{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:TJG63WD2XMJMYYQFK2BKLDPVX4","short_pith_number":"pith:TJG63WD2","schema_version":"1.0","canonical_sha256":"9a4dedd87abb12cc62055682a58df5bf01ee6b0c6ee7764cd92e33ab01ddc43e","source":{"kind":"arxiv","id":"2107.00900","version":1},"attestation_state":"computed","paper":{"title":"Radio emission from dust-obscured galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Krisztina \\'E. Gab\\'anyi, Krisztina Perger, S\\'andor Frey","submitted_at":"2021-07-02T08:28:40Z","abstract_excerpt":"The coevolution of galaxies and their central supermassive black holes is a subject of intense research. A class of objects, the dust-obscured galaxies (DOGs) are particularly interesting in this respect as they are thought to represent a short evolutionary phase when violent star formation activity in the host galaxy may coexist with matter accretion onto the black hole powering the active nucleus. Here we investigate different types of DOGs classified by their mid-infrared spectral energy distributions to reveal whether they can be distinguished by their arcsec-scale radio properties. Radio "},"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":"2107.00900","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-07-02T08:28:40Z","cross_cats_sorted":[],"title_canon_sha256":"bf89ddcea4952d8dd0be8ea6e7204387374c172c2ce004b440823d3ab148de56","abstract_canon_sha256":"c37b66a2b515b83a8b0980365f4c80a307e3d00f9e817bd58ecda449809a0811"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:56:59.036606Z","signature_b64":"AUSTTdz11WJbwf9JO+krLa7o5WPUbbaEYlEVWX+9WMEiJ57kf/QrXVweVWGS5NoDgCZojw+fVn0Rnkkv+WlACA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a4dedd87abb12cc62055682a58df5bf01ee6b0c6ee7764cd92e33ab01ddc43e","last_reissued_at":"2026-07-05T02:56:59.036169Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:56:59.036169Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio emission from dust-obscured galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Krisztina \\'E. Gab\\'anyi, Krisztina Perger, S\\'andor Frey","submitted_at":"2021-07-02T08:28:40Z","abstract_excerpt":"The coevolution of galaxies and their central supermassive black holes is a subject of intense research. A class of objects, the dust-obscured galaxies (DOGs) are particularly interesting in this respect as they are thought to represent a short evolutionary phase when violent star formation activity in the host galaxy may coexist with matter accretion onto the black hole powering the active nucleus. Here we investigate different types of DOGs classified by their mid-infrared spectral energy distributions to reveal whether they can be distinguished by their arcsec-scale radio properties. Radio "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2107.00900","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/2107.00900/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":"2107.00900","created_at":"2026-07-05T02:56:59.036224+00:00"},{"alias_kind":"arxiv_version","alias_value":"2107.00900v1","created_at":"2026-07-05T02:56:59.036224+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2107.00900","created_at":"2026-07-05T02:56:59.036224+00:00"},{"alias_kind":"pith_short_12","alias_value":"TJG63WD2XMJM","created_at":"2026-07-05T02:56:59.036224+00:00"},{"alias_kind":"pith_short_16","alias_value":"TJG63WD2XMJMYYQF","created_at":"2026-07-05T02:56:59.036224+00:00"},{"alias_kind":"pith_short_8","alias_value":"TJG63WD2","created_at":"2026-07-05T02:56:59.036224+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/TJG63WD2XMJMYYQFK2BKLDPVX4","json":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4.json","graph_json":"https://pith.science/api/pith-number/TJG63WD2XMJMYYQFK2BKLDPVX4/graph.json","events_json":"https://pith.science/api/pith-number/TJG63WD2XMJMYYQFK2BKLDPVX4/events.json","paper":"https://pith.science/paper/TJG63WD2"},"agent_actions":{"view_html":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4","download_json":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4.json","view_paper":"https://pith.science/paper/TJG63WD2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2107.00900&json=true","fetch_graph":"https://pith.science/api/pith-number/TJG63WD2XMJMYYQFK2BKLDPVX4/graph.json","fetch_events":"https://pith.science/api/pith-number/TJG63WD2XMJMYYQFK2BKLDPVX4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4/action/storage_attestation","attest_author":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4/action/author_attestation","sign_citation":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4/action/citation_signature","submit_replication":"https://pith.science/pith/TJG63WD2XMJMYYQFK2BKLDPVX4/action/replication_record"}},"created_at":"2026-07-05T02:56:59.036224+00:00","updated_at":"2026-07-05T02:56:59.036224+00:00"}