1 code implementation • 27 Apr 2023 • Helem Salinas, Karim Pichara, Rafael Brahm, Francisco Pérez-Galarce, Domingo Mery
Models, such as the Transformer architecture, were recently proposed for sequential data with successful results.
no code implementations • 12 Mar 2023 • Francisco Pérez-Galarce, Karim Pichara, Pablo Huijse, Márcio Catelan, Domingo Mery
Consequently, we propose a scalable and easily adaptable approach based on an informative regularization and an ad-hoc training procedure to mitigate the shift problem during the training of a multi-layer perceptron for RR Lyrae classification.
no code implementations • 14 Dec 2022 • Olga Graf, Pablo Flores, Pavlos Protopapas, Karim Pichara
Physics-Informed Neural Networks (PINNs) are gaining popularity as a method for solving differential equations.
no code implementations • NeurIPS Workshop DLDE 2021 • Olga Graf, Pablo Flores, Pavlos Protopapas, Karim Pichara
Uncertainty quantification (UQ) helps to make trustworthy predictions based on collected observations and uncertain domain knowledge.
no code implementations • 13 Apr 2020 • Felipe Rojas, Loïc Maurin, Rolando Dünner, Karim Pichara
Finally, we performed a cross-season test over 148 GHz data from 2009 and 2010 for which our model reaches a precision of 99. 8% and 99. 5%, respectively.
1 code implementation • 3 Feb 2020 • Ignacio Becker, Karim Pichara, Márcio Catelan, Pavlos Protopapas, Carlos Aguirre, Fatemeh Nikzat
Our method uses minimal data preprocessing, can be updated with a low computational cost for new observations and light curves, and can scale up to massive datasets.
1 code implementation • 4 Dec 2019 • Lukas Zorich, Karim Pichara, Pavlos Protopapas
Naively re-training from scratch is not an option in streaming settings, mainly because of the expensive pre-processing routines required to obtain a vector representation of light curves (features) each time we include new observations.
1 code implementation • 6 Nov 2019 • Javiera Astudillo, Pavlos Protopapas, Karim Pichara, Pablo Huijse
We propose a methodology in a probabilistic setting that determines a-priory which objects are worth taking spectrum to obtain better insights, where we focus 'insight' as the type of the object (classification).
no code implementations • 8 Mar 2019 • Christian Pieringer, Karim Pichara, Márcio Catelán, Pavlos Protopapas
Within the Machine Learning literature, dictionary-based methods have been widely used to encode relevant parts of image data.
BIG-bench Machine Learning Classification Of Variable Stars +3
1 code implementation • 2 Jan 2019 • Belen Saldias, Pavlos Protopapas, Karim Pichara
In this work, we provide a full probabilistic model for a shorter type of queries.
no code implementations • 21 Oct 2018 • Carlos Aguirre, Karim Pichara, Ignacio Becker
In this work, we present a novel Deep Learning model for light curve classification, mainly based on convolutional units.
1 code implementation • 29 Feb 2016 • Cristóbal Mackenzie, Karim Pichara, Pavlos Protopapas
Representatives of these patterns, called exemplars, are then used to transform lightcurves of a labeled set into a new representation that can then be used to train an automatic classifier.
no code implementations • 18 Apr 2014 • Isadora Nun, Karim Pichara, Pavlos Protopapas, Dae-Won Kim
With the aim of taking full advantage of all the information we have about known objects, our method is based on a supervised algorithm.
no code implementations • 29 Oct 2013 • Karim Pichara, Pavlos Protopapas
We present an automatic classification method for astronomical catalogs with missing data.
no code implementations • 1 Apr 2013 • Karim Pichara, Pavlos Protopapas, Dae-Won Kim, Jean-Baptiste Marquette, Patrick Tisserand
We present a new classification method for quasar identification in the EROS-2 and MACHO datasets based on a boosted version of Random Forest classifier.