Abstract

MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as a facility instrument by the Sapienza University for INAF, that manages the radio telescope, under a PON contract. It will consist of a compact cryostat hosting the re–imaging optics, cooled at 4K, and a 408–pixel array of photon–noise limited lumped element kinetic inductance detectors fabricated at CNR-IFN and cooled at a base temperature lower than 300mK. MISTRAL will be able to investigate a long list of scientific targets spanning from extragalactic astrophysics to solar system science, with high angular resolution (~ 12 arcsec), including Sunyaev Zel’dovich effect measurements and the study of the Cosmic Web.

Highlights

  • Sardinia Radio telescope (SRT) is a multipurpose telescope aimed to measure the electromagnetic radiation from 300 MHz to 116 GHz

  • MISTRAL will be installed in March 2022 and commissioning activities will start in spring 2022

  • SRT is a multipurpose observatory designed to measure a wide range of radio wavelengths: from 300 MHz to 116 GHz

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Summary

Introduction

Sardinia Radio telescope (SRT) is a multipurpose telescope aimed to measure the electromagnetic radiation from 300 MHz to 116 GHz. After the scientific commissioning, in 2015, 4 receivers have been installed and successfully operated at frequency lower than 26.5 GHz. New instruments are going to be installed in the future, among which, MISTRAL will measure in the W-band. High angular resolution W-band measurements open at a number of possibilities of scientific cases, including galaxies spectral energy distribution measurement and their continuum observation [1], AGN and radio galaxies [2], detection of circumstellar disks [3], dense core in giant molecular gas investigation [4], synchrotron non thermal jet and hot spot [5], intraclusters filaments, cosmic web, and other S-Z related observation [6, 7]; and even more, by correlating with other experiment. MISTRAL aims to perform high angular resolution measurement with an array of lumped element kids detectors coupled, thanks to a re-imaging optic system, with SRT.

Sardinia Radio Telescope
Site condition
MISTRAL instrument
Cryostat
Magnetic shield
Optics
Focal Plane
Sensitivity estimation
Conclusions
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