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SOXS (Son Of X-Shooter) is a single object spectrograph, covering from UV to infrared in one single shot.
SOXS was selected in 2015 by ESO (European Southern Observatory) after a call for new instruments at the 3.6m ESO New Technology Telescope at the La Silla Observatory, Chile. SOXS is built by an international consortium led by INAF (50%) and including Israel, UK, Finland, Chile and Denmark as partners.

INAF-Brera Astronomical Observatory is the project nerve centre. We are integrating the infrared arm in our cleaning room. We are developing the producing software for observing schedule on a night-by-night basis and we are contributing for data reduction pipeline.
During operative phase the observatory will be the centre for SOXS operations.

The New Technology Telescope or NTT is a 3.58-metre Ritchey–Chretien telescope operated by the European Southern Observatory. It began operations in 1989. It is located in Chile at the La Silla Observatory.

The New Technology Telescope or NTT is a 3.58-metre Ritchey-Chrétien telescope operated by the European Southern Observatory. It began operations in 1989. It is located in Chile at the La Silla Observatory.

As a reward for our efforts, ESO will compensate the SOXS Consortium with 180 observing nights per year for 5 years (900 nights). The science goals of the SOXS Consortium are focussed: the spectrograph will observe all kind of transient and variable sources discovered by different surveys with a highly flexible schedule, updated daily, based on the Target of Opportunity concept. It will provide a key spectroscopic partner to any kind of imaging survey, becoming one of the premier transient follow-up instruments in the Southern hemisphere. SOXS will study a mixture of transients encompassing all distance scales and branches of astronomy, including fast alerts (such as gamma-ray bursts and gravitational waves), mid-term alerts (such as supernovae and X-ray transients), and fixed-time events (such as the close-by passage of a minor planet or exoplanets). It will also have the scope to observe active galactic nuclei and blazars, tidal disruption events, fast radio bursts, and more.

SOXS will be installed at one of the Nasmyth foci of the NTT, replacing SOFI a productive infrared spectrograph and imaging camera running more than 20 years. SoXS is being built to provide an unique specialized facility to follow up any kind of transient events with the best possible response time paired with high efficiency and availability. (Crediti ESO).

SOXS will be installed at one of the Nasmyth foci of the NTT, replacing SOFI, a venerable and highly productive ESO instrument. Designed as a unique spectroscopic facility, SOXS will study transient sources following triggers and alerts from telescopes, satellites, and detectors worldwide. (Crediti ESO).

 

Besides of the consortium programs on guaranteed time, the instrument is offered to the ESO community for any kind of astrophysical target. The SOXS Consortium is in charge of the NTT operations, producing the observing schedule on a night-by-night basis. The schedule will be dynamical, merging SOXS and ESO target depending on our needs. The schedule is flexible and will give us the opportunity to react in real time to the new surprises the sky will offer us.
Now, (November 2021) SOXS is in its integration phase and a preliminary acceptance of the instrument from ESO is foreseen for the Summer 2022.

Artistic view of some objects that can be studied by SOXS spectrograph - Left top: Gamma Ray Bursts, supernova explosion - Bottom: tidal disruption event.

Artistic view of some objects that can be studied by SOXS spectrograph - Left top: Gamma Ray Bursts, supernova explosion - Bottom: tidal disruption event..

 
SOXS Team
 
 
Project Office
 
Name Role Affiliation
Sergio Campana Principal Investigator INAF-OABrera
Pietro Schipani Project Scientist INAF-OACapodimonte
Riccardo Claudi System Engineer INAF-OAPadova
Paolo D’Avanzo Instrument Scientist INAF-OABrera
 
WP Managers
 
Paolo D’Avanzo Instrument Scientist INAF-OABrera
Matteo Munari Optics WP Manager INAF-OACatania
Matteo Aliverti Mechanics WP Manager INAF-OABrera
Giulio Capasso Electronics WP Manager INAF-OACapodimonte
Andrea Baruffolo Software WP Manager INAF-OAPadova
Salvo Scuderi Vacuum & Cryogenics WP Managert INAF-OACatania
Kalyan Radhakrishnan AIT WP Manager INAF-OAPadova
Matteo Genoni Instrument Model WP Manager INAF-OABrera
Sagi Ben-Ami VIS Spectrograph WP Manager Weizmann Institute
Adam Rubin VIS Spectrograph Optics WP Manager Weizmann Institute
Ofir Hershko VIS Spectrograph Mechanics WP Manager Weizmann Institute
Rosario Cosentino VIS Detector WP Manager INAF-OACatania
Fabrizio Vitali NIR Spectrograph WP Manager INAF-OARoma
Francesco D’Alessio NIR WP Manager INAF-OARoma
Anna Brucalassi Acquisition Camera WP Manager Millenium Institute & ESO
Haynino Kuncaraycti Calibration Unit Optics WP Manager Turku University
 
Science Board
 
I. Arcavi (Tel Aviv University) - Israel
E. Cappellaro (INAF-OA Padova) - Italy
M. Della Valle (INAF-OA Napoli) - Italy
M. Stritzinger (NBI & Aarhus Univ.) - Denmark
A. Gal-Yam (Weizmann Institute) - Israel
S.Mattila (FINCA) - Finland
G. Pignata (Millenium Institute of Astrophysics) - Chile
S. Smartt (Queen’s Univ. Belfast) - UK
S. Campana (INAF-OA Brera) - Italy
 
 
 
Loghi partecipanti al progetto Link al portale dell'ESO - European Southern Observatory Link al portale dell'INAF - Istituto Nazionale di Astrofisica Link al portale Weizmann Institute of Science - Israele Link al portale dell'Universita` di Telaviv Link al portale Aarhus Univ. - Danimarca Link al portale Niels Bohr Institute - University of Copenhagen - Danimarca Link al portale FINCA - Finnish Centre for Astronomy with ESO Link al portale Millenium Institute of Astrophysics - Cile Link al portale Queen's University Belfast - UK
Science Working Group
 
WG WG Topic WG Leader WG Deputy
1 Small bodies and comets Fitzsimmond Dotto
2 Stellar variability, exoplanets and Young Stellar Objects Pagano Alcalà
3 Transient X-ray binaries, magnetars, ultra-luminous Casella Veledina
4 Cataclysmic variables, novae and white dwarfs Della Valle Ben Ami
5 Supernovae Ia and thermonuclear transients Stritzinger Kotak
6 Fast and extreme transients (including SLSNe) Arcavi Mattila
7 Intermediate luminosity transients Kotak Pastorello
8 Core Collapse Supernovae Gal-Yam Pignata
9 AGN and blazars Landoni -
10 Tidal Disruption and Nuclear Events Mattila Arcavi
11 Gamma Ray bursts & Fast radio bursts D’Avanzo Fynbo
12 Gravitational wave and neutrino counterparts Campana Smartt
13 Classification Benetti Botticella
 
Logo SOXS: Laura Ripamonti, Federica Loiacono & Sergio Campana - Credit for web page: S. Campana - M.R. Panzera