The integration and alignment phase for the Acquisition and Guiding System of SOXS
: Araiza-Durán José A., Pignata Giuliano, Brucalassi Anna, Battaini Federico, Radhakrishnan Kalyan, Claudi Riccardo, Campana Sergio, Schipani Pietro, Aliverti Matteo, Baruffolo Andrea, Ben-Ami Sagi, Capasso Giulio, Cosentino Rosario, D'Alessio Francesco, D'Avanzo Paolo, Hershko Ofir, Kuncarayakti Hanindyo, Landoni Marco, Munari Matteo, Rubin Adam, Scuderi Salvatore, Vitali Fabrizio, Young David, Achrén Jani, Arcavi Iair, Bruch Rachel, Cappellaro Enrico, Colapietro Mirko, Della Valle Massimo, Di Benedetto Rosario, D'Orsi Sergio, Gal-Yam Avishay, Genoni Matteo, Díaz Marcos Hernandez, Kotilainen Jari, Li Causi Gianluca, Marty Laurent, Mattila Seppo, Rappaport Michael, Ricci Davide, Riva Marco, Salasnich Bernardo, Smartt Stephen, Sanchez Ricardo Zanmar, Stritzinger Maximilian, Ventura Hector Pérez
: Christopher J. Evans, Julia J. Bryant, Kentaro Motohara
: SPIE Astronomical Telescopes + Instrumentation
Publisher: SPIE-INT SOC OPTICAL ENGINEERING, PO BOX 10, BELLINGHAM, WA 98227-0010 USA
: 2022
: Proceedings of SPIE : the International Society for Optical Engineering
: Proceedings of SPIE: Ground-based and Airborne Instrumentation for Astronomy IX
: GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY IX
: PROC SPIE
: 1218483
: Proceedings of SPIE : the International Society for Optical Engineering
: 12184
: 1218483
: 8
: 0277-786X
: 1996-756X
DOI: https://doi.org/10.1117/12.2630001
: https://doi.org/10.1117/12.2630001
SOXS (Son Of X-Shooter) will be the new double-armed spectrograph for the ESO NTT at La Silla and it will be optimized to provide an unique specialized facility to follow up and classify any kind of transient events. It consists of a central structure (common path) which supports two spectrographs optimized for the UV-Visible and a Near-IR range. Attached to the common path there is the Acquisition and Guiding Camera System (ACS), equipped with a filter wheel which can provide some science grade imaging and moderate high speed photometry. The project is currently in its Assembly Integration and Verification phase following a modular approach so that each sub-system can be integrated in parallel before their final assembly at system level, foreseen at the INAF-Osservatorio Astronomico di Padova (Italy). The optics and the mechanical parts of the ACS arrived in the second semester of 2021, so from that moment the Assembly and Verification Phase began. This work presents the assembly and testing operation of the ACS of SOXS and we report the strategy and the results achieved to meet the requirements.
