51 citations · 116 across the 7 of their papers we have counts for
7 papers
On the performance of pre-trained vision transformers for supernova spectral classification using different spectral representations
J. Serrano Bell, P. Gálvez Molina, V. Contreras Rojas +4
The spectroscopic classification of supernovae is a key component of time-domain astronomy and plays an important role in the identification of Type Ia events. The increasing volum…
ABC-SN: Attention Based Classifier for Supernova Spectra
Willow Fox Fortino, Federica B. Bianco, Pavlos Protopapas +2
While significant advances have been made in photometric classification ahead of the millions of transient events and hundreds of supernovae (SNe) each night that the Vera C. Rubin…
The TAOS Project: Results From Seven Years of Survey Data
Z. -W. Zhang, M. J. Lehner, J. -H. Wang +19
The Taiwanese-American Occultation Survey (TAOS) aims to detect serendipitous occultations of stars by small (about 1 km diameter) objects in the Kuiper Belt and beyond. Such event…
The TAOS Project Stellar Variability II. Detection of 15 Variable Stars
S. Mondal, C. C. Lin, W. P. Chen +20
The Taiwanese-American Occultation Survey (TAOS) project has collected more than a billion photometric measurements since 2005 January. These sky survey data-covering timescales fr…
The TAOS Project: Statistical Analysis of Multi-Telescope Time Series Data
M. J. Lehner, N. K. Coehlo, Z. -W. Zhang +17
The Taiwanese-American Occultation Survey (TAOS) monitors fields of up to ~1000 stars at 5 Hz simultaneously with four small telescopes to detect occultation events from small (~1…
Upper Limits on the Number of Small Bodies in Sedna-Like Orbits by the TAOS Project
J. -H. Wang, M. J. Lehner, Z. -W. Zhang +21
We present the results of a search for occultation events by objects at distances between 100 and 1000 AU in lightcurves from the Taiwanese-American Occultation Survey (TAOS). We s…
First Results From The Taiwanese-American Occultation Survey (TAOS)
Z. -W. Zhang, F. B. Bianco, M. J. Lehner +22
Results from the first two years of data from the Taiwanese-American Occultation Survey (TAOS) are presented. Stars have been monitored photometrically at 4 Hz or 5 Hz to search fo…