{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:MPL736UOM5HDXVF3SL7YMSSOW2","short_pith_number":"pith:MPL736UO","schema_version":"1.0","canonical_sha256":"63d7fdfa8e674e3bd4bb92ff864a4eb685af88092233d285fcde187983e8161c","source":{"kind":"arxiv","id":"1112.0379","version":1},"attestation_state":"computed","paper":{"title":"The SED of the nearby HI-massive LIRG HIZOA J0836-43: from the NIR to the radio domain","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Australian Astronomical Observatory, ACGC, Epping), Michelle E. Cluver (2) ((1) Astronomy Department, Renee C. Kraan-Korteweg (1), University of Cape Town","submitted_at":"2011-12-02T03:26:29Z","abstract_excerpt":"HIZOA J0836-43is one of the most HI-massive galaxies in the local (z<0.1) Universe. Not only are such galaxies extremely rare, but this \"coelacanth\" galaxy exhibits characteristics -- in particular its active, inside-out stellar disk-building -- that appear more typical of past (z ~ 1) star formation, when large gas fractions were more common. Unlike most local giant HI galaxies, it is actively star forming. Moreover, the strong infrared emission is not induced by a merger event or AGN, as is commonly found in other local LIRGs. The galaxy is suggestive of a scaled-up version of local spiral g"},"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":"1112.0379","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-12-02T03:26:29Z","cross_cats_sorted":[],"title_canon_sha256":"5e0edfff3712a478bc035135dbc8eb43efee9dc3d79c8e50c30f2df40a3f2af1","abstract_canon_sha256":"daf37c3d2c9dda6394cd694ef2967c50c2715d5a3bc63b02bb61f3d478188060"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:18.228058Z","signature_b64":"TXPdTHETdf53ppxxU5YtLzGsFIFKGFVDAZlUFXKOAFx4inWi5INgkv+C4tQ+XIF2mX8nwVk6IxwAM/qDQjjlBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"63d7fdfa8e674e3bd4bb92ff864a4eb685af88092233d285fcde187983e8161c","last_reissued_at":"2026-05-18T01:59:18.227459Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:18.227459Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The SED of the nearby HI-massive LIRG HIZOA J0836-43: from the NIR to the radio domain","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Australian Astronomical Observatory, ACGC, Epping), Michelle E. Cluver (2) ((1) Astronomy Department, Renee C. Kraan-Korteweg (1), University of Cape Town","submitted_at":"2011-12-02T03:26:29Z","abstract_excerpt":"HIZOA J0836-43is one of the most HI-massive galaxies in the local (z<0.1) Universe. Not only are such galaxies extremely rare, but this \"coelacanth\" galaxy exhibits characteristics -- in particular its active, inside-out stellar disk-building -- that appear more typical of past (z ~ 1) star formation, when large gas fractions were more common. Unlike most local giant HI galaxies, it is actively star forming. Moreover, the strong infrared emission is not induced by a merger event or AGN, as is commonly found in other local LIRGs. The galaxy is suggestive of a scaled-up version of local spiral g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.0379","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":"1112.0379","created_at":"2026-05-18T01:59:18.227546+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.0379v1","created_at":"2026-05-18T01:59:18.227546+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.0379","created_at":"2026-05-18T01:59:18.227546+00:00"},{"alias_kind":"pith_short_12","alias_value":"MPL736UOM5HD","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_16","alias_value":"MPL736UOM5HDXVF3","created_at":"2026-05-18T12:26:34.985390+00:00"},{"alias_kind":"pith_short_8","alias_value":"MPL736UO","created_at":"2026-05-18T12:26:34.985390+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/MPL736UOM5HDXVF3SL7YMSSOW2","json":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2.json","graph_json":"https://pith.science/api/pith-number/MPL736UOM5HDXVF3SL7YMSSOW2/graph.json","events_json":"https://pith.science/api/pith-number/MPL736UOM5HDXVF3SL7YMSSOW2/events.json","paper":"https://pith.science/paper/MPL736UO"},"agent_actions":{"view_html":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2","download_json":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2.json","view_paper":"https://pith.science/paper/MPL736UO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.0379&json=true","fetch_graph":"https://pith.science/api/pith-number/MPL736UOM5HDXVF3SL7YMSSOW2/graph.json","fetch_events":"https://pith.science/api/pith-number/MPL736UOM5HDXVF3SL7YMSSOW2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2/action/storage_attestation","attest_author":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2/action/author_attestation","sign_citation":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2/action/citation_signature","submit_replication":"https://pith.science/pith/MPL736UOM5HDXVF3SL7YMSSOW2/action/replication_record"}},"created_at":"2026-05-18T01:59:18.227546+00:00","updated_at":"2026-05-18T01:59:18.227546+00:00"}