A4 Vertaisarvioitu artikkeli konferenssijulkaisussa
End-to-End simulation framework for astronomical spectrographs: SOXS, CUBES and ANDES
Tekijät: Scaudo, 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.
Toimittaja: Egner, Sébastien Elias; Roberts, Scott
Konferenssin vakiintunut nimi: SPIE Astronomical Telescopes + Instrumentation
Kustantaja: SPIE-INT SOC OPTICAL ENGINEERING
Kustannuspaikka: BELLINGHAM
Julkaisuvuosi: 2024
Journal: Proceedings of SPIE : the International Society for Optical Engineering
Kokoomateoksen nimi: Modeling, Systems Engineering, and Project Management for Astronomy XI
Lehden akronyymi: PROC SPIE
Artikkelin numero: 1309905
Sarjan nimi: Proceedings of SPIE
Vuosikerta: 13099
Sivujen määrä: 19
ISBN: 978-1-5106-7521-6
eISBN: 978-1-5106-7522-3
ISSN: 0277-786X
eISSN: 1996-756X
DOI: https://doi.org/10.1117/12.3019941
Verkko-osoite: https://doi.org/10.1117/12.3019941
Preprintin osoite: http://arxiv.org/pdf/2407.17542
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.