OAUNI photometry of ASASSN-16hw
Descripción del Articulo
We report optical photometry of Type Ia SN ASASSN-16hw (=SN 2016ekt, ATel #9278, ATel #9289, ATel #9300) on 2016-08-06 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015;arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging measurements using V and R broadband filters were acqui...
Autores: | , , |
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Formato: | ponencia |
Fecha de Publicación: | 2016 |
Institución: | Instituto Geofísico del Perú |
Repositorio: | IGP-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/3333 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/3333 |
Nivel de acceso: | acceso abierto |
Materia: | Optical Supernovae Transient Stars Astronomical photometry Supernova http://purl.org/pe-repo/ocde/ford#1.03.08 |
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Pereyra, AntonioRicra, J.Zevallos, M.2018-11-06T13:13:34Z2018-11-06T13:13:34Z2016-09-30http://hdl.handle.net/20.500.12816/3333We report optical photometry of Type Ia SN ASASSN-16hw (=SN 2016ekt, ATel #9278, ATel #9289, ATel #9300) on 2016-08-06 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015;arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging measurements using V and R broadband filters were acquired with seeing ~1.9" and airmass = 1.5. A total integration time of 42x20s=840s in each filter yielded: Date (UT) filter mag 2016-08-06.119 R 14.656 +/- 0.003 2016-08-06.120 V 14.497 +/- 0.004 Field stars were used for the zero point calibration. Following PESSTO and Du Pont classifications (ATel #9289, ATel #9300), our measurements are very close to maximum. The OAUNI project is supported by UNI, TWAS, IGP and Cienciactiva (Convenio 102-2015 Fondecyt).application/pdfengThe Astronomer's Telegraminfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/OpticalSupernovaeTransientStarsAstronomical photometrySupernovahttp://purl.org/pe-repo/ocde/ford#1.03.08OAUNI photometry of ASASSN-16hwinfo:eu-repo/semantics/lecturereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel #9577.pdfATel #9577.pdfapplication/pdf167164https://repositorio.igp.gob.pe/bitstreams/5a4be1c5-d505-4b6d-8943-0562384c1b07/downloadf2149ad458e5940701678c97995124cfMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8393https://repositorio.igp.gob.pe/bitstreams/27471472-4b25-43ac-8718-821dfed7aba7/downloadf6e2e38ecabbf5c802f4b273da8f9399MD52THUMBNAILATel #9577.pdf.jpgATel #9577.pdf.jpgIM Thumbnailimage/jpeg47343https://repositorio.igp.gob.pe/bitstreams/59c1d29f-4bb9-4ce2-9487-a0f13ca598ab/download5155552581c0296f89b45a37abad7a47MD53TEXTATel #9577.pdf.txtATel #9577.pdf.txtExtracted texttext/plain2422https://repositorio.igp.gob.pe/bitstreams/3a19b3fd-77a2-41b8-91b3-cec377ec3781/download970954f227e2d11032c4ad942ea0e951MD5420.500.12816/3333oai:repositorio.igp.gob.pe:20.500.12816/33332020-12-17 10:19:50.649https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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 |
dc.title.es_ES.fl_str_mv |
OAUNI photometry of ASASSN-16hw |
title |
OAUNI photometry of ASASSN-16hw |
spellingShingle |
OAUNI photometry of ASASSN-16hw Pereyra, Antonio Optical Supernovae Transient Stars Astronomical photometry Supernova http://purl.org/pe-repo/ocde/ford#1.03.08 |
title_short |
OAUNI photometry of ASASSN-16hw |
title_full |
OAUNI photometry of ASASSN-16hw |
title_fullStr |
OAUNI photometry of ASASSN-16hw |
title_full_unstemmed |
OAUNI photometry of ASASSN-16hw |
title_sort |
OAUNI photometry of ASASSN-16hw |
author |
Pereyra, Antonio |
author_facet |
Pereyra, Antonio Ricra, J. Zevallos, M. |
author_role |
author |
author2 |
Ricra, J. Zevallos, M. |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Pereyra, Antonio Ricra, J. Zevallos, M. |
dc.subject.es_ES.fl_str_mv |
Optical Supernovae Transient Stars Astronomical photometry Supernova |
topic |
Optical Supernovae Transient Stars Astronomical photometry Supernova 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 optical photometry of Type Ia SN ASASSN-16hw (=SN 2016ekt, ATel #9278, ATel #9289, ATel #9300) on 2016-08-06 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015;arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging measurements using V and R broadband filters were acquired with seeing ~1.9" and airmass = 1.5. A total integration time of 42x20s=840s in each filter yielded: Date (UT) filter mag 2016-08-06.119 R 14.656 +/- 0.003 2016-08-06.120 V 14.497 +/- 0.004 Field stars were used for the zero point calibration. Following PESSTO and Du Pont classifications (ATel #9289, ATel #9300), our measurements are very close to maximum. The OAUNI project is supported by UNI, TWAS, IGP and Cienciactiva (Convenio 102-2015 Fondecyt). |
publishDate |
2016 |
dc.date.accessioned.none.fl_str_mv |
2018-11-06T13:13:34Z |
dc.date.available.none.fl_str_mv |
2018-11-06T13:13:34Z |
dc.date.issued.fl_str_mv |
2016-09-30 |
dc.type.es_ES.fl_str_mv |
info:eu-repo/semantics/lecture |
format |
lecture |
dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/3333 |
url |
http://hdl.handle.net/20.500.12816/3333 |
dc.language.iso.es_ES.fl_str_mv |
eng |
language |
eng |
dc.rights.es_ES.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.uri.es_ES.fl_str_mv |
https://creativecommons.org/licences/by/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licences/by/4.0/ |
dc.format.es_ES.fl_str_mv |
application/pdf |
dc.publisher.es_ES.fl_str_mv |
The Astronomer's Telegram |
dc.source.none.fl_str_mv |
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Instituto Geofísico del Perú |
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IGP-Institucional |
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Nota importante:
La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).
La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).