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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Detalles Bibliográficos
Publicado:	2013
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:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_97885890_v2013-October_n_p_Giacani 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

id	paper:paper_97885890_v2013-October_n_p_Giacani
record_format	dspace
spelling	paper:paper_97885890_v2013-October_n_p_Giacani2023-06-08T16:39:05Z Search for radio counterpart of the Fermi/VERITAS PWN candidate in the SNR CTA 1 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. 2013 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_97885890_v2013-October_n_p_Giacani 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 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.
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
publishDate	2013
url	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_97885890_v2013-October_n_p_Giacani http://hdl.handle.net/20.500.12110/paper_97885890_v2013-October_n_p_Giacani
_version_	1769175807119327232

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

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