{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:MJMUPGC5KSFWUYKP3RDT7DPFFQ","short_pith_number":"pith:MJMUPGC5","schema_version":"1.0","canonical_sha256":"625947985d548b6a614fdc473f8de52c21be8d546b1b3997ee6b6a1a53c4f4e0","source":{"kind":"arxiv","id":"2407.21103","version":1},"attestation_state":"computed","paper":{"title":"The MillenniumTNG Project: Impact of massive neutrinos on the cosmic large-scale structure and the distribution of galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adrian Jenkins, Ana Maria Delgado, Boryana Hadzhiyska, Carlos Frenk, C\\'esar Hern\\'andez-Aguayo, Fulvio Ferlito, Lars Hernquist, Monica Barrera, Rahul Kannan, R\\\"udiger Pakmor, Simon D. M. White, Sownak Bose, Volker Springel","submitted_at":"2024-07-30T18:00:04Z","abstract_excerpt":"We discuss the cold dark matter plus massive neutrinos simulations of the MillenniumTNG (MTNG) project, which aim to improve understanding of how well ongoing and future large-scale galaxy surveys will measure neutrino masses. Our largest simulations, $3000\\,{\\rm Mpc}$ on a side, use $10240^3$ particles of mass $m_{p} = 6.66\\times 10^{8}\\,h^{-1}{\\rm M}_\\odot$ to represent cold dark matter, and $2560^3$ to represent a population of neutrinos with summed mass $M_\\nu = 100\\,{\\rm meV}$. Smaller volume runs with $\\sim 630\\,{\\rm Mpc}$ also include cases with $M_\\nu = 0\\,\\textrm{and}\\, 300\\,{\\rm meV}"},"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":"2407.21103","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-07-30T18:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"33c73713e0ea4622b32a7a1066aef384fcdaa9f4636124a91d901c2aeafcddf7","abstract_canon_sha256":"28b3822093ed547361d094123905a8f92f34e296dcc90a359ec9f8985ce6f397"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:50:34.044342Z","signature_b64":"xMhCeMtzbuvInezPB72TlgvuRmyXctPQjOIVtCPuKbfrlLJ4ncuLnY/Mq+O24MGG6yw6omp5O5u1YS5nEpxHCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"625947985d548b6a614fdc473f8de52c21be8d546b1b3997ee6b6a1a53c4f4e0","last_reissued_at":"2026-07-05T08:50:34.043902Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:50:34.043902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The MillenniumTNG Project: Impact of massive neutrinos on the cosmic large-scale structure and the distribution of galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adrian Jenkins, Ana Maria Delgado, Boryana Hadzhiyska, Carlos Frenk, C\\'esar Hern\\'andez-Aguayo, Fulvio Ferlito, Lars Hernquist, Monica Barrera, Rahul Kannan, R\\\"udiger Pakmor, Simon D. M. White, Sownak Bose, Volker Springel","submitted_at":"2024-07-30T18:00:04Z","abstract_excerpt":"We discuss the cold dark matter plus massive neutrinos simulations of the MillenniumTNG (MTNG) project, which aim to improve understanding of how well ongoing and future large-scale galaxy surveys will measure neutrino masses. Our largest simulations, $3000\\,{\\rm Mpc}$ on a side, use $10240^3$ particles of mass $m_{p} = 6.66\\times 10^{8}\\,h^{-1}{\\rm M}_\\odot$ to represent cold dark matter, and $2560^3$ to represent a population of neutrinos with summed mass $M_\\nu = 100\\,{\\rm meV}$. Smaller volume runs with $\\sim 630\\,{\\rm Mpc}$ also include cases with $M_\\nu = 0\\,\\textrm{and}\\, 300\\,{\\rm meV}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.21103","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/2407.21103/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":"2407.21103","created_at":"2026-07-05T08:50:34.043957+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.21103v1","created_at":"2026-07-05T08:50:34.043957+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.21103","created_at":"2026-07-05T08:50:34.043957+00:00"},{"alias_kind":"pith_short_12","alias_value":"MJMUPGC5KSFW","created_at":"2026-07-05T08:50:34.043957+00:00"},{"alias_kind":"pith_short_16","alias_value":"MJMUPGC5KSFWUYKP","created_at":"2026-07-05T08:50:34.043957+00:00"},{"alias_kind":"pith_short_8","alias_value":"MJMUPGC5","created_at":"2026-07-05T08:50:34.043957+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26237","citing_title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","ref_index":114,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ","json":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ.json","graph_json":"https://pith.science/api/pith-number/MJMUPGC5KSFWUYKP3RDT7DPFFQ/graph.json","events_json":"https://pith.science/api/pith-number/MJMUPGC5KSFWUYKP3RDT7DPFFQ/events.json","paper":"https://pith.science/paper/MJMUPGC5"},"agent_actions":{"view_html":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ","download_json":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ.json","view_paper":"https://pith.science/paper/MJMUPGC5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.21103&json=true","fetch_graph":"https://pith.science/api/pith-number/MJMUPGC5KSFWUYKP3RDT7DPFFQ/graph.json","fetch_events":"https://pith.science/api/pith-number/MJMUPGC5KSFWUYKP3RDT7DPFFQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ/action/storage_attestation","attest_author":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ/action/author_attestation","sign_citation":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ/action/citation_signature","submit_replication":"https://pith.science/pith/MJMUPGC5KSFWUYKP3RDT7DPFFQ/action/replication_record"}},"created_at":"2026-07-05T08:50:34.043957+00:00","updated_at":"2026-07-05T08:50:34.043957+00:00"}