Seeing measurements at OAUNI on 2016 and 2017 campaigns

We present seeing measurements at OAUNI site gathered on 2016 and 2017 campaigns using V and R broadband filters. In order to quantify the seeing we used the full-width-at-half-maximum from stellar profiles on photometric sequences during the observational windows of our supernovae program. A typical median seeing of ${1}^{^{\prime\prime} }.8$ was found on 2016 and a worst value of ${2}^{^{\prime\prime} }.0$ on 2017. The last one was probably affected by anomalous conditions related to the 2017 extreme climatic event. The monthly first quartile analysis indicates that best seeing conditions can be achieved at a level of ${1}^{^{\prime\prime} }.5$ . In general, our results indicate a reasonable sky quality for the OAUNI site.