{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:R2WNP6Q3QDATVARK4DICQF63WC","short_pith_number":"pith:R2WNP6Q3","schema_version":"1.0","canonical_sha256":"8eacd7fa1b80c13a822ae0d02817dbb0ab9c135ef5755b2a4053cf925f5c6725","source":{"kind":"arxiv","id":"2302.08402","version":1},"attestation_state":"computed","paper":{"title":"Continuum reverberation mapping of MCG 08-11-011","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. Fian, C. Sobrino Figaredo, D. Chelouche, S. Catalan, S. Kaspi, T. Lewis","submitted_at":"2023-02-16T16:26:57Z","abstract_excerpt":"We report the results from a photometric reverberation mapping campaign carried out with the C18 telescope at the Wise Observatory from 2019 to 2020, targeting the active galactic nucleus (AGN) MCG 08-11-011. The monitoring was conducted on a daily basis with specially designed narrow-band filters, spanning from optical to near-infrared wavelengths ($\\sim4000$ to $8000${\\AA}) and avoiding prominent broad emission lines. We aim to measure inter-band continuum time lags, determine the size-wavelength relation, and estimate the host-subtracted AGN luminosity for this system. We used the point-spr"},"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":"2302.08402","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-02-16T16:26:57Z","cross_cats_sorted":[],"title_canon_sha256":"631d36b7a2eec863ef839dafa7a0299b366eb5f8665b584316efb238623fc655","abstract_canon_sha256":"9ff6ae702db5dd5fd619137a8230bd416d511ac8988a6be10bf13b7918fcb8f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:00:08.001863Z","signature_b64":"ZysI9wjVnAO+K1FNhR+ASUSVjoDt04f8iUmV1X7BppmfJPPB6OgMQMQ6wQTo9eCoC6X8wuubt5GyHHb1nwGwCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8eacd7fa1b80c13a822ae0d02817dbb0ab9c135ef5755b2a4053cf925f5c6725","last_reissued_at":"2026-07-05T06:00:08.001411Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:00:08.001411Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Continuum reverberation mapping of MCG 08-11-011","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. Fian, C. Sobrino Figaredo, D. Chelouche, S. Catalan, S. Kaspi, T. Lewis","submitted_at":"2023-02-16T16:26:57Z","abstract_excerpt":"We report the results from a photometric reverberation mapping campaign carried out with the C18 telescope at the Wise Observatory from 2019 to 2020, targeting the active galactic nucleus (AGN) MCG 08-11-011. The monitoring was conducted on a daily basis with specially designed narrow-band filters, spanning from optical to near-infrared wavelengths ($\\sim4000$ to $8000${\\AA}) and avoiding prominent broad emission lines. We aim to measure inter-band continuum time lags, determine the size-wavelength relation, and estimate the host-subtracted AGN luminosity for this system. We used the point-spr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.08402","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/2302.08402/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":"2302.08402","created_at":"2026-07-05T06:00:08.001472+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.08402v1","created_at":"2026-07-05T06:00:08.001472+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.08402","created_at":"2026-07-05T06:00:08.001472+00:00"},{"alias_kind":"pith_short_12","alias_value":"R2WNP6Q3QDAT","created_at":"2026-07-05T06:00:08.001472+00:00"},{"alias_kind":"pith_short_16","alias_value":"R2WNP6Q3QDATVARK","created_at":"2026-07-05T06:00:08.001472+00:00"},{"alias_kind":"pith_short_8","alias_value":"R2WNP6Q3","created_at":"2026-07-05T06:00:08.001472+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.03291","citing_title":"Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC","json":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC.json","graph_json":"https://pith.science/api/pith-number/R2WNP6Q3QDATVARK4DICQF63WC/graph.json","events_json":"https://pith.science/api/pith-number/R2WNP6Q3QDATVARK4DICQF63WC/events.json","paper":"https://pith.science/paper/R2WNP6Q3"},"agent_actions":{"view_html":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC","download_json":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC.json","view_paper":"https://pith.science/paper/R2WNP6Q3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.08402&json=true","fetch_graph":"https://pith.science/api/pith-number/R2WNP6Q3QDATVARK4DICQF63WC/graph.json","fetch_events":"https://pith.science/api/pith-number/R2WNP6Q3QDATVARK4DICQF63WC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC/action/storage_attestation","attest_author":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC/action/author_attestation","sign_citation":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC/action/citation_signature","submit_replication":"https://pith.science/pith/R2WNP6Q3QDATVARK4DICQF63WC/action/replication_record"}},"created_at":"2026-07-05T06:00:08.001472+00:00","updated_at":"2026-07-05T06:00:08.001472+00:00"}