OAUNI photometry of SN 2025qpk

dc.contributor.authorPereyra, Antonio
dc.date.accessioned2025-08-27T14:31:58Z
dc.date.available2025-08-27T14:31:58Z
dc.date.issued2025-08-13
dc.description.abstractWe report photometry of Type Ia SN 2025qpk gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under nonphotometric conditions with airmasses lower than 1.3. The integration time was 60x20s=1200s for all observations. Our measurements yielded: Date (UT) | filter | seeing (") | mag, 2025-07-24.333 | R | 1.8 | 14.56 +/- 0.01, 2025-07-25.138 | R | 2.3 | 14.49 +/- 0.01. UCAC4 field stars were used for the zero point calibration. Our observations are ~17 days after the discovery (TNSTR-2025-2620). The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).
dc.description.sponsorshipEl proyecto OAUNI cuenta con el apoyo de UNI, TWAS, IGP y ProCiencia-Concytec [Convenio 133-2020 Fondecyt].
dc.formatapplication/pdf
dc.identifier.journalThe Astronomer's Telegram
dc.identifier.urihttp://hdl.handle.net/20.500.12816/5736
dc.language.isoeng
dc.publisherR. E. Rutledge
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectOptical
dc.subjectSupernovae
dc.subjectTransient
dc.subject.ocdehttps://purl.org/pe-repo/ocde/ford#1.03.08
dc.titleOAUNI photometry of SN 2025qpk
dc.typeinfo:eu-repo/semantics/report

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