Search for fast radio bursts a forecast for the BINGO interferometry system

• Autor(a) principal: Hoerning, Gabriel Amâncio
• Data de Publicação: 2023
• Tipo de documento: Dissertação
• Idioma: eng
• Título da fonte: Biblioteca Digital de Teses e Dissertações da USP
• Texto Completo: https://www.teses.usp.br/teses/disponiveis/43/43134/tde-18072023-084517/
• topic: BINGO telescope.; Fast Radio Bursts; Fast Radio Bursts; Interferometria,Telescópio BINGO.; Interferometry; Radio Astronomy; Radioastronomia

The Baryon Acoustic Oscillations (BAO) from Integrated Neutral Gas Observations (BINGO) radio telescope will use the neutral Hydrogen emission line to map the Universe in the redshift range 0.127 z 0.449, with the main goal of probing BAO. In addition, the instrument optical design and hardware configuration support the search for Fast Radio Bursts (FRBs). In this Master\'s thesis, we propose the use of a BINGO Interferometry System (BIS), including new auxiliary, smaller radio telescopes, hereafter referred to as \"outriggers.\" The interferometric approach makes it possible to pinpoint the FRB sources in the sky. We present here the results of several BIS configurations, combining BINGO horns with and without mirrors (4 m, 5 m, and 6 m) and using 5, 7, 9, or 10 single horns. We developed a new Python package, FRBlip, which generates synthetic FRB mock catalogs and computes, based on a telescope model, the observed signal-to-noise ratio (S/N). This ratio is used to compute the detection rates of the telescopes and the number of interferometry pairs of telescopes (baselines) that can observe an FRB. FRBs observed by more than one baseline are those whose location can be determined. Thus, we evaluate the performance of BIS regarding FRB localization. We found that BIS will be able to localize 23 FRBs yearly with single horn outriggers in the best configuration (using 10 outriggers of 6 m mirrors), with redshift z 0.96. The full localization capability depends on the number and type of the outriggers. Wider beams are best to pinpoint FRB sources because potential candidates will be observed by more baselines, while narrow beams look deep in redshift. For example, 6 m stations are ideal for this purpose. The BIS can be a powerful extension of the regular BINGO telescope, dedicated to observing hundreds of FRBs during Phase 1. Many of them will be well localized with single horns + 6 m dish as outriggers.