{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:FBYAV3UF5CGSKSVWCYKWNWJ2VH","short_pith_number":"pith:FBYAV3UF","schema_version":"1.0","canonical_sha256":"28700aee85e88d254ab6161566d93aa9d123711b8fad38bc3803758391e09b40","source":{"kind":"arxiv","id":"2306.07320","version":1},"attestation_state":"computed","paper":{"title":"UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adi Zitrin, Andy D. Goulding, Bingjie Wang, Casey Papovich, Christina C. Williams, Dan Coe, Danilo Marchesini, Erica J. Nelson, Gabriel Brammer, Hakim Atek, Iryna Chemerynska, Ivo Labbe, Jenny E. Greene, Joel Leja, Jorryt Matthee, Karl Glazebrook, Katherine A. Suess, Katherine E. Whitaker, Lukas J. Furtak, Marijn Franx, Michael Maseda, Pascal A. Oesch, Pratika Dayal, Rachel Bezanson, Richard Pan, Robert Feldmann, Rohan P. Naidu, Sam E. Cutler, Sedona H. Price, Seiji Fujimoto, Themiya Nanayakkara","submitted_at":"2023-06-12T18:00:01Z","abstract_excerpt":"The James Webb Space Telescope (JWST) is revolutionizing our knowledge of $z>5$ galaxies and their actively accreting black holes. Using the JWST Cycle 1 Treasury program Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) in the lensing field Abell 2744, we report the identification of a sample of little red dots at $3 < z_{\\rm{phot}} < 7$ that likely contain highly-reddened accreting supermassive black holes. Using a NIRCam-only selection to F444W$<27.7$ mag, we find 26 sources over the $\\sim45$ arcmin$^{2}$ field that are blue in F115W$-$F200W$\\sim0$ (or $\\b"},"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":"2306.07320","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-06-12T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"49b6c06de34351654243c537b58f11cfe27e57ec2ac50b5be83b72f376250814","abstract_canon_sha256":"15bf160240bae630884807cf472bfbcd4c801fa33301c9fa77cc76797ae08bb3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:20:02.622740Z","signature_b64":"DOz4f+Qm5UhwiSVypeMRZo6dErA6Ss5ycobCBiafXONqrD8gv5/qodGJJT5MJLCVE7jXAJG+YqFER61aAXrJBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28700aee85e88d254ab6161566d93aa9d123711b8fad38bc3803758391e09b40","last_reissued_at":"2026-07-05T06:20:02.622237Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:20:02.622237Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"UNCOVER: Candidate Red Active Galactic Nuclei at 3<z<7 with JWST and ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adi Zitrin, Andy D. Goulding, Bingjie Wang, Casey Papovich, Christina C. Williams, Dan Coe, Danilo Marchesini, Erica J. Nelson, Gabriel Brammer, Hakim Atek, Iryna Chemerynska, Ivo Labbe, Jenny E. Greene, Joel Leja, Jorryt Matthee, Karl Glazebrook, Katherine A. Suess, Katherine E. Whitaker, Lukas J. Furtak, Marijn Franx, Michael Maseda, Pascal A. Oesch, Pratika Dayal, Rachel Bezanson, Richard Pan, Robert Feldmann, Rohan P. Naidu, Sam E. Cutler, Sedona H. Price, Seiji Fujimoto, Themiya Nanayakkara","submitted_at":"2023-06-12T18:00:01Z","abstract_excerpt":"The James Webb Space Telescope (JWST) is revolutionizing our knowledge of $z>5$ galaxies and their actively accreting black holes. Using the JWST Cycle 1 Treasury program Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) in the lensing field Abell 2744, we report the identification of a sample of little red dots at $3 < z_{\\rm{phot}} < 7$ that likely contain highly-reddened accreting supermassive black holes. Using a NIRCam-only selection to F444W$<27.7$ mag, we find 26 sources over the $\\sim45$ arcmin$^{2}$ field that are blue in F115W$-$F200W$\\sim0$ (or $\\b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.07320","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2306.07320/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2306.07320","created_at":"2026-07-05T06:20:02.622296+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.07320v1","created_at":"2026-07-05T06:20:02.622296+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.07320","created_at":"2026-07-05T06:20:02.622296+00:00"},{"alias_kind":"pith_short_12","alias_value":"FBYAV3UF5CGS","created_at":"2026-07-05T06:20:02.622296+00:00"},{"alias_kind":"pith_short_16","alias_value":"FBYAV3UF5CGSKSVW","created_at":"2026-07-05T06:20:02.622296+00:00"},{"alias_kind":"pith_short_8","alias_value":"FBYAV3UF","created_at":"2026-07-05T06:20:02.622296+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08264","citing_title":"Subaru meets JWST: A Direct Measurement of Ly$\\boldsymbol{\\alpha}$ Escape Fraction at $\\boldsymbol{z\\simeq6.2}$ with Dual Narrow-Band Imaging","ref_index":272,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05281","citing_title":"Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27427","citing_title":"SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2606.04081","citing_title":"The role of major mergers in triggering super-Eddington accretion","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2412.14246","citing_title":"Hidden in Pixels I: Discovery of dual \"little red dots\" indicates excess clustering on kilo-parsec scales","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2601.11203","citing_title":"Little Red Dots as Hidden Neutrino Sources","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17117","citing_title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13211","citing_title":"Sparks: The Magellan/FIRE survey from starburst to post-starburst","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14535","citing_title":"Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18173","citing_title":"Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA","ref_index":64,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH","json":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH.json","graph_json":"https://pith.science/api/pith-number/FBYAV3UF5CGSKSVWCYKWNWJ2VH/graph.json","events_json":"https://pith.science/api/pith-number/FBYAV3UF5CGSKSVWCYKWNWJ2VH/events.json","paper":"https://pith.science/paper/FBYAV3UF"},"agent_actions":{"view_html":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH","download_json":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH.json","view_paper":"https://pith.science/paper/FBYAV3UF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.07320&json=true","fetch_graph":"https://pith.science/api/pith-number/FBYAV3UF5CGSKSVWCYKWNWJ2VH/graph.json","fetch_events":"https://pith.science/api/pith-number/FBYAV3UF5CGSKSVWCYKWNWJ2VH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH/action/storage_attestation","attest_author":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH/action/author_attestation","sign_citation":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH/action/citation_signature","submit_replication":"https://pith.science/pith/FBYAV3UF5CGSKSVWCYKWNWJ2VH/action/replication_record"}},"created_at":"2026-07-05T06:20:02.622296+00:00","updated_at":"2026-07-05T06:20:02.622296+00:00"}