{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:YJZBYNFBLZXMS6MZP6EZPVITER","short_pith_number":"pith:YJZBYNFB","schema_version":"1.0","canonical_sha256":"c2721c34a15e6ec979997f8997d51324500846e5e15aa8eee95c551d15110e73","source":{"kind":"arxiv","id":"1410.6428","version":1},"attestation_state":"computed","paper":{"title":"Star formation around the mid-infrared bubble CN 148","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. K. Ojha, J. M. C. Grave, K. K. Mallick, L. K. Dewangan","submitted_at":"2014-10-23T17:43:04Z","abstract_excerpt":"We present a multi-wavelength study to analyse the star formation process associated with the mid-infrared bubble CN 148 (H II region G10.3-0.1), which harbors an O5V-O6V star. The arc-shaped distribution of molecular CO(2-1) emission, the cold dust emission, and the polycyclic aromatic hydrocarbon features trace a photodissociation region (PDR) around the H II region. We have identified 371 young stellar objects (YSOs) in the selected region and, interestingly, their spatial distribution correlates well with the PDR. 41% of these YSOs are present in 13 clusters, each having visual extinction "},"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":"1410.6428","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-10-23T17:43:04Z","cross_cats_sorted":[],"title_canon_sha256":"41b73b313ecc040bdaa5f4e93c3c7a680962b792db467ebf94f0f006a9a064d3","abstract_canon_sha256":"3d5d6a7ed94c01c059f19100229f3b8dc2fecfaa32131426f16b18da535a611a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:40.437480Z","signature_b64":"k6AyTcWSQezcmSrM/aoGIiI6MiHWmb0xHiM88qXnf3cCi4ufAVJsnBUG0k2kaq0LoJKxu3J/01WxHHeH3bE8AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c2721c34a15e6ec979997f8997d51324500846e5e15aa8eee95c551d15110e73","last_reissued_at":"2026-05-18T01:41:40.436622Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:40.436622Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star formation around the mid-infrared bubble CN 148","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. K. Ojha, J. M. C. Grave, K. K. Mallick, L. K. Dewangan","submitted_at":"2014-10-23T17:43:04Z","abstract_excerpt":"We present a multi-wavelength study to analyse the star formation process associated with the mid-infrared bubble CN 148 (H II region G10.3-0.1), which harbors an O5V-O6V star. The arc-shaped distribution of molecular CO(2-1) emission, the cold dust emission, and the polycyclic aromatic hydrocarbon features trace a photodissociation region (PDR) around the H II region. We have identified 371 young stellar objects (YSOs) in the selected region and, interestingly, their spatial distribution correlates well with the PDR. 41% of these YSOs are present in 13 clusters, each having visual extinction "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.6428","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":"1410.6428","created_at":"2026-05-18T01:41:40.436761+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.6428v1","created_at":"2026-05-18T01:41:40.436761+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.6428","created_at":"2026-05-18T01:41:40.436761+00:00"},{"alias_kind":"pith_short_12","alias_value":"YJZBYNFBLZXM","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"YJZBYNFBLZXMS6MZ","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"YJZBYNFB","created_at":"2026-05-18T12:28:57.508820+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/YJZBYNFBLZXMS6MZP6EZPVITER","json":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER.json","graph_json":"https://pith.science/api/pith-number/YJZBYNFBLZXMS6MZP6EZPVITER/graph.json","events_json":"https://pith.science/api/pith-number/YJZBYNFBLZXMS6MZP6EZPVITER/events.json","paper":"https://pith.science/paper/YJZBYNFB"},"agent_actions":{"view_html":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER","download_json":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER.json","view_paper":"https://pith.science/paper/YJZBYNFB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.6428&json=true","fetch_graph":"https://pith.science/api/pith-number/YJZBYNFBLZXMS6MZP6EZPVITER/graph.json","fetch_events":"https://pith.science/api/pith-number/YJZBYNFBLZXMS6MZP6EZPVITER/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER/action/storage_attestation","attest_author":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER/action/author_attestation","sign_citation":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER/action/citation_signature","submit_replication":"https://pith.science/pith/YJZBYNFBLZXMS6MZP6EZPVITER/action/replication_record"}},"created_at":"2026-05-18T01:41:40.436761+00:00","updated_at":"2026-05-18T01:41:40.436761+00:00"}