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:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3317
Enlace del recurso:http://hdl.handle.net/20.500.12816/3317
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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dc.title.es_ES.fl_str_mv OAUNI photometry of SN2017gmr/DLT17cq
title OAUNI photometry of SN2017gmr/DLT17cq
spellingShingle OAUNI photometry of SN2017gmr/DLT17cq
Pereyra, Antonio
Optical
Supernovae
Transient
Stars
Astronomical photometry
Supernova
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.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 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 2018-11-06T11:21:49Z
dc.date.available.none.fl_str_mv 2018-11-06T11:21:49Z
dc.date.issued.fl_str_mv 2017-12-22
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/20.500.12816/3317
url http://hdl.handle.net/20.500.12816/3317
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
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dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv The Astronomer's Telegram
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instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Pereyra, AntonioRicra, J.2018-11-06T11:21:49Z2018-11-06T11:21:49Z2017-12-22http://hdl.handle.net/20.500.12816/3317Optical 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).Este trabajo fue financiado por el Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica (Fondecyt - Perú) en el marco del proyecto Observaciones Astronómicas de Precisión con Telescopio Robótico en el Observatorio de Huancayo [número de contrato 102-2015].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 SN2017gmr/DLT17cqinfo:eu-repo/semantics/lecturereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel #11083.pdfATel #11083.pdfapplication/pdf159497https://repositorio.igp.gob.pe/bitstreams/8cd90953-0a46-4739-aa3c-c0f678ff9963/download945864cfcde5d9cada4a2563c86a7e67MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/252fc5a7-c5cc-44a6-a017-c962ce7653da/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILATel #11083.pdf.jpgATel #11083.pdf.jpgIM Thumbnailimage/jpeg39158https://repositorio.igp.gob.pe/bitstreams/79211d47-e496-4918-8b5f-8883c551f2dc/download4998363fcfb19c13e466e83692a5be49MD53TEXTATel #11083.pdf.txtATel #11083.pdf.txtExtracted texttext/plain1697https://repositorio.igp.gob.pe/bitstreams/e25093e4-39a0-492f-849d-894b21f0c976/download1ef4ce6fe1b11b324e5c61e9eb974111MD5420.500.12816/3317oai:repositorio.igp.gob.pe:20.500.12816/33172025-09-25 11:25:32.68https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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OAUNI photometry of SN2017gmr/DLT17cq
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