{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:NXWB7GE57O7MRHLFOCH5DFX3DZ","short_pith_number":"pith:NXWB7GE5","schema_version":"1.0","canonical_sha256":"6dec1f989dfbbec89d65708fd196fb1e4242f21c97a6ff78eb8e01c776d5aa7f","source":{"kind":"arxiv","id":"0910.3763","version":1},"attestation_state":"computed","paper":{"title":"The Arecibo Methanol Maser Galactic Plane Survey - III: Distances and Luminosities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. D. Pandian, K. M. Menten, P. F. Goldsmith","submitted_at":"2009-10-20T08:15:51Z","abstract_excerpt":"We derive kinematic distances to the 86 6.7 GHz methanol masers discovered in the Arecibo Methanol Maser Galactic Plane Survey. The systemic velocities of the sources were derived from 13CO (J=2-1), CS (J=5-4), and NH3 observations made with the ARO Submillimeter Telescope, the APEX telescope, and the Effelsberg 100 m telescope, respectively. Kinematic distance ambiguities were resolved using HI self-absorption with HI data from the VLA Galactic Plane Survey. We observe roughly three times as many sources at the far distance compared to the near distance. The vertical distribution of the sourc"},"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":"0910.3763","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-10-20T08:15:51Z","cross_cats_sorted":[],"title_canon_sha256":"3aab8f04026a2d103e9833dac450c2351b2ca6f6528bf570279dc6e4d8ff461c","abstract_canon_sha256":"d7f09dd66ecff14c788ba8cd43c9638ffc2f7e9d76f1f6ec0be76e78af9863b6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:34:18.156236Z","signature_b64":"BZZ3mtmF/t3WNCu+doup0pMtZKLRwsyoqnOY69QxK8qqKmoqvt+LaW/zxOGgY2tFmnk4zDtD/xEAcv5oO3PiDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6dec1f989dfbbec89d65708fd196fb1e4242f21c97a6ff78eb8e01c776d5aa7f","last_reissued_at":"2026-05-18T02:34:18.155739Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:34:18.155739Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Arecibo Methanol Maser Galactic Plane Survey - III: Distances and Luminosities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. D. Pandian, K. M. Menten, P. F. Goldsmith","submitted_at":"2009-10-20T08:15:51Z","abstract_excerpt":"We derive kinematic distances to the 86 6.7 GHz methanol masers discovered in the Arecibo Methanol Maser Galactic Plane Survey. The systemic velocities of the sources were derived from 13CO (J=2-1), CS (J=5-4), and NH3 observations made with the ARO Submillimeter Telescope, the APEX telescope, and the Effelsberg 100 m telescope, respectively. Kinematic distance ambiguities were resolved using HI self-absorption with HI data from the VLA Galactic Plane Survey. We observe roughly three times as many sources at the far distance compared to the near distance. The vertical distribution of the sourc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.3763","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":"0910.3763","created_at":"2026-05-18T02:34:18.155811+00:00"},{"alias_kind":"arxiv_version","alias_value":"0910.3763v1","created_at":"2026-05-18T02:34:18.155811+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.3763","created_at":"2026-05-18T02:34:18.155811+00:00"},{"alias_kind":"pith_short_12","alias_value":"NXWB7GE57O7M","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"NXWB7GE57O7MRHLF","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"NXWB7GE5","created_at":"2026-05-18T12:26:01.383474+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/NXWB7GE57O7MRHLFOCH5DFX3DZ","json":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ.json","graph_json":"https://pith.science/api/pith-number/NXWB7GE57O7MRHLFOCH5DFX3DZ/graph.json","events_json":"https://pith.science/api/pith-number/NXWB7GE57O7MRHLFOCH5DFX3DZ/events.json","paper":"https://pith.science/paper/NXWB7GE5"},"agent_actions":{"view_html":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ","download_json":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ.json","view_paper":"https://pith.science/paper/NXWB7GE5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0910.3763&json=true","fetch_graph":"https://pith.science/api/pith-number/NXWB7GE57O7MRHLFOCH5DFX3DZ/graph.json","fetch_events":"https://pith.science/api/pith-number/NXWB7GE57O7MRHLFOCH5DFX3DZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ/action/storage_attestation","attest_author":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ/action/author_attestation","sign_citation":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ/action/citation_signature","submit_replication":"https://pith.science/pith/NXWB7GE57O7MRHLFOCH5DFX3DZ/action/replication_record"}},"created_at":"2026-05-18T02:34:18.155811+00:00","updated_at":"2026-05-18T02:34:18.155811+00:00"}