{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:VKLLJTF3GLGPL6VDRTLDJTRMZV","short_pith_number":"pith:VKLLJTF3","schema_version":"1.0","canonical_sha256":"aa96b4ccbb32ccf5faa38cd634ce2ccd625374623c7c92eb0c50143c783a7558","source":{"kind":"arxiv","id":"2006.08625","version":1},"attestation_state":"computed","paper":{"title":"Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Bonaca, Benjamin D. Johnson, Charlie Conroy, Dennis Zaritsky, Nelson Caldwell, Phillip A. Cargile, Rohan P. Naidu, Yuan-Sen Ting","submitted_at":"2020-06-15T18:00:01Z","abstract_excerpt":"In the $\\Lambda$CDM paradigm the Galactic stellar halo is predicted to harbor the accreted debris of smaller systems. To identify these systems, the H3 Spectroscopic Survey, combined with $Gaia$, is gathering 6D phase-space and chemical information in the distant Galaxy. Here we present a comprehensive inventory of structure within 50 kpc from the Galactic center using a sample of 5684 giants at $|b|>40^{\\circ}$ and $|Z|>2$ kpc. We identify known structures including the high-$\\alpha$ disk, the in-situ halo (disk stars heated to eccentric orbits), Sagittarius (Sgr), $Gaia$-Sausage-Enceladus (G"},"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":"2006.08625","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-06-15T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"82822d31a4d6a90696aa9858844c97ac3f77f5a134b26d62575db62712dadd1d","abstract_canon_sha256":"edf66b18cfb5ff956de6022d48093e14ffa3bd9d67cd1bcbd9bd2bb0f67a15c4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:38:38.062265Z","signature_b64":"mQiKDRMMviQAccBTGpGtR+O9ZrTO03q4vHISJWFmW4IEfl8NFFfQ/N9FTy0kbUlCUwDqubTEI07rNgVq9CECDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aa96b4ccbb32ccf5faa38cd634ce2ccd625374623c7c92eb0c50143c783a7558","last_reissued_at":"2026-07-05T01:38:38.061769Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:38:38.061769Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Ana Bonaca, Benjamin D. Johnson, Charlie Conroy, Dennis Zaritsky, Nelson Caldwell, Phillip A. Cargile, Rohan P. Naidu, Yuan-Sen Ting","submitted_at":"2020-06-15T18:00:01Z","abstract_excerpt":"In the $\\Lambda$CDM paradigm the Galactic stellar halo is predicted to harbor the accreted debris of smaller systems. To identify these systems, the H3 Spectroscopic Survey, combined with $Gaia$, is gathering 6D phase-space and chemical information in the distant Galaxy. Here we present a comprehensive inventory of structure within 50 kpc from the Galactic center using a sample of 5684 giants at $|b|>40^{\\circ}$ and $|Z|>2$ kpc. We identify known structures including the high-$\\alpha$ disk, the in-situ halo (disk stars heated to eccentric orbits), Sagittarius (Sgr), $Gaia$-Sausage-Enceladus (G"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.08625","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2006.08625/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2006.08625","created_at":"2026-07-05T01:38:38.061851+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.08625v1","created_at":"2026-07-05T01:38:38.061851+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.08625","created_at":"2026-07-05T01:38:38.061851+00:00"},{"alias_kind":"pith_short_12","alias_value":"VKLLJTF3GLGP","created_at":"2026-07-05T01:38:38.061851+00:00"},{"alias_kind":"pith_short_16","alias_value":"VKLLJTF3GLGPL6VD","created_at":"2026-07-05T01:38:38.061851+00:00"},{"alias_kind":"pith_short_8","alias_value":"VKLLJTF3","created_at":"2026-07-05T01:38:38.061851+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05510","citing_title":"Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams","ref_index":49,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV","json":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV.json","graph_json":"https://pith.science/api/pith-number/VKLLJTF3GLGPL6VDRTLDJTRMZV/graph.json","events_json":"https://pith.science/api/pith-number/VKLLJTF3GLGPL6VDRTLDJTRMZV/events.json","paper":"https://pith.science/paper/VKLLJTF3"},"agent_actions":{"view_html":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV","download_json":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV.json","view_paper":"https://pith.science/paper/VKLLJTF3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.08625&json=true","fetch_graph":"https://pith.science/api/pith-number/VKLLJTF3GLGPL6VDRTLDJTRMZV/graph.json","fetch_events":"https://pith.science/api/pith-number/VKLLJTF3GLGPL6VDRTLDJTRMZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV/action/storage_attestation","attest_author":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV/action/author_attestation","sign_citation":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV/action/citation_signature","submit_replication":"https://pith.science/pith/VKLLJTF3GLGPL6VDRTLDJTRMZV/action/replication_record"}},"created_at":"2026-07-05T01:38:38.061851+00:00","updated_at":"2026-07-05T01:38:38.061851+00:00"}