Póster presentado a la XXX Astronomical Data Analysis Software and Systems Conference, celebrada online del 8 al 12 de noviembre de 2020 en la University of Maryland, College Park Campus, USA.[Aims]: to detect and to reconstruct the pulses that X-ray photons produce at TES (Transition Edge Sensor) detectors (like the one in the Athena/X-IFU instrument), using Deep Learning techniques. The dataset used contains simulations performed with the Athena official simulator SIXTE.[Methods]: We construct and train a Convolution Neural Network (CNN) to differentiate between single, double and triple pulses. We use a hyper-parameter bayesian optimization to select the optimal CNN architecture.[Results]: we present the results of our CNN classification...
14 pages, 10 tables, 16 figures, accepted for publication in MNRASInternational audienceGalaxy clust...
The ability to discover new transient candidates via image differencing without direct human interve...
New deep learning techniques present promising new analysis methods for Imaging Atmospheric Cherenko...
Transition Edge Sensors detector devices, like the core of the X-IFU instrument that will be on-boar...
Transition Edge Sensors detector devices, like the core of the X-IFU instrument that will be on-boar...
We present here the computational basis of the software chain (XRAYCHAIN) developed to detect and an...
This work was developed in the context of space-born gamma-ray astronomy, with particular focus on a...
Convolutional neural networks (CNNs) are widely used state-of-the-art computer vision tools that are...
Trabajo presentado a la XXVII Astronomical Data Analysis Software and Systems Conference, celebrada ...
We present a technique for optical transient detection using artificial neural networks, particularl...
Upcoming fast radio burst (FRB) surveys will search ~103 beams on the sky with a very high duty cycl...
This thesis presents new machine learning techniques for producing high energy astronomy survey cata...
A convolutional neural network (CNN) architecture is developed to improve the pulse shape discrimina...
Parallel Flash Talk at the "XIX International Workshop on Neutrino Telescopes" on line - 18-26 Febru...
14 pages, 10 tables, 16 figures, accepted for publication in MNRASInternational audienceGalaxy clust...
The ability to discover new transient candidates via image differencing without direct human interve...
New deep learning techniques present promising new analysis methods for Imaging Atmospheric Cherenko...
Transition Edge Sensors detector devices, like the core of the X-IFU instrument that will be on-boar...
Transition Edge Sensors detector devices, like the core of the X-IFU instrument that will be on-boar...
We present here the computational basis of the software chain (XRAYCHAIN) developed to detect and an...
This work was developed in the context of space-born gamma-ray astronomy, with particular focus on a...
Convolutional neural networks (CNNs) are widely used state-of-the-art computer vision tools that are...
Trabajo presentado a la XXVII Astronomical Data Analysis Software and Systems Conference, celebrada ...
We present a technique for optical transient detection using artificial neural networks, particularl...
Upcoming fast radio burst (FRB) surveys will search ~103 beams on the sky with a very high duty cycl...
This thesis presents new machine learning techniques for producing high energy astronomy survey cata...
A convolutional neural network (CNN) architecture is developed to improve the pulse shape discrimina...
Parallel Flash Talk at the "XIX International Workshop on Neutrino Telescopes" on line - 18-26 Febru...
14 pages, 10 tables, 16 figures, accepted for publication in MNRASInternational audienceGalaxy clust...
The ability to discover new transient candidates via image differencing without direct human interve...
New deep learning techniques present promising new analysis methods for Imaging Atmospheric Cherenko...