{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BT4DN3F3XWAEWOI6WIZWXNWSXE","short_pith_number":"pith:BT4DN3F3","schema_version":"1.0","canonical_sha256":"0cf836ecbbbd804b391eb2336bb6d2b93f38cd5bc6f14aed755d88c945153e56","source":{"kind":"arxiv","id":"2411.12005","version":2},"attestation_state":"computed","paper":{"title":"Exploring the Nature of Little Red Dots: Constraints on AGN and Stellar Contributions from PRIMER MIRI Imaging","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam C. Carnall, Alexa M. Morales, Anthony J. Taylor, Anton M. Koekemoer, Callum T. Donnan, Casey Papovich, Dale D. Kocevski, Derek J. McLeod, Fergus Cullen, Gene C. K. Leung, Guillermo Barro, Hollis B. Akins, James S. Dunlop, L. Y. Aaron Yung, Michaela Hirschmann, Nikko J. Cleri, Norman A. Grogin, \\'Oscar A. Ch\\'avez Ortiz, Pablo G. P\\'erez-Gonz\\'alez, Ray A. Lucas, Richard S. Ellis, Steven L. Finkelstein, Vasily Kokorev","submitted_at":"2024-11-18T19:41:17Z","abstract_excerpt":"JWST has revealed a large population of compact, red galaxies at $z>4$ known as Little Red Dots (LRDs). We analyze the spectral energy distributions (SEDs) of 95 LRDs from the JWST PRIMER survey with complete photometric coverage from $1-18\\ \\mu$m using NIRCam and MIRI imaging, representing the most extensive SED analysis on a large LRD sample with long-wavelength MIRI data. We examine SED models in which either galaxy or active galactic nucleus (AGN) emission dominates the rest-frame UV or optical continuum, extracting physical properties to explore each scenario's implications. In the galaxy"},"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":"2411.12005","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-11-18T19:41:17Z","cross_cats_sorted":[],"title_canon_sha256":"f698f52bebf436c7d561f530085f59e02d0ae5b95017c56bbd6bb20507e1a0ab","abstract_canon_sha256":"2c7bc8e01e391089f1db9038b2cb9c18025e6990cbf564641ef81a26c511a2cd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:39:10.511741Z","signature_b64":"h0m26RlwAVVtVwcon3YarAeMb+d4XHKGBqpgQ2D8c7G9U1bFjZL+20AsSPcyHuWq5PpiAHbsRjHHFIF3xxtOCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0cf836ecbbbd804b391eb2336bb6d2b93f38cd5bc6f14aed755d88c945153e56","last_reissued_at":"2026-07-05T09:39:10.511270Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:39:10.511270Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring the Nature of Little Red Dots: Constraints on AGN and Stellar Contributions from PRIMER MIRI Imaging","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam C. Carnall, Alexa M. Morales, Anthony J. Taylor, Anton M. Koekemoer, Callum T. Donnan, Casey Papovich, Dale D. Kocevski, Derek J. McLeod, Fergus Cullen, Gene C. K. Leung, Guillermo Barro, Hollis B. Akins, James S. Dunlop, L. Y. Aaron Yung, Michaela Hirschmann, Nikko J. Cleri, Norman A. Grogin, \\'Oscar A. Ch\\'avez Ortiz, Pablo G. P\\'erez-Gonz\\'alez, Ray A. Lucas, Richard S. Ellis, Steven L. Finkelstein, Vasily Kokorev","submitted_at":"2024-11-18T19:41:17Z","abstract_excerpt":"JWST has revealed a large population of compact, red galaxies at $z>4$ known as Little Red Dots (LRDs). We analyze the spectral energy distributions (SEDs) of 95 LRDs from the JWST PRIMER survey with complete photometric coverage from $1-18\\ \\mu$m using NIRCam and MIRI imaging, representing the most extensive SED analysis on a large LRD sample with long-wavelength MIRI data. We examine SED models in which either galaxy or active galactic nucleus (AGN) emission dominates the rest-frame UV or optical continuum, extracting physical properties to explore each scenario's implications. In the galaxy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.12005","kind":"arxiv","version":2},"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/2411.12005/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":"2411.12005","created_at":"2026-07-05T09:39:10.511336+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.12005v2","created_at":"2026-07-05T09:39:10.511336+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.12005","created_at":"2026-07-05T09:39:10.511336+00:00"},{"alias_kind":"pith_short_12","alias_value":"BT4DN3F3XWAE","created_at":"2026-07-05T09:39:10.511336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BT4DN3F3XWAEWOI6","created_at":"2026-07-05T09:39:10.511336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BT4DN3F3","created_at":"2026-07-05T09:39:10.511336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2502.02637","citing_title":"Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2509.23490","citing_title":"The mechanism for creating \"dynamical gravastar\" black hole mimickers also explains formation of \"little red dots\"","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04685","citing_title":"Compact, AGN-hosting Dwarf Galaxies with \"Little Red Dots\"-like SEDs in the Local Universe","ref_index":50,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE","json":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE.json","graph_json":"https://pith.science/api/pith-number/BT4DN3F3XWAEWOI6WIZWXNWSXE/graph.json","events_json":"https://pith.science/api/pith-number/BT4DN3F3XWAEWOI6WIZWXNWSXE/events.json","paper":"https://pith.science/paper/BT4DN3F3"},"agent_actions":{"view_html":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE","download_json":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE.json","view_paper":"https://pith.science/paper/BT4DN3F3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.12005&json=true","fetch_graph":"https://pith.science/api/pith-number/BT4DN3F3XWAEWOI6WIZWXNWSXE/graph.json","fetch_events":"https://pith.science/api/pith-number/BT4DN3F3XWAEWOI6WIZWXNWSXE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE/action/storage_attestation","attest_author":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE/action/author_attestation","sign_citation":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE/action/citation_signature","submit_replication":"https://pith.science/pith/BT4DN3F3XWAEWOI6WIZWXNWSXE/action/replication_record"}},"created_at":"2026-07-05T09:39:10.511336+00:00","updated_at":"2026-07-05T09:39:10.511336+00:00"}