{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:W3YOWPTOLZECSRVTL2IGT64356","short_pith_number":"pith:W3YOWPTO","schema_version":"1.0","canonical_sha256":"b6f0eb3e6e5e482946b35e9069fb9bef90c3ea582f4657c2b7196fef1c657bf5","source":{"kind":"arxiv","id":"2210.10803","version":1},"attestation_state":"computed","paper":{"title":"GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Alexis Finoguenov, Andrea Biviano, Andreea S. Font, Andrew M. M. Reeves, Benedetta Vulcani, Bianca Poggianti, Chris Lidman, Dennis Zaritsky, Devontae C. Baxter, Egidijus Kukstas, Florian Sarron, Gabriella De Lucia, Gillian Wilson, Gregory Rudnick, Howard K. C. Yee, Ian G. McCarthy, Irene Pintos-Castro, Jeffrey C. Chan, Julie Nantais, Justin Marchioni, Kristi Webb, Lyndsay Old, M. C. Cooper, Michael L. Balogh, Pascale Jablonka, Pierluigi Cerulo, Remco van der Burg, Ricardo Demarco, Sean McGee, Yannick M. Bahe","submitted_at":"2022-10-19T18:00:05Z","abstract_excerpt":"Recent observations have shown that the environmental quenching of galaxies at z ~ 1 is qualitatively different to that in the local Universe. However, the physical origin of these differences has not yet been elucidated. In addition, while low-redshift comparisons between observed environmental trends and the predictions of cosmological hydrodynamical simulations are now routine, there have been relatively few comparisons at higher redshifts to date. Here we confront three state-of-the-art suites of simulations (BAHAMAS+MACSIS, EAGLE+Hydrangea, IllustrisTNG) with state-of-the-art observations"},"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":"2210.10803","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-10-19T18:00:05Z","cross_cats_sorted":[],"title_canon_sha256":"4d428f6d6f3e0a9db50647320481ca58277e995a643eac78e8dc90fd15df43c8","abstract_canon_sha256":"2d4e50debecc3baf669fa6951d6fde4052b89aaed958f309b511d38bee1e70e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:22:58.192401Z","signature_b64":"2TsSAy+FDvMMGEhh6vvcheWICPXQVXbDP21RN4bIJVQLzITuZSz1OxIM7bywlGZpB08Qnn1QXFLal03g+jSZBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b6f0eb3e6e5e482946b35e9069fb9bef90c3ea582f4657c2b7196fef1c657bf5","last_reissued_at":"2026-07-05T05:22:58.191925Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:22:58.191925Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Alexis Finoguenov, Andrea Biviano, Andreea S. Font, Andrew M. M. Reeves, Benedetta Vulcani, Bianca Poggianti, Chris Lidman, Dennis Zaritsky, Devontae C. Baxter, Egidijus Kukstas, Florian Sarron, Gabriella De Lucia, Gillian Wilson, Gregory Rudnick, Howard K. C. Yee, Ian G. McCarthy, Irene Pintos-Castro, Jeffrey C. Chan, Julie Nantais, Justin Marchioni, Kristi Webb, Lyndsay Old, M. C. Cooper, Michael L. Balogh, Pascale Jablonka, Pierluigi Cerulo, Remco van der Burg, Ricardo Demarco, Sean McGee, Yannick M. Bahe","submitted_at":"2022-10-19T18:00:05Z","abstract_excerpt":"Recent observations have shown that the environmental quenching of galaxies at z ~ 1 is qualitatively different to that in the local Universe. However, the physical origin of these differences has not yet been elucidated. In addition, while low-redshift comparisons between observed environmental trends and the predictions of cosmological hydrodynamical simulations are now routine, there have been relatively few comparisons at higher redshifts to date. Here we confront three state-of-the-art suites of simulations (BAHAMAS+MACSIS, EAGLE+Hydrangea, IllustrisTNG) with state-of-the-art observations"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.10803","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/2210.10803/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":"2210.10803","created_at":"2026-07-05T05:22:58.191985+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.10803v1","created_at":"2026-07-05T05:22:58.191985+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.10803","created_at":"2026-07-05T05:22:58.191985+00:00"},{"alias_kind":"pith_short_12","alias_value":"W3YOWPTOLZEC","created_at":"2026-07-05T05:22:58.191985+00:00"},{"alias_kind":"pith_short_16","alias_value":"W3YOWPTOLZECSRVT","created_at":"2026-07-05T05:22:58.191985+00:00"},{"alias_kind":"pith_short_8","alias_value":"W3YOWPTO","created_at":"2026-07-05T05:22:58.191985+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356","json":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356.json","graph_json":"https://pith.science/api/pith-number/W3YOWPTOLZECSRVTL2IGT64356/graph.json","events_json":"https://pith.science/api/pith-number/W3YOWPTOLZECSRVTL2IGT64356/events.json","paper":"https://pith.science/paper/W3YOWPTO"},"agent_actions":{"view_html":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356","download_json":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356.json","view_paper":"https://pith.science/paper/W3YOWPTO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.10803&json=true","fetch_graph":"https://pith.science/api/pith-number/W3YOWPTOLZECSRVTL2IGT64356/graph.json","fetch_events":"https://pith.science/api/pith-number/W3YOWPTOLZECSRVTL2IGT64356/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356/action/storage_attestation","attest_author":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356/action/author_attestation","sign_citation":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356/action/citation_signature","submit_replication":"https://pith.science/pith/W3YOWPTOLZECSRVTL2IGT64356/action/replication_record"}},"created_at":"2026-07-05T05:22:58.191985+00:00","updated_at":"2026-07-05T05:22:58.191985+00:00"}