{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:UODWD6N3CGW74KC5INX6YRJIS6","short_pith_number":"pith:UODWD6N3","schema_version":"1.0","canonical_sha256":"a38761f9bb11adfe285d436fec452897a8567d31260e1a3561e2887a29d8196d","source":{"kind":"arxiv","id":"1111.5670","version":1},"attestation_state":"computed","paper":{"title":"Maser Source Finding Methods in HOPS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"Andrew J. Walsh, Christopher H. Jordan, Cormac Purcell, Steven Longmore, Vicki Lowe","submitted_at":"2011-11-24T02:36:57Z","abstract_excerpt":"The {\\bf H}$_2${\\bf O} Southern Galactic {\\bf P}lane {\\bf S}urvey (HOPS) has observed 100 square degrees of the Galactic plane, using the Mopra radio telescope to search for emission from multiple spectral lines in the 12\\,mm band (19.5\\,--\\,27.5\\,GHz). Perhaps the most important of these spectral lines is the 22.2\\,GHz water maser transition. We describe the methods used to identify water maser candidates and subsequent confirmation of the sources. Our methods involve a simple determination of likely candidates by searching peak emission maps, utilising the intrinsic nature of water maser emi"},"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":"1111.5670","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2011-11-24T02:36:57Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"761cbcbf93c684e7f78c9f7a10dc342b1fb03c1da695db4d798502c16fd13179","abstract_canon_sha256":"adc42a1dc4994f2bedc8896bb3b893d423c78329b81fa2a0738807318a3907c8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:26.003287Z","signature_b64":"EaDGQusW19s+1JM5SMzv5+SQIkS3L12rAm5CnSKvvFZyN1+jJtF2iLQeUH8Cgs1I4a0CViXdH6R6WpYXUxqkCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a38761f9bb11adfe285d436fec452897a8567d31260e1a3561e2887a29d8196d","last_reissued_at":"2026-05-18T01:59:26.002574Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:26.002574Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Maser Source Finding Methods in HOPS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"Andrew J. Walsh, Christopher H. Jordan, Cormac Purcell, Steven Longmore, Vicki Lowe","submitted_at":"2011-11-24T02:36:57Z","abstract_excerpt":"The {\\bf H}$_2${\\bf O} Southern Galactic {\\bf P}lane {\\bf S}urvey (HOPS) has observed 100 square degrees of the Galactic plane, using the Mopra radio telescope to search for emission from multiple spectral lines in the 12\\,mm band (19.5\\,--\\,27.5\\,GHz). Perhaps the most important of these spectral lines is the 22.2\\,GHz water maser transition. We describe the methods used to identify water maser candidates and subsequent confirmation of the sources. Our methods involve a simple determination of likely candidates by searching peak emission maps, utilising the intrinsic nature of water maser emi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1111.5670","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":"1111.5670","created_at":"2026-05-18T01:59:26.002681+00:00"},{"alias_kind":"arxiv_version","alias_value":"1111.5670v1","created_at":"2026-05-18T01:59:26.002681+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1111.5670","created_at":"2026-05-18T01:59:26.002681+00:00"},{"alias_kind":"pith_short_12","alias_value":"UODWD6N3CGW7","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_16","alias_value":"UODWD6N3CGW74KC5","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_8","alias_value":"UODWD6N3","created_at":"2026-05-18T12:26:42.757692+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/UODWD6N3CGW74KC5INX6YRJIS6","json":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6.json","graph_json":"https://pith.science/api/pith-number/UODWD6N3CGW74KC5INX6YRJIS6/graph.json","events_json":"https://pith.science/api/pith-number/UODWD6N3CGW74KC5INX6YRJIS6/events.json","paper":"https://pith.science/paper/UODWD6N3"},"agent_actions":{"view_html":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6","download_json":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6.json","view_paper":"https://pith.science/paper/UODWD6N3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1111.5670&json=true","fetch_graph":"https://pith.science/api/pith-number/UODWD6N3CGW74KC5INX6YRJIS6/graph.json","fetch_events":"https://pith.science/api/pith-number/UODWD6N3CGW74KC5INX6YRJIS6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6/action/storage_attestation","attest_author":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6/action/author_attestation","sign_citation":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6/action/citation_signature","submit_replication":"https://pith.science/pith/UODWD6N3CGW74KC5INX6YRJIS6/action/replication_record"}},"created_at":"2026-05-18T01:59:26.002681+00:00","updated_at":"2026-05-18T01:59:26.002681+00:00"}