{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:AJNQY4FP3ER5AF4A2NC4EVGKXC","short_pith_number":"pith:AJNQY4FP","schema_version":"1.0","canonical_sha256":"025b0c70afd923d01780d345c254cab8ab30564b42288171f39e859ec83027ec","source":{"kind":"arxiv","id":"1202.6478","version":1},"attestation_state":"computed","paper":{"title":"A 95 GHz Class I Methanol Maser Survey Toward A Sample of GLIMPSE Point Sources Associated with BGPS Clumps","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bing-Gang Ju, Cong-Gui Gan, Jin-hua He, Simon P. Ellingsen, Tao An, Xi Chen, Yan Sun, Ye Xu, Zhi-Qiang Shen","submitted_at":"2012-02-29T08:24:42Z","abstract_excerpt":"We report a survey with the Purple Mountain Observatory (PMO) 13.7-m radio telescope for class I methanol masers from the 95 GHz (8_0 - 7_1 A^+) transition. The 214 target sources were selected by combining information from both the Spitzer GLIMPSE and 1.1 mm BGPS survey catalogs. The observed sources satisfy both the GLIMPSE mid-IR criteria of [3.6]-[4.5]>1.3, [3.6]-[5.8]>2.5, [3.6]-[8.0]>2.5 and 8.0 um magnitude less than 10, and also have an associated 1.1 mm BGPS source. Class I methanol maser emission was detected in 63 sources, corresponding to a detection rate of 29% for this survey. Fo"},"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":"1202.6478","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/3.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-02-29T08:24:42Z","cross_cats_sorted":[],"title_canon_sha256":"37d11dee8a49c90309c43af73f10dacc742ac8c8eb6d22a2eb5edc5edbc36534","abstract_canon_sha256":"8ad2278c64c33333e558b01bf2107cc80ada7ed59efe3869a10414e4b5b2358c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:18.367298Z","signature_b64":"l0avfWRvHTYv6Jog0bKAF+LVU+V9ZtamiDkx+PiPSZNZpUOmngCmXHg0ZFVv+UcN7HhOpGkqA1tFr7bnHt4YCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"025b0c70afd923d01780d345c254cab8ab30564b42288171f39e859ec83027ec","last_reissued_at":"2026-05-18T01:58:18.366765Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:18.366765Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A 95 GHz Class I Methanol Maser Survey Toward A Sample of GLIMPSE Point Sources Associated with BGPS Clumps","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bing-Gang Ju, Cong-Gui Gan, Jin-hua He, Simon P. Ellingsen, Tao An, Xi Chen, Yan Sun, Ye Xu, Zhi-Qiang Shen","submitted_at":"2012-02-29T08:24:42Z","abstract_excerpt":"We report a survey with the Purple Mountain Observatory (PMO) 13.7-m radio telescope for class I methanol masers from the 95 GHz (8_0 - 7_1 A^+) transition. The 214 target sources were selected by combining information from both the Spitzer GLIMPSE and 1.1 mm BGPS survey catalogs. The observed sources satisfy both the GLIMPSE mid-IR criteria of [3.6]-[4.5]>1.3, [3.6]-[5.8]>2.5, [3.6]-[8.0]>2.5 and 8.0 um magnitude less than 10, and also have an associated 1.1 mm BGPS source. Class I methanol maser emission was detected in 63 sources, corresponding to a detection rate of 29% for this survey. Fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.6478","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":"1202.6478","created_at":"2026-05-18T01:58:18.366841+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.6478v1","created_at":"2026-05-18T01:58:18.366841+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.6478","created_at":"2026-05-18T01:58:18.366841+00:00"},{"alias_kind":"pith_short_12","alias_value":"AJNQY4FP3ER5","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"AJNQY4FP3ER5AF4A","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"AJNQY4FP","created_at":"2026-05-18T12:26:58.693483+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/AJNQY4FP3ER5AF4A2NC4EVGKXC","json":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC.json","graph_json":"https://pith.science/api/pith-number/AJNQY4FP3ER5AF4A2NC4EVGKXC/graph.json","events_json":"https://pith.science/api/pith-number/AJNQY4FP3ER5AF4A2NC4EVGKXC/events.json","paper":"https://pith.science/paper/AJNQY4FP"},"agent_actions":{"view_html":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC","download_json":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC.json","view_paper":"https://pith.science/paper/AJNQY4FP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.6478&json=true","fetch_graph":"https://pith.science/api/pith-number/AJNQY4FP3ER5AF4A2NC4EVGKXC/graph.json","fetch_events":"https://pith.science/api/pith-number/AJNQY4FP3ER5AF4A2NC4EVGKXC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC/action/storage_attestation","attest_author":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC/action/author_attestation","sign_citation":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC/action/citation_signature","submit_replication":"https://pith.science/pith/AJNQY4FP3ER5AF4A2NC4EVGKXC/action/replication_record"}},"created_at":"2026-05-18T01:58:18.366841+00:00","updated_at":"2026-05-18T01:58:18.366841+00:00"}