{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:QXRS242KKF5GKIZFPKNGLUXTV3","short_pith_number":"pith:QXRS242K","schema_version":"1.0","canonical_sha256":"85e32d734a517a6523257a9a65d2f3aef70b03dd9e4646c23d8dbc5a8104950c","source":{"kind":"arxiv","id":"1808.02899","version":1},"attestation_state":"computed","paper":{"title":"Quasi-simultaneous 43 and 86 GHz SiO Maser Observations and Potential Bias in the BAaDE Survey Are Resolved","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Lor\\`ant O. Sjouwerman, Mark J. Claussen, Mark R. Morris, Michael C. Stroh, Michael R. Rich, Ylva M. Pihlstr\\\"om","submitted_at":"2018-08-08T18:00:25Z","abstract_excerpt":"We observed the 43 GHz v=1, 2, and 3 and 86 GHz v=1 SiO maser transitions quasi-simultaneously for a Mira-variable-dominated sample of over 80 sources from the Bulge Asymmetries and Dynamical Evolution (BAaDE) project, using ATCA, and statistically compared the relative line strengths. On average, the 43 GHz v=1 line is brighter than the 86 GHz v=1 line by a factor of 1.36+/-0.15. As a result, an 86 GHz v=1 observed sample can be observed to 85.9% of the distance of a 43 GHz v=1 observed sample using the same sensitivity. We discuss what impact this may have on the BAaDE Galactic plane survey "},"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":"1808.02899","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-08-08T18:00:25Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"109e873926aa73d2ded940d089a3c8d9e509d5fb6d755bd0390141332ddbcb0d","abstract_canon_sha256":"ec8698c637e8e390f253cec001ee10842db0941747bc3099f38393f86822dca7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:08:30.703390Z","signature_b64":"8x315rfY2n6NmNdAg4kYu4SEhpSREnNpBlUIEKvlAU0+WSu486o+yzD6EqJfiZxLouQYC1FaoTL4N8/5V2KoDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"85e32d734a517a6523257a9a65d2f3aef70b03dd9e4646c23d8dbc5a8104950c","last_reissued_at":"2026-05-18T00:08:30.702983Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:08:30.702983Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasi-simultaneous 43 and 86 GHz SiO Maser Observations and Potential Bias in the BAaDE Survey Are Resolved","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Lor\\`ant O. Sjouwerman, Mark J. Claussen, Mark R. Morris, Michael C. Stroh, Michael R. Rich, Ylva M. Pihlstr\\\"om","submitted_at":"2018-08-08T18:00:25Z","abstract_excerpt":"We observed the 43 GHz v=1, 2, and 3 and 86 GHz v=1 SiO maser transitions quasi-simultaneously for a Mira-variable-dominated sample of over 80 sources from the Bulge Asymmetries and Dynamical Evolution (BAaDE) project, using ATCA, and statistically compared the relative line strengths. On average, the 43 GHz v=1 line is brighter than the 86 GHz v=1 line by a factor of 1.36+/-0.15. As a result, an 86 GHz v=1 observed sample can be observed to 85.9% of the distance of a 43 GHz v=1 observed sample using the same sensitivity. We discuss what impact this may have on the BAaDE Galactic plane survey "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.02899","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":"1808.02899","created_at":"2026-05-18T00:08:30.703045+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.02899v1","created_at":"2026-05-18T00:08:30.703045+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.02899","created_at":"2026-05-18T00:08:30.703045+00:00"},{"alias_kind":"pith_short_12","alias_value":"QXRS242KKF5G","created_at":"2026-05-18T12:32:50.500415+00:00"},{"alias_kind":"pith_short_16","alias_value":"QXRS242KKF5GKIZF","created_at":"2026-05-18T12:32:50.500415+00:00"},{"alias_kind":"pith_short_8","alias_value":"QXRS242K","created_at":"2026-05-18T12:32:50.500415+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/QXRS242KKF5GKIZFPKNGLUXTV3","json":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3.json","graph_json":"https://pith.science/api/pith-number/QXRS242KKF5GKIZFPKNGLUXTV3/graph.json","events_json":"https://pith.science/api/pith-number/QXRS242KKF5GKIZFPKNGLUXTV3/events.json","paper":"https://pith.science/paper/QXRS242K"},"agent_actions":{"view_html":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3","download_json":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3.json","view_paper":"https://pith.science/paper/QXRS242K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.02899&json=true","fetch_graph":"https://pith.science/api/pith-number/QXRS242KKF5GKIZFPKNGLUXTV3/graph.json","fetch_events":"https://pith.science/api/pith-number/QXRS242KKF5GKIZFPKNGLUXTV3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3/action/storage_attestation","attest_author":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3/action/author_attestation","sign_citation":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3/action/citation_signature","submit_replication":"https://pith.science/pith/QXRS242KKF5GKIZFPKNGLUXTV3/action/replication_record"}},"created_at":"2026-05-18T00:08:30.703045+00:00","updated_at":"2026-05-18T00:08:30.703045+00:00"}