OAUNI photometry of SN 2023mkt

Descripción del Articulo

We report photometry of Type Ia SN 2023mkt gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under non-photometric conditions with an airmass lower than 1.7. The integration time was 90x20s=1800s in both nights. Our...

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Detalles Bibliográficos
Autores: Pereyra, Antonio, Tello, J., Alvarado, D., Torre, E., Zevallos, M., de Almeida, L.
Formato: informe técnico
Fecha de Publicación:2023
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5492
Enlace del recurso:http://hdl.handle.net/20.500.12816/5492
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 2023mkt
title OAUNI photometry of SN 2023mkt
spellingShingle OAUNI photometry of SN 2023mkt
Pereyra, Antonio
Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
title_short OAUNI photometry of SN 2023mkt
title_full OAUNI photometry of SN 2023mkt
title_fullStr OAUNI photometry of SN 2023mkt
title_full_unstemmed OAUNI photometry of SN 2023mkt
title_sort OAUNI photometry of SN 2023mkt
author Pereyra, Antonio
author_facet Pereyra, Antonio
Tello, J.
Alvarado, D.
Torre, E.
Zevallos, M.
de Almeida, L.
author_role author
author2 Tello, J.
Alvarado, D.
Torre, E.
Zevallos, M.
de Almeida, L.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Pereyra, Antonio
Tello, J.
Alvarado, D.
Torre, E.
Zevallos, M.
de Almeida, L.
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 Ia SN 2023mkt gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under non-photometric conditions with an airmass lower than 1.7. The integration time was 90x20s=1800s in both nights. Our measurements are indicated below: Date (UT) | filter |seeing (") | mag, 2023-08-18.082 | R | 2.1 | 16.02 +/- 0.01, 2023-08-19.079 | R | 2.4 |16.05 +/- 0.01. UCAC4 field stars were used for the zero point calibration. Our observations are ~6 weeks after SN 2023mkt discovery date. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).
publishDate 2023
dc.date.accessioned.none.fl_str_mv 2023-11-27T19:00:54Z
dc.date.available.none.fl_str_mv 2023-11-27T19:00:54Z
dc.date.issued.fl_str_mv 2023-09-07
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/20.500.12816/5492
url http://hdl.handle.net/20.500.12816/5492
dc.language.iso.es_ES.fl_str_mv eng
language eng
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, AntonioTello, J.Alvarado, D.Torre, E.Zevallos, M.de Almeida, L.2023-11-27T19:00:54Z2023-11-27T19:00:54Z2023-09-07http://hdl.handle.net/20.500.12816/5492We report photometry of Type Ia SN 2023mkt gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under non-photometric conditions with an airmass lower than 1.7. The integration time was 90x20s=1800s in both nights. Our measurements are indicated below: Date (UT) | filter |seeing (") | mag, 2023-08-18.082 | R | 2.1 | 16.02 +/- 0.01, 2023-08-19.079 | R | 2.4 |16.05 +/- 0.01. UCAC4 field stars were used for the zero point calibration. Our observations are ~6 weeks after SN 2023mkt discovery date. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).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/pdfengR. 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 2023mktinfo:eu-repo/semantics/reportreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel-16234.pdfATel-16234.pdfapplication/pdf342841https://repositorio.igp.gob.pe/bitstreams/3ca77932-93cf-429e-bbef-9f671da56bb7/download6c3d6280506bb593ca77f9d23efebd42MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/8bb0c1a9-ed37-43eb-8881-078c97a83d10/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTATel-16234.pdf.txtATel-16234.pdf.txtExtracted texttext/plain1349https://repositorio.igp.gob.pe/bitstreams/dbb779ae-63a4-41fe-ac7c-714217f73e13/download4f5c4f27a103a14c4e253fff717b3b74MD53THUMBNAILATel-16234.pdf.jpgATel-16234.pdf.jpgIM Thumbnailimage/jpeg56809https://repositorio.igp.gob.pe/bitstreams/b7c6e603-8d59-47cd-8237-5ba0375a41e6/download41ccbddc432e199b7f855d6954254d64MD5420.500.12816/5492oai:repositorio.igp.gob.pe:20.500.12816/54922025-09-25 10:29:43.413https://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 2023mkt
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