SOXS: a wide band spectrograph to follow up transients

Pietro Schipani; Sergio Campana; Riccardo U. Claudi; Hans-ulrich Kaufl; Matteo Accardo; Mika Hirvonen; Jussi Lehti; Jari Kotilainen; Tarun Kumar; Jani Achrén; Luca Marafatto; O. Hershko; Matteo Aliverti; Andrea Baruffolo; Sagi Ben-ami; Federico Biondi; Anna Brucalassi; Giulio Capasso; Rosario Cosentino; Francesco D'alessio; Paolo D'avanzo; Oz Diner; Daniele Gardiol; Hanindyo Kuncarayacti; Matteo Munari; Adam Rubin; Salvatore Scuderi; Fabrizio Vitali; José Antonio Araiza-durán; Iair Arcavi; Andrea Bianco; Enrico Cappellaro; Mirko Colapietro; Massimo Della Valle; Sergio D'orsi; Daniela Fantinel; Johan Fynbo; Avishay Gal-yam; Matteo Genoni; Marco Landoni; Gianluca Li Causi; Davide Loreggia; Seppo Mattila; Giorgio Pariani; Giuliano Pignata; Michael Rappaport; Marco Riva; Davide Ricci; Bernardo Salasnich; Stephen Smartt; Massimo Turatto; Ricardo Zánmar Sánchez; Hideki Takami; Christopher J. Evans; Luc Simard

doi:10.1117/12.2307349

SOXS: a wide band spectrograph to follow up transients

Pietro Schipani, Sergio Campana, Riccardo U. Claudi, Hans-ulrich Kaufl, Matteo Accardo, Mika Hirvonen, Jussi Lehti, Jari Kotilainen, Tarun Kumar, Jani Achrén, Luca Marafatto, O. Hershko, Matteo Aliverti, Andrea Baruffolo, Sagi Ben-ami, Federico Biondi, Anna Brucalassi, Giulio Capasso, Rosario Cosentino, Francesco D'alessioPaolo D'avanzo, Oz Diner, Daniele Gardiol, Hanindyo Kuncarayacti, Matteo Munari, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, José Antonio Araiza-durán, Iair Arcavi, Andrea Bianco, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Sergio D'orsi, Daniela Fantinel, Johan Fynbo, Avishay Gal-yam, Matteo Genoni, Marco Landoni, Gianluca Li Causi, Davide Loreggia, Seppo Mattila, Giorgio Pariani, Giuliano Pignata, Michael Rappaport, Marco Riva, Davide Ricci, Bernardo Salasnich, Stephen Smartt, Massimo Turatto, Ricardo Zánmar Sánchez, Hideki Takami, Christopher J. Evans, Luc Simard

The Cosmic Dawn Center

15 Citationer (Scopus)

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.

Originalsprog	Engelsk
Tidsskrift	Proceedings of the SPIE
Vol/bind	10702
Antal sider	12
ISSN	0277-786X
DOI	https://doi.org/10.1117/12.2307349
Status	Udgivet - 2018
Begivenhed	Ground-based and Airborne Instrumentation for Astronomy VII - Austin, United States Varighed: 10 jun. 2018 → 15 jun. 2018

Konference

Konference	Ground-based and Airborne Instrumentation for Astronomy VII
Lokation	Austin, United States
Periode	10/06/2018 → 15/06/2018

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10.1117/12.2307349

Citationsformater

Schipani, P., Campana, S., Claudi, R. U., Kaufl, H., Accardo, M., Hirvonen, M., Lehti, J., Kotilainen, J., Kumar, T., Achrén, J., Marafatto, L., Hershko, O., Aliverti, M., Baruffolo, A., Ben-ami, S., Biondi, F., Brucalassi, A., Capasso, G., Cosentino, R., ... Simard, L. (2018). SOXS: a wide band spectrograph to follow up transients. Proceedings of the SPIE, 10702. https://doi.org/10.1117/12.2307349

Schipani, P, Campana, S, Claudi, RU, Kaufl, H, Accardo, M, Hirvonen, M, Lehti, J, Kotilainen, J, Kumar, T, Achrén, J, Marafatto, L, Hershko, O, Aliverti, M, Baruffolo, A, Ben-ami, S, Biondi, F, Brucalassi, A, Capasso, G, Cosentino, R, D'alessio, F, D'avanzo, P, Diner, O, Gardiol, D, Kuncarayacti, H, Munari, M, Rubin, A, Scuderi, S, Vitali, F, Araiza-durán, JA, Arcavi, I, Bianco, A, Cappellaro, E, Colapietro, M, Della Valle, M, D'orsi, S, Fantinel, D, Fynbo, J, Gal-yam, A, Genoni, M, Landoni, M, Li Causi, G, Loreggia, D, Mattila, S, Pariani, G, Pignata, G, Rappaport, M, Riva, M, Ricci, D, Salasnich, B, Smartt, S, Turatto, M, Zánmar Sánchez, R, Takami, H, Evans, CJ & Simard, L 2018, 'SOXS: a wide band spectrograph to follow up transients', Proceedings of the SPIE, bind 10702. https://doi.org/10.1117/12.2307349

