OAUNI photometry of SN 2023ixf

Descripción del Articulo

We report photometry of Type II SN 2023ixf gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two epochs under stable conditions (seeing ~1.7") and airmass lower than 2.5 (target with low altitude). Our integration times were 54x20s=10...

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Detalles Bibliográficos
Autores: Pereyra, Antonio, Espinoza, M., Tello, J., Zevallos, M., de Almeida, L., Torre, E.
Formato: informe técnico
Fecha de Publicación:2023
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:español
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5421
Enlace del recurso:http://hdl.handle.net/20.500.12816/5421
Nivel de acceso:acceso abierto
Materia:Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
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dc.title.es_ES.fl_str_mv OAUNI photometry of SN 2023ixf
title OAUNI photometry of SN 2023ixf
spellingShingle OAUNI photometry of SN 2023ixf
Pereyra, Antonio
Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
title_short OAUNI photometry of SN 2023ixf
title_full OAUNI photometry of SN 2023ixf
title_fullStr OAUNI photometry of SN 2023ixf
title_full_unstemmed OAUNI photometry of SN 2023ixf
title_sort OAUNI photometry of SN 2023ixf
author Pereyra, Antonio
author_facet Pereyra, Antonio
Espinoza, M.
Tello, J.
Zevallos, M.
de Almeida, L.
Torre, E.
author_role author
author2 Espinoza, M.
Tello, J.
Zevallos, M.
de Almeida, L.
Torre, E.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Pereyra, Antonio
Espinoza, M.
Tello, J.
Zevallos, M.
de Almeida, L.
Torre, E.
dc.subject.es_ES.fl_str_mv Optical
Supernovae
Transient
topic Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
dc.subject.ocde.es_ES.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.03.08
description We report photometry of Type II SN 2023ixf gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two epochs under stable conditions (seeing ~1.7") and airmass lower than 2.5 (target with low altitude). Our integration times were 54x20s=1080s and 50x20s=1000s on 2023-06-20 and 2023-06-21, respectively. Our measurements yielded: on (UT) 2023-06-20.021, R = 11.28 +/- 0.02, and, on (UT) 2023-06-21.022, R = 11.30 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our observations are ~32-33 days after the earliest detection.
publishDate 2023
dc.date.accessioned.none.fl_str_mv 2023-07-04T22:44:03Z
dc.date.available.none.fl_str_mv 2023-07-04T22:44:03Z
dc.date.issued.fl_str_mv 2023-06-27
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/report
format report
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/5421
url http://hdl.handle.net/20.500.12816/5421
dc.language.iso.es_ES.fl_str_mv spa
language spa
dc.rights.es_ES.fl_str_mv info:eu-repo/semantics/openAccess
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eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv R. E. Rutledge
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Pereyra, AntonioEspinoza, M.Tello, J.Zevallos, M.de Almeida, L.Torre, E.2023-07-04T22:44:03Z2023-07-04T22:44:03Z2023-06-27http://hdl.handle.net/20.500.12816/5421We report photometry of Type II SN 2023ixf gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two epochs under stable conditions (seeing ~1.7") and airmass lower than 2.5 (target with low altitude). Our integration times were 54x20s=1080s and 50x20s=1000s on 2023-06-20 and 2023-06-21, respectively. Our measurements yielded: on (UT) 2023-06-20.021, R = 11.28 +/- 0.02, and, on (UT) 2023-06-21.022, R = 11.30 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our observations are ~32-33 days after the earliest detection.Este trabajo fue financiado por el Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica (Fondecyt - Perú) en el marco del proyecto OAUNI [número de contrato 133-2020].application/pdfspaR. E. Rutledgeinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/OpticalSupernovaeTransienthttp://purl.org/pe-repo/ocde/ford#1.03.08OAUNI photometry of SN 2023ixfinfo:eu-repo/semantics/reportreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel-16098.pdfATel-16098.pdfapplication/pdf46483https://repositorio.igp.gob.pe/bitstreams/9d3e94ec-1b1a-44c1-8c2c-ded68b51fab4/downloadbef6464339d638c770da730f9cfb7a0fMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/d187a46f-eb5f-4472-88bb-ef3f2ab60931/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTATel-16098.pdf.txtATel-16098.pdf.txtExtracted texttext/plain1572https://repositorio.igp.gob.pe/bitstreams/bdd7c3a3-eeb6-4cae-bf0c-28fc90843e88/download04faac64badfc38722fdd15235d237bfMD53THUMBNAILATel-16098.pdf.jpgATel-16098.pdf.jpgIM Thumbnailimage/jpeg59931https://repositorio.igp.gob.pe/bitstreams/c2098f3a-8b3f-4a77-b97c-3a439b91a658/download7162bd56153ce432ec81f9f2f2e62e1fMD5420.500.12816/5421oai:repositorio.igp.gob.pe:20.500.12816/54212025-09-25 10:34:08.973https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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OAUNI photometry of SN 2023ixf
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