{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FC6SKQ7V5OGXPEFBOXRJQDLMJG","short_pith_number":"pith:FC6SKQ7V","schema_version":"1.0","canonical_sha256":"28bd2543f5eb8d7790a175e2980d6c4984aa3f92245df9166857ad3ead0717ba","source":{"kind":"arxiv","id":"1812.06808","version":1},"attestation_state":"computed","paper":{"title":"Investigation of the stellar content in the IRAS 05168+3634 star-forming region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"N. Azatyan","submitted_at":"2018-12-17T14:47:39Z","abstract_excerpt":"We present the investigation results of structure and stellar content of a molecular cloud surrounding the five IRAS sources: 05168+3634, 05184+3635, 05177+3636, 05162+3639, and IRAS 05156+3643. Using multi-color criteria, we identified a rich population of embedded YSO candidates with infrared excess (Class 0/I and Class II) and their characteristics in a quite large molecular cloud which is located in the region of 24 arcmin radius. The molecular cloud includes 240 candidates of YSOs within the radii of sub-regions around 5 IRAS sources. The color-magnitude diagrams of the sub-regions sugges"},"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":"1812.06808","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-12-17T14:47:39Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"c6e98cd940da94e01975e9cdb19904a80415cb274a1dd16f2a2169548f1aeb54","abstract_canon_sha256":"3b691f130920a51c0903a0ff6e6ea3c24dc20d004a2b786ecd9b5573ff899380"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:55:10.534938Z","signature_b64":"CO9ZL6d8gfH5ZjoF0LbVgiHnhFOchc4EsXRLdAUXjcaRiz06sv7hC+OoQBtd4B+TQ8/LnLgHDHS1CcGuqYJVBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28bd2543f5eb8d7790a175e2980d6c4984aa3f92245df9166857ad3ead0717ba","last_reissued_at":"2026-05-17T23:55:10.534489Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:55:10.534489Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigation of the stellar content in the IRAS 05168+3634 star-forming region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"N. Azatyan","submitted_at":"2018-12-17T14:47:39Z","abstract_excerpt":"We present the investigation results of structure and stellar content of a molecular cloud surrounding the five IRAS sources: 05168+3634, 05184+3635, 05177+3636, 05162+3639, and IRAS 05156+3643. Using multi-color criteria, we identified a rich population of embedded YSO candidates with infrared excess (Class 0/I and Class II) and their characteristics in a quite large molecular cloud which is located in the region of 24 arcmin radius. The molecular cloud includes 240 candidates of YSOs within the radii of sub-regions around 5 IRAS sources. The color-magnitude diagrams of the sub-regions sugges"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.06808","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":"1812.06808","created_at":"2026-05-17T23:55:10.534558+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.06808v1","created_at":"2026-05-17T23:55:10.534558+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.06808","created_at":"2026-05-17T23:55:10.534558+00:00"},{"alias_kind":"pith_short_12","alias_value":"FC6SKQ7V5OGX","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_16","alias_value":"FC6SKQ7V5OGXPEFB","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_8","alias_value":"FC6SKQ7V","created_at":"2026-05-18T12:32:22.470017+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/FC6SKQ7V5OGXPEFBOXRJQDLMJG","json":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG.json","graph_json":"https://pith.science/api/pith-number/FC6SKQ7V5OGXPEFBOXRJQDLMJG/graph.json","events_json":"https://pith.science/api/pith-number/FC6SKQ7V5OGXPEFBOXRJQDLMJG/events.json","paper":"https://pith.science/paper/FC6SKQ7V"},"agent_actions":{"view_html":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG","download_json":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG.json","view_paper":"https://pith.science/paper/FC6SKQ7V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.06808&json=true","fetch_graph":"https://pith.science/api/pith-number/FC6SKQ7V5OGXPEFBOXRJQDLMJG/graph.json","fetch_events":"https://pith.science/api/pith-number/FC6SKQ7V5OGXPEFBOXRJQDLMJG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG/action/storage_attestation","attest_author":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG/action/author_attestation","sign_citation":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG/action/citation_signature","submit_replication":"https://pith.science/pith/FC6SKQ7V5OGXPEFBOXRJQDLMJG/action/replication_record"}},"created_at":"2026-05-17T23:55:10.534558+00:00","updated_at":"2026-05-17T23:55:10.534558+00:00"}