{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:HHURRDCZ72EE74B65DJWVHA2Y7","short_pith_number":"pith:HHURRDCZ","schema_version":"1.0","canonical_sha256":"39e9188c59fe884ff03ee8d36a9c1ac7e3758ab2e42b1a9049d5fb9e0716e2c4","source":{"kind":"arxiv","id":"1002.3324","version":2},"attestation_state":"computed","paper":{"title":"High Sensitivity Array Observations of the z=1.87 Sub-Millimeter Galaxy GOODS 850-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. J. Barger, C. L. Carilli, E. Momjian, K. K. Knudsen, L. L. Cowie, W-H. Wang","submitted_at":"2010-02-17T17:38:49Z","abstract_excerpt":"We present sensitive phase-referenced VLBI results on the radio continuum emission from the z=1.87 luminous submillimeter galaxy (SMG) GOODS 850-3. The observations were carried out at 1.4 GHz using the High Sensitivity Array (HSA). Our sensitive tapered VLBI image of GOODS 850-3 at 0.47 x 0.34 arcsec (3.9 x 2.9 kpc) resolution shows a marginally resolved continuum structure with a peak flux density of 148 \\pm 38 uJy/beam, and a total flux density of 168 \\pm 73 uJy, consistent with previous VLA and MERLIN measurements. The derived intrinsic brightness temperature is > 5 \\pm 2 x 10^3 K. The rad"},"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":"1002.3324","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-02-17T17:38:49Z","cross_cats_sorted":[],"title_canon_sha256":"ff9d54ffa946511970645472edd34ef2960908552e617d16d349547cc5c4146d","abstract_canon_sha256":"31908f3227a5f9006256bf8930b7c17fa3ce485d01d6b4b004bdae78a9b66cac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:00.111671Z","signature_b64":"7Dq4vRrT+N3+PFNbZSyCzwYLpTLVj5MRo7hwJxQ96PcqLvHTbcjynaa/2wsvgMdZL8JgeyAMT+zIJl8NHc96AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"39e9188c59fe884ff03ee8d36a9c1ac7e3758ab2e42b1a9049d5fb9e0716e2c4","last_reissued_at":"2026-05-18T02:09:00.110968Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:00.110968Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High Sensitivity Array Observations of the z=1.87 Sub-Millimeter Galaxy GOODS 850-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. J. Barger, C. L. Carilli, E. Momjian, K. K. Knudsen, L. L. Cowie, W-H. Wang","submitted_at":"2010-02-17T17:38:49Z","abstract_excerpt":"We present sensitive phase-referenced VLBI results on the radio continuum emission from the z=1.87 luminous submillimeter galaxy (SMG) GOODS 850-3. The observations were carried out at 1.4 GHz using the High Sensitivity Array (HSA). Our sensitive tapered VLBI image of GOODS 850-3 at 0.47 x 0.34 arcsec (3.9 x 2.9 kpc) resolution shows a marginally resolved continuum structure with a peak flux density of 148 \\pm 38 uJy/beam, and a total flux density of 168 \\pm 73 uJy, consistent with previous VLA and MERLIN measurements. The derived intrinsic brightness temperature is > 5 \\pm 2 x 10^3 K. The rad"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.3324","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":""},"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":"1002.3324","created_at":"2026-05-18T02:09:00.111095+00:00"},{"alias_kind":"arxiv_version","alias_value":"1002.3324v2","created_at":"2026-05-18T02:09:00.111095+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.3324","created_at":"2026-05-18T02:09:00.111095+00:00"},{"alias_kind":"pith_short_12","alias_value":"HHURRDCZ72EE","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"HHURRDCZ72EE74B6","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"HHURRDCZ","created_at":"2026-05-18T12:26:07.630475+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/HHURRDCZ72EE74B65DJWVHA2Y7","json":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7.json","graph_json":"https://pith.science/api/pith-number/HHURRDCZ72EE74B65DJWVHA2Y7/graph.json","events_json":"https://pith.science/api/pith-number/HHURRDCZ72EE74B65DJWVHA2Y7/events.json","paper":"https://pith.science/paper/HHURRDCZ"},"agent_actions":{"view_html":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7","download_json":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7.json","view_paper":"https://pith.science/paper/HHURRDCZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1002.3324&json=true","fetch_graph":"https://pith.science/api/pith-number/HHURRDCZ72EE74B65DJWVHA2Y7/graph.json","fetch_events":"https://pith.science/api/pith-number/HHURRDCZ72EE74B65DJWVHA2Y7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7/action/storage_attestation","attest_author":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7/action/author_attestation","sign_citation":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7/action/citation_signature","submit_replication":"https://pith.science/pith/HHURRDCZ72EE74B65DJWVHA2Y7/action/replication_record"}},"created_at":"2026-05-18T02:09:00.111095+00:00","updated_at":"2026-05-18T02:09:00.111095+00:00"}