{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:LOY6GEKHBXXEOML6ODMPB3U6C7","short_pith_number":"pith:LOY6GEKH","schema_version":"1.0","canonical_sha256":"5bb1e311470dee47317e70d8f0ee9e17fb85be5a92f2fe80064771f8f66b0e34","source":{"kind":"arxiv","id":"1505.05506","version":1},"attestation_state":"computed","paper":{"title":"Tidal stripping of globular clusters in a simulated galaxy cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Felipe Ramos, Hern\\'an Muriel, Mario Abadi, Valeria Coenda","submitted_at":"2015-05-20T20:00:26Z","abstract_excerpt":"Using a cosmological N-body numerical simulation of the formation of a galaxy cluster- sized halo, we analyze the temporal evolution of its globular cluster population. We follow the dynamical evolution of 38 galactic dark matter halos orbiting in a galaxy cluster that at redshift z=0 has a virial mass of 1.71 * 10 ^14 Msol h^-1. In order to mimic both \"blue\" and \"red\" populations of globular clusters, for each galactic halo we select two different sets of particles at high redshift (z ~ 1), constrained by the condition that, at redshift z=0, their average radial density profiles are similar t"},"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":"1505.05506","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-05-20T20:00:26Z","cross_cats_sorted":[],"title_canon_sha256":"c998c974e40685b209ede5d62f222f97f951e13099b138483b584d7d948d5557","abstract_canon_sha256":"ec9299426da079165463fef88b3c573eacf64a4796782fb55d4f041028bb33b4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:54.455779Z","signature_b64":"dQO3+MZmoonux4kJQdy/bVgPz5swh0tBtlZIBlAd+H2fCZElMy5AVdC21TGeS21Ap2uHzj5EC08sYcb9wIJaBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5bb1e311470dee47317e70d8f0ee9e17fb85be5a92f2fe80064771f8f66b0e34","last_reissued_at":"2026-05-18T02:03:54.455120Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:54.455120Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tidal stripping of globular clusters in a simulated galaxy cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Felipe Ramos, Hern\\'an Muriel, Mario Abadi, Valeria Coenda","submitted_at":"2015-05-20T20:00:26Z","abstract_excerpt":"Using a cosmological N-body numerical simulation of the formation of a galaxy cluster- sized halo, we analyze the temporal evolution of its globular cluster population. We follow the dynamical evolution of 38 galactic dark matter halos orbiting in a galaxy cluster that at redshift z=0 has a virial mass of 1.71 * 10 ^14 Msol h^-1. In order to mimic both \"blue\" and \"red\" populations of globular clusters, for each galactic halo we select two different sets of particles at high redshift (z ~ 1), constrained by the condition that, at redshift z=0, their average radial density profiles are similar t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.05506","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":"1505.05506","created_at":"2026-05-18T02:03:54.455254+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.05506v1","created_at":"2026-05-18T02:03:54.455254+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.05506","created_at":"2026-05-18T02:03:54.455254+00:00"},{"alias_kind":"pith_short_12","alias_value":"LOY6GEKHBXXE","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"LOY6GEKHBXXEOML6","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"LOY6GEKH","created_at":"2026-05-18T12:29:29.992203+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/LOY6GEKHBXXEOML6ODMPB3U6C7","json":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7.json","graph_json":"https://pith.science/api/pith-number/LOY6GEKHBXXEOML6ODMPB3U6C7/graph.json","events_json":"https://pith.science/api/pith-number/LOY6GEKHBXXEOML6ODMPB3U6C7/events.json","paper":"https://pith.science/paper/LOY6GEKH"},"agent_actions":{"view_html":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7","download_json":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7.json","view_paper":"https://pith.science/paper/LOY6GEKH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.05506&json=true","fetch_graph":"https://pith.science/api/pith-number/LOY6GEKHBXXEOML6ODMPB3U6C7/graph.json","fetch_events":"https://pith.science/api/pith-number/LOY6GEKHBXXEOML6ODMPB3U6C7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7/action/storage_attestation","attest_author":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7/action/author_attestation","sign_citation":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7/action/citation_signature","submit_replication":"https://pith.science/pith/LOY6GEKHBXXEOML6ODMPB3U6C7/action/replication_record"}},"created_at":"2026-05-18T02:03:54.455254+00:00","updated_at":"2026-05-18T02:03:54.455254+00:00"}