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:Consejo Nacional de Ciencia Tecnología e Innovación
Repositorio:CONCYTEC-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.concytec.gob.pe:20.500.12390/830
Enlace del recurso:https://hdl.handle.net/20.500.12390/830
Nivel de acceso:acceso abierto
Materia:Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
https://purl.org/pe-repo/ocde/ford#1.03.08
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spelling Publicationrp02114600rp02138600rp02139600Pereyra, AntonioRicra, J.Zevallos, M.2024-05-30T23:13:38Z2024-05-30T23:13:38Z2016-12-07https://hdl.handle.net/20.500.12390/830We 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)filtermag 2016-08-09.397R15.84 +/- 0.04 2016-08-09.412V15.82 +/- 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)."Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - ConcytecengThe Astronomer's Telegraminfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/SupernovaEstrellas-1Fotometría astronómica-1Óptica-1info:eu-repo/semantics/lecture-1https://purl.org/pe-repo/ocde/ford#1.03.08-1OAUNI photometry of ASASSN-16hzinfo:eu-repo/semantics/lecturereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC20.500.12390/830oai:repositorio.concytec.gob.pe:20.500.12390/8302024-05-30 15:59:17.648https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only accesshttps://repositorio.concytec.gob.peRepositorio Institucional CONCYTECrepositorio@concytec.gob.pe#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#<Publication xmlns="https://www.openaire.eu/cerif-profile/1.1/" id="4463c7a2-9626-4a8c-b364-3111db31bc4d"> <Type xmlns="https://www.openaire.eu/cerif-profile/vocab/COAR_Publication_Types">http://purl.org/coar/resource_type/c_1843</Type> <Language>eng</Language> <Title>OAUNI photometry of ASASSN-16hz</Title> <PublishedIn> <Publication> </Publication> </PublishedIn> <PublicationDate>2016-12-07</PublicationDate> <Authors> <Author> <DisplayName>Pereyra, Antonio</DisplayName> <Person id="rp02114" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Ricra, J.</DisplayName> <Person id="rp02138" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Zevallos, M.</DisplayName> <Person id="rp02139" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> </Authors> <Editors> </Editors> <Publishers> <Publisher> <DisplayName>The Astronomer&apos;s Telegram</DisplayName> <OrgUnit /> </Publisher> </Publishers> <License>https://creativecommons.org/licenses/by-nc-nd/4.0/</License> <Keyword>Supernova</Keyword> <Keyword>Estrellas</Keyword> <Keyword>Fotometría astronómica</Keyword> <Keyword>Óptica</Keyword> <Keyword>info:eu-repo/semantics/lecture</Keyword> <Abstract>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&quot; and airmass = 1.3. A total integration time of 900s (45x20s) and 880s (44x20s) in R and V filter, respectively, yielded: Date (UT)</Abstract> <Abstract>filter</Abstract> <Abstract>mag 2016-08-09.397</Abstract> <Abstract>R</Abstract> <Abstract>15.84 +/- 0.04 2016-08-09.412</Abstract> <Abstract>V</Abstract> <Abstract>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).&quot;</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1
dc.title.none.fl_str_mv OAUNI photometry of ASASSN-16hz
title OAUNI photometry of ASASSN-16hz
spellingShingle OAUNI photometry of ASASSN-16hz
Pereyra, Antonio
Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
https://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.none.fl_str_mv Supernova
topic Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
https://purl.org/pe-repo/ocde/ford#1.03.08
dc.subject.es_PE.fl_str_mv Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
dc.subject.ocde.none.fl_str_mv https://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)
publishDate 2016
dc.date.accessioned.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.available.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.issued.fl_str_mv 2016-12-07
dc.type.none.fl_str_mv info:eu-repo/semantics/lecture
format lecture
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/830
url https://hdl.handle.net/20.500.12390/830
dc.language.iso.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.none.fl_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
dc.publisher.none.fl_str_mv The Astronomer's Telegram
publisher.none.fl_str_mv The Astronomer's Telegram
dc.source.none.fl_str_mv reponame:CONCYTEC-Institucional
instname:Consejo Nacional de Ciencia Tecnología e Innovación
instacron:CONCYTEC
instname_str Consejo Nacional de Ciencia Tecnología e Innovación
instacron_str CONCYTEC
institution CONCYTEC
reponame_str CONCYTEC-Institucional
collection CONCYTEC-Institucional
repository.name.fl_str_mv Repositorio Institucional CONCYTEC
repository.mail.fl_str_mv repositorio@concytec.gob.pe
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score 13.263243
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