{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PKMSM2GHDDL7WX7BLLJLZP7HU7","short_pith_number":"pith:PKMSM2GH","schema_version":"1.0","canonical_sha256":"7a992668c718d7fb5fe15ad2bcbfe7a7e761d4ae314ddf0cc063bf623e3f9cab","source":{"kind":"arxiv","id":"1705.08221","version":1},"attestation_state":"computed","paper":{"title":"CO excitation in the Seyfert galaxy NGC7130","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. Gruppioni, C. Vignali, F. Pozzi, L. Vallini, M. Massardi, M. Mingozzi, M. Talia, P. Andreani","submitted_at":"2017-05-23T12:53:59Z","abstract_excerpt":"We present a coherent multi-band modelling of the CO Spectral Energy Distribution of the local Seyfert Galaxy NGC7130 to assess the impact of the AGN activity on the molecular gas. We take advantage of all the available data from X-ray to the sub-mm, including ALMA data. The high-resolution (~0.2\") ALMA CO(6-5) data constrain the spatial extension of the CO emission down to ~70 pc scale. From the analysis of the archival CHANDRA and NuSTAR data, we infer the presence of a buried, Compton-thick AGN of moderate luminosity, L_2-10keV ~ 1.6x10^{43} ergs-1. We explore photodissociation and X-ray-do"},"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":"1705.08221","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-23T12:53:59Z","cross_cats_sorted":[],"title_canon_sha256":"30cecf54083207db8f0766a07a197616b50e48f2c14712b6e9b4f031332d284f","abstract_canon_sha256":"8301879657d9f4a3ea6263624ff8b20e1da943d989b46ca9f4378433efd74032"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:39:34.823860Z","signature_b64":"nzoL2lk0ZH/K2/Zfu5qqZ5WFpq2CAOOPY9KbWgdzg1DbmfO/XSVPhLMsVLwL9wC3dtgktVHtfeO8nMtKsYfKCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a992668c718d7fb5fe15ad2bcbfe7a7e761d4ae314ddf0cc063bf623e3f9cab","last_reissued_at":"2026-05-18T00:39:34.823133Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:39:34.823133Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CO excitation in the Seyfert galaxy NGC7130","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. Gruppioni, C. Vignali, F. Pozzi, L. Vallini, M. Massardi, M. Mingozzi, M. Talia, P. Andreani","submitted_at":"2017-05-23T12:53:59Z","abstract_excerpt":"We present a coherent multi-band modelling of the CO Spectral Energy Distribution of the local Seyfert Galaxy NGC7130 to assess the impact of the AGN activity on the molecular gas. We take advantage of all the available data from X-ray to the sub-mm, including ALMA data. The high-resolution (~0.2\") ALMA CO(6-5) data constrain the spatial extension of the CO emission down to ~70 pc scale. From the analysis of the archival CHANDRA and NuSTAR data, we infer the presence of a buried, Compton-thick AGN of moderate luminosity, L_2-10keV ~ 1.6x10^{43} ergs-1. We explore photodissociation and X-ray-do"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.08221","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":""},"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":"1705.08221","created_at":"2026-05-18T00:39:34.823247+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.08221v1","created_at":"2026-05-18T00:39:34.823247+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.08221","created_at":"2026-05-18T00:39:34.823247+00:00"},{"alias_kind":"pith_short_12","alias_value":"PKMSM2GHDDL7","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PKMSM2GHDDL7WX7B","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PKMSM2GH","created_at":"2026-05-18T12:31:37.085036+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/PKMSM2GHDDL7WX7BLLJLZP7HU7","json":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7.json","graph_json":"https://pith.science/api/pith-number/PKMSM2GHDDL7WX7BLLJLZP7HU7/graph.json","events_json":"https://pith.science/api/pith-number/PKMSM2GHDDL7WX7BLLJLZP7HU7/events.json","paper":"https://pith.science/paper/PKMSM2GH"},"agent_actions":{"view_html":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7","download_json":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7.json","view_paper":"https://pith.science/paper/PKMSM2GH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.08221&json=true","fetch_graph":"https://pith.science/api/pith-number/PKMSM2GHDDL7WX7BLLJLZP7HU7/graph.json","fetch_events":"https://pith.science/api/pith-number/PKMSM2GHDDL7WX7BLLJLZP7HU7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7/action/storage_attestation","attest_author":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7/action/author_attestation","sign_citation":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7/action/citation_signature","submit_replication":"https://pith.science/pith/PKMSM2GHDDL7WX7BLLJLZP7HU7/action/replication_record"}},"created_at":"2026-05-18T00:39:34.823247+00:00","updated_at":"2026-05-18T00:39:34.823247+00:00"}