{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:RGUBPB6JA7LVCNNBE45JPQ6E32","short_pith_number":"pith:RGUBPB6J","schema_version":"1.0","canonical_sha256":"89a81787c907d75135a1273a97c3c4deaa0d60971af48b2ccc074943e1311be3","source":{"kind":"arxiv","id":"1904.11966","version":3},"attestation_state":"computed","paper":{"title":"HACC Cosmological Simulations: First Data Release","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"Adrian Pope, Benjamin S. Allen, Danila Korytov, Esteban Rangel, Hal Finkel, Ian Foster, Joseph Hollowed, Katrin Heitmann, Kyle Chard, Nicholas Frontiere, Patricia Larsen, Salman Habib, Thomas D. Uram","submitted_at":"2019-04-26T17:50:48Z","abstract_excerpt":"We describe the first major public data release from cosmological simulations carried out with Argonne's HACC code. This initial release covers a range of datasets from large gravity-only simulations. The data products include halo information for multiple redshifts, down-sampled particles, and lightcone outputs. We provide data from two very large LCDM simulations as well as beyond-LCDM simulations spanning eleven w0-wa cosmologies. Our release platform uses Petrel, a research data service, located at the Argonne Leadership Computing Facility. Petrel offers fast data transfer mechanisms and a"},"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":"1904.11966","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-04-26T17:50:48Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"73a77d569cd0fdcbde2289d435e6be952274ba925401e0633a8dffebc9e3859d","abstract_canon_sha256":"17ab389d8939a4a745e5a551afd01f53dc5a5c7ecc18703b89778b1bcc0744d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:09:25.502174Z","signature_b64":"/zhQjWOsuD7IzPFw/qBttiwKW2EM+YfrSS8y+4br9epNRLooj0M1YVSkKz2W210Oy+E2+zUOTEfIoGcZhKfXAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"89a81787c907d75135a1273a97c3c4deaa0d60971af48b2ccc074943e1311be3","last_reissued_at":"2026-07-05T00:09:25.501672Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:09:25.501672Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"HACC Cosmological Simulations: First Data Release","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"Adrian Pope, Benjamin S. Allen, Danila Korytov, Esteban Rangel, Hal Finkel, Ian Foster, Joseph Hollowed, Katrin Heitmann, Kyle Chard, Nicholas Frontiere, Patricia Larsen, Salman Habib, Thomas D. Uram","submitted_at":"2019-04-26T17:50:48Z","abstract_excerpt":"We describe the first major public data release from cosmological simulations carried out with Argonne's HACC code. This initial release covers a range of datasets from large gravity-only simulations. The data products include halo information for multiple redshifts, down-sampled particles, and lightcone outputs. We provide data from two very large LCDM simulations as well as beyond-LCDM simulations spanning eleven w0-wa cosmologies. Our release platform uses Petrel, a research data service, located at the Argonne Leadership Computing Facility. Petrel offers fast data transfer mechanisms and a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.11966","kind":"arxiv","version":3},"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/1904.11966/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":"1904.11966","created_at":"2026-07-05T00:09:25.501735+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.11966v3","created_at":"2026-07-05T00:09:25.501735+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.11966","created_at":"2026-07-05T00:09:25.501735+00:00"},{"alias_kind":"pith_short_12","alias_value":"RGUBPB6JA7LV","created_at":"2026-07-05T00:09:25.501735+00:00"},{"alias_kind":"pith_short_16","alias_value":"RGUBPB6JA7LVCNNB","created_at":"2026-07-05T00:09:25.501735+00:00"},{"alias_kind":"pith_short_8","alias_value":"RGUBPB6J","created_at":"2026-07-05T00:09:25.501735+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2301.09655","citing_title":"Perturbation-theory informed integrators for cosmological simulations","ref_index":12,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32","json":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32.json","graph_json":"https://pith.science/api/pith-number/RGUBPB6JA7LVCNNBE45JPQ6E32/graph.json","events_json":"https://pith.science/api/pith-number/RGUBPB6JA7LVCNNBE45JPQ6E32/events.json","paper":"https://pith.science/paper/RGUBPB6J"},"agent_actions":{"view_html":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32","download_json":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32.json","view_paper":"https://pith.science/paper/RGUBPB6J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.11966&json=true","fetch_graph":"https://pith.science/api/pith-number/RGUBPB6JA7LVCNNBE45JPQ6E32/graph.json","fetch_events":"https://pith.science/api/pith-number/RGUBPB6JA7LVCNNBE45JPQ6E32/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32/action/storage_attestation","attest_author":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32/action/author_attestation","sign_citation":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32/action/citation_signature","submit_replication":"https://pith.science/pith/RGUBPB6JA7LVCNNBE45JPQ6E32/action/replication_record"}},"created_at":"2026-07-05T00:09:25.501735+00:00","updated_at":"2026-07-05T00:09:25.501735+00:00"}