OAUNI multiband photometry of SN2022hrs

Descripción del Articulo

We report multiband photometry of Type Ia SN2022hrs (TNSTR-2022-994, TNSCR-2022- 997) on 2022-05-02 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015; arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging using BVRI filters was performed under non-photometric conditions (seeing...

Descripción completa

Detalles Bibliográficos
Autores: Pereyra, Antonio, Tello, J., Zeballos, M., de Almeida, L., Espinoza, M., Alvarado, D.
Formato: informe técnico
Fecha de Publicación:2022
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5226
Enlace del recurso:http://hdl.handle.net/20.500.12816/5226
Nivel de acceso:acceso abierto
Materia:Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
id IGPR_e766b2a93ef81cfb50342bb0367e455c
oai_identifier_str oai:repositorio.igp.gob.pe:20.500.12816/5226
network_acronym_str IGPR
network_name_str IGP-Institucional
repository_id_str 4701
dc.title.es_ES.fl_str_mv OAUNI multiband photometry of SN2022hrs
title OAUNI multiband photometry of SN2022hrs
spellingShingle OAUNI multiband photometry of SN2022hrs
Pereyra, Antonio
Optical
Supernovae
Transient
http://purl.org/pe-repo/ocde/ford#1.03.08
title_short OAUNI multiband photometry of SN2022hrs
title_full OAUNI multiband photometry of SN2022hrs
title_fullStr OAUNI multiband photometry of SN2022hrs
title_full_unstemmed OAUNI multiband photometry of SN2022hrs
title_sort OAUNI multiband photometry of SN2022hrs
author Pereyra, Antonio
author_facet Pereyra, Antonio
Tello, J.
Zeballos, M.
de Almeida, L.
Espinoza, M.
Alvarado, D.
author_role author
author2 Tello, J.
Zeballos, M.
de Almeida, L.
Espinoza, M.
Alvarado, D.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Pereyra, Antonio
Tello, J.
Zeballos, M.
de Almeida, L.
Espinoza, M.
Alvarado, D.
dc.subject.es_ES.fl_str_mv Optical
Supernovae
Transient
topic Optical
Supernovae
Transient
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 multiband photometry of Type Ia SN2022hrs (TNSTR-2022-994, TNSCR-2022- 997) on 2022-05-02 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015; arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging using BVRI filters was performed under non-photometric conditions (seeing ~1.8") and airmass lower than 1.2. Total integration times of (45x20s=900s) for V, R and I filters, and (60x20s=1200s) for B filter yielded: Date (UT) filter mag 2022-05-02.208 B 12.54 +/- 0.22 2022-05-02.087 V 12.38 +/- 0.14 2022-05-02.104 R 12.52 +/- 0.10 2022-05-02.190 I 13.21 +/- 0.13. UCAC4 field stars were used for the zero point calibration. Following the GELATO classification (TNSCR-2022-997), our measurements are very close to the maximum brightness. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).
publishDate 2022
dc.date.accessioned.none.fl_str_mv 2022-05-18T10:20:29Z
dc.date.available.none.fl_str_mv 2022-05-18T10:20:29Z
dc.date.issued.fl_str_mv 2022-05-13
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/report
format report
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/5226
url http://hdl.handle.net/20.500.12816/5226
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/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.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv R. E. Rutledge
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
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
bitstream.url.fl_str_mv https://repositorio.igp.gob.pe/bitstreams/9c151123-6cc8-454b-993d-f49e307cd037/download
https://repositorio.igp.gob.pe/bitstreams/8338452e-09ad-44b0-b08d-1842696872ae/download
https://repositorio.igp.gob.pe/bitstreams/c632cad5-85a0-4386-b82f-5e027387d692/download
https://repositorio.igp.gob.pe/bitstreams/b83505c2-1ff9-474a-99b3-dce5459bb1b7/download
bitstream.checksum.fl_str_mv bebaf435fdb16f2e87ff838e6ec275c3
8a4605be74aa9ea9d79846c1fba20a33
63802a58814dfbe40fee18f14b0ef743
af31bd908c3891997ad8ac92b5f2962a
bitstream.checksumAlgorithm.fl_str_mv MD5
MD5
MD5
MD5
repository.name.fl_str_mv Repositorio Geofísico del Peru
repository.mail.fl_str_mv dspace-help@myu.edu
_version_ 1842618195789217792
spelling Pereyra, AntonioTello, J.Zeballos, M.de Almeida, L.Espinoza, M.Alvarado, D.2022-05-18T10:20:29Z2022-05-18T10:20:29Z2022-05-13http://hdl.handle.net/20.500.12816/5226We report multiband photometry of Type Ia SN2022hrs (TNSTR-2022-994, TNSCR-2022- 997) on 2022-05-02 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015; arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging using BVRI filters was performed under non-photometric conditions (seeing ~1.8") and airmass lower than 1.2. Total integration times of (45x20s=900s) for V, R and I filters, and (60x20s=1200s) for B filter yielded: Date (UT) filter mag 2022-05-02.208 B 12.54 +/- 0.22 2022-05-02.087 V 12.38 +/- 0.14 2022-05-02.104 R 12.52 +/- 0.10 2022-05-02.190 I 13.21 +/- 0.13. UCAC4 field stars were used for the zero point calibration. Following the GELATO classification (TNSCR-2022-997), our measurements are very close to the maximum brightness. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).application/pdfengR. E. Rutledgeinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/OpticalSupernovaeTransienthttp://purl.org/pe-repo/ocde/ford#1.03.08OAUNI multiband photometry of SN2022hrsinfo:eu-repo/semantics/reportreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALATel-15378.pdfATel-15378.pdfapplication/pdf476589https://repositorio.igp.gob.pe/bitstreams/9c151123-6cc8-454b-993d-f49e307cd037/downloadbebaf435fdb16f2e87ff838e6ec275c3MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/8338452e-09ad-44b0-b08d-1842696872ae/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTATel-15378.pdf.txtATel-15378.pdf.txtExtracted texttext/plain1664https://repositorio.igp.gob.pe/bitstreams/c632cad5-85a0-4386-b82f-5e027387d692/download63802a58814dfbe40fee18f14b0ef743MD53THUMBNAILATel-15378.pdf.jpgATel-15378.pdf.jpgIM Thumbnailimage/jpeg63384https://repositorio.igp.gob.pe/bitstreams/b83505c2-1ff9-474a-99b3-dce5459bb1b7/downloadaf31bd908c3891997ad8ac92b5f2962aMD5420.500.12816/5226oai:repositorio.igp.gob.pe:20.500.12816/52262022-05-18 10:40:26.354https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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
score 13.448654
OAUNI multiband photometry of SN2022hrs
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).

Ejemplares Similares