High angular resolution Sunyaev Zel'dovich observations: the case of MISTRAL
E. S. Battistelli (Sapienza University of Rome), E. Barbavara, (Sapienza University of Rome), P. de Bernardis (Sapienza University of Rome),, F. Cacciotti (Sapienza University of Rome), V. Capalbo (Sapienza University, of Rome), E. Carretti (INAF-IRA)

TL;DR
MISTRAL is a new millimeter-wave camera for the Sardinia Radio Telescope, designed to observe the Sunyaev Zel'dovich effect and other astrophysical phenomena with high angular resolution and multiple scientific applications.
Contribution
This paper introduces MISTRAL, a novel 12-arcsecond resolution, 408-KID array camera for the Sardinia Radio Telescope, enabling advanced SZ effect and astrophysical studies.
Findings
Design and construction of MISTRAL completed in 2022
MISTRAL will provide high-resolution SZ observations of galaxy clusters
The instrument will support diverse astrophysical research
Abstract
The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements kids, MISTRAL, is a millimetric () multipixel camera being built for the Sardinia Radio Telescope. It is going to be a facility instrument and will sample the sky with 12 arcsec angular resolution, 4 arcmin field of view, through 408 Kinetic Inductance Detectors (KIDs). The construction and the beginning of commissioning is planned to be in 2022. MISTRAL will allow the scientific community to propose a wide variety of scientific cases including protoplanetary discs study, star forming regions, galaxies radial profiles, and high angular resolution measurements of the Sunyaev Zel'dovich (SZ) effect with the investigation of the morphology of galaxy cluster and the search for the Cosmic Web.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Gamma-ray bursts and supernovae · Astronomical Observations and Instrumentation
