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  5. SOXS: a wide band spectrograph to follow up transients
 

SOXS: a wide band spectrograph to follow up transients

Date Issued
2018
Author(s)
SCHIPANI, Pietro  
•
CAMPANA, Sergio  
•
CLAUDI, Riccardo  
•
Käufl, H. U.
•
Accardo, M.
•
Aliverti, Matteo  
•
BARUFFOLO, Andrea  
•
Ben Ami, S.
•
BIONDI, FEDERICO  
•
BRUCALASSI, ANNA  
•
CAPASSO, Giulio  
•
COSENTINO, Rosario  
•
D'Alessio, F.  
•
D'AVANZO, Paolo  
•
Hershko, O.
•
GARDIOL, Daniele  
•
Kuncarayacti, H.
•
Munari, M.  
•
Rubin, A.
•
SCUDERI, Salvatore  
•
VITALI, Fabrizio  
•
Achrén, J.
•
Araiza-Duran, J. Antonio
•
Arcavi, I.
•
BIANCO, Andrea  
•
CAPPELLARO, Enrico  
•
COLAPIETRO, MIRKO  
•
DELLA VALLE, Massimo  
•
Diner, O.
•
D'ORSI, SERGIO  
•
FANTINEL, Daniela  
•
Fynbo, J.
•
Gal-Yam, A.
•
Genoni, Matteo  
•
Hirvonen, M.
•
Kotilainen, J.
•
Kumar, T.
•
LANDONI, Marco  
•
Lehti, J.
•
LI CAUSI, Gianluca  
•
Loreggia, D.  
•
Marafatto, L.  
•
Mattila, S.
•
PARIANI, Giorgio  
•
Pignata, G.
•
Rappaport, M.
•
RICCI, DAVIDE  
•
RIVA, Marco  
•
SALASNICH, Bernardo  
•
Zanmar Sanchez, R.
•
Smartt, S.
•
TURATTO, Massimo  
DOI
10.1117/12.2307349
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.
Coverage
Ground-based and Airborne Instrumentation for Astronomy VII
All editors
Evans, Christopher J.; Simard, Luc; Takami, Hideki
Series
PROCEEDINGS OF SPIE  
Volume
10702
Start page
107020F
Conferenece
Ground-based and Airborne Instrumentation for Astronomy VII
Conferenece place
Austin, Texas, United States
Conferenece date
10-15 June, 2018
Uri
http://hdl.handle.net/20.500.12386/28791
Url
https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10702/2307349/SOXS--a-wide-band-spectrograph-to-follow-up-transients/10.1117/12.2307349.short?SSO=1
Issn Identifier
0277-786X
Ads BibCode
2018SPIE10702E..0FS
Rights
open.access
File(s)
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