SOXS End-to-End simulator: development and applications for pipeline design

被引：11

作者：

Genoni, M. ^{[1
]}

Landoni, M. ^{[1
,19
]}

Li Causi, G. ^{[2
]}

Pariani, G. ^{[1
]}

Aliverti, M. ^{[1
]}

Campana, S. ^{[1
]}

Schipani, P. ^{[3
]}

Claudi, R. ^{[4
]}

Munari, M. ^{[10
]}

Rubin, A. ^{[13
]}

D'Avanzo, P. ^{[1
]}

Riva, M. ^{[1
]}

Baruffolo, A. ^{[4
]}

Biondi, F. ^{[18
]}

Capasso, G. ^{[3
]}

Cosentino, R. ^{[6
]}

D'Alessio, F. ^{[7
]}

Hershko, O. ^{[5
]}

Kuncarayakti, H. ^{[8
,9
]}

Pignata, G. ^{[11
,12
]}

Scuderi, S. ^{[10
]}

Radhakrishnan, K. ^{[4
]}

Ben-Ami, S. ^{[5
]}

Vitali, F. ^{[7
]}

Young, D. ^{[13
]}

Brucalassi, A.

Achren, J. ^{[14
]}

Araiza-Duran, J. A. ^{[12
,15
]}

Arcavi, I ^{[16
]}

Bruch, R. ^{[5
]}

Cappellaro, E. ^{[4
]}

Colapietro, M. ^{[3
]}

Della Valle, M. ^{[3
]}

De Pascale, M. ^{[4
]}

Di Benedetto, R. ^{[10
]}

D'Orsi, S. ^{[3
]}

Gal-Yam, A. ^{[5
]}

Hernandez Diaz, M. ^{[6
]}

Kotilainen, J. ^{[8
,9
]}

Mattila, S. ^{[9
]}

Rappaport, M. ^{[5
]}

Ricci, D. ^{[4
]}

Salasnich, B. ^{[4
]}

Smartt, S. ^{[13
]}

Sanchez, R. Zanmar ^{[10
]}

Stritzinger, M. ^{[17
]}

Ventura, H. ^{[6
]}

机构：

[1] INAF Osservatorio Astron Brera Merate, Via E Bianchi 46, I-23807 Merate, LC, Italy

[2] INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, Rome, Italy

[3] INAF Osservatorio Astron Capodimonte, Sal Moiariello 16, I-80131 Naples, Italy

[4] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy

[5] Weizmann Inst Sci, Herzl St 234, IL-7610001 Rehovot, Israel

[6] TNG, FGG INAF, Rambla JA Fernandez Perez 7, E-38712 Brena Baja, TF, Spain

[7] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 M Porzio Catone, Italy

[8] Univ Turku, Finnish Ctr Astron ESO FINCA, FI-20014 Turku, Finland

[9] Univ Turku, Dept Phys & Astron, Tuorla Observ, FI-20014 Turku, Finland

[10] INAF Osservatorio Astrofis Catania, Via S Sofia 78 30, I-95123 Catania, Italy

[11] Univ Andres Bello, Avda Republ 252, Santiago, Chile

[12] Millennium Inst Astrophys MAS, Santiago, Chile

[13] Queens Univ Belfast, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland

[14] Incident Angle Oy, Capsiankatu 4 A 29, FI-20320 Turku, Finland

[15] Ctr Invest Opt AC, Leon 37150, Mexico

[16] Tel Aviv Univ, Dept Astrophys, IL-69978 Tel Aviv, Israel

[17] Aarhus Univ, Ny Munkegade 120, DK-8000 Aarhus, Denmark

[18] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

[19] INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy

来源：

MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY IX | 2020年 / 11450卷

关键词：

ESO-NTT telescope; SOXS; End-to-End simulations; Echelle cross-dispersed spectrograph;

D O I：

10.1117/12.2560640

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the development of the End-to-End simulator for the SOXS instrument at the ESO-NTT 3.5-m telescope. SOXS will be a spectroscopic facility, made by two arms high efficiency spectrographs, able to cover the spectral range 350-2000 nm with resolving power R approximate to 4500. The E2E model allows to simulate the propagation of photons starting from the scientific target of interest up to the detectors. The outputs of the simulator are synthetic frames, which will be mainly exploited for optimizing the pipeline development and possibly assisting for proper alignment and integration phases in laboratory and at the telescope. In this paper, we will detail the architecture of the simulator and the computational model, which are strongly characterized by modularity and flexibility. Synthetic spectral formats, related to different seeing and observing conditions, and calibration frames to be ingested by the pipeline are also presented.

引用

页数：16

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