{"paper":{"title":"X-ray analysis of the galaxy group UGC03957 beyond R200 with Suzaku","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"J. Hasenbusch, L. Lovisari, S. Th\\\"olken, T. H. Reiprich","submitted_at":"2016-03-16T20:00:23Z","abstract_excerpt":"We investigated the gas properties of the galaxy group UGC03957 up to $1.4R_{200} \\approx 1.4$Mpc in four azimuthal directions with the Suzaku satellit and performed a spectral analysis of five Suzaku observations of UGC03957 with 138ks good exposure time in total and five Chandra snapshot observations for point source detection. We found a temperature drop of a factor of ${\\sim} 3$ from the center to the outskirts that is consistent with previous results for galaxy clusters. The metal abundance profile shows a flat behavior towards large radii, which is a hint for galactic winds as the primar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.05255","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}