{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:OAOYLGN3LVE2WFDMD2PCZCH7P6","short_pith_number":"pith:OAOYLGN3","schema_version":"1.0","canonical_sha256":"701d8599bb5d49ab146c1e9e2c88ff7f9d8e56528b3e663feba8acb6c67a35f6","source":{"kind":"arxiv","id":"1501.06659","version":1},"attestation_state":"computed","paper":{"title":"ASASSN-14cc: Likely Helium Analog of RZ Leonis Minoris","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"BAV, Berto Monard (Center for Backyard Astronomy Kleinkaroo), Franz-Josef Hambsch (GEOS, Taichi Kato (Kyoto U), Vereniging Voor Sterrenkunde)","submitted_at":"2015-01-27T05:27:16Z","abstract_excerpt":"We identified that ASASSN-14cc is a very active dwarf nova spending approximately 60% of the time in outburst. Our long-term photometry revealed that the object shows long outbursts recurring with a period of 21-33 d and very brief short outbursts lasting less than 1 d. The maximum decline rate exceeds 2.8 mag/d. The duration of long outbursts is 9-18 d, comprising 50-60% of the recurrence time of long outbursts. We detected 0.01560-0.01562 d (22.5 min) modulations during long outbursts, which we identified to be superhumps. These features indicate that ASASSN-14cc has outburst parameters very"},"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":"1501.06659","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-01-27T05:27:16Z","cross_cats_sorted":[],"title_canon_sha256":"7463e27adbf028349f80d19280969e1d5ff5015500aade9d45a0ae3dc76ccc60","abstract_canon_sha256":"5f34795f699122afe29016c98b33ff0dfafa8aec62eaca803d38f53098b9cfa9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:06.463115Z","signature_b64":"eNCOhGtT7yDwSb9x0iIgdCA5ZcYMnXXMPWUGyY9n6+UO+jDr/ux15wkeUr2+ubc58NshqW5xPf8HMoD3G3APCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"701d8599bb5d49ab146c1e9e2c88ff7f9d8e56528b3e663feba8acb6c67a35f6","last_reissued_at":"2026-05-18T01:41:06.462407Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:06.462407Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ASASSN-14cc: Likely Helium Analog of RZ Leonis Minoris","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"BAV, Berto Monard (Center for Backyard Astronomy Kleinkaroo), Franz-Josef Hambsch (GEOS, Taichi Kato (Kyoto U), Vereniging Voor Sterrenkunde)","submitted_at":"2015-01-27T05:27:16Z","abstract_excerpt":"We identified that ASASSN-14cc is a very active dwarf nova spending approximately 60% of the time in outburst. Our long-term photometry revealed that the object shows long outbursts recurring with a period of 21-33 d and very brief short outbursts lasting less than 1 d. The maximum decline rate exceeds 2.8 mag/d. The duration of long outbursts is 9-18 d, comprising 50-60% of the recurrence time of long outbursts. We detected 0.01560-0.01562 d (22.5 min) modulations during long outbursts, which we identified to be superhumps. These features indicate that ASASSN-14cc has outburst parameters very"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.06659","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":"1501.06659","created_at":"2026-05-18T01:41:06.462518+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.06659v1","created_at":"2026-05-18T01:41:06.462518+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.06659","created_at":"2026-05-18T01:41:06.462518+00:00"},{"alias_kind":"pith_short_12","alias_value":"OAOYLGN3LVE2","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_16","alias_value":"OAOYLGN3LVE2WFDM","created_at":"2026-05-18T12:29:34.919912+00:00"},{"alias_kind":"pith_short_8","alias_value":"OAOYLGN3","created_at":"2026-05-18T12:29:34.919912+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/OAOYLGN3LVE2WFDMD2PCZCH7P6","json":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6.json","graph_json":"https://pith.science/api/pith-number/OAOYLGN3LVE2WFDMD2PCZCH7P6/graph.json","events_json":"https://pith.science/api/pith-number/OAOYLGN3LVE2WFDMD2PCZCH7P6/events.json","paper":"https://pith.science/paper/OAOYLGN3"},"agent_actions":{"view_html":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6","download_json":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6.json","view_paper":"https://pith.science/paper/OAOYLGN3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.06659&json=true","fetch_graph":"https://pith.science/api/pith-number/OAOYLGN3LVE2WFDMD2PCZCH7P6/graph.json","fetch_events":"https://pith.science/api/pith-number/OAOYLGN3LVE2WFDMD2PCZCH7P6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6/action/storage_attestation","attest_author":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6/action/author_attestation","sign_citation":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6/action/citation_signature","submit_replication":"https://pith.science/pith/OAOYLGN3LVE2WFDMD2PCZCH7P6/action/replication_record"}},"created_at":"2026-05-18T01:41:06.462518+00:00","updated_at":"2026-05-18T01:41:06.462518+00:00"}