Pulsar Observations at low latitudes and low frequencies

Autores
Lousto, Carlos Oscar; Gancio Gonzalez, Guillermo Matias; Zubieta, Ezequiel; del Palacio, Santiago
Año de publicación
2023
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The Pulsar Monitoring in Argentina (PuMA) is a collaboration between the Argentine Institute for Radioas-tronomy (IAR) and the Rochester Institute of Technology (RIT) that since 2017 has been observing southernsky pulsars with high cadence using the two restored IAR antennas in the L-Band (1400MHz). We brieflyreview the first set of results of this program to study transient phenomena, such as magnetars and glitchingpulsars, as well as to perform precise timing of millisecond pulsars. Access to lower frequency bands, wheremost of the pulsars are brighter, would allow us to reach additional pulsars, currently buried into the back-ground noise. We identify two dozen additional glitching pulsars that could be observable in the 400MHz bandby the IAR’s projected Multipurpose Interferometer Array (MIA). We also discuss the relevance and challengesof single-pulse pulsar timing at low frequencies and the search for Fast Radio Burst (FRB) in the collecteddata since 2017 using machine learning techniques.
Fil: Lousto, Carlos Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Gancio Gonzalez, Guillermo Matias. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Zubieta, Ezequiel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: del Palacio, Santiago. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Prospects for low-frequency radio astronomy in South America
CABA
Argentina
Instituto Argentino de Radioastronomía
Materia
DETECTORS
STATISTICAL
PULSAR
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/231985
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Pulsar Observations at low latitudes and low frequenciesLousto, Carlos OscarGancio Gonzalez, Guillermo MatiasZubieta, Ezequieldel Palacio, SantiagoDETECTORSSTATISTICALPULSARhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Pulsar Monitoring in Argentina (PuMA) is a collaboration between the Argentine Institute for Radioas-tronomy (IAR) and the Rochester Institute of Technology (RIT) that since 2017 has been observing southernsky pulsars with high cadence using the two restored IAR antennas in the L-Band (1400MHz). We brieflyreview the first set of results of this program to study transient phenomena, such as magnetars and glitchingpulsars, as well as to perform precise timing of millisecond pulsars. Access to lower frequency bands, wheremost of the pulsars are brighter, would allow us to reach additional pulsars, currently buried into the back-ground noise. We identify two dozen additional glitching pulsars that could be observable in the 400MHz bandby the IAR’s projected Multipurpose Interferometer Array (MIA). We also discuss the relevance and challengesof single-pulse pulsar timing at low frequencies and the search for Fast Radio Burst (FRB) in the collecteddata since 2017 using machine learning techniques.Fil: Lousto, Carlos Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Gancio Gonzalez, Guillermo Matias. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Zubieta, Ezequiel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: del Palacio, Santiago. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaProspects for low-frequency radio astronomy in South AmericaCABAArgentinaInstituto Argentino de RadioastronomíaUniversidad Nacional Autónoma de MéxicoBenaglia, PaulaAndruchow, Ileana2023info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectWorkshopJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/231985Pulsar Observations at low latitudes and low frequencies; Prospects for low-frequency radio astronomy in South America; CABA; Argentina; 2022; 1-111405-2059CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol56.htmlinfo:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/rmaa/RMxAC..56/PDF/RMxAC..56_clousto-XXIVa.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:38:33Zoai:ri.conicet.gov.ar:11336/231985instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:38:33.45CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Pulsar Observations at low latitudes and low frequencies
title Pulsar Observations at low latitudes and low frequencies
spellingShingle Pulsar Observations at low latitudes and low frequencies
Lousto, Carlos Oscar
DETECTORS
STATISTICAL
PULSAR
title_short Pulsar Observations at low latitudes and low frequencies
title_full Pulsar Observations at low latitudes and low frequencies
title_fullStr Pulsar Observations at low latitudes and low frequencies
title_full_unstemmed Pulsar Observations at low latitudes and low frequencies
title_sort Pulsar Observations at low latitudes and low frequencies
dc.creator.none.fl_str_mv Lousto, Carlos Oscar
Gancio Gonzalez, Guillermo Matias
Zubieta, Ezequiel
del Palacio, Santiago
author Lousto, Carlos Oscar
author_facet Lousto, Carlos Oscar
Gancio Gonzalez, Guillermo Matias
Zubieta, Ezequiel
del Palacio, Santiago
author_role author
author2 Gancio Gonzalez, Guillermo Matias
Zubieta, Ezequiel
del Palacio, Santiago
author2_role author
author
author
dc.contributor.none.fl_str_mv Benaglia, Paula
Andruchow, Ileana
dc.subject.none.fl_str_mv DETECTORS
STATISTICAL
PULSAR
topic DETECTORS
STATISTICAL
PULSAR
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The Pulsar Monitoring in Argentina (PuMA) is a collaboration between the Argentine Institute for Radioas-tronomy (IAR) and the Rochester Institute of Technology (RIT) that since 2017 has been observing southernsky pulsars with high cadence using the two restored IAR antennas in the L-Band (1400MHz). We brieflyreview the first set of results of this program to study transient phenomena, such as magnetars and glitchingpulsars, as well as to perform precise timing of millisecond pulsars. Access to lower frequency bands, wheremost of the pulsars are brighter, would allow us to reach additional pulsars, currently buried into the back-ground noise. We identify two dozen additional glitching pulsars that could be observable in the 400MHz bandby the IAR’s projected Multipurpose Interferometer Array (MIA). We also discuss the relevance and challengesof single-pulse pulsar timing at low frequencies and the search for Fast Radio Burst (FRB) in the collecteddata since 2017 using machine learning techniques.
Fil: Lousto, Carlos Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Gancio Gonzalez, Guillermo Matias. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Zubieta, Ezequiel. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: del Palacio, Santiago. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Prospects for low-frequency radio astronomy in South America
CABA
Argentina
Instituto Argentino de Radioastronomía
description The Pulsar Monitoring in Argentina (PuMA) is a collaboration between the Argentine Institute for Radioas-tronomy (IAR) and the Rochester Institute of Technology (RIT) that since 2017 has been observing southernsky pulsars with high cadence using the two restored IAR antennas in the L-Band (1400MHz). We brieflyreview the first set of results of this program to study transient phenomena, such as magnetars and glitchingpulsars, as well as to perform precise timing of millisecond pulsars. Access to lower frequency bands, wheremost of the pulsars are brighter, would allow us to reach additional pulsars, currently buried into the back-ground noise. We identify two dozen additional glitching pulsars that could be observable in the 400MHz bandby the IAR’s projected Multipurpose Interferometer Array (MIA). We also discuss the relevance and challengesof single-pulse pulsar timing at low frequencies and the search for Fast Radio Burst (FRB) in the collecteddata since 2017 using machine learning techniques.
publishDate 2023
dc.date.none.fl_str_mv 2023
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Workshop
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/231985
Pulsar Observations at low latitudes and low frequencies; Prospects for low-frequency radio astronomy in South America; CABA; Argentina; 2022; 1-11
1405-2059
CONICET Digital
CONICET
url http://hdl.handle.net/11336/231985
identifier_str_mv Pulsar Observations at low latitudes and low frequencies; Prospects for low-frequency radio astronomy in South America; CABA; Argentina; 2022; 1-11
1405-2059
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol56.html
info:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/rmaa/RMxAC..56/PDF/RMxAC..56_clousto-XXIVa.pdf
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Universidad Nacional Autónoma de México
publisher.none.fl_str_mv Universidad Nacional Autónoma de México
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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