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A hidden radio halo in A1682?
Cosmology and Nongalactic Astrophysics · Submitted 12 Jul 2011
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Our data analysis suggests that the radio galaxies are superposed to very low surface brightness radio emission extended on the cluster scale, which we present here.
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The abstract, sentence by sentence
High sensitivity observations of radio halos in galaxy clusters at frequencies lower than 330 MHz are still relatively rare, and very little is known compared to the classical 1.4 GHz images. The few radio halos imaged down to 150-240 MHz show a considerable spread in size, morphology and spectral properties. All clusters belonging to the GMRT Radio Halo Survey with detected or candidate cluster-scale diffuse emission have been imaged at 325 MHz with the GMRT. Few of them were also observed with the GMRT at 240 MHz and 150 MHz. For A1682, imaging is particularly challenging due to the presence of strong and extended radio galaxies at the center. Our data analysis suggests that the radio galaxies are superposed to very low surface brightness radio emission extended on the cluster scale, which we present here.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | High sensitivity observations of radio halos in galaxy clusters at frequencies lower than 330 MHz are still relatively rare, and very little is known compared to the classical 1.4 GHz images. | background 0.71 | 0.05 | 0.03 | asserted 1.00 |
| s1 | The few radio halos imaged down to 150-240 MHz show a considerable spread in size, morphology and spectral properties. | background 0.95 | 0.11 | 0.03 | asserted 1.00 |
| s2 | All clusters belonging to the GMRT Radio Halo Survey with detected or candidate cluster-scale diffuse emission have been imaged at 325 MHz with the GMRT. | method 0.63 | 0.76 | 0.04 | asserted 1.00 |
| s3 | Few of them were also observed with the GMRT at 240 MHz and 150 MHz. | method 0.46 | 0.61 | 0.03 | asserted 1.00 |
| s4 | For A1682, imaging is particularly challenging due to the presence of strong and extended radio galaxies at the center. | background 0.60 | 0.16 | 0.03 | asserted 1.00 |
| s5 | Our data analysis suggests that the radio galaxies are superposed to very low surface brightness radio emission extended on the cluster scale, which we present here. | result 0.95 | 0.95 | 0.88 | hedged possibility 0.96 |
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The paper
Original abstract
High sensitivity observations of radio halos in galaxy clusters at frequencies lower than 330 MHz are still relatively rare, and very little is known compared to the classical 1.4 GHz images. The few radio halos imaged down to 150-240 MHz show a considerable spread in size, morphology and spectral properties. All clusters belonging to the GMRT Radio Halo Survey with detected or candidate cluster-scale diffuse emission have been imaged at 325 MHz with the GMRT. Few of them were also observed with the GMRT at 240 MHz and 150 MHz. For A1682, imaging is particularly challenging due to the presence of strong and extended radio galaxies at the center. Our data analysis suggests that the radio galaxies are superposed to very low surface brightness radio emission extended on the cluster scale, which we present here.
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