OLIVEIRA, A. R. M.; http://lattes.cnpq.br/1112730768122348; OLIVEIRA, Ana Rafaely Medeiros de.
Resumo:
In 2007, a very bright radio pulse was identified in archival data from the Parkes Telescope
in Australia, marking the beginning of a new branch of research in astrophysics. In the
early years, Fast Radio Bursts (FRBs) appeared very mysterious because the sample of
events was limited, and their origins were unknown. With the improvement of instruments
and data analysis techniques over the last five years, hundreds of new FRBs have been
discovered. The field is now undergoing a revolution, and the understanding of FRBs
has rapidly increased as new events continue to be uncovered. However, as new data are
received at a high rate of candidates, it is necessary to assess whether they are FRBs
or transients originating from other sources. In this work, we employ Deep Learning
techniques to train deep neural networks for the classification of FRB and transient
candidates. The convolutional neural networks used work with frequency and time data
to generate spectrograms, also known as Waterfalls. We trained these networks using
simulated FRBs and analyzed their output. We present several deep learning models with
an accuracy and recall of approximately 90% on our test dataset, which is composed of
simulated data and real pulses or FRB candidates. Currently, the use of machine learning
algorithms for candidate classification is essential. These algorithms will also play a key
role in building real-time triggers for detection in the BINGO project instruments.