Matches in UGent Biblio for { <https://biblio.ugent.be/publication/1245258#aggregation> ?p ?o. }
Showing items 1 to 41 of
41
with 100 items per page.
- aggregation classification "A1".
- aggregation creator B334862.
- aggregation creator B334863.
- aggregation creator B334864.
- aggregation creator B334865.
- aggregation creator B334866.
- aggregation creator B334867.
- aggregation creator B334868.
- aggregation creator B334869.
- aggregation creator B334870.
- aggregation creator person.
- aggregation date "2009".
- aggregation format "application/pdf".
- aggregation hasFormat 1245258.bibtex.
- aggregation hasFormat 1245258.csv.
- aggregation hasFormat 1245258.dc.
- aggregation hasFormat 1245258.didl.
- aggregation hasFormat 1245258.doc.
- aggregation hasFormat 1245258.json.
- aggregation hasFormat 1245258.mets.
- aggregation hasFormat 1245258.mods.
- aggregation hasFormat 1245258.rdf.
- aggregation hasFormat 1245258.ris.
- aggregation hasFormat 1245258.txt.
- aggregation hasFormat 1245258.xls.
- aggregation hasFormat 1245258.yaml.
- aggregation isPartOf urn:issn:0004-6361.
- aggregation language "eng".
- aggregation rights "I have transferred the copyright for this publication to the publisher".
- aggregation subject "Physics and Astronomy".
- aggregation title "Revealing the magnetic field in a distant galaxy cluster: discovery of the complex radio emission from MACS J0717.5+3745".
- aggregation abstract "Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster MACS J0717.5+3745 (z = 0.55). Known to be an extremely complex cluster merger, the system is uniquely suited for an investigation of the phenomena at work in the intra-cluster medium (ICM) during cluster collisions. Methods. We use multi-frequency and multi-resolution data obtained with the Very Large Array radio telescope, and X-ray features revealed by Chandra, to probe the non-thermal and thermal components of the ICM, their relations and interactions. Results. The cluster shows highly complex radio emission. A bright, giant radio halo is detected at frequencies as high as 4.8 GHz. MACS J0717.5+3745 is the most distant cluster currently known to host a radio halo. This radio halo is also the most powerful ever observed, and the second case for which polarized radio emission has been detected, indicating that the magnetic field is ordered on large scales.".
- aggregation authorList BK630617.
- aggregation endPage "720".
- aggregation issue "3".
- aggregation startPage "707".
- aggregation volume "503".
- aggregation aggregates 1252801.
- aggregation isDescribedBy 1245258.
- aggregation similarTo 200912520.
- aggregation similarTo LU-1245258.