{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:B5PTFCCWAQAY47Y5B4AZWFO3Z7","short_pith_number":"pith:B5PTFCCW","schema_version":"1.0","canonical_sha256":"0f5f32885604018e7f1d0f019b15dbcfdde825282600a6822d342422e4df53b0","source":{"kind":"arxiv","id":"1205.5807","version":1},"attestation_state":"computed","paper":{"title":"Galactic star formation and accretion histories from matching galaxies to dark matter haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Benjamin P. Moster, Simon D. M. White, Thorsten Naab","submitted_at":"2012-05-25T20:00:04Z","abstract_excerpt":"We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z~4 to the present. This multi-epoch abundance matching (MEAM) model self-consistently takes into account that satellite galaxies first become satellites at times earlier than they are observed. We employ a redshift-dependent parameterization of the stellar-to-halo mass relation to populate haloes and subhaloes in the Millennium simulations with galaxies, requiring that the observed stellar mass functions at"},"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":"1205.5807","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-05-25T20:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"7ab193d6cde680a03c64f784dbec6b2e8ae6f8e0b075ca0b627bd48889786bf6","abstract_canon_sha256":"067cbac623c91a134aa4edda53ef93bdce2ae971c1c43942640cc5dd7e5696eb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:17.041332Z","signature_b64":"0kkVk4KDQOTy0rwlIV53+HpIVK1x1sZyt3mxGMsSQ5dazV+rrTR588fV3YL66cBf5Q/EZudQkzto0aWCywVPBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0f5f32885604018e7f1d0f019b15dbcfdde825282600a6822d342422e4df53b0","last_reissued_at":"2026-05-18T01:57:17.040855Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:17.040855Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic star formation and accretion histories from matching galaxies to dark matter haloes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Benjamin P. Moster, Simon D. M. White, Thorsten Naab","submitted_at":"2012-05-25T20:00:04Z","abstract_excerpt":"We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z~4 to the present. This multi-epoch abundance matching (MEAM) model self-consistently takes into account that satellite galaxies first become satellites at times earlier than they are observed. We employ a redshift-dependent parameterization of the stellar-to-halo mass relation to populate haloes and subhaloes in the Millennium simulations with galaxies, requiring that the observed stellar mass functions at"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.5807","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":"1205.5807","created_at":"2026-05-18T01:57:17.040930+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.5807v1","created_at":"2026-05-18T01:57:17.040930+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.5807","created_at":"2026-05-18T01:57:17.040930+00:00"},{"alias_kind":"pith_short_12","alias_value":"B5PTFCCWAQAY","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"B5PTFCCWAQAY47Y5","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"B5PTFCCW","created_at":"2026-05-18T12:26:58.693483+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":20,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2605.23554","citing_title":"Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope","ref_index":188,"is_internal_anchor":true},{"citing_arxiv_id":"2512.05584","citing_title":"Stellar feedback drives the baryon deficiency in low-mass galaxies","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18975","citing_title":"Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2509.07097","citing_title":"Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2509.09576","citing_title":"Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way","ref_index":97,"is_internal_anchor":false},{"citing_arxiv_id":"2511.00975","citing_title":"The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years","ref_index":99,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00988","citing_title":"Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation","ref_index":213,"is_internal_anchor":false},{"citing_arxiv_id":"2604.03389","citing_title":"The Role of Baryonic and Dark Matter in Bar Kinematics","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06769","citing_title":"Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model","ref_index":238,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08682","citing_title":"The Hubble sequence in JWST CEERS from unbiased galaxy morphologies","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13866","citing_title":"Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies","ref_index":110,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17660","citing_title":"Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17162","citing_title":"Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts","ref_index":95,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17963","citing_title":"BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies","ref_index":117,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19449","citing_title":"Cosmological constraints from the small scale clustering of Emission Line Galaxies","ref_index":146,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00988","citing_title":"Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation","ref_index":213,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23236","citing_title":"The functional form of galaxy and halo luminosity and mass functions","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23147","citing_title":"A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22105","citing_title":"Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers","ref_index":73,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04144","citing_title":"The galaxy-halo connection and the dynamical evolution of a giant disc in a massive node of the Cosmic Web at z~3","ref_index":116,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7","json":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7.json","graph_json":"https://pith.science/api/pith-number/B5PTFCCWAQAY47Y5B4AZWFO3Z7/graph.json","events_json":"https://pith.science/api/pith-number/B5PTFCCWAQAY47Y5B4AZWFO3Z7/events.json","paper":"https://pith.science/paper/B5PTFCCW"},"agent_actions":{"view_html":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7","download_json":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7.json","view_paper":"https://pith.science/paper/B5PTFCCW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.5807&json=true","fetch_graph":"https://pith.science/api/pith-number/B5PTFCCWAQAY47Y5B4AZWFO3Z7/graph.json","fetch_events":"https://pith.science/api/pith-number/B5PTFCCWAQAY47Y5B4AZWFO3Z7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7/action/storage_attestation","attest_author":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7/action/author_attestation","sign_citation":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7/action/citation_signature","submit_replication":"https://pith.science/pith/B5PTFCCWAQAY47Y5B4AZWFO3Z7/action/replication_record"}},"created_at":"2026-05-18T01:57:17.040930+00:00","updated_at":"2026-05-18T01:57:17.040930+00:00"}