{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:YGCWYFS53C5DPIVZHDVX2RNWYG","short_pith_number":"pith:YGCWYFS5","schema_version":"1.0","canonical_sha256":"c1856c165dd8ba37a2b938eb7d45b6c1ad74daa61242dcdbf0693e40b4a84879","source":{"kind":"arxiv","id":"2507.07991","version":1},"attestation_state":"computed","paper":{"title":"Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrina Nicola, Aurel Schneider, Joop Schaye, Jozef Bucko, Matthieu Schaller, Michael Kova\\v{c}, Robert Reischke, Romain Teyssier, Sambit K. Giri","submitted_at":"2025-07-10T17:59:06Z","abstract_excerpt":"Baryonic feedback alters the matter distribution on small and intermediate scales, posing a challenge for precision cosmology. The new, component-wise baryonification (BFC) approach provides a self-consistent framework to model feedback effects for different observables. In this paper we use this framework to fit kinematic Sunyaev-Zel'dovich (kSZ) observations from the Atacama Cosmology Telescope (ACT) alongside halo X-ray gas fractions from eROSITA, investigating baryonic feedback in a cosmological context. We first show that the kSZ data from ACT is consistent with the gas fractions from eRO"},"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":"2507.07991","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-07-10T17:59:06Z","cross_cats_sorted":[],"title_canon_sha256":"f5d4461e7c201d2c5dee911ae57d47cea09ef8454823c20b8dfa0e938f452854","abstract_canon_sha256":"b123d0d7716ab34aeca6f1affd4697ac8e9e78cfb0e54cabfb9128b86727964f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:35:08.292137Z","signature_b64":"BYNI6i3++EAa5x0Bic1Ajvi5M8CT7lYy0ePP5lMwJ2yO84BYeCgMTXBBU5HGLJ01JkUeIbBHa+gzdulNpxCWBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c1856c165dd8ba37a2b938eb7d45b6c1ad74daa61242dcdbf0693e40b4a84879","last_reissued_at":"2026-07-05T11:35:08.291592Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:35:08.291592Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrina Nicola, Aurel Schneider, Joop Schaye, Jozef Bucko, Matthieu Schaller, Michael Kova\\v{c}, Robert Reischke, Romain Teyssier, Sambit K. Giri","submitted_at":"2025-07-10T17:59:06Z","abstract_excerpt":"Baryonic feedback alters the matter distribution on small and intermediate scales, posing a challenge for precision cosmology. The new, component-wise baryonification (BFC) approach provides a self-consistent framework to model feedback effects for different observables. In this paper we use this framework to fit kinematic Sunyaev-Zel'dovich (kSZ) observations from the Atacama Cosmology Telescope (ACT) alongside halo X-ray gas fractions from eROSITA, investigating baryonic feedback in a cosmological context. We first show that the kSZ data from ACT is consistent with the gas fractions from eRO"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.07991","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/2507.07991/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":"2507.07991","created_at":"2026-07-05T11:35:08.291662+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.07991v1","created_at":"2026-07-05T11:35:08.291662+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.07991","created_at":"2026-07-05T11:35:08.291662+00:00"},{"alias_kind":"pith_short_12","alias_value":"YGCWYFS53C5D","created_at":"2026-07-05T11:35:08.291662+00:00"},{"alias_kind":"pith_short_16","alias_value":"YGCWYFS53C5DPIVZ","created_at":"2026-07-05T11:35:08.291662+00:00"},{"alias_kind":"pith_short_8","alias_value":"YGCWYFS5","created_at":"2026-07-05T11:35:08.291662+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.29388","citing_title":"Probing the Baryon Distribution with Fast Radio Bursts","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2512.11041","citing_title":"KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19744","citing_title":"Precision Kinematic Sunyaev--Zel'dovich Measurements Across Halo Mass and Redshift with DESI DR2 and ACT DR6: Part I. Luminous Red Galaxies","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG","json":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG.json","graph_json":"https://pith.science/api/pith-number/YGCWYFS53C5DPIVZHDVX2RNWYG/graph.json","events_json":"https://pith.science/api/pith-number/YGCWYFS53C5DPIVZHDVX2RNWYG/events.json","paper":"https://pith.science/paper/YGCWYFS5"},"agent_actions":{"view_html":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG","download_json":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG.json","view_paper":"https://pith.science/paper/YGCWYFS5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.07991&json=true","fetch_graph":"https://pith.science/api/pith-number/YGCWYFS53C5DPIVZHDVX2RNWYG/graph.json","fetch_events":"https://pith.science/api/pith-number/YGCWYFS53C5DPIVZHDVX2RNWYG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG/action/storage_attestation","attest_author":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG/action/author_attestation","sign_citation":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG/action/citation_signature","submit_replication":"https://pith.science/pith/YGCWYFS53C5DPIVZHDVX2RNWYG/action/replication_record"}},"created_at":"2026-07-05T11:35:08.291662+00:00","updated_at":"2026-07-05T11:35:08.291662+00:00"}