{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:D55DM5QIFQNFX6THVB4OUE5RYU","short_pith_number":"pith:D55DM5QI","schema_version":"1.0","canonical_sha256":"1f7a3676082c1a5bfa67a878ea13b1c5365d182a6d6951e6c11ff5e0369bd6cd","source":{"kind":"arxiv","id":"2410.07340","version":1},"attestation_state":"computed","paper":{"title":"Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anthony J. Taylor, Anton M. Koekemoer, Benne W. Holwerda, Bren Backhaus, Dale D. Kocevski, Fabio Pacucci, Jonathan R. Trump, Kelcey Davis, Lise-Marie Seill\\'e, Madisyn Brooks, Michaela Hirschmann, Nikko J. Cleri, Ray A. Lucas, Raymond C. Simons, Steven L. Finkelstein, V\\'eronique Buat","submitted_at":"2024-10-09T18:00:19Z","abstract_excerpt":"JWST spectroscopy has discovered a population of $z \\gtrsim 3.5$ galaxies with broad Balmer emission lines, and narrow forbidden lines, that are consistent with hosting active galactic nuclei (AGN). Many of these systems, now known as ``little red dots\" (LRDs), are compact and have unique colors that are very red in the optical/near-infrared and blue in the ultraviolet. The relative contribution of galaxy starlight and AGN to these systems remains uncertain, especially for the galaxies with unusual blue+red spectral energy distributions. In this work, we use Balmer decrements to measure the in"},"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":"2410.07340","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-10-09T18:00:19Z","cross_cats_sorted":[],"title_canon_sha256":"3fb768f065a8bdaa46928f2a1739533df6722dd060a1915d37a06ac7ab710f52","abstract_canon_sha256":"9b710179b5887749b2730becb8a4320dc787592258c44f33bca503fac36a2c45"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:18:34.850349Z","signature_b64":"zO8jCAKCnx3sFZejbJNh+qDMwR+3drdhYOI5GAf/S/zUNTmibs11kFtFEoUP/XwypyaG3mNu6Y3RjvaLPr1RCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1f7a3676082c1a5bfa67a878ea13b1c5365d182a6d6951e6c11ff5e0369bd6cd","last_reissued_at":"2026-07-05T09:18:34.849867Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:18:34.849867Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anthony J. Taylor, Anton M. Koekemoer, Benne W. Holwerda, Bren Backhaus, Dale D. Kocevski, Fabio Pacucci, Jonathan R. Trump, Kelcey Davis, Lise-Marie Seill\\'e, Madisyn Brooks, Michaela Hirschmann, Nikko J. Cleri, Ray A. Lucas, Raymond C. Simons, Steven L. Finkelstein, V\\'eronique Buat","submitted_at":"2024-10-09T18:00:19Z","abstract_excerpt":"JWST spectroscopy has discovered a population of $z \\gtrsim 3.5$ galaxies with broad Balmer emission lines, and narrow forbidden lines, that are consistent with hosting active galactic nuclei (AGN). Many of these systems, now known as ``little red dots\" (LRDs), are compact and have unique colors that are very red in the optical/near-infrared and blue in the ultraviolet. The relative contribution of galaxy starlight and AGN to these systems remains uncertain, especially for the galaxies with unusual blue+red spectral energy distributions. In this work, we use Balmer decrements to measure the in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.07340","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/2410.07340/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":"2410.07340","created_at":"2026-07-05T09:18:34.849922+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.07340v1","created_at":"2026-07-05T09:18:34.849922+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.07340","created_at":"2026-07-05T09:18:34.849922+00:00"},{"alias_kind":"pith_short_12","alias_value":"D55DM5QIFQNF","created_at":"2026-07-05T09:18:34.849922+00:00"},{"alias_kind":"pith_short_16","alias_value":"D55DM5QIFQNFX6TH","created_at":"2026-07-05T09:18:34.849922+00:00"},{"alias_kind":"pith_short_8","alias_value":"D55DM5QI","created_at":"2026-07-05T09:18:34.849922+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00084","citing_title":"Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5","ref_index":178,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15263","citing_title":"Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates","ref_index":207,"is_internal_anchor":false},{"citing_arxiv_id":"2503.16596","citing_title":"A \"Black Hole Star\" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU","json":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU.json","graph_json":"https://pith.science/api/pith-number/D55DM5QIFQNFX6THVB4OUE5RYU/graph.json","events_json":"https://pith.science/api/pith-number/D55DM5QIFQNFX6THVB4OUE5RYU/events.json","paper":"https://pith.science/paper/D55DM5QI"},"agent_actions":{"view_html":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU","download_json":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU.json","view_paper":"https://pith.science/paper/D55DM5QI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.07340&json=true","fetch_graph":"https://pith.science/api/pith-number/D55DM5QIFQNFX6THVB4OUE5RYU/graph.json","fetch_events":"https://pith.science/api/pith-number/D55DM5QIFQNFX6THVB4OUE5RYU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU/action/storage_attestation","attest_author":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU/action/author_attestation","sign_citation":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU/action/citation_signature","submit_replication":"https://pith.science/pith/D55DM5QIFQNFX6THVB4OUE5RYU/action/replication_record"}},"created_at":"2026-07-05T09:18:34.849922+00:00","updated_at":"2026-07-05T09:18:34.849922+00:00"}