{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:432LJKVZUOVWJLSY4JMWOAYYXE","short_pith_number":"pith:432LJKVZ","schema_version":"1.0","canonical_sha256":"e6f4b4aab9a3ab64ae58e259670318b9181b1f2432175dedb27d95cfb3c0e8de","source":{"kind":"arxiv","id":"1707.02609","version":1},"attestation_state":"computed","paper":{"title":"The correlation between the sizes of globular cluster systems and their host dark matter haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Bailey Robison, Michael J. Hudson","submitted_at":"2017-07-09T18:00:00Z","abstract_excerpt":"The sizes of entire systems of globular clusters (GCs) depend on the formation and destruction histories of the GCs themselves, but also on the assembly, merger and accretion history of the dark matter (DM) haloes that they inhabit. Recent work has shown a linear relation between total mass of globular clusters in the globular cluster system and the mass of its host dark matter halo, calibrated from weak lensing. Here we extend this to GC system sizes, by studying the radial density profiles of GCs around galaxies in nearby galaxy groups. We find that radial density profiles of the GC systems "},"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":"1707.02609","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-07-09T18:00:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"e056eff55dc9a6bed74de34ec68b85534717ca7d3e571887d161fb7993cb2621","abstract_canon_sha256":"d604ca08e70fb48abaf46d49f40cbc9fcff90ffe3ed63d63f7d68a6745460cb9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:18:19.894692Z","signature_b64":"E8T95fwfqPPxtFr4inB6j5LgKUZvpGsWwqE/SkPvUt1mLob/wpC1xfd70BT9z6XdPswege5A2yfMnkEcMOjjAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6f4b4aab9a3ab64ae58e259670318b9181b1f2432175dedb27d95cfb3c0e8de","last_reissued_at":"2026-05-18T00:18:19.894013Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:18:19.894013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The correlation between the sizes of globular cluster systems and their host dark matter haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Bailey Robison, Michael J. Hudson","submitted_at":"2017-07-09T18:00:00Z","abstract_excerpt":"The sizes of entire systems of globular clusters (GCs) depend on the formation and destruction histories of the GCs themselves, but also on the assembly, merger and accretion history of the dark matter (DM) haloes that they inhabit. Recent work has shown a linear relation between total mass of globular clusters in the globular cluster system and the mass of its host dark matter halo, calibrated from weak lensing. Here we extend this to GC system sizes, by studying the radial density profiles of GCs around galaxies in nearby galaxy groups. We find that radial density profiles of the GC systems "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.02609","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":"1707.02609","created_at":"2026-05-18T00:18:19.894123+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.02609v1","created_at":"2026-05-18T00:18:19.894123+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.02609","created_at":"2026-05-18T00:18:19.894123+00:00"},{"alias_kind":"pith_short_12","alias_value":"432LJKVZUOVW","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"432LJKVZUOVWJLSY","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"432LJKVZ","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07120","citing_title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","ref_index":118,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE","json":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE.json","graph_json":"https://pith.science/api/pith-number/432LJKVZUOVWJLSY4JMWOAYYXE/graph.json","events_json":"https://pith.science/api/pith-number/432LJKVZUOVWJLSY4JMWOAYYXE/events.json","paper":"https://pith.science/paper/432LJKVZ"},"agent_actions":{"view_html":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE","download_json":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE.json","view_paper":"https://pith.science/paper/432LJKVZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.02609&json=true","fetch_graph":"https://pith.science/api/pith-number/432LJKVZUOVWJLSY4JMWOAYYXE/graph.json","fetch_events":"https://pith.science/api/pith-number/432LJKVZUOVWJLSY4JMWOAYYXE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE/action/storage_attestation","attest_author":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE/action/author_attestation","sign_citation":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE/action/citation_signature","submit_replication":"https://pith.science/pith/432LJKVZUOVWJLSY4JMWOAYYXE/action/replication_record"}},"created_at":"2026-05-18T00:18:19.894123+00:00","updated_at":"2026-05-18T00:18:19.894123+00:00"}