OAUNI photometry of SN 2024jlf
Descripción del Articulo
We report photometry of Type II SN 2024jlf gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging in R filter was performed on five consecutive nights under non-photometric conditions with airmasses lower than 1.3. The integration time was 40x20s=800s fo...
| Autores: | , , , , , , |
|---|---|
| Formato: | informe técnico |
| Fecha de Publicación: | 2024 |
| Institución: | Instituto Geofísico del Perú |
| Repositorio: | IGP-Institucional |
| Lenguaje: | inglés |
| OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/5644 |
| Enlace del recurso: | http://hdl.handle.net/20.500.12816/5644 |
| Nivel de acceso: | acceso abierto |
| Materia: | Optical Supernovae Transient https://purl.org/pe-repo/ocde/ford#1.03.08 |
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| dc.title.none.fl_str_mv |
OAUNI photometry of SN 2024jlf |
| title |
OAUNI photometry of SN 2024jlf |
| spellingShingle |
OAUNI photometry of SN 2024jlf Pereyra, Antonio Optical Supernovae Transient https://purl.org/pe-repo/ocde/ford#1.03.08 |
| title_short |
OAUNI photometry of SN 2024jlf |
| title_full |
OAUNI photometry of SN 2024jlf |
| title_fullStr |
OAUNI photometry of SN 2024jlf |
| title_full_unstemmed |
OAUNI photometry of SN 2024jlf |
| title_sort |
OAUNI photometry of SN 2024jlf |
| author |
Pereyra, Antonio |
| author_facet |
Pereyra, Antonio Zevallos, M. Alvarado, D. Delgado, J. Tello, J. de Almeida, L. Torre, E. |
| author_role |
author |
| author2 |
Zevallos, M. Alvarado, D. Delgado, J. Tello, J. de Almeida, L. Torre, E. |
| author2_role |
author author author author author author |
| dc.contributor.author.fl_str_mv |
Pereyra, Antonio Zevallos, M. Alvarado, D. Delgado, J. Tello, J. de Almeida, L. Torre, E. |
| dc.subject.none.fl_str_mv |
Optical Supernovae Transient |
| topic |
Optical Supernovae Transient https://purl.org/pe-repo/ocde/ford#1.03.08 |
| dc.subject.ocde.none.fl_str_mv |
https://purl.org/pe-repo/ocde/ford#1.03.08 |
| description |
We report photometry of Type II SN 2024jlf gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging in R filter was performed on five consecutive nights under non-photometric conditions with airmasses lower than 1.3. The integration time was 40x20s=800s for all observations. Our measurements yielded: Date (UT) | filter | seeing (") | mag, 2024-06-05.056 | R | 2.5 | 14.71 +/- 0.01, 2024-06-06.024 | R | 2.7 | 14.57 +/- 0.03, 2024-06-07.013 | R | 2.9 | 14.45 +/- 0.03, 2024-06-08.010 | R | 2.7 | 14.54 +/- 0.02, 2024-06-09.005 | R | 2.5 | 14.66 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our first observation is ~8 days after ZTF discovery. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt). |
| publishDate |
2024 |
| dc.date.accessioned.none.fl_str_mv |
2024-12-02T16:16:19Z |
| dc.date.available.none.fl_str_mv |
