{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:KYK6KPSE45GTWGZH6EAHH57LLP","short_pith_number":"pith:KYK6KPSE","schema_version":"1.0","canonical_sha256":"5615e53e44e74d3b1b27f10073f7eb5be5c5b11c2206437ec7680bbe2779bcfd","source":{"kind":"arxiv","id":"2407.03445","version":1},"attestation_state":"computed","paper":{"title":"Submillimeter and Mid-Infrared Variability of Young Stellar Objects in the M17SWex Intermediate-Mass Star-Forming Region","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Carlos Contreras Pena, Doug Johnstone, Geumsook Park, Gregory Herczeg, Jennifer Hatchell, Jeong-Eun Lee, Kee-Tae Kim, Keping Qiu, Mi-Ryang Kim, Sheng-Yuan Liu, Steve Mairs, The JCMT Transient Team, Xu Zhang, Yao-Te Wang, Zhiwei Chen","submitted_at":"2024-07-03T18:44:18Z","abstract_excerpt":"We present a comprehensive analysis of young stellar object (YSO) variability within the M17 Southwest Extension (M17 SWex), using 3.5 years of monitoring data from the JCMT Transient Survey at sub-millimeter (sub-mm) and 9 years from the NEOWISE mission at mid-infrared (mid-IR). Our study encompasses observations of 147 bright sub-mm peaks identified within our deep JCMT co-added map as well as 156 YSOs in NEOWISE W1 and 179 in W2 that were previously identified in Spitzer surveys. We find three robust sub-mm variables: two are candidate YSOs and one is a likely extragalactic source. At mid-I"},"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":"2407.03445","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-07-03T18:44:18Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"fe61b4a9b86f7485136dbc00d42e1d7dbfc9101da1e0a25d836521986704c6ad","abstract_canon_sha256":"b47a10c56e82608814cdd6817011cdd48074a533dff92a41b9f657e81b0c89a1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:39:55.023556Z","signature_b64":"IAP0rXEaAiTN+lU2NMT1KxnSw2T2FSlqb47RwHg+sPlZ2ZoleYwLGJkCASx6Met1rsigMkud4ubrWXNf12kFCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5615e53e44e74d3b1b27f10073f7eb5be5c5b11c2206437ec7680bbe2779bcfd","last_reissued_at":"2026-07-05T08:39:55.023120Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:39:55.023120Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Submillimeter and Mid-Infrared Variability of Young Stellar Objects in the M17SWex Intermediate-Mass Star-Forming Region","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Carlos Contreras Pena, Doug Johnstone, Geumsook Park, Gregory Herczeg, Jennifer Hatchell, Jeong-Eun Lee, Kee-Tae Kim, Keping Qiu, Mi-Ryang Kim, Sheng-Yuan Liu, Steve Mairs, The JCMT Transient Team, Xu Zhang, Yao-Te Wang, Zhiwei Chen","submitted_at":"2024-07-03T18:44:18Z","abstract_excerpt":"We present a comprehensive analysis of young stellar object (YSO) variability within the M17 Southwest Extension (M17 SWex), using 3.5 years of monitoring data from the JCMT Transient Survey at sub-millimeter (sub-mm) and 9 years from the NEOWISE mission at mid-infrared (mid-IR). Our study encompasses observations of 147 bright sub-mm peaks identified within our deep JCMT co-added map as well as 156 YSOs in NEOWISE W1 and 179 in W2 that were previously identified in Spitzer surveys. We find three robust sub-mm variables: two are candidate YSOs and one is a likely extragalactic source. At mid-I"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.03445","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/2407.03445/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":"2407.03445","created_at":"2026-07-05T08:39:55.023174+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.03445v1","created_at":"2026-07-05T08:39:55.023174+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.03445","created_at":"2026-07-05T08:39:55.023174+00:00"},{"alias_kind":"pith_short_12","alias_value":"KYK6KPSE45GT","created_at":"2026-07-05T08:39:55.023174+00:00"},{"alias_kind":"pith_short_16","alias_value":"KYK6KPSE45GTWGZH","created_at":"2026-07-05T08:39:55.023174+00:00"},{"alias_kind":"pith_short_8","alias_value":"KYK6KPSE","created_at":"2026-07-05T08:39:55.023174+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/KYK6KPSE45GTWGZH6EAHH57LLP","json":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP.json","graph_json":"https://pith.science/api/pith-number/KYK6KPSE45GTWGZH6EAHH57LLP/graph.json","events_json":"https://pith.science/api/pith-number/KYK6KPSE45GTWGZH6EAHH57LLP/events.json","paper":"https://pith.science/paper/KYK6KPSE"},"agent_actions":{"view_html":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP","download_json":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP.json","view_paper":"https://pith.science/paper/KYK6KPSE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.03445&json=true","fetch_graph":"https://pith.science/api/pith-number/KYK6KPSE45GTWGZH6EAHH57LLP/graph.json","fetch_events":"https://pith.science/api/pith-number/KYK6KPSE45GTWGZH6EAHH57LLP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP/action/storage_attestation","attest_author":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP/action/author_attestation","sign_citation":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP/action/citation_signature","submit_replication":"https://pith.science/pith/KYK6KPSE45GTWGZH6EAHH57LLP/action/replication_record"}},"created_at":"2026-07-05T08:39:55.023174+00:00","updated_at":"2026-07-05T08:39:55.023174+00:00"}