The discovery of a radio halo in PLCK G147.3-16.6 at z=0.65
| Autor: | van Weeren, R. J., Intema, H. T., Lal, D. V., Bonafede, A., Jones, C., Forman, W. R., Röttgering, H. J. A., Brüggen, M., Stroe, A., Hoeft, M., Nuza, S. E., de Gasperin, F. |
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| Rok vydání: | 2014 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1088/2041-8205/781/2/L32 |
| Popis: | Recent X-ray and Sunyaev-Zel'dovich (SZ) observations have dramatically increased the number of known distant galaxy clusters. In some merging, low-redshift (z<0.4) clusters, centrally-located, diffuse, extended radio emission (called radio halos) has been found. Using the Giant Metrewave Radio Telescope (GMRT), we report the detection of diffuse radio emission in the binary-merging cluster PLCK G147.3-16.6 located at z = 0.65. We classify the emission as a giant radio halo due to the large physical extent of about 0.9 Mpc and low-surface brightness. We measure an integrated flux density of $7.3\pm1.1$ mJy at 610 MHz for the radio halo, resulting in a 1.4 GHz radio power of $5.1 \times 10^{24}$ W/Hz. The radio halo power is consistent with that expected from the known correlation between X-ray luminosity or the cluster integrated SZ signal and radio power. Our observations also suggest that more of these distant radio halos could be discovered with the GMRT. Comment: 5 pages, 4 figures, 1 table. Accepted for publication in ApJL |
| Databáze: | arXiv |
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