{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:YALMXX53WYUOOG4A3C4P3ZAYZV","short_pith_number":"pith:YALMXX53","schema_version":"1.0","canonical_sha256":"c016cbdfbbb628e71b80d8b8fde418cd4ad0f162f5587dc8f4375a451fdeb86f","source":{"kind":"arxiv","id":"2605.23841","version":1},"attestation_state":"computed","paper":{"title":"cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"Andrea Pezzotta (cloe-org maintainers), Carmelita Carbone, Casper Vedder (cloe-org contributors), Chiara Moretti, Davide Sciotti, Felicitas Keil, Guadalupe Ca\\~nas-Herrera, Isaac Tutusaus, Jip de Buck, Klara Bertmann, Marco Bonici, Martin Crocce, Martin K\\\"archer, Nastassia Grimm, Nicolas Tessore, Pedro Carrilho, Peter L. Taylor, Santiago Casas, Zahra Baghkhani","submitted_at":"2026-05-22T16:50:05Z","abstract_excerpt":"cloelike is a Python package providing modular, composable Gaussian likelihood classes for the main cosmological large-scale structure observables targeted by the ESA Euclid space mission. It is a core component of the CLOE (Cosmology Likelihood for Observables in Euclid) ecosystem and interfaces directly with cloelib for theoretical predictions and euclidlib for reading official Euclid data products. The package implements Gaussian likelihoods covering harmonic angular power spectra and real-space two-point correlation functions for weak lensing (WL), photometric galaxy clustering (GCph), and"},"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":"2605.23841","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-22T16:50:05Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"744755d031e414feea636bee11b14903c407e7a427cc21c92f77ff23b4ae2f5e","abstract_canon_sha256":"dcf8a7ef1a9969d19e93f704cd9c88ad31731a2f3dc21e70feff4e8ece2a29b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-25T02:02:35.653096Z","signature_b64":"DEuyPhsY3CEwsnVsrw4Kyb19bqOQk3uX9fZ/1VAJUlUKhD8V9Ix2v+K3jPyeToOeNMcKjyctwz8VnK2BPdIdBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c016cbdfbbb628e71b80d8b8fde418cd4ad0f162f5587dc8f4375a451fdeb86f","last_reissued_at":"2026-05-25T02:02:35.652336Z","signature_status":"signed_v1","first_computed_at":"2026-05-25T02:02:35.652336Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.CO","authors_text":"Andrea Pezzotta (cloe-org maintainers), Carmelita Carbone, Casper Vedder (cloe-org contributors), Chiara Moretti, Davide Sciotti, Felicitas Keil, Guadalupe Ca\\~nas-Herrera, Isaac Tutusaus, Jip de Buck, Klara Bertmann, Marco Bonici, Martin Crocce, Martin K\\\"archer, Nastassia Grimm, Nicolas Tessore, Pedro Carrilho, Peter L. Taylor, Santiago Casas, Zahra Baghkhani","submitted_at":"2026-05-22T16:50:05Z","abstract_excerpt":"cloelike is a Python package providing modular, composable Gaussian likelihood classes for the main cosmological large-scale structure observables targeted by the ESA Euclid space mission. It is a core component of the CLOE (Cosmology Likelihood for Observables in Euclid) ecosystem and interfaces directly with cloelib for theoretical predictions and euclidlib for reading official Euclid data products. The package implements Gaussian likelihoods covering harmonic angular power spectra and real-space two-point correlation functions for weak lensing (WL), photometric galaxy clustering (GCph), and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.23841","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/2605.23841/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":"2605.23841","created_at":"2026-05-25T02:02:35.652461+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.23841v1","created_at":"2026-05-25T02:02:35.652461+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.23841","created_at":"2026-05-25T02:02:35.652461+00:00"},{"alias_kind":"pith_short_12","alias_value":"YALMXX53WYUO","created_at":"2026-05-25T02:02:35.652461+00:00"},{"alias_kind":"pith_short_16","alias_value":"YALMXX53WYUOOG4A","created_at":"2026-05-25T02:02:35.652461+00:00"},{"alias_kind":"pith_short_8","alias_value":"YALMXX53","created_at":"2026-05-25T02:02:35.652461+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/YALMXX53WYUOOG4A3C4P3ZAYZV","json":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV.json","graph_json":"https://pith.science/api/pith-number/YALMXX53WYUOOG4A3C4P3ZAYZV/graph.json","events_json":"https://pith.science/api/pith-number/YALMXX53WYUOOG4A3C4P3ZAYZV/events.json","paper":"https://pith.science/paper/YALMXX53"},"agent_actions":{"view_html":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV","download_json":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV.json","view_paper":"https://pith.science/paper/YALMXX53","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.23841&json=true","fetch_graph":"https://pith.science/api/pith-number/YALMXX53WYUOOG4A3C4P3ZAYZV/graph.json","fetch_events":"https://pith.science/api/pith-number/YALMXX53WYUOOG4A3C4P3ZAYZV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV/action/storage_attestation","attest_author":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV/action/author_attestation","sign_citation":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV/action/citation_signature","submit_replication":"https://pith.science/pith/YALMXX53WYUOOG4A3C4P3ZAYZV/action/replication_record"}},"created_at":"2026-05-25T02:02:35.652461+00:00","updated_at":"2026-05-25T02:02:35.652461+00:00"}