OAUNI non-detection of AT 2023pow in R band
dc.contributor.author | Pereyra, Antonio | |
dc.contributor.author | Tello, J. | |
dc.contributor.author | Alvarado, D. | |
dc.contributor.author | Torre, E. | |
dc.contributor.author | Zevallos, M. | |
dc.contributor.author | Espinoza, M. | |
dc.contributor.author | de Almeida, L. | |
dc.date.accessioned | 2023-09-22T15:16:51Z | |
dc.date.available | 2023-09-22T15:16:51Z | |
dc.date.issued | 2023-08-23 | |
dc.description.abstract | CCD imaging was performed of the NGC 1640 field using the OAUNI 51cm telescope at Huancayo Observatory, Peru, on 2023-08-19.310 (UT). No source is detected at the position of AT 2023pow (TNSTR-2023-1982) with limiting magnitude R ~ 18.5. This is consistent with the AT 2023pow report by T. Noguchi few hours after the detection alert. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio133-2020 Fondecyt). | es_ES |
dc.format | application/pdf | es_ES |
dc.identifier.uri | http://hdl.handle.net/20.500.12816/5461 | |
dc.language.iso | eng | es_ES |
dc.publisher | R. E. Rutledge | es_ES |
dc.rights | info:eu-repo/semantics/openAccess | es_ES |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | es_ES |
dc.subject | Optical | es_ES |
dc.subject | Transient | es_ES |
dc.subject.ocde | http://purl.org/pe-repo/ocde/ford#1.03.08 | es_ES |
dc.title | OAUNI non-detection of AT 2023pow in R band | es_ES |
dc.type | info:eu-repo/semantics/report | es_ES |