{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:O632Z3FCTOQEBO3JFQ775ORLWH","short_pith_number":"pith:O632Z3FC","schema_version":"1.0","canonical_sha256":"77b7aceca29ba040bb692c3ffeba2bb1fb4275918be0aa9e1d948da962562a88","source":{"kind":"arxiv","id":"1407.5004","version":1},"attestation_state":"computed","paper":{"title":"Interpreting broad emission-line variations I : Factors influencing the emission-line response","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"K. T. Korista, M. R. Goad","submitted_at":"2014-07-18T14:08:25Z","abstract_excerpt":"We investigate the sensitivity of the measured broad emission-line responsivity dlog f_line/dlog f_cont to continuum variations in the context of straw-man BLR geometries of varying size with fixed BLR boundaries, and for which the intrinsic emission-line responsivity is known a priori. We find for a generic emission-line that the measured responsivity, delay and maximum of the cross-correlation function are correlated for characteristic continuum variability timescales T_char less than the maximum delay for that line tau_max(line) for a particular choice of BLR geometry and observer orientati"},"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":"1407.5004","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-18T14:08:25Z","cross_cats_sorted":[],"title_canon_sha256":"81600afde98efb34a6d7a3a1cca614341586c4076ba11e2c587ae11a3d1d05a0","abstract_canon_sha256":"a7d00956f83529a30930e33797a730c94a8ae26b210094a2d4cfa7fe64a83300"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:33.986773Z","signature_b64":"s93RbohjXhqWuI/Vz9A98rHbK+DNvHQZdLv1/zsDlOvKp4FKamc68YRR4s7jLDK049vGy8QrkO7+SwLON3rWAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77b7aceca29ba040bb692c3ffeba2bb1fb4275918be0aa9e1d948da962562a88","last_reissued_at":"2026-05-18T01:42:33.986205Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:33.986205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interpreting broad emission-line variations I : Factors influencing the emission-line response","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"K. T. Korista, M. R. Goad","submitted_at":"2014-07-18T14:08:25Z","abstract_excerpt":"We investigate the sensitivity of the measured broad emission-line responsivity dlog f_line/dlog f_cont to continuum variations in the context of straw-man BLR geometries of varying size with fixed BLR boundaries, and for which the intrinsic emission-line responsivity is known a priori. We find for a generic emission-line that the measured responsivity, delay and maximum of the cross-correlation function are correlated for characteristic continuum variability timescales T_char less than the maximum delay for that line tau_max(line) for a particular choice of BLR geometry and observer orientati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.5004","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":"1407.5004","created_at":"2026-05-18T01:42:33.986286+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.5004v1","created_at":"2026-05-18T01:42:33.986286+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.5004","created_at":"2026-05-18T01:42:33.986286+00:00"},{"alias_kind":"pith_short_12","alias_value":"O632Z3FCTOQE","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"O632Z3FCTOQEBO3J","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"O632Z3FC","created_at":"2026-05-18T12:28:41.024544+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.27675","citing_title":"OzSSy1: The Australian Southern Seyfert-1 Spectroscopic Atlas and Catalogue at z < 0.1","ref_index":167,"is_internal_anchor":true},{"citing_arxiv_id":"2606.00992","citing_title":"Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes","ref_index":72,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH","json":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH.json","graph_json":"https://pith.science/api/pith-number/O632Z3FCTOQEBO3JFQ775ORLWH/graph.json","events_json":"https://pith.science/api/pith-number/O632Z3FCTOQEBO3JFQ775ORLWH/events.json","paper":"https://pith.science/paper/O632Z3FC"},"agent_actions":{"view_html":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH","download_json":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH.json","view_paper":"https://pith.science/paper/O632Z3FC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.5004&json=true","fetch_graph":"https://pith.science/api/pith-number/O632Z3FCTOQEBO3JFQ775ORLWH/graph.json","fetch_events":"https://pith.science/api/pith-number/O632Z3FCTOQEBO3JFQ775ORLWH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH/action/storage_attestation","attest_author":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH/action/author_attestation","sign_citation":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH/action/citation_signature","submit_replication":"https://pith.science/pith/O632Z3FCTOQEBO3JFQ775ORLWH/action/replication_record"}},"created_at":"2026-05-18T01:42:33.986286+00:00","updated_at":"2026-05-18T01:42:33.986286+00:00"}