2024-12-02T16:16:19Z |
| dc.date.issued.fl_str_mv |
2024-11-25 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/report |
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report |
| dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/5644 |
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http://hdl.handle.net/20.500.12816/5644 |
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eng |
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eng |
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info:eu-repo/semantics/openAccess |
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https://creativecommons.org/licenses/by/4.0/ |
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openAccess |
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https://creativecommons.org/licenses/by/4.0/ |
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application/pdf |
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R. E. Rutledge |
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R. E. Rutledge |
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Pereyra, AntonioZevallos, M.Alvarado, D.Delgado, J.Tello, J.de Almeida, L.Torre, E.2024-12-02T16:16:19Z2024-12-02T16:16:19Z2024-11-25http://hdl.handle.net/20.500.12816/5644We report photometry of Type II SN 2024jlf gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging in R filter was performed on five consecutive nights under non-photometric conditions with airmasses lower than 1.3. The integration time was 40x20s=800s for all observations. Our measurements yielded: Date (UT) | filter | seeing (") | mag, 2024-06-05.056 | R | 2.5 | 14.71 +/- 0.01, 2024-06-06.024 | R | 2.7 | 14.57 +/- 0.03, 2024-06-07.013 | R | 2.9 | 14.45 +/- 0.03, 2024-06-08.010 | R | 2.7 | 14.54 +/- 0.02, 2024-06-09.005 | R | 2.5 | 14.66 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our first observation is ~8 days after ZTF discovery. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).Este trabajo fue financiado por el Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica (Fondecyt - Perú) en el marco del proyecto OAUNI [número de contrato 133-2020].application/pdfengR. E. Rutledgeinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/4.0/OpticalSupernovaeTransienthttps://purl.org/pe-repo/ocde/ford#1.03.08OAUNI photometry of SN 2024jlfinfo:eu-repo/semantics/reportreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPLICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/971680b7-b7bb-4af9-92e1-7915b3e88b13/downloadbb9bdc0b3349e4284e09149f943790b4MD51ORIGINALATel -16921.pdfATel -16921.pdfapplication/pdf346377https://repositorio.igp.gob.pe/bitstreams/05f0929f-f53a-4317-949b-c980862c0655/download5a51972ce798d058e8d8d1397e6f6c3dMD52TEXTATel -16921.pdf.txtATel -16921.pdf.txtExtracted texttext/plain2529https://repositorio.igp.gob.pe/bitstreams/d20ab980-8539-4504-a643-b227e52b6bf0/downloaddef4ab202b4dd80caa17d71e9e093dc3MD53THUMBNAILATel -16921.pdf.jpgATel -16921.pdf.jpgGenerated Thumbnailimage/jpeg33573https://repositorio.igp.gob.pe/bitstreams/fae269a9-bd0c-4c3b-8b55-8e1363a5a7b4/downloadf4a703c5614661a3a0c47fdc84620aa1MD5420.500.12816/5644oai:repositorio.igp.gob.pe:20.500.12816/56442025-09-25 10:26:20.156https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.peTk9URTogUExBQ0UgWU9VUiBPV04gTElDRU5TRSBIRVJFClRoaXMgc2FtcGxlIGxpY2Vuc2UgaXMgcHJvdmlkZWQgZm9yIGluZm9ybWF0aW9uYWwgcHVycG9zZXMgb25seS4KCk5PTi1FWENMVVNJVkUgRElTVFJJQlVUSU9OIExJQ0VOU0UKCkJ5IHNpZ25pbmcgYW5kIHN1Ym1pdHRpbmcgdGhpcyBsaWNlbnNlLCB5b3UgKHRoZSBhdXRob3Iocykgb3IgY29weXJpZ2h0IG93bmVyKSBncmFudHMgdG8gRFNwYWNlIFVuaXZlcnNpdHkgKERTVSkgdGhlIG5vbi1leGNsdXNpdmUgcmlnaHQgdG8gcmVwcm9kdWNlLCB0cmFuc2xhdGUgKGFzIGRlZmluZWQgYmVsb3cpLCBhbmQvb3IgZGlzdHJpYnV0ZSB5b3VyIHN1Ym1pc3Npb24gKGluY2x1ZGluZyB0aGUgYWJzdHJhY3QpIHdvcmxkd2lkZSBpbiBwcmludCBhbmQgZWxlY3Ryb25pYyBmb3JtYXQgYW5kIGluIGFueSBtZWRpdW0sIGluY2x1ZGluZyBidXQgbm90IGxpbWl0ZWQgdG8gYXVkaW8gb3IgdmlkZW8uCgpZb3UgYWdyZWUgdGhhdCBEU1UgbWF5LCB3aXRob3V0IGNoYW5naW5nIHRoZSBjb250ZW50LCB0cmFuc2xhdGUgdGhlIHN1Ym1pc3Npb24gdG8gYW55IG1lZGl1bSBvciBmb3JtYXQgZm9yIHRoZSBwdXJwb3NlIG9mIHByZXNlcnZhdGlvbi4KCllvdSBhbHNvIGFncmVlIHRoYXQgRFNVIG1heSBrZWVwIG1vcmUgdGhhbiBvbmUgY29weSBvZiB0aGlzIHN1Ym1pc3Npb24gZm9yIHB1cnBvc2VzIG9mIHNlY3VyaXR5LCBiYWNrLXVwIGFuZCBwcmVzZXJ2YXRpb24uCgpZb3UgcmVwcmVzZW50IHRoYXQgdGhlIHN1Ym1pc3Npb24gaXMgeW91ciBvcmlnaW5hbCB3b3JrLCBhbmQgdGhhdCB5b3UgaGF2ZSB0aGUgcmlnaHQgdG8gZ3JhbnQgdGhlIHJpZ2h0cyBjb250YWluZWQgaW4gdGhpcyBsaWNlbnNlLiBZb3UgYWxzbyByZXByZXNlbnQgdGhhdCB5b3VyIHN1Ym1pc3Npb24gZG9lcyBub3QsIHRvIHRoZSBiZXN0IG9mIHlvdXIga25vd2xlZGdlLCBpbmZyaW5nZSB1cG9uIGFueW9uZSdzIGNvcHlyaWdodC4KCklmIHRoZSBzdWJtaXNzaW9uIGNvbnRhaW5zIG1hdGVyaWFsIGZvciB3aGljaCB5b3UgZG8gbm90IGhvbGQgY29weXJpZ2h0LCB5b3UgcmVwcmVzZW50IHRoYXQgeW91IGhhdmUgb2J0YWluZWQgdGhlIHVucmVzdHJpY3RlZCBwZXJtaXNzaW9uIG9mIHRoZSBjb3B5cmlnaHQgb3duZXIgdG8gZ3JhbnQgRFNVIHRoZSByaWdodHMgcmVxdWlyZWQgYnkgdGhpcyBsaWNlbnNlLCBhbmQgdGhhdCBzdWNoIHRoaXJkLXBhcnR5IG93bmVkIG1hdGVyaWFsIGlzIGNsZWFybHkgaWRlbnRpZmllZCBhbmQgYWNrbm93bGVkZ2VkIHdpdGhpbiB0aGUgdGV4dCBvciBjb250ZW50IG9mIHRoZSBzdWJtaXNzaW9uLgoKSUYgVEhFIFNVQk1JU1NJT04gSVMgQkFTRUQgVVBPTiBXT1JLIFRIQVQgSEFTIEJFRU4gU1BPTlNPUkVEIE9SIFNVUFBPUlRFRCBCWSBBTiBBR0VOQ1kgT1IgT1JHQU5JWkFUSU9OIE9USEVSIFRIQU4gRFNVLCBZT1UgUkVQUkVTRU5UIFRIQVQgWU9VIEhBVkUgRlVMRklMTEVEIEFOWSBSSUdIVCBPRiBSRVZJRVcgT1IgT1RIRVIgT0JMSUdBVElPTlMgUkVRVUlSRUQgQlkgU1VDSCBDT05UUkFDVCBPUiBBR1JFRU1FTlQuCgpEU1Ugd2lsbCBjbGVhcmx5IGlkZW50aWZ5IHlvdXIgbmFtZShzKSBhcyB0aGUgYXV0aG9yKHMpIG9yIG93bmVyKHMpIG9mIHRoZSBzdWJtaXNzaW9uLCBhbmQgd2lsbCBub3QgbWFrZSBhbnkgYWx0ZXJhdGlvbiwgb3RoZXIgdGhhbiBhcyBhbGxvd2VkIGJ5IHRoaXMgbGljZW5zZSwgdG8geW91ciBzdWJtaXNzaW9uLgo= |
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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).