17542


Tiivistelmä
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.



Last updated on 2025-21-03 at 10:41