@inproceedings{bcae568453c449b0bcce636021fa6842,

title = "SOXS: a wide band spectrograph to follow up transients",

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.",

author = "Pietro Schipani and Sergio Campana and Claudi, {Riccardo U.} and Hans-ulrich Kaufl and Matteo Accardo and Mika Hirvonen and Jussi Lehti and Jari Kotilainen and Tarun Kumar and Jani Achr{\'e}n and Luca Marafatto and O. Hershko and Matteo Aliverti and Andrea Baruffolo and Sagi Ben-ami and Federico Biondi and Anna Brucalassi and Giulio Capasso and Rosario Cosentino and Francesco D'alessio and Paolo D'avanzo and Oz Diner and Daniele Gardiol and Hanindyo Kuncarayacti and Matteo Munari and Adam Rubin and Salvatore Scuderi and Fabrizio Vitali and Araiza-dur{\'a}n, {Jos{\'e} Antonio} and Iair Arcavi and Andrea Bianco and Enrico Cappellaro and Mirko Colapietro and {Della Valle}, Massimo and Sergio D'orsi and Daniela Fantinel and Johan Fynbo and Avishay Gal-yam and Matteo Genoni and Marco Landoni and {Li Causi}, Gianluca and Davide Loreggia and Seppo Mattila and Giorgio Pariani and Giuliano Pignata and Michael Rappaport and Marco Riva and Davide Ricci and Bernardo Salasnich and Stephen Smartt and Massimo Turatto and {Z{\'a}nmar S{\'a}nchez}, Ricardo and Hideki Takami and Evans, {Christopher J.} and Luc Simard",

year = "2018",

doi = "10.1117/12.2307349",

language = "English",

volume = "10702",

journal = "Proceedings of the SPIE",

issn = "0277-786X",

publisher = "International Society for Optical Engineering",

note = "Ground-based and Airborne Instrumentation for Astronomy VII ; Conference date: 10-06-2018 Through 15-06-2018",

}

TY - GEN

T1 - SOXS

T2 - Ground-based and Airborne Instrumentation for Astronomy VII

AU - Schipani, Pietro

AU - Campana, Sergio

AU - Claudi, Riccardo U.

AU - Kaufl, Hans-ulrich

AU - Accardo, Matteo

AU - Hirvonen, Mika

AU - Lehti, Jussi

AU - Kotilainen, Jari

AU - Kumar, Tarun

AU - Achrén, Jani

AU - Marafatto, Luca

AU - Hershko, O.

AU - Aliverti, Matteo

AU - Baruffolo, Andrea

AU - Ben-ami, Sagi

AU - Biondi, Federico

AU - Brucalassi, Anna

AU - Capasso, Giulio

AU - Cosentino, Rosario

AU - D'alessio, Francesco

AU - D'avanzo, Paolo

AU - Diner, Oz

AU - Gardiol, Daniele

AU - Kuncarayacti, Hanindyo

AU - Munari, Matteo

AU - Rubin, Adam

AU - Scuderi, Salvatore

AU - Vitali, Fabrizio

AU - Araiza-durán, José Antonio

AU - Arcavi, Iair

AU - Bianco, Andrea

AU - Cappellaro, Enrico

AU - Colapietro, Mirko

AU - Della Valle, Massimo

AU - D'orsi, Sergio

AU - Fantinel, Daniela

AU - Fynbo, Johan

AU - Gal-yam, Avishay

AU - Genoni, Matteo

AU - Landoni, Marco

AU - Li Causi, Gianluca

AU - Loreggia, Davide

AU - Mattila, Seppo

AU - Pariani, Giorgio

AU - Pignata, Giuliano

AU - Rappaport, Michael

AU - Riva, Marco

AU - Ricci, Davide

AU - Salasnich, Bernardo

AU - Smartt, Stephen

AU - Turatto, Massimo

AU - Zánmar Sánchez, Ricardo

AU - Takami, Hideki

AU - Evans, Christopher J.

AU - Simard, Luc

PY - 2018

Y1 - 2018

N2 - 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.

AB - 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.

U2 - 10.1117/12.2307349

DO - 10.1117/12.2307349

M3 - Conference article

SN - 0277-786X

VL - 10702

JO - Proceedings of the SPIE

JF - Proceedings of the SPIE

Y2 - 10 June 2018 through 15 June 2018

ER -

SOXS: a wide band spectrograph to follow up transients

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