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

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...

Full description

Saved in:
Bibliographic Details
Main Authors Santhakumari, Kalyan Kumar Radhakrishnan, Battaini, Federico, Di Filippo, Simone, Di Rosa, Silvio, Cabona, Lorenzo, Claudi, Riccardo, Lessio, Luigi, Dima, Marco, Young, David, Landoni, Marco, Colapietro, Mirko, D'Orsi, Sergio, Aliverti, Matteo, Genoni, Matteo, Munari, Matteo, Sanchez, Ricardo Zanmar, Vitali, Fabrizio, Ricci, Davide, Schipani, Pietro, Campana, Sergio, Achren, Jani, Araiza-Duran, Jose, Arcavi, Iair, Baruffolo, Andrea, Ben-Ami, Sagi, Bitchkovsky, Alex, Brucalassi, Anna, Bruch, Rachel, Capasso, Giulio, Cappellaro, Enrico, Cosentino, Rosario, D'Alessio, Francesco, D'Avanzo, Paolo, Della Valle, Massimo, Di Benedetto, Rosario, Gal-Yam, Avishay, Diaz, Marcos Hernandez, Hershko, Ofir, Kotilainen, Jari, Kuncarayakti, Hanindyo, Causi, Gianluca Li, Marafatto, Luca, Martinetti, Eugenio, Marty, Laurent, Mattila, Seppo, Micciche, Antonio, Nicotra, Gaetano, Oggioni, Luca, Ventura, Hector Perez, Pariani, Giorgio, Pignata, Giuliano, Rappaport, Michael, Riva, Marco, Rubin, Adam, Salasnich, Bernardo, Savarese, Salvatore, Scuderi, Salvatore, Smartt, Steven, Stritzinger, Maximilian
Format Journal Article
LanguageEnglish
Published 24.07.2024
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary: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).
DOI:10.48550/arxiv.2407.17288