{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:SGTIWERXDPMYS65B3W2BHX3WEL","short_pith_number":"pith:SGTIWERX","schema_version":"1.0","canonical_sha256":"91a68b12371bd9897ba1ddb413df7622e17f40f680ba3434c34caf44108a7d9d","source":{"kind":"arxiv","id":"2305.02443","version":2},"attestation_state":"computed","paper":{"title":"The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. G. Robotham, Jessica E. Thorne, Luke J. M. Davies, Sabine Bellstedt","submitted_at":"2023-05-03T22:08:22Z","abstract_excerpt":"Traditionally, the far ultraviolet (FUV) to far-infrared (FIR) and radio spectral energy distributions (SEDs) of galaxies have been considered separately despite the common physical process shaping them. In this work, we explore the utility of simultaneously fitting FUV-radio SEDs using an extended version of the ProSpect SED fitting code considering contributions from both free-free and synchrotron emission. We use a small sample of galaxies from the Deep Extragalactic VIsible Legacy Survey (DEVILS) and the Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel (KINGFISH) where "},"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":"2305.02443","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-05-03T22:08:22Z","cross_cats_sorted":[],"title_canon_sha256":"c1f84ae0bcc52cda0001a70b6c71f2d3706b53b20bc1250eb7f690bc9e71f567","abstract_canon_sha256":"ba7b284d091f61375d4f9b16c1bd2fb90fa00fe1e93c2809fc1931063530708a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:10:39.914019Z","signature_b64":"a2aTXSmaTlIiMPyR2DPY7HVJCdB0sWg+vcCSOPT3X0WnWWZ+Ye9+6YHZQqr7zZDkxujXsP0uAvJLq3DxJ593DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91a68b12371bd9897ba1ddb413df7622e17f40f680ba3434c34caf44108a7d9d","last_reissued_at":"2026-07-05T06:10:39.913592Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:10:39.913592Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Long and the Short of It: The Benefits and Leverage of Ultraviolet-Radio Galaxy Fitting","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron S. G. Robotham, Jessica E. Thorne, Luke J. M. Davies, Sabine Bellstedt","submitted_at":"2023-05-03T22:08:22Z","abstract_excerpt":"Traditionally, the far ultraviolet (FUV) to far-infrared (FIR) and radio spectral energy distributions (SEDs) of galaxies have been considered separately despite the common physical process shaping them. In this work, we explore the utility of simultaneously fitting FUV-radio SEDs using an extended version of the ProSpect SED fitting code considering contributions from both free-free and synchrotron emission. We use a small sample of galaxies from the Deep Extragalactic VIsible Legacy Survey (DEVILS) and the Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel (KINGFISH) where "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.02443","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/2305.02443/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":"2305.02443","created_at":"2026-07-05T06:10:39.913649+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.02443v2","created_at":"2026-07-05T06:10:39.913649+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.02443","created_at":"2026-07-05T06:10:39.913649+00:00"},{"alias_kind":"pith_short_12","alias_value":"SGTIWERXDPMY","created_at":"2026-07-05T06:10:39.913649+00:00"},{"alias_kind":"pith_short_16","alias_value":"SGTIWERXDPMYS65B","created_at":"2026-07-05T06:10:39.913649+00:00"},{"alias_kind":"pith_short_8","alias_value":"SGTIWERX","created_at":"2026-07-05T06:10:39.913649+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/SGTIWERXDPMYS65B3W2BHX3WEL","json":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL.json","graph_json":"https://pith.science/api/pith-number/SGTIWERXDPMYS65B3W2BHX3WEL/graph.json","events_json":"https://pith.science/api/pith-number/SGTIWERXDPMYS65B3W2BHX3WEL/events.json","paper":"https://pith.science/paper/SGTIWERX"},"agent_actions":{"view_html":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL","download_json":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL.json","view_paper":"https://pith.science/paper/SGTIWERX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.02443&json=true","fetch_graph":"https://pith.science/api/pith-number/SGTIWERXDPMYS65B3W2BHX3WEL/graph.json","fetch_events":"https://pith.science/api/pith-number/SGTIWERXDPMYS65B3W2BHX3WEL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL/action/storage_attestation","attest_author":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL/action/author_attestation","sign_citation":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL/action/citation_signature","submit_replication":"https://pith.science/pith/SGTIWERXDPMYS65B3W2BHX3WEL/action/replication_record"}},"created_at":"2026-07-05T06:10:39.913649+00:00","updated_at":"2026-07-05T06:10:39.913649+00:00"}