OAUNI photometry of ASASSN-16hz
Descripción del Articulo
We report optical photometry of Type Ia SN ASASSN-16hz (=SN 2016eqb, ATel #9332, ATel #9333) on 2016-08-09 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.8" and airmass = 1.3. A total integration time of 900s (45x20s) and 880s...
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:20.500.12816/3331 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/3331 |
Nivel de acceso: | acceso abierto |
Materia: | Optical Supernovae Transient Stars Supernova Astronomical photometry http://purl.org/pe-repo/ocde/ford#1.03.08 |
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Pereyra, AntonioRicra, J.Zevallos, M.2018-11-06T13:05:56Z2018-11-06T13:05:56Z2016-12-07http://hdl.handle.net/20.500.12816/3331We report optical photometry of Type Ia SN ASASSN-16hz (=SN 2016eqb, ATel #9332, ATel #9333) on 2016-08-09 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.8" and airmass = 1.3. A total integration time of 900s (45x20s) and 880s (44x20s) in R and V filter, respectively, yielded: Date (UT) | filter | mag 2016-08-09.397 | R | 15.84 +/- 0.04 2016-08-09.412 | V | 15.82 +/- 0.05 UCAC4 field stars were used for the zero point calibration. Following Mayall/KOSMOS classification (ATel #9333), our measurements are ~2 days after 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/OpticalSupernovaeTransientStarsSupernovaAstronomical photometryhttp://purl.org/pe-repo/ocde/ford#1.03.08OAUNI photometry of ASASSN-16hzinfo:eu-repo/semantics/lecturereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel #9835.pdfATel #9835.pdfapplication/pdf183647https://repositorio.igp.gob.pe/bitstreams/f0cd3477-848b-4153-ad09-5cd0ded95a23/download66e7d0b6bd83eb687cd085e0fb825aadMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8393https://repositorio.igp.gob.pe/bitstreams/2e6bc2fe-e6ce-4bd2-9307-f2135712f2a4/downloadf6e2e38ecabbf5c802f4b273da8f9399MD52THUMBNAILATel #9835.pdf.jpgATel #9835.pdf.jpgIM Thumbnailimage/jpeg43853https://repositorio.igp.gob.pe/bitstreams/53c49809-00b0-4955-bbf1-0f975c5984c0/download80fd2e5f82e99949aa79e3569096d7caMD53TEXTATel #9835.pdf.txtATel #9835.pdf.txtExtracted texttext/plain2000https://repositorio.igp.gob.pe/bitstreams/c9bb38a6-8883-4bf0-b41b-1041c4c2f78e/downloadf72df83dcb748a11420e469db195c070MD5420.500.12816/3331oai:repositorio.igp.gob.pe:20.500.12816/33312020-12-17 10:19:50.668https://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-16hz |
title |
OAUNI photometry of ASASSN-16hz |
spellingShingle |
OAUNI photometry of ASASSN-16hz Pereyra, Antonio Optical Supernovae Transient Stars Supernova Astronomical photometry http://purl.org/pe-repo/ocde/ford#1.03.08 |
title_short |
OAUNI photometry of ASASSN-16hz |
title_full |
OAUNI photometry of ASASSN-16hz |
title_fullStr |
OAUNI photometry of ASASSN-16hz |
title_full_unstemmed |
OAUNI photometry of ASASSN-16hz |
title_sort |
OAUNI photometry of ASASSN-16hz |
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 Supernova Astronomical photometry |
topic |
Optical Supernovae Transient Stars Supernova Astronomical photometry 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-16hz (=SN 2016eqb, ATel #9332, ATel #9333) on 2016-08-09 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.8" and airmass = 1.3. A total integration time of 900s (45x20s) and 880s (44x20s) in R and V filter, respectively, yielded: Date (UT) | filter | mag 2016-08-09.397 | R | 15.84 +/- 0.04 2016-08-09.412 | V | 15.82 +/- 0.05 UCAC4 field stars were used for the zero point calibration. Following Mayall/KOSMOS classification (ATel #9333), our measurements are ~2 days after 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 |
2018-11-06T13:05:56Z |
dc.date.available.none.fl_str_mv |
2018-11-06T13:05:56Z |
dc.date.issued.fl_str_mv |
2016-12-07 |
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/20.500.12816/3331 |
url |
http://hdl.handle.net/20.500.12816/3331 |
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).