{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BS5HZGNKE6WAVROMEST3YLEUMA","short_pith_number":"pith:BS5HZGNK","schema_version":"1.0","canonical_sha256":"0cba7c99aa27ac0ac5cc24a7bc2c946010b90c53c06754092c630911d4a47178","source":{"kind":"arxiv","id":"2407.09419","version":1},"attestation_state":"computed","paper":{"title":"Investigating Optical Variability of the Blazar S5 0716+714 On Diverse Time-scales","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Aditi Agarwal, Aykut \\\"Ozd\\\"onmez, Erg\\\"un Ege, Tansel Ak","submitted_at":"2024-07-12T16:47:44Z","abstract_excerpt":"We present the results of the observational study of the blazar S5 0716+716 in the optical bands B, V, R, and I between March 2019 and August 2023 to investigate its variability on diverse time-scales. The blazar was followed up by the T60 robotic telescope in Turkey for 416 nights to obtain long-term variability during this period. In order to search for intraday variability of the object, we have carried out 21 nights of observations with the T100 telescope for at least 1 hour. The blazar showed a ~2.47 mag variation in the optical R-band during our monitoring period, the brightest state on "},"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":"2407.09419","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-07-12T16:47:44Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"20e654a96f298fe99144f39ab22f00ba6f449bc1c2471bd45255aeee6c4bbc97","abstract_canon_sha256":"3b538405c706124ddb96d948acfb99ba5a3f6f90095d78a1b027d5cbc9d4d729"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:43:18.862582Z","signature_b64":"0H88nQrw71F757wwwA8SwisLAwL2/l35CsYyosTq23kLg96RAQpah15VoKmfBdR1x1pJCvIyo0JY/y0U6aVTDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0cba7c99aa27ac0ac5cc24a7bc2c946010b90c53c06754092c630911d4a47178","last_reissued_at":"2026-07-05T08:43:18.862233Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:43:18.862233Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating Optical Variability of the Blazar S5 0716+714 On Diverse Time-scales","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Aditi Agarwal, Aykut \\\"Ozd\\\"onmez, Erg\\\"un Ege, Tansel Ak","submitted_at":"2024-07-12T16:47:44Z","abstract_excerpt":"We present the results of the observational study of the blazar S5 0716+716 in the optical bands B, V, R, and I between March 2019 and August 2023 to investigate its variability on diverse time-scales. The blazar was followed up by the T60 robotic telescope in Turkey for 416 nights to obtain long-term variability during this period. In order to search for intraday variability of the object, we have carried out 21 nights of observations with the T100 telescope for at least 1 hour. The blazar showed a ~2.47 mag variation in the optical R-band during our monitoring period, the brightest state on "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.09419","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/2407.09419/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":"2407.09419","created_at":"2026-07-05T08:43:18.862285+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.09419v1","created_at":"2026-07-05T08:43:18.862285+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.09419","created_at":"2026-07-05T08:43:18.862285+00:00"},{"alias_kind":"pith_short_12","alias_value":"BS5HZGNKE6WA","created_at":"2026-07-05T08:43:18.862285+00:00"},{"alias_kind":"pith_short_16","alias_value":"BS5HZGNKE6WAVROM","created_at":"2026-07-05T08:43:18.862285+00:00"},{"alias_kind":"pith_short_8","alias_value":"BS5HZGNK","created_at":"2026-07-05T08:43:18.862285+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.03420","citing_title":"PKS 2155-304: Long-Term Optical Photometric Monitoring and Variability Analysis","ref_index":26,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA","json":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA.json","graph_json":"https://pith.science/api/pith-number/BS5HZGNKE6WAVROMEST3YLEUMA/graph.json","events_json":"https://pith.science/api/pith-number/BS5HZGNKE6WAVROMEST3YLEUMA/events.json","paper":"https://pith.science/paper/BS5HZGNK"},"agent_actions":{"view_html":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA","download_json":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA.json","view_paper":"https://pith.science/paper/BS5HZGNK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.09419&json=true","fetch_graph":"https://pith.science/api/pith-number/BS5HZGNKE6WAVROMEST3YLEUMA/graph.json","fetch_events":"https://pith.science/api/pith-number/BS5HZGNKE6WAVROMEST3YLEUMA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA/action/storage_attestation","attest_author":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA/action/author_attestation","sign_citation":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA/action/citation_signature","submit_replication":"https://pith.science/pith/BS5HZGNKE6WAVROMEST3YLEUMA/action/replication_record"}},"created_at":"2026-07-05T08:43:18.862285+00:00","updated_at":"2026-07-05T08:43:18.862285+00:00"}