{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:YBE2ZTUWQSAJC7GMMEJXORT6DQ","short_pith_number":"pith:YBE2ZTUW","schema_version":"1.0","canonical_sha256":"c049acce968480917ccc611377467e1c1da221ed433b7d4f763fabf79ca13b19","source":{"kind":"arxiv","id":"2403.14615","version":1},"attestation_state":"computed","paper":{"title":"Search for protostellar jets with UWISH2 in the molecular cloud complexes Vulpecula and IRDC G53.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anandmayee Tej, Dirk Froebrich, Manash Samal, Manish Chauhan","submitted_at":"2024-03-21T17:58:18Z","abstract_excerpt":"Jets and outflows are the early signposts of stellar birth. Using the UKIRT Wide Field Infrared Survey for H2 (UWISH2) at 2.12 micron, 127 outflows are identified in molecular cloud complexes Vulpecula OB1 and IRDC G53.2 covering 12 square degrees of the Galactic plane. Using multi-wavelength datasets, from 1.2 to 70 micron, 79 young stellar objects (YSOs) are proposed as potential driving sources, where, $\\sim$ 79% are likely Class 0/I protostars, 17% are Class II YSOs and the remaining 4% are Class III YSOs. The outflows are characterized in terms of their length, flux, luminosity and knot-s"},"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":"2403.14615","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-03-21T17:58:18Z","cross_cats_sorted":[],"title_canon_sha256":"367d652657e21f706e8720cafa5526e9da42cd567f373618cb06de17ac3b7560","abstract_canon_sha256":"c0d1afaca59eba3908ffc16aad339dc5f4c420a513fb99240a29e5e354f09e68"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:59:11.488837Z","signature_b64":"zrwUzdqlG9rgVPradn//V4LCDluHhOapyLV+nAIas0R/ttOpN3EyJ25fb+lfnb+Dd75G6Nu1TetyBw+OIYAjAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c049acce968480917ccc611377467e1c1da221ed433b7d4f763fabf79ca13b19","last_reissued_at":"2026-07-05T07:59:11.488373Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:59:11.488373Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for protostellar jets with UWISH2 in the molecular cloud complexes Vulpecula and IRDC G53.2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anandmayee Tej, Dirk Froebrich, Manash Samal, Manish Chauhan","submitted_at":"2024-03-21T17:58:18Z","abstract_excerpt":"Jets and outflows are the early signposts of stellar birth. Using the UKIRT Wide Field Infrared Survey for H2 (UWISH2) at 2.12 micron, 127 outflows are identified in molecular cloud complexes Vulpecula OB1 and IRDC G53.2 covering 12 square degrees of the Galactic plane. Using multi-wavelength datasets, from 1.2 to 70 micron, 79 young stellar objects (YSOs) are proposed as potential driving sources, where, $\\sim$ 79% are likely Class 0/I protostars, 17% are Class II YSOs and the remaining 4% are Class III YSOs. The outflows are characterized in terms of their length, flux, luminosity and knot-s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.14615","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.14615/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2403.14615","created_at":"2026-07-05T07:59:11.488433+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.14615v1","created_at":"2026-07-05T07:59:11.488433+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.14615","created_at":"2026-07-05T07:59:11.488433+00:00"},{"alias_kind":"pith_short_12","alias_value":"YBE2ZTUWQSAJ","created_at":"2026-07-05T07:59:11.488433+00:00"},{"alias_kind":"pith_short_16","alias_value":"YBE2ZTUWQSAJC7GM","created_at":"2026-07-05T07:59:11.488433+00:00"},{"alias_kind":"pith_short_8","alias_value":"YBE2ZTUW","created_at":"2026-07-05T07:59:11.488433+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/YBE2ZTUWQSAJC7GMMEJXORT6DQ","json":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ.json","graph_json":"https://pith.science/api/pith-number/YBE2ZTUWQSAJC7GMMEJXORT6DQ/graph.json","events_json":"https://pith.science/api/pith-number/YBE2ZTUWQSAJC7GMMEJXORT6DQ/events.json","paper":"https://pith.science/paper/YBE2ZTUW"},"agent_actions":{"view_html":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ","download_json":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ.json","view_paper":"https://pith.science/paper/YBE2ZTUW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.14615&json=true","fetch_graph":"https://pith.science/api/pith-number/YBE2ZTUWQSAJC7GMMEJXORT6DQ/graph.json","fetch_events":"https://pith.science/api/pith-number/YBE2ZTUWQSAJC7GMMEJXORT6DQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ/action/storage_attestation","attest_author":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ/action/author_attestation","sign_citation":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ/action/citation_signature","submit_replication":"https://pith.science/pith/YBE2ZTUWQSAJC7GMMEJXORT6DQ/action/replication_record"}},"created_at":"2026-07-05T07:59:11.488433+00:00","updated_at":"2026-07-05T07:59:11.488433+00:00"}