{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:JHBILU732GEMV4ZT5DKNTICTRZ","short_pith_number":"pith:JHBILU73","schema_version":"1.0","canonical_sha256":"49c285d3fbd188caf333e8d4d9a0538e7e574fc7fc170e7030aa6b8d263d22c8","source":{"kind":"arxiv","id":"1112.1074","version":2},"attestation_state":"computed","paper":{"title":"Cataclysmic Variables in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Christian Knigge (University of Southampton)","submitted_at":"2011-12-05T21:00:03Z","abstract_excerpt":"Every massive globular cluster (GC) is expected to harbour a significant population of cataclysmic variables (CVs). In this review, I first explain why GC CVs matter astrophysically, how many and what types are theoretically predicted to exist and what observational tools we can use to discover, confirm and study them. I then take a look at how theoretical predictions and observed samples actually stack up to date. In the process, I also reconsider the evidence for two widely held ideas about CVs in GCs: (i) that there must be many fewer dwarf novae than expected; (ii) that the incidence of ma"},"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":"1112.1074","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-12-05T21:00:03Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"dd444b38168f431f085cf0c9f9e16849e4efd2407bff6f7c46f9236bfd8c20ae","abstract_canon_sha256":"ef86a7ab7f76658c04916a723c8f1184de70b6c7d5291f7364edd25add88dd80"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:02:37.271261Z","signature_b64":"a1in2/wKXXA+bBtwWzhNXcupt8NmO0Nn2reAtztOUHhpMXOf8/ZAi1jnjnzu2vls0zXxCgRKRHKCya/mxyISBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"49c285d3fbd188caf333e8d4d9a0538e7e574fc7fc170e7030aa6b8d263d22c8","last_reissued_at":"2026-05-18T04:02:37.270537Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:02:37.270537Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cataclysmic Variables in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Christian Knigge (University of Southampton)","submitted_at":"2011-12-05T21:00:03Z","abstract_excerpt":"Every massive globular cluster (GC) is expected to harbour a significant population of cataclysmic variables (CVs). In this review, I first explain why GC CVs matter astrophysically, how many and what types are theoretically predicted to exist and what observational tools we can use to discover, confirm and study them. I then take a look at how theoretical predictions and observed samples actually stack up to date. In the process, I also reconsider the evidence for two widely held ideas about CVs in GCs: (i) that there must be many fewer dwarf novae than expected; (ii) that the incidence of ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.1074","kind":"arxiv","version":2},"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":"1112.1074","created_at":"2026-05-18T04:02:37.270646+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.1074v2","created_at":"2026-05-18T04:02:37.270646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.1074","created_at":"2026-05-18T04:02:37.270646+00:00"},{"alias_kind":"pith_short_12","alias_value":"JHBILU732GEM","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"JHBILU732GEMV4ZT","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"JHBILU73","created_at":"2026-05-18T12:26:32.869790+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21331","citing_title":"Searching for links between energetic millisecond pulsars and repeating fast radio bursts","ref_index":275,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ","json":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ.json","graph_json":"https://pith.science/api/pith-number/JHBILU732GEMV4ZT5DKNTICTRZ/graph.json","events_json":"https://pith.science/api/pith-number/JHBILU732GEMV4ZT5DKNTICTRZ/events.json","paper":"https://pith.science/paper/JHBILU73"},"agent_actions":{"view_html":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ","download_json":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ.json","view_paper":"https://pith.science/paper/JHBILU73","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.1074&json=true","fetch_graph":"https://pith.science/api/pith-number/JHBILU732GEMV4ZT5DKNTICTRZ/graph.json","fetch_events":"https://pith.science/api/pith-number/JHBILU732GEMV4ZT5DKNTICTRZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ/action/storage_attestation","attest_author":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ/action/author_attestation","sign_citation":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ/action/citation_signature","submit_replication":"https://pith.science/pith/JHBILU732GEMV4ZT5DKNTICTRZ/action/replication_record"}},"created_at":"2026-05-18T04:02:37.270646+00:00","updated_at":"2026-05-18T04:02:37.270646+00:00"}