GMRT observations of SNR G15.4+0.1/HESS J1818-154

We report here on the first dedicated simultaneous imaging and pulsar observations towards the supernova remnant (SNR) G15.4+0.1, the possible counterpart of the very high energy (VHE) source HESS J1818-154. The observations were carried out using the Giant Metrewave Radio Telescope (GMRT) at 610 an...

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Detalles Bibliográficos
Publicado: 2014
Materias:
(ISM:) supernova remnants
(stars:) pulsars: general
(stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906)
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v9_nS296_p366_Castelletti
http://hdl.handle.net/20.500.12110/paper_17439213_v9_nS296_p366_Castelletti
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_17439213_v9_nS296_p366_Castelletti
record_format dspace
spelling paper:paper_17439213_v9_nS296_p366_Castelletti2023-06-08T16:28:12Z GMRT observations of SNR G15.4+0.1/HESS J1818-154 (ISM:) supernova remnants (stars:) pulsars: general (stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906) We report here on the first dedicated simultaneous imaging and pulsar observations towards the supernova remnant (SNR) G15.4+0.1, the possible counterpart of the very high energy (VHE) source HESS J1818-154. The observations were carried out using the Giant Metrewave Radio Telescope (GMRT) at 610 and 1400 MHz. Preliminary analysis of data suggests absence of pulsations towards the centroid of HESS J1818-154, with upper limits of 0.6 and 0.3 mJy at 610 and 1400 MHz, respectively. Analysis of data with a larger beam is in progress, which may confirm the presence of a putative pulsar and its wind nebula if it is offset from the centroid of HESS J1818-154. © International Astronomical Union 2014. 2014 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v9_nS296_p366_Castelletti http://hdl.handle.net/20.500.12110/paper_17439213_v9_nS296_p366_Castelletti
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic (ISM:) supernova remnants
(stars:) pulsars: general
(stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906)
spellingShingle (ISM:) supernova remnants
(stars:) pulsars: general
(stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906)
GMRT observations of SNR G15.4+0.1/HESS J1818-154
topic_facet (ISM:) supernova remnants
(stars:) pulsars: general
(stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906)
description We report here on the first dedicated simultaneous imaging and pulsar observations towards the supernova remnant (SNR) G15.4+0.1, the possible counterpart of the very high energy (VHE) source HESS J1818-154. The observations were carried out using the Giant Metrewave Radio Telescope (GMRT) at 610 and 1400 MHz. Preliminary analysis of data suggests absence of pulsations towards the centroid of HESS J1818-154, with upper limits of 0.6 and 0.3 mJy at 610 and 1400 MHz, respectively. Analysis of data with a larger beam is in progress, which may confirm the presence of a putative pulsar and its wind nebula if it is offset from the centroid of HESS J1818-154. © International Astronomical Union 2014.
title GMRT observations of SNR G15.4+0.1/HESS J1818-154
title_short GMRT observations of SNR G15.4+0.1/HESS J1818-154
title_full GMRT observations of SNR G15.4+0.1/HESS J1818-154
title_fullStr GMRT observations of SNR G15.4+0.1/HESS J1818-154
title_full_unstemmed GMRT observations of SNR G15.4+0.1/HESS J1818-154
title_sort gmrt observations of snr g15.4+0.1/hess j1818-154
publishDate 2014
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v9_nS296_p366_Castelletti
http://hdl.handle.net/20.500.12110/paper_17439213_v9_nS296_p366_Castelletti
_version_ 1768541771027972096

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