Short term period variable stars observed at OAUNI

TL;DR

This paper reports initial scientific findings from the OAUNI observatory on short-term period variable stars, including delta Scuti stars, eclipsing binaries, and cataclysmic variables, demonstrating high-quality light curves and satisfactory photometric precision.

Contribution

First scientific results from OAUNI on short-term variable stars, showcasing high-quality light curves and effective photometric precision in a Peruvian Andes observatory.

Findings

High-quality light curves of delta Scuti stars

Successful observation of eclipsing and cataclysmic binaries

Photometric precision meets initial expectations

Abstract

We present the first scientific results of the program on short term period variable stars observed using the OAUNI facility at the peruvian Andes. These results include good quality light curves of delta Scuti stars, rapidly oscillating stars along with eclipsing and cataclysmic binaries. The photometric precision reached by the available instrumental and equipment, and used in the several scientific subprograms, has satisfied the initial expectations.