{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:4FUESBXUO67C7BV4QNMZ6IXNGN","short_pith_number":"pith:4FUESBXU","schema_version":"1.0","canonical_sha256":"e1684906f477be2f86bc83599f22ed337f5c902a2a2755b1c296084c057d56e8","source":{"kind":"arxiv","id":"2107.06851","version":1},"attestation_state":"computed","paper":{"title":"A systematic study of photoionized emission and warm absorption signatures of the NLS1 Mrk 335","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Cosimo Bambi, D. Grupe, E. Kara, H. Liu, J. Jiang, M. L. Parker, S. Komossa","submitted_at":"2021-07-14T17:10:04Z","abstract_excerpt":"We present an analysis of all the archival high resolution spectra of the Narrow-line Seyfert 1 galaxy Mrk~335 obtained with Reflection Grating Spectrometer (RGS) on board \\textit{XMM-Newton}. The spectra show rich emission and absorption features in low and intermediate flux intervals. We model the emission lines with the \\textsc{pion\\_xs} grid and try to find any possible correlation between the properties of the emitting gas and the source flux. Current data does not allow detailed trace of the response of the line emitting gas to the X-ray flux of Mrk~335, but the flux of the X-ray lines i"},"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":"2107.06851","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-07-14T17:10:04Z","cross_cats_sorted":[],"title_canon_sha256":"bf769e97e22f8ce8c858c88039cc652799781bd163b45c780d0dab7ec280d55b","abstract_canon_sha256":"ea800d4c678bc25c7d6e1f50acd4f8f23ea5a4a3c6674b0da5e32cb04fad4445"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:07:50.588978Z","signature_b64":"V3MwTSnXTYVSps/HND2O0OOadrYoVDbxXKeUc+g1hcYkgd0NP2dcDp5RoICBKESsK4QF0S1CZj7y8WvBEMGrDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e1684906f477be2f86bc83599f22ed337f5c902a2a2755b1c296084c057d56e8","last_reissued_at":"2026-07-05T03:07:50.588532Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:07:50.588532Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A systematic study of photoionized emission and warm absorption signatures of the NLS1 Mrk 335","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Cosimo Bambi, D. Grupe, E. Kara, H. Liu, J. Jiang, M. L. Parker, S. Komossa","submitted_at":"2021-07-14T17:10:04Z","abstract_excerpt":"We present an analysis of all the archival high resolution spectra of the Narrow-line Seyfert 1 galaxy Mrk~335 obtained with Reflection Grating Spectrometer (RGS) on board \\textit{XMM-Newton}. The spectra show rich emission and absorption features in low and intermediate flux intervals. We model the emission lines with the \\textsc{pion\\_xs} grid and try to find any possible correlation between the properties of the emitting gas and the source flux. Current data does not allow detailed trace of the response of the line emitting gas to the X-ray flux of Mrk~335, but the flux of the X-ray lines i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2107.06851","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/2107.06851/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":"2107.06851","created_at":"2026-07-05T03:07:50.588591+00:00"},{"alias_kind":"arxiv_version","alias_value":"2107.06851v1","created_at":"2026-07-05T03:07:50.588591+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2107.06851","created_at":"2026-07-05T03:07:50.588591+00:00"},{"alias_kind":"pith_short_12","alias_value":"4FUESBXUO67C","created_at":"2026-07-05T03:07:50.588591+00:00"},{"alias_kind":"pith_short_16","alias_value":"4FUESBXUO67C7BV4","created_at":"2026-07-05T03:07:50.588591+00:00"},{"alias_kind":"pith_short_8","alias_value":"4FUESBXU","created_at":"2026-07-05T03:07:50.588591+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/4FUESBXUO67C7BV4QNMZ6IXNGN","json":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN.json","graph_json":"https://pith.science/api/pith-number/4FUESBXUO67C7BV4QNMZ6IXNGN/graph.json","events_json":"https://pith.science/api/pith-number/4FUESBXUO67C7BV4QNMZ6IXNGN/events.json","paper":"https://pith.science/paper/4FUESBXU"},"agent_actions":{"view_html":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN","download_json":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN.json","view_paper":"https://pith.science/paper/4FUESBXU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2107.06851&json=true","fetch_graph":"https://pith.science/api/pith-number/4FUESBXUO67C7BV4QNMZ6IXNGN/graph.json","fetch_events":"https://pith.science/api/pith-number/4FUESBXUO67C7BV4QNMZ6IXNGN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN/action/storage_attestation","attest_author":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN/action/author_attestation","sign_citation":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN/action/citation_signature","submit_replication":"https://pith.science/pith/4FUESBXUO67C7BV4QNMZ6IXNGN/action/replication_record"}},"created_at":"2026-07-05T03:07:50.588591+00:00","updated_at":"2026-07-05T03:07:50.588591+00:00"}