OAUNI photometry of SN2017gmr/DLT17cq

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Optical photometry of Type II SN2017gmr/DLT17cq (ATel #10706, ATel #10717, TNSCR 2017-1220) on 2017-09-19.207 (UT) was gathered using the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed in R band with seeing ~1.5" and airmass = 1.3. A total integration time of 55x2...

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Detalles Bibliográficos
Autores: Pereyra, Antonio, Ricra, J.
Formato: ponencia
Fecha de Publicación:2017
Institución:Consejo Nacional de Ciencia Tecnología e Innovación
Repositorio:CONCYTEC-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.concytec.gob.pe:20.500.12390/828
Enlace del recurso:https://hdl.handle.net/20.500.12390/828
Nivel de acceso:acceso abierto
Materia:Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
http://purl.org/pe-repo/ocde/ford#1.03.08
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spelling Publicationrp02114600rp02138600Pereyra, AntonioRicra, J.2024-05-30T23:13:38Z2024-05-30T23:13:38Z2017-12-22https://hdl.handle.net/20.500.12390/828Optical photometry of Type II SN2017gmr/DLT17cq (ATel #10706, ATel #10717, TNSCR 2017-1220) on 2017-09-19.207 (UT) was gathered using the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed in R band with seeing ~1.5" and airmass = 1.3. A total integration time of 55x20s=1100s yielded R = (14.05 +/- 0.04) mag. NOMAD field stars were used for the zero point calibration. 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-1http://purl.org/pe-repo/ocde/ford#1.03.08-1OAUNI photometry of SN2017gmr/DLT17cqinfo:eu-repo/semantics/lecturereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC20.500.12390/828oai:repositorio.concytec.gob.pe:20.500.12390/8282024-05-30 15:59:16.214https://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#<Publication xmlns="https://www.openaire.eu/cerif-profile/1.1/" id="2a313350-5ef2-42fe-a0d9-746d018ccd1d"> <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 SN2017gmr/DLT17cq</Title> <PublishedIn> <Publication> </Publication> </PublishedIn> <PublicationDate>2017-12-22</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> </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>Optical photometry of Type II SN2017gmr/DLT17cq (ATel #10706, ATel #10717, TNSCR 2017-1220) on 2017-09-19.207 (UT) was gathered using the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed in R band with seeing ~1.5&quot; and airmass = 1.3. A total integration time of 55x20s=1100s yielded R = (14.05 +/- 0.04) mag. NOMAD field stars were used for the zero point calibration. The OAUNI project is supported by UNI, TWAS, IGP and Cienciactiva (Convenio 102-2015 Fondecyt).</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1
dc.title.none.fl_str_mv OAUNI photometry of SN2017gmr/DLT17cq
title OAUNI photometry of SN2017gmr/DLT17cq
spellingShingle OAUNI photometry of SN2017gmr/DLT17cq
Pereyra, Antonio
Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
http://purl.org/pe-repo/ocde/ford#1.03.08
title_short OAUNI photometry of SN2017gmr/DLT17cq
title_full OAUNI photometry of SN2017gmr/DLT17cq
title_fullStr OAUNI photometry of SN2017gmr/DLT17cq
title_full_unstemmed OAUNI photometry of SN2017gmr/DLT17cq
title_sort OAUNI photometry of SN2017gmr/DLT17cq
author Pereyra, Antonio
author_facet Pereyra, Antonio
Ricra, J.
author_role author
author2 Ricra, J.
author2_role author
dc.contributor.author.fl_str_mv Pereyra, Antonio
Ricra, J.
dc.subject.none.fl_str_mv Supernova
topic Supernova
Estrellas
Fotometría astronómica
Óptica
info:eu-repo/semantics/lecture
http://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 http://purl.org/pe-repo/ocde/ford#1.03.08
description Optical photometry of Type II SN2017gmr/DLT17cq (ATel #10706, ATel #10717, TNSCR 2017-1220) on 2017-09-19.207 (UT) was gathered using the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed in R band with seeing ~1.5" and airmass = 1.3. A total integration time of 55x20s=1100s yielded R = (14.05 +/- 0.04) mag. NOMAD field stars were used for the zero point calibration. The OAUNI project is supported by UNI, TWAS, IGP and Cienciactiva (Convenio 102-2015 Fondecyt).
publishDate 2017
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 2017-12-22
dc.type.none.fl_str_mv info:eu-repo/semantics/lecture
format lecture
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/828
url https://hdl.handle.net/20.500.12390/828
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
_version_ 1844883068813312000
score 13.390007
OAUNI photometry of SN2017gmr/DLT17cq
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).

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