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.