{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:PSKANO6G5JTHHLY5ZLL6AG43M7","short_pith_number":"pith:PSKANO6G","schema_version":"1.0","canonical_sha256":"7c9406bbc6ea6673af1dcad7e01b9b67c37b9a8d4282387293450d71714aba2a","source":{"kind":"arxiv","id":"2004.10230","version":1},"attestation_state":"computed","paper":{"title":"The Star Formation in Radio Survey: 3 - 33 GHz Imaging of Nearby Galaxy Nuclei and Extranuclear Star-forming Regions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Dong, D.S. Meier, E.J. Murphy, E. Momjian, E. Schinnerer, J.L. Turner, R. C. Kennicutt Jr., S.T. Linden","submitted_at":"2020-04-21T18:29:13Z","abstract_excerpt":"We present 3, 15, and 33 GHz imaging towards galaxy nuclei and extranuclear star-forming regions using the Karl G. Jansky Very Large Array as part of the Star Formation in Radio Survey. With $3-33$ GHz radio spectra, we measured the spectral indices and corresponding thermal (free-free) emission fractions for a sample of 335 discrete regions having significant detections in at least two radio bands. After removing 14 likely background galaxies, we find that the median thermal fraction at 33 GHz is $92 \\pm 0.8\\%$ with a median absolute deviation of $11\\%$, when a two-component power-law model i"},"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":"2004.10230","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-04-21T18:29:13Z","cross_cats_sorted":[],"title_canon_sha256":"3bb0341c67de88340c55e9ec5951850cecbbb0299f8933159436630d0a55da71","abstract_canon_sha256":"6e1c2d700be7960396e1edd3d94fbe78bbd09b55f0b9e46e804322845f3f1519"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:07:29.645395Z","signature_b64":"VMeynyjNW8JmynNtLGd5ylGi6F0cL/dzkTzJEf9CznSRsLMU/SQ/E11UO0geWIPp8r9FGW1nhkoQZvU27bqFCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c9406bbc6ea6673af1dcad7e01b9b67c37b9a8d4282387293450d71714aba2a","last_reissued_at":"2026-07-05T01:07:29.644907Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:07:29.644907Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Star Formation in Radio Survey: 3 - 33 GHz Imaging of Nearby Galaxy Nuclei and Extranuclear Star-forming Regions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Dong, D.S. Meier, E.J. Murphy, E. Momjian, E. Schinnerer, J.L. Turner, R. C. Kennicutt Jr., S.T. Linden","submitted_at":"2020-04-21T18:29:13Z","abstract_excerpt":"We present 3, 15, and 33 GHz imaging towards galaxy nuclei and extranuclear star-forming regions using the Karl G. Jansky Very Large Array as part of the Star Formation in Radio Survey. With $3-33$ GHz radio spectra, we measured the spectral indices and corresponding thermal (free-free) emission fractions for a sample of 335 discrete regions having significant detections in at least two radio bands. After removing 14 likely background galaxies, we find that the median thermal fraction at 33 GHz is $92 \\pm 0.8\\%$ with a median absolute deviation of $11\\%$, when a two-component power-law model i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2004.10230","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/2004.10230/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":"2004.10230","created_at":"2026-07-05T01:07:29.644959+00:00"},{"alias_kind":"arxiv_version","alias_value":"2004.10230v1","created_at":"2026-07-05T01:07:29.644959+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2004.10230","created_at":"2026-07-05T01:07:29.644959+00:00"},{"alias_kind":"pith_short_12","alias_value":"PSKANO6G5JTH","created_at":"2026-07-05T01:07:29.644959+00:00"},{"alias_kind":"pith_short_16","alias_value":"PSKANO6G5JTHHLY5","created_at":"2026-07-05T01:07:29.644959+00:00"},{"alias_kind":"pith_short_8","alias_value":"PSKANO6G","created_at":"2026-07-05T01:07:29.644959+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/PSKANO6G5JTHHLY5ZLL6AG43M7","json":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7.json","graph_json":"https://pith.science/api/pith-number/PSKANO6G5JTHHLY5ZLL6AG43M7/graph.json","events_json":"https://pith.science/api/pith-number/PSKANO6G5JTHHLY5ZLL6AG43M7/events.json","paper":"https://pith.science/paper/PSKANO6G"},"agent_actions":{"view_html":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7","download_json":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7.json","view_paper":"https://pith.science/paper/PSKANO6G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2004.10230&json=true","fetch_graph":"https://pith.science/api/pith-number/PSKANO6G5JTHHLY5ZLL6AG43M7/graph.json","fetch_events":"https://pith.science/api/pith-number/PSKANO6G5JTHHLY5ZLL6AG43M7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7/action/storage_attestation","attest_author":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7/action/author_attestation","sign_citation":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7/action/citation_signature","submit_replication":"https://pith.science/pith/PSKANO6G5JTHHLY5ZLL6AG43M7/action/replication_record"}},"created_at":"2026-07-05T01:07:29.644959+00:00","updated_at":"2026-07-05T01:07:29.644959+00:00"}