1. SOXS: a wide band spectrograph to follow up transients
- Author
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Johan P. U. Fynbo, H. U. Käufl, J. Lehti, A. Brucalassi, Massimo Turatto, T. Kumar, Matteo Accardo, H. Kuncarayacti, Matteo Genoni, Marco Riva, P. D'Avanzo, Daniela Fantinel, Matteo Aliverti, Jari Kotilainen, Federico Biondi, Davide Loreggia, Adam Rubin, Rosario Cosentino, Stephen J. Smartt, Sergio Campana, Fabrizio Vitali, Andrea Baruffolo, Seppo Mattila, R. Zanmar Sanchez, Salvo Scuderi, Matteo Munari, Giuliano Pignata, Francesco D'Alessio, Antonino Bianco, M. Hirvonen, Sergio D'Orsi, M. Della Valle, S. Ben Ami, Iair Arcavi, G. Capasso, Daniele Gardiol, D. Ricci, Luca Marafatto, G. Li Causi, Enrico Cappellaro, J. Achrén, Riccardo Claudi, Avishay Gal-Yam, J. Antonio Araiza-Duran, Giorgio Pariani, Bernardo Salasnich, Marco Landoni, O. Diner, O. Hershko, Pietro Schipani, M. Colapietro, and Michael Rappaport
- Subjects
Physics ,ta115 ,010504 meteorology & atmospheric sciences ,Gravitational wave ,FOS: Physical sciences ,Astronomy ,01 natural sciences ,law.invention ,SOXS ,Telescope ,Photometry (optics) ,Supernova ,Limiting magnitude ,law ,Target of opportunity ,0103 physical sciences ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,010303 astronomy & astrophysics ,Spectrograph ,astro-ph.IM ,0105 earth and related environmental sciences - Abstract
SOXS (Son Of X-Shooter) will be a spectrograph for the ESO NTT telescope capable to cover the optical and NIR bands, based on the heritage of the X-Shooter at the ESO-VLT. SOXS will be built and run by an international consortium, carrying out rapid and longer term Target of Opportunity requests on a variety of astronomical objects. SOXS will observe all kind of transient and variable sources from different surveys. These will be a mixture of fast alerts (e.g. gamma-ray bursts, gravitational waves, neutrino events), mid-term alerts (e.g. supernovae, X-ray transients), fixed time events (e.g. close-by passage of minor bodies). While the focus is on transients and variables, still there is a wide range of other astrophysical targets and science topics that will benefit from SOXS. The design foresees a spectrograph with a Resolution-Slit product ~ 4500, capable of simultaneously observing over the entire band the complete spectral range from the U- to the H-band. The limiting magnitude of R~20 (1 hr at S/N~10) is suited to study transients identified from on-going imaging surveys. Light imaging capabilities in the optical band (grizy) are also envisaged to allow for multi-band photometry of the faintest transients. This paper outlines the status of the project, now in Final Design Phase., Comment: 12 pages, 14 figures, to be published in SPIE Proceedings 10702
- Published
- 2018
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