OAUNI photometry of ASASSN-16hz

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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...

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Detalles Bibliográficos
Autores: Pereyra, Antonio, Ricra, J., Zevallos, M.
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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spelling 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
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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 reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
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reponame_str IGP-Institucional
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