Muestra métricas de impacto externas asociadas a la publicación. Para mayor detalle:
| Indexado |
|
||||
| DOI | 10.1016/J.ASCOM.2023.100694 | ||||
| Año | 2023 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In recent decades, machine learning has provided valuable models and algorithms for processing and extracting knowledge from time-series surveys. Different classifiers have been proposed and performed to an excellent standard. Nevertheless, few papers have tackled the data shift problem in labeled training sets, which occurs when there is a mismatch between the data distribution in the training set and the testing set. This drawback can damage the prediction performance in unseen data. 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. We collect ranges for characteristic features to construct a symbolic representation of prior knowledge, which was used to model the informative regularizer component. Simultaneously, we design a two-step back-propagation algorithm to integrate this knowledge into the neural network, whereby one step is applied in each epoch to minimize classification error, while another is applied to ensure regularization. Our algorithm defines a subset of parameters (a mask) for each loss function. This approach handles the forgetting effect, which stems from a trade-off between these loss functions (learning from data versus learning expert knowledge) during training. Experiments were conducted using recently proposed shifted benchmark sets for RR Lyrae stars, outperforming baseline models by up to 3% through a more reliable classifier. Our method provides a new path to incorporate knowledge from characteristic features into artificial neural networks to manage the underlying data shift problem.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Perez-Galarce, Francisco | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| 2 | Pichara, Karim E. | Hombre |
Pontificia Universidad Católica de Chile - Chile
Instituto Milenio de Astrofísica - Chile |
| 3 | Huijse, P. | Hombre |
Instituto Milenio de Astrofísica - Chile
Universidad Austral de Chile - Chile |
| 4 | Catelan, Marcio | Hombre |
Instituto Milenio de Astrofísica - Chile
Pontificia Universidad Católica de Chile - Chile |
| 5 | MERY-QUIROZ, DOMINGO | Hombre |
Pontificia Universidad Católica de Chile - Chile
|
| Fuente |
|---|
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Proyecto Basal |
| ANID |
| Agencia Nacional de Investigación y Desarrollo |
| ANID's Millennium Science Initiative |
| Agenția Națională pentru Cercetare și Dezvoltare |
| CENIA |
| National Center for Artificial Intelligence |
| ANID, through FONDECYT |
| National Center for Artificial Intelligence (CENIA) Proyecto Basal |
| National Agency for Research and Development (ANID) , through the FONDECYT |
| Agradecimiento |
|---|
| The authors would like to acknowledge the support from the National Agency for Research and Development (ANID) , through the FONDECYT Regular project number 1180054. F. Pérez-Galarce acknowledges support from ANID , through Scholarship Program/ Doctorado Nacional/2017-21171036. P.H. acknowledges support from ANID , through FONDECYT regular 1211374 . Support for M.C. is provided by ANID’s Millennium Science Initiative through grant ICN12_12009 , awarded to the Millennium Institute of Astrophysics (MAS), and by Proyecto Basal FB210003. D. Mery acknowledges support from National Center for Artificial Intelligence (CENIA) Proyecto Basal FB210017. |
| The authors would like to acknowledge the support from the National Agency for Research and Development (ANID) , through the FONDECYT Regular project number 1180054. F. Perez-Galarce acknowledges support from ANID, through Scholarship Program/Doctorado Nacional/2017-21171036. P.H. acknowledges support from ANID, through FONDECYT regular 1211374. Support for M.C. is provided by ANID's Millennium Science Initiative through grant ICN12_12009, awarded to the Millennium Institute of Astrophysics (MAS) , and by Proyecto Basal FB210003. D. Mery acknowledges support from National Center for Artificial Intelligence (CENIA) Proyecto Basal FB210017. |