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<ri:Resource created="2025-12-15T09:07:05Z" status="active" updated="2026-03-20T07:08:39Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Seven candidate revived radio fossils images</title><shortName>J/A+A/704/A245</shortName><identifier>ivo://CDS.VizieR/J/A+A/704/A245</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bruno L.</name></creator><creator><name>Botteon A.</name></creator><creator><name>Dallacasa D.</name></creator><creator><name>Venturi T.</name></creator><creator><name>Balboni M.</name></creator><creator><name>Biava N.,Brienza M.</name></creator><creator><name>Brueggen M.</name></creator><creator><name>Brunetti G.</name></creator><creator><name>de Gasperin F.</name></creator><creator><name>De Rubeis E.,Di Gennaro G.</name></creator><creator><name>Gastaldello F.</name></creator><creator><name>Ignesti A.</name></creator><creator><name>Pasini T.</name></creator><creator><name>Rajpurohit K.,Shulevski A.</name></creator><creator><name>Srikanth K.S.L.</name></creator><creator><name>van Weeren R.J.</name></creator><creator><name>Zhang X.</name></creator><date role="Updated">2026-03-20T07:08:39Z</date><date role="Created">2025-12-15T09:07:05Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxy-clusters</subject><subject>radio-galaxies</subject><description>Complex energy transfer processes in the intracluster medium (ICM) can revive fossil (with spectral ages &gt;&gt;100Myr) plasma initially generated by radio galaxies. This leads to the re-ignition of faint radio sources with irregular and filamentary morphologies, and ultra-steep (alpha&gt;1.5) synchrotron spectra, which can be more easily detected at low frequencies (~100MHz). These sources offer the opportunity to investigate the microphysics of the ICM and its interplay with radio galaxies, the origin of seed relativistic electrons, the merging history of the host cluster, and the phenomenology of radio filaments. The study of revived sources has so far been hampered by the requirement of sensitive and high-resolution multi-frequency radio data at low frequencies to characterise their spatial properties and provide a proper classification. We aim to perform the analysis of a sample of candidate revived sources identified among nearby (z&lt;=0.35) and low-mass (M_500_&lt;=5x10^14^M_{sun}_) Planck clusters in the footprint of the Second Data Release of the LOw Frequency ARray (LOFAR) Two Metre Sky Survey (LoTSS-DR2). By inspecting LoTSS-DR2 images at 144MHz, we identified 7 targets with patchy and filamentary morphologies, which have been followed-up with the upgraded Giant Metrewave Radio Telescope (uGMRT) at 400MHz. By combining LOFAR and uGMRT data, we obtained high-resolution images and spectral index maps, which we used to interpret the nature of the sources. All targets show regions with very steep spectra, confirming the effectiveness of our morphology-based selection in identifying fossil plasma. Based on their morphology, spectral properties, and optical associations, we investigated the origin of the targets. 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