{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:7YNMT6KFPTOWN4Z62XPFKN27QT","short_pith_number":"pith:7YNMT6KF","schema_version":"1.0","canonical_sha256":"fe1ac9f9457cdd66f33ed5de55375f84de4ec298ba003bedd8b6f8aee6470811","source":{"kind":"arxiv","id":"1201.1855","version":1},"attestation_state":"computed","paper":{"title":"Multiwavelength campaign on Mrk 509 VIII. Location of the X-ray absorber","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"C. P. de Vries, C. Pinto, E. Behar, E. Costantini, G. A. Kriss, G. Branduardi-Raymont, G. Ponti, J. Ebrero, J. S. Kaastra, K. C. Steenbrugge, M. Cappi, M. Mehdipour, N. Arav, P.-O. Petrucci, R. G. Detmers, S. Bianchi, S. Paltani","submitted_at":"2012-01-09T17:48:44Z","abstract_excerpt":"The bright Seyfert 1 galaxy Mrk 509 was monitored by XMM-Newton and other satellites in 2009 to constrain the location of the outflow. We have studied the response of the photoionised gas to changes in the ionising flux produced by the central regions. We used the 5 discrete ionisation components A-E detected in the time-averaged spectrum taken with the RGS. Using the ratio of fluxed EPIC and RGS spectra, we put tight constraints on the variability of the absorbers. Monitoring with the Swift satellite started 6 weeks before the XMM-Newton observations, allowing to use the ionising flux history"},"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":"1201.1855","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-09T17:48:44Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"876d85b5eb44d81037292004e67329b7930669311e202297af5ca49a554bf418","abstract_canon_sha256":"cb1af68f49b1edfa06b11eb5f06af8dad9767ded6102f6865ce61a0750436616"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:53.952679Z","signature_b64":"dOOGJhwEuNinNTpMd4kOLqRWges9ok3n9pFBLWOBDA0RLx3xGjElB5ya+kmNqI0Rt7a0zgRv1CpIJiNMRiJRBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fe1ac9f9457cdd66f33ed5de55375f84de4ec298ba003bedd8b6f8aee6470811","last_reissued_at":"2026-05-18T01:58:53.951997Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:53.951997Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength campaign on Mrk 509 VIII. Location of the X-ray absorber","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"C. P. de Vries, C. Pinto, E. Behar, E. Costantini, G. A. Kriss, G. Branduardi-Raymont, G. Ponti, J. Ebrero, J. S. Kaastra, K. C. Steenbrugge, M. Cappi, M. Mehdipour, N. Arav, P.-O. Petrucci, R. G. Detmers, S. Bianchi, S. Paltani","submitted_at":"2012-01-09T17:48:44Z","abstract_excerpt":"The bright Seyfert 1 galaxy Mrk 509 was monitored by XMM-Newton and other satellites in 2009 to constrain the location of the outflow. We have studied the response of the photoionised gas to changes in the ionising flux produced by the central regions. We used the 5 discrete ionisation components A-E detected in the time-averaged spectrum taken with the RGS. Using the ratio of fluxed EPIC and RGS spectra, we put tight constraints on the variability of the absorbers. Monitoring with the Swift satellite started 6 weeks before the XMM-Newton observations, allowing to use the ionising flux history"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1855","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":"1201.1855","created_at":"2026-05-18T01:58:53.952104+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.1855v1","created_at":"2026-05-18T01:58:53.952104+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1855","created_at":"2026-05-18T01:58:53.952104+00:00"},{"alias_kind":"pith_short_12","alias_value":"7YNMT6KFPTOW","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"7YNMT6KFPTOWN4Z6","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"7YNMT6KF","created_at":"2026-05-18T12:26:58.693483+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/7YNMT6KFPTOWN4Z62XPFKN27QT","json":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT.json","graph_json":"https://pith.science/api/pith-number/7YNMT6KFPTOWN4Z62XPFKN27QT/graph.json","events_json":"https://pith.science/api/pith-number/7YNMT6KFPTOWN4Z62XPFKN27QT/events.json","paper":"https://pith.science/paper/7YNMT6KF"},"agent_actions":{"view_html":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT","download_json":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT.json","view_paper":"https://pith.science/paper/7YNMT6KF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.1855&json=true","fetch_graph":"https://pith.science/api/pith-number/7YNMT6KFPTOWN4Z62XPFKN27QT/graph.json","fetch_events":"https://pith.science/api/pith-number/7YNMT6KFPTOWN4Z62XPFKN27QT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT/action/storage_attestation","attest_author":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT/action/author_attestation","sign_citation":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT/action/citation_signature","submit_replication":"https://pith.science/pith/7YNMT6KFPTOWN4Z62XPFKN27QT/action/replication_record"}},"created_at":"2026-05-18T01:58:53.952104+00:00","updated_at":"2026-05-18T01:58:53.952104+00:00"}