SOXS: A wide band spectrograph to follow up transients

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dc.contributor.authorSchipani, P.
dc.contributor.authorCampana, S.
dc.contributor.authorClaudi, R.
dc.contributor.authorKäufl, H.U.
dc.contributor.authorAccardo, M.
dc.contributor.authorAliverti, M.
dc.contributor.authorBaruffolo, A.
dc.contributor.authorBen Ami, S.
dc.contributor.authorBiondi, F.
dc.contributor.authorBrucalassi, A.
dc.contributor.authorCapasso, G.
dc.contributor.authorCosentino, R.
dc.contributor.authorD'Alessio, F.
dc.contributor.authorD'Avanzo, P.
dc.contributor.authorHershko, O.
dc.contributor.authorGardiol, D.
dc.contributor.authorKuncarayacti, H.
dc.contributor.authorMunari, M.
dc.contributor.authorRubin, A.
dc.contributor.authorScuderi, S.
dc.contributor.authorVitali, F.
dc.contributor.authorAchrén, J.
dc.contributor.authorAraiza-Duran, J. Antonio
dc.contributor.authorArcavi, I.
dc.contributor.authorBianco, A.
dc.contributor.authorCappellaro, E.
dc.contributor.authorColapietro, M.
dc.contributor.authorDella Valle, M.
dc.contributor.authorDiner, O.
dc.contributor.authorD'Orsi, S.
dc.contributor.authorFantinel, D.
dc.contributor.authorFynbo, J.
dc.contributor.authorGal-Yam, A.
dc.contributor.authorGenoni, M.
dc.contributor.authorHirvonen, M.
dc.contributor.authorKotilainen, J.
dc.contributor.authorKumar, T.
dc.contributor.authorLandoni, M.
dc.contributor.authorLehti, J.
dc.contributor.authorLi Causi, G.
dc.contributor.authorLoreggia, D.
dc.contributor.authorMarafatto, L.
dc.contributor.authorMattila, S.
dc.contributor.authorPariani, G.
dc.contributor.authorPignata, G.
dc.contributor.authorRappaport, M.
dc.contributor.authorRicci, D.
dc.contributor.authorRiva, M.
dc.contributor.authorSalasnich, B.
dc.contributor.authorZanmar Sanchez, R.
dc.contributor.authorSmartt, S.
dc.contributor.authorTuratto, M.
dc.date.accessioned2022-09-26T14:07:03Z
dc.date.available2022-09-26T14:07:03Z
dc.date.issued2018-06
dc.descriptionIndexación: Scopuses
dc.description.abstractSOXS (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. © 2018 SPIE.es
dc.description.uri://efaidnbmnnnibpcajpcglclefindmkaj/https://pureadmin.qub.ac.uk/ws/files/187277420/1807.08828v1.pdf
dc.identifier.doi10.1117/12.2307349
dc.identifier.issn0277786X
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/24062
dc.language.isoenes
dc.publisherSPIEes
dc.rights.licenseAtribución 4.0 Internacional (CC BY 4.0)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.subjectTelescopees
dc.subjectEchellees
dc.subjectEuropean Southern Observatoryes
dc.titleSOXS: A wide band spectrograph to follow up transientses
dc.typeArtículoes
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Proceedings of SPIE - The International Society for Optical EngineeringOpen AccessVolume 107022018 Article number 107020FGround-based and Airborne Instrumentation for Astronomy VII 2018Austin10 June 2018through 14 June 2018Code 138743
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