{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:3QVE76JVF74YHDIOLDXPA2COOJ","short_pith_number":"pith:3QVE76JV","schema_version":"1.0","canonical_sha256":"dc2a4ff9352ff9838d0e58eef0684e725aec8655c154d18ae1a4744053b4aeda","source":{"kind":"arxiv","id":"0906.3353","version":1},"attestation_state":"computed","paper":{"title":"Ks-band (2.14 micron) imaging of southern massive star formation regions traced by methanol masers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"(2) University of New South Wales), M. G. Burton ((1) Harvard-Smithsonian Center for Astrophysics, S. N. Longmore","submitted_at":"2009-06-18T06:04:26Z","abstract_excerpt":"We present deep, wide-field, Ks-band (2.14 micron) images towards 87 southern massive star formation regions traced by methanol maser emission. Using point-spread function fitting, we generate 2.14 micron point source catalogues towards each of the regions. For the regions between 10 degrees and 350 degrees galactic longitude and galactic latitude +/- 1 degree, we match the 2.14 micron sources with the GLIMPSE point source catalogue to generate a combined 2.14 to 8.0 micron point source catalogue. We provide this data for the astronomical community to utilise in studies of the stellar content "},"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":"0906.3353","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-06-18T06:04:26Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"cdd0f637acbf75761bd4b7e74d348f76653b64f84712cf2e5fee6487a9ddeeb7","abstract_canon_sha256":"fa23a3e8051c6dbae9c5ceb32afefd796fc73c58c060fda1630a82d47e559e00"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:31:41.545624Z","signature_b64":"sQQkIKBrPrqMre9Ng3698AzVi0MNiirO+S0b3Wihy4BwL47GAk6vFwd1HmkEa4OsYgv5j5BgtKYEWTwvZvOfCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc2a4ff9352ff9838d0e58eef0684e725aec8655c154d18ae1a4744053b4aeda","last_reissued_at":"2026-05-18T04:31:41.545147Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:31:41.545147Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ks-band (2.14 micron) imaging of southern massive star formation regions traced by methanol masers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"(2) University of New South Wales), M. G. Burton ((1) Harvard-Smithsonian Center for Astrophysics, S. N. Longmore","submitted_at":"2009-06-18T06:04:26Z","abstract_excerpt":"We present deep, wide-field, Ks-band (2.14 micron) images towards 87 southern massive star formation regions traced by methanol maser emission. Using point-spread function fitting, we generate 2.14 micron point source catalogues towards each of the regions. For the regions between 10 degrees and 350 degrees galactic longitude and galactic latitude +/- 1 degree, we match the 2.14 micron sources with the GLIMPSE point source catalogue to generate a combined 2.14 to 8.0 micron point source catalogue. We provide this data for the astronomical community to utilise in studies of the stellar content "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0906.3353","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":"0906.3353","created_at":"2026-05-18T04:31:41.545226+00:00"},{"alias_kind":"arxiv_version","alias_value":"0906.3353v1","created_at":"2026-05-18T04:31:41.545226+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0906.3353","created_at":"2026-05-18T04:31:41.545226+00:00"},{"alias_kind":"pith_short_12","alias_value":"3QVE76JVF74Y","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_16","alias_value":"3QVE76JVF74YHDIO","created_at":"2026-05-18T12:25:58.018023+00:00"},{"alias_kind":"pith_short_8","alias_value":"3QVE76JV","created_at":"2026-05-18T12:25:58.018023+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/3QVE76JVF74YHDIOLDXPA2COOJ","json":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ.json","graph_json":"https://pith.science/api/pith-number/3QVE76JVF74YHDIOLDXPA2COOJ/graph.json","events_json":"https://pith.science/api/pith-number/3QVE76JVF74YHDIOLDXPA2COOJ/events.json","paper":"https://pith.science/paper/3QVE76JV"},"agent_actions":{"view_html":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ","download_json":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ.json","view_paper":"https://pith.science/paper/3QVE76JV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0906.3353&json=true","fetch_graph":"https://pith.science/api/pith-number/3QVE76JVF74YHDIOLDXPA2COOJ/graph.json","fetch_events":"https://pith.science/api/pith-number/3QVE76JVF74YHDIOLDXPA2COOJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ/action/storage_attestation","attest_author":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ/action/author_attestation","sign_citation":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ/action/citation_signature","submit_replication":"https://pith.science/pith/3QVE76JVF74YHDIOLDXPA2COOJ/action/replication_record"}},"created_at":"2026-05-18T04:31:41.545226+00:00","updated_at":"2026-05-18T04:31:41.545226+00:00"}