{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:FJS4O5C3XBJXNRVN6QRNZ5XJDK","short_pith_number":"pith:FJS4O5C3","schema_version":"1.0","canonical_sha256":"2a65c7745bb85376c6adf422dcf6e91aa4de46a74bd59668fb5dc6976b72f588","source":{"kind":"arxiv","id":"1712.04204","version":4},"attestation_state":"computed","paper":{"title":"Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Constantin, C. A. Witherspoon, C. M. V. Impellizzeri, C. Y. Kuo, D. Pesce, F. Gao, H. H. Chung, I. Zaw, J. A. Braatz, J.-H. Woo, L. Hao","submitted_at":"2017-12-12T10:15:37Z","abstract_excerpt":"Water megamasers from circumnuclear disks in galaxy centers provide the most accurate measurements of supermassive black hole masses and uniquely probe the sub-parsec accretion processes. At the same time, these systems offer independent crucial constraints of the Hubble Constant in the nearby universe, and thus, the arguably best single constraint on the nature of dark energy. The chances of finding these golden standards are however abysmally low, at an overall =< 3% for any level of water maser emission detected at 22 GHz, and =< 1% for those exhibiting the disk-like configuration. We provi"},"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":"1712.04204","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-12T10:15:37Z","cross_cats_sorted":[],"title_canon_sha256":"f85b64fc55baeeef0c4343f9bffcdc9748e88684f77838f8cc1e22a0cd4464dc","abstract_canon_sha256":"90fb032fe135c3981a343a4caba8e355f887f38907cf4b7881dbc407207ecfa5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:06.633803Z","signature_b64":"jvLaZMwk7B/mflLflZMJLfp8QSqShRpuIP1lo4j/f0zHV61sQ8tcO3DFw9M3NmlT0is7cZyPkOC3J6yX1HKlAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2a65c7745bb85376c6adf422dcf6e91aa4de46a74bd59668fb5dc6976b72f588","last_reissued_at":"2026-05-18T00:11:06.633115Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:06.633115Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Constantin, C. A. Witherspoon, C. M. V. Impellizzeri, C. Y. Kuo, D. Pesce, F. Gao, H. H. Chung, I. Zaw, J. A. Braatz, J.-H. Woo, L. Hao","submitted_at":"2017-12-12T10:15:37Z","abstract_excerpt":"Water megamasers from circumnuclear disks in galaxy centers provide the most accurate measurements of supermassive black hole masses and uniquely probe the sub-parsec accretion processes. At the same time, these systems offer independent crucial constraints of the Hubble Constant in the nearby universe, and thus, the arguably best single constraint on the nature of dark energy. The chances of finding these golden standards are however abysmally low, at an overall =< 3% for any level of water maser emission detected at 22 GHz, and =< 1% for those exhibiting the disk-like configuration. We provi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.04204","kind":"arxiv","version":4},"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":"1712.04204","created_at":"2026-05-18T00:11:06.633219+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.04204v4","created_at":"2026-05-18T00:11:06.633219+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.04204","created_at":"2026-05-18T00:11:06.633219+00:00"},{"alias_kind":"pith_short_12","alias_value":"FJS4O5C3XBJX","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"FJS4O5C3XBJXNRVN","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"FJS4O5C3","created_at":"2026-05-18T12:31:15.632608+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/FJS4O5C3XBJXNRVN6QRNZ5XJDK","json":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK.json","graph_json":"https://pith.science/api/pith-number/FJS4O5C3XBJXNRVN6QRNZ5XJDK/graph.json","events_json":"https://pith.science/api/pith-number/FJS4O5C3XBJXNRVN6QRNZ5XJDK/events.json","paper":"https://pith.science/paper/FJS4O5C3"},"agent_actions":{"view_html":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK","download_json":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK.json","view_paper":"https://pith.science/paper/FJS4O5C3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.04204&json=true","fetch_graph":"https://pith.science/api/pith-number/FJS4O5C3XBJXNRVN6QRNZ5XJDK/graph.json","fetch_events":"https://pith.science/api/pith-number/FJS4O5C3XBJXNRVN6QRNZ5XJDK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK/action/storage_attestation","attest_author":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK/action/author_attestation","sign_citation":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK/action/citation_signature","submit_replication":"https://pith.science/pith/FJS4O5C3XBJXNRVN6QRNZ5XJDK/action/replication_record"}},"created_at":"2026-05-18T00:11:06.633219+00:00","updated_at":"2026-05-18T00:11:06.633219+00:00"}