{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:LRGXW4MYVIO76RB2QW6G2R3CZZ","short_pith_number":"pith:LRGXW4MY","schema_version":"1.0","canonical_sha256":"5c4d7b7198aa1dff443a85bc6d4762ce590d441b7ab96df0bba895dcbd549dee","source":{"kind":"arxiv","id":"2008.11207","version":2},"attestation_state":"computed","paper":{"title":"Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alyson M. Brooks, Charlotte R. Christensen, Elaad Applebaum, Ferah Munshi, Michael Tremmel, Sijing Shen, Thomas R. Quinn","submitted_at":"2020-08-25T18:00:02Z","abstract_excerpt":"We present results from the \"Mint\" resolution DC Justice League suite of Milky Way-like zoom-in cosmological simulations, which extend our study of nearby galaxies down into the ultra-faint dwarf (UFD) regime for the first time. The mass resolution of these simulations is the highest ever published for cosmological Milky Way zoom-in simulations run to $z=0$, with initial star (dark matter) particle masses of 994 (17900) M$_\\odot$, and a force resolution of 87 pc. We study the surrounding dwarfs and UFDs, and find the simulations match the observed dynamical properties of galaxies with $-3 < M_"},"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":"2008.11207","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-08-25T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"b675a03c4265e8748c0fc4b62c5dabbe79cc9ea7d48e71d88c1c95a217abd052","abstract_canon_sha256":"80243f9690b120d392f7568eb796a48910b38e9666201cc528950568a8cfacb1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:07:49.307856Z","signature_b64":"A6R0Hux50CoAzCT+KTrE0wRvKF/7zBT1OYMsTXIAaot4IuJ5x1TRSB2zUxFvTqry2EczdVxobgEaOKalSjycCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c4d7b7198aa1dff443a85bc6d4762ce590d441b7ab96df0bba895dcbd549dee","last_reissued_at":"2026-07-05T02:07:49.307425Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:07:49.307425Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ultra-faint dwarfs in a Milky Way context: Introducing the Mint Condition DC Justice League Simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alyson M. Brooks, Charlotte R. Christensen, Elaad Applebaum, Ferah Munshi, Michael Tremmel, Sijing Shen, Thomas R. Quinn","submitted_at":"2020-08-25T18:00:02Z","abstract_excerpt":"We present results from the \"Mint\" resolution DC Justice League suite of Milky Way-like zoom-in cosmological simulations, which extend our study of nearby galaxies down into the ultra-faint dwarf (UFD) regime for the first time. The mass resolution of these simulations is the highest ever published for cosmological Milky Way zoom-in simulations run to $z=0$, with initial star (dark matter) particle masses of 994 (17900) M$_\\odot$, and a force resolution of 87 pc. We study the surrounding dwarfs and UFDs, and find the simulations match the observed dynamical properties of galaxies with $-3 < M_"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.11207","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2008.11207/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":"2008.11207","created_at":"2026-07-05T02:07:49.307483+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.11207v2","created_at":"2026-07-05T02:07:49.307483+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.11207","created_at":"2026-07-05T02:07:49.307483+00:00"},{"alias_kind":"pith_short_12","alias_value":"LRGXW4MYVIO7","created_at":"2026-07-05T02:07:49.307483+00:00"},{"alias_kind":"pith_short_16","alias_value":"LRGXW4MYVIO76RB2","created_at":"2026-07-05T02:07:49.307483+00:00"},{"alias_kind":"pith_short_8","alias_value":"LRGXW4MY","created_at":"2026-07-05T02:07:49.307483+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.07470","citing_title":"Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps","ref_index":79,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ","json":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ.json","graph_json":"https://pith.science/api/pith-number/LRGXW4MYVIO76RB2QW6G2R3CZZ/graph.json","events_json":"https://pith.science/api/pith-number/LRGXW4MYVIO76RB2QW6G2R3CZZ/events.json","paper":"https://pith.science/paper/LRGXW4MY"},"agent_actions":{"view_html":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ","download_json":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ.json","view_paper":"https://pith.science/paper/LRGXW4MY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.11207&json=true","fetch_graph":"https://pith.science/api/pith-number/LRGXW4MYVIO76RB2QW6G2R3CZZ/graph.json","fetch_events":"https://pith.science/api/pith-number/LRGXW4MYVIO76RB2QW6G2R3CZZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ/action/storage_attestation","attest_author":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ/action/author_attestation","sign_citation":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ/action/citation_signature","submit_replication":"https://pith.science/pith/LRGXW4MYVIO76RB2QW6G2R3CZZ/action/replication_record"}},"created_at":"2026-07-05T02:07:49.307483+00:00","updated_at":"2026-07-05T02:07:49.307483+00:00"}