{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2025:SI4DQJWHZ7FZ7RB7MZYQ2Q4THD","short_pith_number":"pith:SI4DQJWH","canonical_record":{"source":{"id":"2503.00112","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-28T19:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"50d91645b5b93f403450492f15263cad7e5c02641a02787a695b9c3bcb36e3ee","abstract_canon_sha256":"7a03c6992199bfa09c1129c65d3bc9a289f17142d581fe41b6e83fa17c58352f"},"schema_version":"1.0"},"canonical_sha256":"92383826c7cfcb9fc43f66710d439338c06a6017ef0ea42ffa1d647473df8c4b","source":{"kind":"arxiv","id":"2503.00112","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2503.00112","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"arxiv_version","alias_value":"2503.00112v1","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.00112","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_12","alias_value":"SI4DQJWHZ7FZ","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_16","alias_value":"SI4DQJWHZ7FZ7RB7","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_8","alias_value":"SI4DQJWH","created_at":"2026-07-05T10:59:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2025:SI4DQJWHZ7FZ7RB7MZYQ2Q4THD","target":"record","payload":{"canonical_record":{"source":{"id":"2503.00112","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-28T19:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"50d91645b5b93f403450492f15263cad7e5c02641a02787a695b9c3bcb36e3ee","abstract_canon_sha256":"7a03c6992199bfa09c1129c65d3bc9a289f17142d581fe41b6e83fa17c58352f"},"schema_version":"1.0"},"canonical_sha256":"92383826c7cfcb9fc43f66710d439338c06a6017ef0ea42ffa1d647473df8c4b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:59:06.360496Z","signature_b64":"1H3UUx7Ttdo5KyJmi9oC6h8ragUSWlwE34CO+CPaEc+VrM6Kk4liAfvzJ+IfR394oZjs7mGnbqYJtzk3pQG8Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"92383826c7cfcb9fc43f66710d439338c06a6017ef0ea42ffa1d647473df8c4b","last_reissued_at":"2026-07-05T10:59:06.359980Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:59:06.359980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2503.00112","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-05T10:59:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"cqf1wSpK/24ALslcjskYf2IxzNowfw/w2Vr0wpy+FKXwcUXUP15fVOaVT3aOKrC5iLCiT2MF052VmUV2TYTMDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-05T21:12:39.701184Z"},"content_sha256":"cd00a50b3ff13b5b84f8ae945432f93df6901128e25ed73d4cf94b51cd63c1a6","schema_version":"1.0","event_id":"sha256:cd00a50b3ff13b5b84f8ae945432f93df6901128e25ed73d4cf94b51cd63c1a6"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2025:SI4DQJWHZ7FZ7RB7MZYQ2Q4THD","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Going deeper into the dark with COSMOS-Web: JWST unveils the total contribution of Radio-Selected NIRfaint galaxies to the cosmic Star Formation Rate Density","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alberto Traina, Andrea Cimatti, Andrea Enia, Andrea Lapi, Andreas L. Faisst, Anton M. Koekemoer, Brant E. Robertson, Caitlin M. Casey, Christopher C. Hayward, Cristian Vignali, Daizhong Liu, Fabrizio Gentile, Francesca Pozzi, Giovanni Zamorani, Henry Joy McCracken, Hollis B. Akins, Irham T. Andika, Jason Rhodes, Jed McKinney, Jeyhan S. Kartaltepe, Laia Barrufet, Louise Paquereau, Margherita Talia, Marika Giulietti, Marko Shuntov, Mattia Vaccari, Maximilien Franco, Meriem Behiri, Micheal R. Rich, Natalie Allen, Nicole E. Drakos, Olivier Ilbert, Rashmi Gottumukkala, Santosh Harish, Shuowen Jin, Steven Gillman, Sune Toft","submitted_at":"2025-02-28T19:00:04Z","abstract_excerpt":"We present the first follow-up with JWST of radio-selected NIRfaint galaxies as part of the COSMOS-Web survey. By selecting galaxies detected at radio frequencies ($S_{\\rm 3 GHz}>11.5$ $\\mu$Jy; i.e. S/N$>5$) and with faint counterparts at NIR wavelengths (F150W$>26.1$ mag), we collect a sample of 127 likely dusty star-forming galaxies (DSFGs). We estimate their physical properties through SED fitting, compute the first radio luminosity function for these types of sources, and their contribution to the total cosmic star formation rate density. Our analysis confirms that these sources represent "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.00112","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/2503.00112/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-05T10:59:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"v9N/nm8kp1g7XySK8bnRLcEF/q9t31kw1zLx2tGq7ev2UOlTVcZQEFaLiWB0fLIYzM7bqseGfzkRfJ2oDVbvAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-05T21:12:39.701760Z"},"content_sha256":"977821b159b316c5814686af38b3bac22cc2f260e8fb34f767b74304f246c367","schema_version":"1.0","event_id":"sha256:977821b159b316c5814686af38b3bac22cc2f260e8fb34f767b74304f246c367"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/bundle.json","state_url":"https://pith.science/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-05T21:12:39Z","links":{"resolver":"https://pith.science/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD","bundle":"https://pith.science/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/bundle.json","state":"https://pith.science/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SI4DQJWHZ7FZ7RB7MZYQ2Q4THD/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2025:SI4DQJWHZ7FZ7RB7MZYQ2Q4THD","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"7a03c6992199bfa09c1129c65d3bc9a289f17142d581fe41b6e83fa17c58352f","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-28T19:00:04Z","title_canon_sha256":"50d91645b5b93f403450492f15263cad7e5c02641a02787a695b9c3bcb36e3ee"},"schema_version":"1.0","source":{"id":"2503.00112","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2503.00112","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"arxiv_version","alias_value":"2503.00112v1","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.00112","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_12","alias_value":"SI4DQJWHZ7FZ","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_16","alias_value":"SI4DQJWHZ7FZ7RB7","created_at":"2026-07-05T10:59:06Z"},{"alias_kind":"pith_short_8","alias_value":"SI4DQJWH","created_at":"2026-07-05T10:59:06Z"}],"graph_snapshots":[{"event_id":"sha256:977821b159b316c5814686af38b3bac22cc2f260e8fb34f767b74304f246c367","target":"graph","created_at":"2026-07-05T10:59:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2503.00112/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We present the first follow-up with JWST of radio-selected NIRfaint galaxies as part of the COSMOS-Web survey. By selecting galaxies detected at radio frequencies ($S_{\\rm 3 GHz}>11.5$ $\\mu$Jy; i.e. S/N$>5$) and with faint counterparts at NIR wavelengths (F150W$>26.1$ mag), we collect a sample of 127 likely dusty star-forming galaxies (DSFGs). We estimate their physical properties through SED fitting, compute the first radio luminosity function for these types of sources, and their contribution to the total cosmic star formation rate density. Our analysis confirms that these sources represent ","authors_text":"Alberto Traina, Andrea Cimatti, Andrea Enia, Andrea Lapi, Andreas L. Faisst, Anton M. Koekemoer, Brant E. Robertson, Caitlin M. Casey, Christopher C. Hayward, Cristian Vignali, Daizhong Liu, Fabrizio Gentile, Francesca Pozzi, Giovanni Zamorani, Henry Joy McCracken, Hollis B. Akins, Irham T. Andika, Jason Rhodes, Jed McKinney, Jeyhan S. Kartaltepe, Laia Barrufet, Louise Paquereau, Margherita Talia, Marika Giulietti, Marko Shuntov, Mattia Vaccari, Maximilien Franco, Meriem Behiri, Micheal R. Rich, Natalie Allen, Nicole E. Drakos, Olivier Ilbert, Rashmi Gottumukkala, Santosh Harish, Shuowen Jin, Steven Gillman, Sune Toft","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-28T19:00:04Z","title":"Going deeper into the dark with COSMOS-Web: JWST unveils the total contribution of Radio-Selected NIRfaint galaxies to the cosmic Star Formation Rate Density"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.00112","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:cd00a50b3ff13b5b84f8ae945432f93df6901128e25ed73d4cf94b51cd63c1a6","target":"record","created_at":"2026-07-05T10:59:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"7a03c6992199bfa09c1129c65d3bc9a289f17142d581fe41b6e83fa17c58352f","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-28T19:00:04Z","title_canon_sha256":"50d91645b5b93f403450492f15263cad7e5c02641a02787a695b9c3bcb36e3ee"},"schema_version":"1.0","source":{"id":"2503.00112","kind":"arxiv","version":1}},"canonical_sha256":"92383826c7cfcb9fc43f66710d439338c06a6017ef0ea42ffa1d647473df8c4b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"92383826c7cfcb9fc43f66710d439338c06a6017ef0ea42ffa1d647473df8c4b","first_computed_at":"2026-07-05T10:59:06.359980Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-05T10:59:06.359980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"1H3UUx7Ttdo5KyJmi9oC6h8ragUSWlwE34CO+CPaEc+VrM6Kk4liAfvzJ+IfR394oZjs7mGnbqYJtzk3pQG8Cw==","signature_status":"signed_v1","signed_at":"2026-07-05T10:59:06.360496Z","signed_message":"canonical_sha256_bytes"},"source_id":"2503.00112","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:cd00a50b3ff13b5b84f8ae945432f93df6901128e25ed73d4cf94b51cd63c1a6","sha256:977821b159b316c5814686af38b3bac22cc2f260e8fb34f767b74304f246c367"],"state_sha256":"c91142ff4dc9ab43cfde4a714356fcf725075251bd788e8fc539d1bf21cdd618"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"L+Exylrwc9UxMDW/i3qYwQXBq83j80qyGFVNQc7++PMjlEtJNZmP/jxX3YB56wvHV/p+Qb23LxagB6hImDdoCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-05T21:12:39.706316Z","bundle_sha256":"75993279ba7c448b7fdaf6f2dee0dd047ade2056ba5abc8a0fcb547fc9d75258"}}