Ioannis Politopoulos,1 Johan Pragt,1 Rik ter Horst,1 Ronald Roelfsema,1 Olga Bellido-Tirado,2 Joar Brynnel,2 Steffen Frey,2 Amina Helmi,3 Jeroen Herrewijnen,1 Roelof de Jonghttps://orcid.org/0000-0001-6982-4081,2 Michael Lehmitz,4 Ramon Navarro,1 Allar Saviauk,2 Ray Sharples,5 Luke Tyas,5 Jurgen Schmoll,5 Walter Seifert,6 Menno de Haan,1 Menno Schuil,1 Eddy Elswijk,1 Eduardo Balbinot3
1NOVA Optical Infrared Instrumentation Group, ASTRON (Netherlands) 2Leibniz-Institut für Astrophysik Potsdam (Germany) 3Univ. of Groningen (Netherlands) 4Max-Planck-Institut für Astronomie (Germany) 5Durham Univ. (United Kingdom) 6Zentrum für Astronomie, Landessternwarte Heidelberg (Germany)
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The Calibration Unit for 4MOST is providing hundreds of highly stable sharp spectral features with high power and mimicking the sky over the focal plane. The heart of the system is a combination of a bright broadband lamp and a Fabry-Perot etalon that provides a regular comb of spectral lines. 120 integrating spheres are distributed in 4 Light sabre linear arrays. These Light sabres are attached to the telescope spider struts and provide unvignetted illumination to the telescope focal plane. We describe the final design, the alignment, and the results of the testing.
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Ioannis Politopoulos, Johan Pragt, Rik ter Horst, Ronald Roelfsema, Olga Bellido-Tirado, Joar Brynnel, Steffen Frey, Amina Helmi, Jeroen Herrewijnen, Roelof de Jong, Michael Lehmitz, Ramon Navarro, Allar Saviauk, Ray Sharples, Luke Tyas, Jurgen Schmoll, Walter Seifert, Menno de Haan, Menno Schuil, Eddy Elswijk, Eduardo Balbinot, "4MOST calibration system: design, assembly, and testing," Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 1218473 (29 August 2022); https://doi.org/10.1117/12.2629542