Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1

We present new high angular resolution and high sensitivity radio observations toward the neutron star RX J0007.0+7303, carried out with the Karl G. Jansky Very Large Array at 1.5 GHz. This source powers a pulsar wind nebula (PWN) only detected in the X-ray and gamma-ray domains. The new high qualit...

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Autores principales: Giacani, E., Rovero, A.C., Cillis, A., Pichel, A., Dubner, G.
Formato: CONF
Materias:
CTA 1
Pulsar wind nebula
Radio observations
Cosmic rays
Cosmology
Pulsars
Radio
Signal to noise ratio
High sensitivity
Neutron stars
Noise levels
Pulsar wind nebulae
Radio observation
Very large arrays
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_97885890_v2013-October_n_p_Giacani
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
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spelling todo:paper_97885890_v2013-October_n_p_Giacani2023-10-03T16:45:17Z Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1 Giacani, E. Rovero, A.C. Cillis, A. Pichel, A. Dubner, G. CTA 1 Pulsar wind nebula Radio observations Cosmic rays Cosmology Pulsars Radio Signal to noise ratio CTA 1 High sensitivity Neutron stars Noise levels Pulsar wind nebula Pulsar wind nebulae Radio observation Very large arrays Gamma rays We present new high angular resolution and high sensitivity radio observations toward the neutron star RX J0007.0+7303, carried out with the Karl G. Jansky Very Large Array at 1.5 GHz. This source powers a pulsar wind nebula (PWN) only detected in the X-ray and gamma-ray domains. The new high quality radio observations do not show any evidence of a source, either point-like or extended, that could be interpreted as the radio counterpart of the high energy PWN, down to a noise level of 15 µJy/beam. © 2013 Sociedade Brasileira de Fisica. All Rights Reserved. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_97885890_v2013-October_n_p_Giacani
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic CTA 1
Pulsar wind nebula
Radio observations
Cosmic rays
Cosmology
Pulsars
Radio
Signal to noise ratio
CTA 1
High sensitivity
Neutron stars
Noise levels
Pulsar wind nebula
Pulsar wind nebulae
Radio observation
Very large arrays
Gamma rays
spellingShingle CTA 1
Pulsar wind nebula
Radio observations
Cosmic rays
Cosmology
Pulsars
Radio
Signal to noise ratio
CTA 1
High sensitivity
Neutron stars
Noise levels
Pulsar wind nebula
Pulsar wind nebulae
Radio observation
Very large arrays
Gamma rays
Giacani, E.
Rovero, A.C.
Cillis, A.
Pichel, A.
Dubner, G.
Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
topic_facet CTA 1
Pulsar wind nebula
Radio observations
Cosmic rays
Cosmology
Pulsars
Radio
Signal to noise ratio
CTA 1
High sensitivity
Neutron stars
Noise levels
Pulsar wind nebula
Pulsar wind nebulae
Radio observation
Very large arrays
Gamma rays
description We present new high angular resolution and high sensitivity radio observations toward the neutron star RX J0007.0+7303, carried out with the Karl G. Jansky Very Large Array at 1.5 GHz. This source powers a pulsar wind nebula (PWN) only detected in the X-ray and gamma-ray domains. The new high quality radio observations do not show any evidence of a source, either point-like or extended, that could be interpreted as the radio counterpart of the high energy PWN, down to a noise level of 15 µJy/beam. © 2013 Sociedade Brasileira de Fisica. All Rights Reserved.
format CONF
author Giacani, E.
Rovero, A.C.
Cillis, A.
Pichel, A.
Dubner, G.
author_facet Giacani, E.
Rovero, A.C.
Cillis, A.
Pichel, A.
Dubner, G.
author_sort Giacani, E.
title Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
title_short Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
title_full Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
title_fullStr Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
title_full_unstemmed Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1
title_sort search for radio counterpart of the fermi/veritas pwn candidate in the snr cta 1
url http://hdl.handle.net/20.500.12110/paper_97885890_v2013-October_n_p_Giacani
work_keys_str_mv AT giacanie searchforradiocounterpartofthefermiveritaspwncandidateinthesnrcta1
AT roveroac searchforradiocounterpartofthefermiveritaspwncandidateinthesnrcta1
AT cillisa searchforradiocounterpartofthefermiveritaspwncandidateinthesnrcta1
AT pichela searchforradiocounterpartofthefermiveritaspwncandidateinthesnrcta1
AT dubnerg searchforradiocounterpartofthefermiveritaspwncandidateinthesnrcta1
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