Seeing measurements at OAUNI on 2016 and 2017 campaigns

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dc.contributor.authorPereyra, Antonio
dc.contributor.authorTello, J.
dc.contributor.authorZevallos, M.
dc.date.accessioned2022-11-23T16:53:33Z
dc.date.available2022-11-23T16:53:33Z
dc.date.issued2022
dc.description.abstractWe 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” .8 was found on 2016 and a worst value of 2” .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” .5. In general, our results indicate a reasonable sky quality for the OAUNI site.es_ES
dc.description.peer-reviewPor pareses_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationPereyra, A., Tello, J. & Zevallos, M. (2022). Seeing measurements at OAUNI on 2016 and 2017 campaigns.==$Journal of Physics: Conference Series, 2372,$==012001. https://doi.org/10.1088/1742-6596/2372/1/012001es_ES
dc.identifier.doihttps://doi.org/10.1088/1742-6596/2372/1/012001es_ES
dc.identifier.govdocindex-oti2018
dc.identifier.journalJournal of Physics: Conference Serieses_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/5320
dc.language.isoenges_ES
dc.publisherIOP Publishinges_ES
dc.relation.ispartofurn:issn:1742-6596
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es_ES
dc.subjectSeeinges_ES
dc.subjectSite testinges_ES
dc.subjectAstronomical observatoryes_ES
dc.subject.ocdehttps://purl.org/pe-repo/ocde/ford#1.03.00es_ES
dc.titleSeeing measurements at OAUNI on 2016 and 2017 campaignses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES

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