{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:CX7DA67TS23SFOM6I2XH3NWET5","short_pith_number":"pith:CX7DA67T","schema_version":"1.0","canonical_sha256":"15fe307bf396b722b99e46ae7db6c49f4cf402448dd1b29658ab251deb91e577","source":{"kind":"arxiv","id":"astro-ph/0410083","version":1},"attestation_state":"computed","paper":{"title":"Multi-wavelength study of a sample of nearby Seyfert galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Panessa, K. Iwasawa, L. Bassani, M. Cappi, M. Dadina","submitted_at":"2004-10-04T18:52:44Z","abstract_excerpt":"One of the least biased complete Seyfert sample available to date has been considered to perform an X-ray survey using the capabilities of XMM-Newton and Chandra satellites. The X-ray nuclear luminosities obtained have been used to perform a multi-wavelength analysis as a powerfull tool in the identification of heavily obscured objects. The new X-ray data, together with highest quality nuclear fluxes available from the radio to the optical band, allow us to obtain nuclear Spectral Energy Distributions (SEDs) for type 1 and type 2 objects in our sample. The results obtained from the analysis of"},"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":"astro-ph/0410083","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-04T18:52:44Z","cross_cats_sorted":[],"title_canon_sha256":"50cb9d64dbbeea49998a9e72b20d15cf30e842626a94afc1cb9fe08d5af69f85","abstract_canon_sha256":"d6702ecb5a15b5f87b1bc0846486dd72c5449ef51c7aa96ce1bd1f13aa3514c8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:13:47.953495Z","signature_b64":"gbW8FAFYxik2QC82V6tof+HsO4y1uMHV+YoAyyM76F7hiKeUvOidGotob8hOrrxx8LtX4qnLY64489m4W17tCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15fe307bf396b722b99e46ae7db6c49f4cf402448dd1b29658ab251deb91e577","last_reissued_at":"2026-07-04T14:13:47.953101Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:13:47.953101Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-wavelength study of a sample of nearby Seyfert galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. Panessa, K. Iwasawa, L. Bassani, M. Cappi, M. Dadina","submitted_at":"2004-10-04T18:52:44Z","abstract_excerpt":"One of the least biased complete Seyfert sample available to date has been considered to perform an X-ray survey using the capabilities of XMM-Newton and Chandra satellites. The X-ray nuclear luminosities obtained have been used to perform a multi-wavelength analysis as a powerfull tool in the identification of heavily obscured objects. The new X-ray data, together with highest quality nuclear fluxes available from the radio to the optical band, allow us to obtain nuclear Spectral Energy Distributions (SEDs) for type 1 and type 2 objects in our sample. The results obtained from the analysis of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410083","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0410083/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0410083","created_at":"2026-07-04T14:13:47.953160+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410083v1","created_at":"2026-07-04T14:13:47.953160+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410083","created_at":"2026-07-04T14:13:47.953160+00:00"},{"alias_kind":"pith_short_12","alias_value":"CX7DA67TS23S","created_at":"2026-07-04T14:13:47.953160+00:00"},{"alias_kind":"pith_short_16","alias_value":"CX7DA67TS23SFOM6","created_at":"2026-07-04T14:13:47.953160+00:00"},{"alias_kind":"pith_short_8","alias_value":"CX7DA67T","created_at":"2026-07-04T14:13:47.953160+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5","json":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5.json","graph_json":"https://pith.science/api/pith-number/CX7DA67TS23SFOM6I2XH3NWET5/graph.json","events_json":"https://pith.science/api/pith-number/CX7DA67TS23SFOM6I2XH3NWET5/events.json","paper":"https://pith.science/paper/CX7DA67T"},"agent_actions":{"view_html":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5","download_json":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5.json","view_paper":"https://pith.science/paper/CX7DA67T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0410083&json=true","fetch_graph":"https://pith.science/api/pith-number/CX7DA67TS23SFOM6I2XH3NWET5/graph.json","fetch_events":"https://pith.science/api/pith-number/CX7DA67TS23SFOM6I2XH3NWET5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5/action/storage_attestation","attest_author":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5/action/author_attestation","sign_citation":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5/action/citation_signature","submit_replication":"https://pith.science/pith/CX7DA67TS23SFOM6I2XH3NWET5/action/replication_record"}},"created_at":"2026-07-04T14:13:47.953160+00:00","updated_at":"2026-07-04T14:13:47.953160+00:00"}