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The detailed analysis of all data taken by the XMM-Newton satellite of UGC11763 to characterize the different components that are emitting and absorbing radiation in the vicinity of the active nucleus.\n  Methods. The continuum emission was studied through the EPIC spectra taking profit of the spectral range of these cameras. The high resolution RGS spectra were analyzed in order to characterize the absorbing features and the emission line features that arise in the spectra of this source.\n  Results. A power law with a photon index \\Gamma = 1.72^{+0.03}_{-0.01} accounts for the continuum "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0909.2180","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-09-11T14:39:42Z","cross_cats_sorted":[],"title_canon_sha256":"0a78d1300b652c516680408ae8b5655046c714ea2a196b46a7008a97eae0e22b","abstract_canon_sha256":"a09cd1b2c8f5cd01656d288749a091b5ff80ea7a7c9eb2b23065c27b9ab71dd7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:11:56.920063Z","signature_b64":"2u5eULTeDN1Of5Woxg4KIC22wZabXHoViNfKmnbB6r1CNJ71OteXoKde3/BgxnHfX3Wx1nT+1hPBBU0+gULJBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bbf4e6f7632efd710d1e799abf58e901545872182cca24ca5719439e1ff804ab","last_reissued_at":"2026-05-18T02:11:56.919185Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:11:56.919185Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Characterization of the emitting and absorbing media around the nucleus of the active galaxy UGC11763 using XMM-Newton data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.I. Diaz, G.F. Hagele, M. Santos-Lleo, M.V. Cardaci, P. Rodriguez-Pascual, Y. Krongold","submitted_at":"2009-09-11T14:39:42Z","abstract_excerpt":"Aims. The detailed analysis of all data taken by the XMM-Newton satellite of UGC11763 to characterize the different components that are emitting and absorbing radiation in the vicinity of the active nucleus.\n  Methods. The continuum emission was studied through the EPIC spectra taking profit of the spectral range of these cameras. The high resolution RGS spectra were analyzed in order to characterize the absorbing features and the emission line features that arise in the spectra of this source.\n  Results. 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