{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:O5VWKP5Z2VHZ3OMKDL3TT747QD","short_pith_number":"pith:O5VWKP5Z","schema_version":"1.0","canonical_sha256":"776b653fb9d54f9db98a1af739ff9f80deba36bbba7fb6bfc2a2d97f6afd4d64","source":{"kind":"arxiv","id":"0706.1213","version":1},"attestation_state":"computed","paper":{"title":"Resumption of mass accretion in RS Oph","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. E. Bromage, H. L. Worters, J. P. Osborne, S. P. S Eyres","submitted_at":"2007-06-08T17:26:14Z","abstract_excerpt":"The latest outburst of the recurrent nova RS Oph occurred in 2006 February. Photometric data presented here show evidence of the resumption of optical flickering, indicating re-establishment of accretion by day 241 of the outburst. Magnitude variations of up to 0.32 mag in V-band and 0.14 mag in B on timescales of 600-7000 s are detected. Over the two week observational period we also detect a 0.5 mag decline in the mean brightness, from V~11.4 to V~11.9, and record B~12.9 mag. Limits on the mass accretion rate of ~10^{-10} to 10^{-9} Msun/yr are calculated, which span the range of accretion r"},"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":"0706.1213","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-06-08T17:26:14Z","cross_cats_sorted":[],"title_canon_sha256":"e100655a411b3e6b8727609a1345cc3045a90a3b0259953685b63faf987e35c0","abstract_canon_sha256":"aaec824517920b69d1b5afcf2b0b2f96884ac34f0d324c82b90f505397b1c17f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:21:15.864901Z","signature_b64":"wFxjtsPb2VAkad3jjdeD2B4abJXgoEfEJcH2GvR2lR22sdN7wgj3AOO/dD/QgMpBaqJ85Pls2cPAq6zeAK67Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"776b653fb9d54f9db98a1af739ff9f80deba36bbba7fb6bfc2a2d97f6afd4d64","last_reissued_at":"2026-07-04T15:21:15.864448Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:21:15.864448Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resumption of mass accretion in RS Oph","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"G. E. Bromage, H. L. Worters, J. P. Osborne, S. P. S Eyres","submitted_at":"2007-06-08T17:26:14Z","abstract_excerpt":"The latest outburst of the recurrent nova RS Oph occurred in 2006 February. Photometric data presented here show evidence of the resumption of optical flickering, indicating re-establishment of accretion by day 241 of the outburst. Magnitude variations of up to 0.32 mag in V-band and 0.14 mag in B on timescales of 600-7000 s are detected. Over the two week observational period we also detect a 0.5 mag decline in the mean brightness, from V~11.4 to V~11.9, and record B~12.9 mag. Limits on the mass accretion rate of ~10^{-10} to 10^{-9} Msun/yr are calculated, which span the range of accretion r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0706.1213","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/0706.1213/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":"0706.1213","created_at":"2026-07-04T15:21:15.864528+00:00"},{"alias_kind":"arxiv_version","alias_value":"0706.1213v1","created_at":"2026-07-04T15:21:15.864528+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0706.1213","created_at":"2026-07-04T15:21:15.864528+00:00"},{"alias_kind":"pith_short_12","alias_value":"O5VWKP5Z2VHZ","created_at":"2026-07-04T15:21:15.864528+00:00"},{"alias_kind":"pith_short_16","alias_value":"O5VWKP5Z2VHZ3OMK","created_at":"2026-07-04T15:21:15.864528+00:00"},{"alias_kind":"pith_short_8","alias_value":"O5VWKP5Z","created_at":"2026-07-04T15:21:15.864528+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.17652","citing_title":"Association between Recurrent Novae and Nova Super-Remnants","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD","json":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD.json","graph_json":"https://pith.science/api/pith-number/O5VWKP5Z2VHZ3OMKDL3TT747QD/graph.json","events_json":"https://pith.science/api/pith-number/O5VWKP5Z2VHZ3OMKDL3TT747QD/events.json","paper":"https://pith.science/paper/O5VWKP5Z"},"agent_actions":{"view_html":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD","download_json":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD.json","view_paper":"https://pith.science/paper/O5VWKP5Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0706.1213&json=true","fetch_graph":"https://pith.science/api/pith-number/O5VWKP5Z2VHZ3OMKDL3TT747QD/graph.json","fetch_events":"https://pith.science/api/pith-number/O5VWKP5Z2VHZ3OMKDL3TT747QD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD/action/storage_attestation","attest_author":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD/action/author_attestation","sign_citation":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD/action/citation_signature","submit_replication":"https://pith.science/pith/O5VWKP5Z2VHZ3OMKDL3TT747QD/action/replication_record"}},"created_at":"2026-07-04T15:21:15.864528+00:00","updated_at":"2026-07-04T15:21:15.864528+00:00"}