{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:EVBJVHZVENPDPSSHRX354L7KAY","short_pith_number":"pith:EVBJVHZV","schema_version":"1.0","canonical_sha256":"25429a9f35235e37ca478df7de2fea0622b6245cc818e610fa78d4bb858a4b35","source":{"kind":"arxiv","id":"1308.6575","version":1},"attestation_state":"computed","paper":{"title":"Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ho Seong Hwang, Margaret J. Geller (Smithsonian Astrophysical Observatory), Sean M. Andrews","submitted_at":"2013-08-29T20:00:00Z","abstract_excerpt":"We report Submillimeter Array (SMA) observations of the 880 \\mu m dust continuum emission for four dust-obscured galaxies (DOGs) in the local universe. Two DOGs are clearly detected with S_\\nu(880 \\mu m)=10-13 mJy and S/N>5, but the other two are not detected with 3{\\sigma} upper limits of S_\\nu(880 \\mu m)=5-9 mJy. Including an additional two local DOGs with submillimeter data from the literature, we determine the dust masses and temperatures for six local DOGs. The infrared luminosities and dust masses for these DOGs are in the range 1.2-4.9x10^{11} (L_sun) and 4-14x10^{7} (M_sun), respective"},"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":"1308.6575","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-08-29T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"25b8d20d672353a41ba65a47e94f5ce2c7b02145248e3702cd43f98f46d1a412","abstract_canon_sha256":"65871f0c96bd6bef9077fccf44babc6a40a6bb749609b6ae4a657e3fdcaaaf9c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:56.784184Z","signature_b64":"hldkuBmGxil1/6wu9kUY4BTnSFh3X+JJIgyPPoAjNuouTvGoYEAcMzUWFaSDOG+9GhDpac+TvDdcszaBiWoOBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"25429a9f35235e37ca478df7de2fea0622b6245cc818e610fa78d4bb858a4b35","last_reissued_at":"2026-05-18T01:47:56.783547Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:56.783547Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ho Seong Hwang, Margaret J. Geller (Smithsonian Astrophysical Observatory), Sean M. Andrews","submitted_at":"2013-08-29T20:00:00Z","abstract_excerpt":"We report Submillimeter Array (SMA) observations of the 880 \\mu m dust continuum emission for four dust-obscured galaxies (DOGs) in the local universe. Two DOGs are clearly detected with S_\\nu(880 \\mu m)=10-13 mJy and S/N>5, but the other two are not detected with 3{\\sigma} upper limits of S_\\nu(880 \\mu m)=5-9 mJy. Including an additional two local DOGs with submillimeter data from the literature, we determine the dust masses and temperatures for six local DOGs. The infrared luminosities and dust masses for these DOGs are in the range 1.2-4.9x10^{11} (L_sun) and 4-14x10^{7} (M_sun), respective"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.6575","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":""},"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":"1308.6575","created_at":"2026-05-18T01:47:56.783646+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.6575v1","created_at":"2026-05-18T01:47:56.783646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.6575","created_at":"2026-05-18T01:47:56.783646+00:00"},{"alias_kind":"pith_short_12","alias_value":"EVBJVHZVENPD","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_16","alias_value":"EVBJVHZVENPDPSSH","created_at":"2026-05-18T12:27:43.054852+00:00"},{"alias_kind":"pith_short_8","alias_value":"EVBJVHZV","created_at":"2026-05-18T12:27:43.054852+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/EVBJVHZVENPDPSSHRX354L7KAY","json":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY.json","graph_json":"https://pith.science/api/pith-number/EVBJVHZVENPDPSSHRX354L7KAY/graph.json","events_json":"https://pith.science/api/pith-number/EVBJVHZVENPDPSSHRX354L7KAY/events.json","paper":"https://pith.science/paper/EVBJVHZV"},"agent_actions":{"view_html":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY","download_json":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY.json","view_paper":"https://pith.science/paper/EVBJVHZV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.6575&json=true","fetch_graph":"https://pith.science/api/pith-number/EVBJVHZVENPDPSSHRX354L7KAY/graph.json","fetch_events":"https://pith.science/api/pith-number/EVBJVHZVENPDPSSHRX354L7KAY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY/action/storage_attestation","attest_author":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY/action/author_attestation","sign_citation":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY/action/citation_signature","submit_replication":"https://pith.science/pith/EVBJVHZVENPDPSSHRX354L7KAY/action/replication_record"}},"created_at":"2026-05-18T01:47:56.783646+00:00","updated_at":"2026-05-18T01:47:56.783646+00:00"}