{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:BODFTIXWAFAASNRGH3JO5XGQQI","short_pith_number":"pith:BODFTIXW","schema_version":"1.0","canonical_sha256":"0b8659a2f601400936263ed2eedcd082278cb72fbc243d712a94dc968801f35e","source":{"kind":"arxiv","id":"1102.1032","version":2},"attestation_state":"computed","paper":{"title":"A Mid-Infrared Census of Star Formation Activity in Bolocam Galactic Plane Survey Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Claudia J. Cyganowski, James Urquhart, Miranda K. Dunham, Neal J. Evans II, Thomas P. Robitaille, Wayne M. Schlingman","submitted_at":"2011-02-04T23:13:03Z","abstract_excerpt":"We present the results of a search for mid-infrared signs of star formation activity in the 1.1 mm sources in the Bolocam Galactic Plane Survey (BGPS). We have correlated the BGPS catalog with available mid-IR Galactic plane catalogs based on the Spitzer Space Telescope GLIMPSE legacy survey and the Midcourse Space Experiment (MSX) Galactic plane survey. We find that 44% (3,712 of 8,358) of the BGPS sources contain at least one mid-IR source, including 2,457 of 5,067 (49%) within the area where all surveys overlap (10 deg < l < 65 deg). Accounting for chance alignments between the BGPS and mid"},"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":"1102.1032","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2011-02-04T23:13:03Z","cross_cats_sorted":[],"title_canon_sha256":"5b38cbc4ea1c94e569ea7faa8bc3bfa6e2f641b2c2f5bc70a19e5cf9bdc285d5","abstract_canon_sha256":"4832e4233180d47c44af77f6b14b1332074fb500f7c5a124729425e7813b3bbc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:16.475167Z","signature_b64":"cpDD3J03seHaA+15Ktt7xCcOfinK+uLGLCsPzieidGvB7PhrbYZh01ciSvUR/1TTNhBTvWFeaGbqROUXoLByAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b8659a2f601400936263ed2eedcd082278cb72fbc243d712a94dc968801f35e","last_reissued_at":"2026-05-18T02:03:16.474404Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:16.474404Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Mid-Infrared Census of Star Formation Activity in Bolocam Galactic Plane Survey Sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Claudia J. Cyganowski, James Urquhart, Miranda K. Dunham, Neal J. Evans II, Thomas P. Robitaille, Wayne M. Schlingman","submitted_at":"2011-02-04T23:13:03Z","abstract_excerpt":"We present the results of a search for mid-infrared signs of star formation activity in the 1.1 mm sources in the Bolocam Galactic Plane Survey (BGPS). We have correlated the BGPS catalog with available mid-IR Galactic plane catalogs based on the Spitzer Space Telescope GLIMPSE legacy survey and the Midcourse Space Experiment (MSX) Galactic plane survey. We find that 44% (3,712 of 8,358) of the BGPS sources contain at least one mid-IR source, including 2,457 of 5,067 (49%) within the area where all surveys overlap (10 deg < l < 65 deg). Accounting for chance alignments between the BGPS and mid"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.1032","kind":"arxiv","version":2},"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":"1102.1032","created_at":"2026-05-18T02:03:16.474543+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.1032v2","created_at":"2026-05-18T02:03:16.474543+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.1032","created_at":"2026-05-18T02:03:16.474543+00:00"},{"alias_kind":"pith_short_12","alias_value":"BODFTIXWAFAA","created_at":"2026-05-18T12:26:24.575870+00:00"},{"alias_kind":"pith_short_16","alias_value":"BODFTIXWAFAASNRG","created_at":"2026-05-18T12:26:24.575870+00:00"},{"alias_kind":"pith_short_8","alias_value":"BODFTIXW","created_at":"2026-05-18T12:26:24.575870+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/BODFTIXWAFAASNRGH3JO5XGQQI","json":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI.json","graph_json":"https://pith.science/api/pith-number/BODFTIXWAFAASNRGH3JO5XGQQI/graph.json","events_json":"https://pith.science/api/pith-number/BODFTIXWAFAASNRGH3JO5XGQQI/events.json","paper":"https://pith.science/paper/BODFTIXW"},"agent_actions":{"view_html":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI","download_json":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI.json","view_paper":"https://pith.science/paper/BODFTIXW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.1032&json=true","fetch_graph":"https://pith.science/api/pith-number/BODFTIXWAFAASNRGH3JO5XGQQI/graph.json","fetch_events":"https://pith.science/api/pith-number/BODFTIXWAFAASNRGH3JO5XGQQI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI/action/storage_attestation","attest_author":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI/action/author_attestation","sign_citation":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI/action/citation_signature","submit_replication":"https://pith.science/pith/BODFTIXWAFAASNRGH3JO5XGQQI/action/replication_record"}},"created_at":"2026-05-18T02:03:16.474543+00:00","updated_at":"2026-05-18T02:03:16.474543+00:00"}