{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:ZCENQVWC24YFE3BXZJPHXH3PN3","short_pith_number":"pith:ZCENQVWC","schema_version":"1.0","canonical_sha256":"c888d856c2d730526c37ca5e7b9f6f6ed425826121662abb8badb3d30b478381","source":{"kind":"arxiv","id":"1103.2121","version":4},"attestation_state":"computed","paper":{"title":"The scatter about the \"Universal\" dwarf spheroidal mass profile: A kinematic study of the M31 satellites, And V and And VI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. M. Brooks, A. M. N. Ferguson, A. W. McConnachie, G. F. Lewis, J. Pe\\~narrubia, K. Venn, M. J. Irwin, M. L. M. Collins, N. Arimoto, R. A. Ibata, R. M. Rich, S. C. Chapman","submitted_at":"2011-03-10T20:50:59Z","abstract_excerpt":"While the satellites of the Milky Way (MW) have been shown to be largely consistent in terms of their mass contained within one half--light radius (M_{half}) with a \"Universal\" mass profile, a number of M31 satellites are found to be inconsistent with such relations, and seem kinematically colder in their central regions than their MW cousins. In this work, we present new kinematic and updated structural properties for two M31 dSphs, And V and And VI using data from the Keck Low Resolution Imaging Spectrograph (LRIS) and the DEep Imaging Multi-Object Spectrograph (DEIMOS) instruments and the S"},"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":"1103.2121","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-03-10T20:50:59Z","cross_cats_sorted":[],"title_canon_sha256":"4f6d251bab67a3d47c3b0171ead6ddee5129155f21dabdee1e95c2d5538eaa41","abstract_canon_sha256":"f2290ad01da0fc2347ab8a1f6e5ba6ba5276fb8be8f2bd86a783d6cfc2784151"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:54.912875Z","signature_b64":"eRRhBHcAfD67TKrLSkMpgsAiYDltWWT/QqqhcVQZPm4U3NjW7jG/4SUSsVMWuY7aQu/4679P167NBmi8u4wHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c888d856c2d730526c37ca5e7b9f6f6ed425826121662abb8badb3d30b478381","last_reissued_at":"2026-05-18T02:02:54.912246Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:54.912246Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The scatter about the \"Universal\" dwarf spheroidal mass profile: A kinematic study of the M31 satellites, And V and And VI","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. M. Brooks, A. M. N. Ferguson, A. W. McConnachie, G. F. Lewis, J. Pe\\~narrubia, K. Venn, M. J. Irwin, M. L. M. Collins, N. Arimoto, R. A. Ibata, R. M. Rich, S. C. Chapman","submitted_at":"2011-03-10T20:50:59Z","abstract_excerpt":"While the satellites of the Milky Way (MW) have been shown to be largely consistent in terms of their mass contained within one half--light radius (M_{half}) with a \"Universal\" mass profile, a number of M31 satellites are found to be inconsistent with such relations, and seem kinematically colder in their central regions than their MW cousins. In this work, we present new kinematic and updated structural properties for two M31 dSphs, And V and And VI using data from the Keck Low Resolution Imaging Spectrograph (LRIS) and the DEep Imaging Multi-Object Spectrograph (DEIMOS) instruments and the S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.2121","kind":"arxiv","version":4},"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":"1103.2121","created_at":"2026-05-18T02:02:54.912352+00:00"},{"alias_kind":"arxiv_version","alias_value":"1103.2121v4","created_at":"2026-05-18T02:02:54.912352+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.2121","created_at":"2026-05-18T02:02:54.912352+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZCENQVWC24YF","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZCENQVWC24YFE3BX","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZCENQVWC","created_at":"2026-05-18T12:26:47.523578+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/ZCENQVWC24YFE3BXZJPHXH3PN3","json":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3.json","graph_json":"https://pith.science/api/pith-number/ZCENQVWC24YFE3BXZJPHXH3PN3/graph.json","events_json":"https://pith.science/api/pith-number/ZCENQVWC24YFE3BXZJPHXH3PN3/events.json","paper":"https://pith.science/paper/ZCENQVWC"},"agent_actions":{"view_html":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3","download_json":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3.json","view_paper":"https://pith.science/paper/ZCENQVWC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1103.2121&json=true","fetch_graph":"https://pith.science/api/pith-number/ZCENQVWC24YFE3BXZJPHXH3PN3/graph.json","fetch_events":"https://pith.science/api/pith-number/ZCENQVWC24YFE3BXZJPHXH3PN3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3/action/storage_attestation","attest_author":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3/action/author_attestation","sign_citation":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3/action/citation_signature","submit_replication":"https://pith.science/pith/ZCENQVWC24YFE3BXZJPHXH3PN3/action/replication_record"}},"created_at":"2026-05-18T02:02:54.912352+00:00","updated_at":"2026-05-18T02:02:54.912352+00:00"}