no code implementations • 2 May 2022 • C. Donoso-Oliva, I. Becker, P. Protopapas, G. Cabrera-Vives, Vishnu M., Harsh Vardhan
We used millions of R-band light sequences to adjust the ASTROMER weights.
1 code implementation • 7 Jun 2021 • C. Donoso-Oliva, G. Cabrera-Vives, P. Protopapas, R. Carrasco-Davis, P. A. Estevez
In this work, we study the effectiveness of the LSTM and Phased LSTM based architectures for the classification of astronomical lightcurves.
2 code implementations • 7 Aug 2020 • P. Sánchez-Sáez, I. Reyes, C. Valenzuela, F. Förster, S. Eyheramendy, F. Elorrieta, F. E. Bauer, G. Cabrera-Vives, P. A. Estévez, M. Catelan, G. Pignata, P. Huijse, D. De Cicco, P. Arévalo, R. Carrasco-Davis, J. Abril, R. Kurtev, J. Borissova, J. Arredondo, E. Castillo-Navarrete, D. Rodriguez, D. Ruz-Mieres, A. Moya, L. Sabatini-Gacitúa, C. Sepúlveda-Cobo
The ALeRCE light curve classifier uses variability features computed from the ZTF alert stream, and colors obtained from AllWISE and ZTF photometry.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena Solar and Stellar Astrophysics