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.
Documento: | Artículo |
Título: | GMRT observations of SNR G15.4+0.1/HESS J1818-154 |
Autor: | Castelletti, G.; Joshi, B.C.; Surnis, M.P.; Supán, L.; Dubner, G.; Ray A.K.; McCray R. |
Filiación: | Institute of Astronomy and Space Physics (IAFE), Buenos Aires, Argentina National Centre for Radio Astrophysics (NCRA), Pune, India |
Palabras clave: | (ISM:) supernova remnants; (stars:) pulsars: general; (stars:) pulsars: individual (J1645-0317, J1939+2134, J1901-0906) |
Año: | 2014 |
Volumen: | 9 |
Número: | S296 |
Página de inicio: | 366 |
Página de fin: | 367 |
DOI: | http://dx.doi.org/10.1017/S174392131300985X |
Título revista: | Proceedings of the International Astronomical Union |
Título revista abreviado: | Proc. Int. Astron. Union |
ISSN: | 17439213 |
Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v9_nS296_p366_Castelletti |