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arxiv: 2407.17288 · v1 · pith:GNZ3RDBM · submitted 2024-07-24 · astro-ph.IM · astro-ph.EP

What is your favorite transient event? SOXS is almost ready to observe!

Kalyan Kumar Radhakrishnan Santhakumari , Federico Battaini , Simone Di Filippo , Silvio Di Rosa , Lorenzo Cabona , Riccardo Claudi , Luigi Lessio , Marco Dima
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David Young Marco Landoni Mirko Colapietro Sergio D'Orsi Matteo Aliverti Matteo Genoni Matteo Munari Ricardo Zanmar Sanchez Fabrizio Vitali Davide Ricci Pietro Schipani Sergio Campana Jani Achren Jose Araiza-Duran Iair Arcavi Andrea Baruffolo Sagi Ben-Ami Alex Bitchkovsky Anna Brucalassi Rachel Bruch Giulio Capasso Enrico Cappellaro Rosario Cosentino Francesco D'Alessio Paolo D'Avanzo Massimo Della Valle Rosario Di Benedetto Avishay Gal-Yam Marcos Hernandez Diaz Ofir Hershko Jari Kotilainen Hanindyo Kuncarayakti Gianluca Li Causi Luca Marafatto Eugenio Martinetti Laurent Marty Seppo Mattila Antonio Micciche Gaetano Nicotra Luca Oggioni Hector Perez Ventura Giorgio Pariani Giuliano Pignata Michael Rappaport Marco Riva Adam Rubin Bernardo Salasnich Salvatore Savarese Salvatore Scuderi Steven Smartt Maximilian Stritzinger
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keywords soxseventobservetransientverificationwavelengthacceptancealmost
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The Son Of X-Shooter (SOXS) will be the specialized facility to observe any transient event with a flexible scheduler at the ESO New Technology Telescope (NTT) at La Silla, Chile. SOXS is a single object spectrograph offering simultaneous spectral coverage in UV-VIS (350-850 nm) and NIR (800-2000 nm) wavelength regimes with an average of R~4500 for a 1arcsec slit. SOXS also has imaging capabilities in the visible wavelength regime. Currently, SOXS is being integrated at the INAF-Astronomical Observatory of Padova. Subsystem- and system-level tests and verification are ongoing to ensure and confirm that every requirement and performance are met. In this paper, we report on the integration and verification of SOXS as the team and the instrument prepare for the Preliminary Acceptance Europe (PAE).

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