activity
20172024
most citedObservations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

140 citations · 142 across the 6 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.IM2021

SCORPIO, a package for the visualization of galaxy pairs

Jose A. Benavides, Martín Chalela, Juan B. Cabral +2

We present the description of the project \texttt{SCORPIO}, a Python package for retrieving images and associated data of galaxy pairs based on their position, facilitating visual…

astro-ph.IM2021

Being nice to the server: Wrapping a REST API for a cosmological distance/velocity calculator with Python

Juan Cabral, Ehsan Kourkchi, Martin Beroiz +2

In this paper we present PyCF3, a python client for the cosmological distance-velocity calculator CosmicFlow-3. The project has a cache and retry system designed with the objective…

q-fin.PM2021

Evaluation of the importance of criteria for the selection of cryptocurrencies

Natalia A. Van Heerden, Juan B. Cabral, Nadia Luczywo

In recent years, cryptocurrencies have gone from an obscure niche to a prominent place, with investment in these assets becoming increasingly popular. However, cryptocurrencies car…

stat.CO20211 cited

Arby Fast data-driven surrogates

Aarón Villanueva, Martin Beroiz, Juan Cabral +2

The availability of fast to evaluate and reliable predictive models is highly relevant in multi-query scenarios where evaluating some quantities in real, or near-real-time becomes…

astro-ph.IM20211 cited

Drifting Features: Detection and evaluation in the context of automatic RRLs identification in VVV

J. B. Cabral, M. Lares, S. Gurovich +2

As most of the modern astronomical sky surveys produce data faster than humans can analyze it, Machine Learning (ML) has become a central tool in Astronomy. Modern ML methods can b…

astro-ph.EP2021

Easy asteroid phase curve fitting for the Python ecosystem: Pyedra

Milagros Colazo, Juan Cabral, Martin Chalela +1

A trending astronomical phenomenon to study is the variation in brightness of asteroids, caused by its rotation on its own axis, non-spherical shapes, changes of albedo along its s…