The map-making and data filtering pipeline for the MISTRAL receiver

E. Barbavara; E. S. Battistelli; P. de Bernardis; F. Cacciotti; V. Capalbo; A. Carbone; E. Carretti; D. Ciccalotti; F. Columbro; A. Coppolecchia; A. Cruciani; G. D'Alessandro; M. De Petris; F. Govoni; G. Isopi; L. Lamagna; P. Marongiu; A. Mascia; S. Masi; E. Molinari; M. Murgia; A. Navarrini; A. Novelli; A. Occhiuzzi; A. Orlati; A. Paiella; G. Pettinari; F. Piacentini; T. Pisanu; S. Poppi; I. Porceddu; A. Ritacco; R. Schirru; G. Vargiu

doi:10.1117/12.3019685

16 August 2024 The map-making and data filtering pipeline for the MISTRAL receiver

E. Barbavara, E. S. Battistelli, P. de Bernardis, F. Cacciotti, V. Capalbo, A. Carbone, E. Carretti, D. Ciccalotti, F. Columbro, A. Coppolecchia, A. Cruciani, G. D'Alessandro, M. De Petris, F. Govoni, G. Isopi, L. Lamagna, P. Marongiu, A. Mascia, S. Masi, E. Molinari, M. Murgia, A. Navarrini, A. Novelli, A. Occhiuzzi, A. Orlati, A. Paiella, G. Pettinari, F. Piacentini, T. Pisanu, S. Poppi, I. Porceddu, A. Ritacco, R. Schirru, G. Vargiu

Author Affiliations +

Proceedings Volume 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII; 131022T (2024) https://doi.org/10.1117/12.3019685
Event: SPIE Astronomical Telescopes + Instrumentation, 2024, Yokohama, Japan

Conference Poster

Abstract

A new facility instrument open to the scientific community is MISTRAL. The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements KIDs (MISTRAL) is a millimetric multi–pixel camera, mounted at the Gregorian focus of the Sardinia Radio Telescope (SRT), working in the W-band that will be able to study many scientific cases, from the ‘missing baryons’ problem to extragalactic astrophysics, morphology of galaxy cluster and the search of the Cosmic Web through high angular resolution measurements of the Sunyaev-Zel’dovich effect. We present the current state of the map-making and data filtering software that we plan to use for future observations. This software aims to analyze the simulated observations of a target, filter the data from instrumental noise and produce a map, employing a customized common mode removal.

(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.

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E. Barbavara, E. S. Battistelli, P. de Bernardis, F. Cacciotti, V. Capalbo, A. Carbone, E. Carretti, D. Ciccalotti, F. Columbro, A. Coppolecchia, A. Cruciani, G. D'Alessandro, M. De Petris, F. Govoni, G. Isopi, L. Lamagna, P. Marongiu, A. Mascia, S. Masi, E. Molinari, M. Murgia, A. Navarrini, A. Novelli, A. Occhiuzzi, A. Orlati, A. Paiella, G. Pettinari, F. Piacentini, T. Pisanu, S. Poppi, I. Porceddu, A. Ritacco, R. Schirru, and G. Vargiu "The map-making and data filtering pipeline for the MISTRAL receiver", Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131022T (16 August 2024); https://doi.org/10.1117/12.3019685

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