{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HW6XSDP5HLAEKM4PRIB2D5OKB4","short_pith_number":"pith:HW6XSDP5","schema_version":"1.0","canonical_sha256":"3dbd790dfd3ac045338f8a03a1f5ca0f2feb02a8161f1b381b512fe4cc53b970","source":{"kind":"arxiv","id":"1101.4546","version":1},"attestation_state":"computed","paper":{"title":"The Spitzer Survey of Interstellar Clouds in the Gould Belt. IV. Lupus V and VI Observed with IRAC and MIPS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bruno Mer{\\i}n, Dawn Peterson, Jes K. J{\\o}rgensen, Loredana Spezzi, Lori E. Allen, Lucas A. Cieza, Michael M. Dunham, Neal J. Evans II, Nick F. H. Tothill, Paul M. Harvey, Pierre Vernazza, the Gould's Belt Team, Tracy L. Huard, Tyler L. Bourke","submitted_at":"2011-01-24T14:30:02Z","abstract_excerpt":"We present Gould's Belt (GB) Spitzer IRAC and MIPS observations of the Lupus V and VI clouds and discuss them in combination with near-infrared (2MASS) data. Our observations complement those obtained for other Lupus clouds within the frame of the Spitzer \"Core to Disk\" (c2d) Legacy Survey. We found 43 Young Stellar Object (YSO) candidates in Lupus V and 45 in Lupus VI, including 2 transition disks, using the standard c2d/GB selection method. None of these sources was classified as a pre-main sequence star from previous optical, near-IR and X-ray surveys. A large majority of these YSO candidat"},"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":"1101.4546","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-24T14:30:02Z","cross_cats_sorted":[],"title_canon_sha256":"fa2c9c0456478e9e870a15540a19122c3f5162115aa68f817142bbbdd8cc8140","abstract_canon_sha256":"14bfe67d9891b633b8e2eee02d6a18c295eea10eca2f169e1a01a6a329850a5f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:24.752768Z","signature_b64":"vdH8xBm9j1vczkd7YPvsm8LN88DrCTW332G2YMW1fZ8F0JCNcWz7QC4b/bqp1KTwAbae7eL25mEPFL3DrLCiDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3dbd790dfd3ac045338f8a03a1f5ca0f2feb02a8161f1b381b512fe4cc53b970","last_reissued_at":"2026-05-18T02:03:24.752020Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:24.752020Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Spitzer Survey of Interstellar Clouds in the Gould Belt. IV. Lupus V and VI Observed with IRAC and MIPS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bruno Mer{\\i}n, Dawn Peterson, Jes K. J{\\o}rgensen, Loredana Spezzi, Lori E. Allen, Lucas A. Cieza, Michael M. Dunham, Neal J. Evans II, Nick F. H. Tothill, Paul M. Harvey, Pierre Vernazza, the Gould's Belt Team, Tracy L. Huard, Tyler L. Bourke","submitted_at":"2011-01-24T14:30:02Z","abstract_excerpt":"We present Gould's Belt (GB) Spitzer IRAC and MIPS observations of the Lupus V and VI clouds and discuss them in combination with near-infrared (2MASS) data. Our observations complement those obtained for other Lupus clouds within the frame of the Spitzer \"Core to Disk\" (c2d) Legacy Survey. We found 43 Young Stellar Object (YSO) candidates in Lupus V and 45 in Lupus VI, including 2 transition disks, using the standard c2d/GB selection method. None of these sources was classified as a pre-main sequence star from previous optical, near-IR and X-ray surveys. A large majority of these YSO candidat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.4546","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":"1101.4546","created_at":"2026-05-18T02:03:24.752141+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.4546v1","created_at":"2026-05-18T02:03:24.752141+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.4546","created_at":"2026-05-18T02:03:24.752141+00:00"},{"alias_kind":"pith_short_12","alias_value":"HW6XSDP5HLAE","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HW6XSDP5HLAEKM4P","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HW6XSDP5","created_at":"2026-05-18T12:26:30.835961+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/HW6XSDP5HLAEKM4PRIB2D5OKB4","json":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4.json","graph_json":"https://pith.science/api/pith-number/HW6XSDP5HLAEKM4PRIB2D5OKB4/graph.json","events_json":"https://pith.science/api/pith-number/HW6XSDP5HLAEKM4PRIB2D5OKB4/events.json","paper":"https://pith.science/paper/HW6XSDP5"},"agent_actions":{"view_html":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4","download_json":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4.json","view_paper":"https://pith.science/paper/HW6XSDP5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.4546&json=true","fetch_graph":"https://pith.science/api/pith-number/HW6XSDP5HLAEKM4PRIB2D5OKB4/graph.json","fetch_events":"https://pith.science/api/pith-number/HW6XSDP5HLAEKM4PRIB2D5OKB4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4/action/storage_attestation","attest_author":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4/action/author_attestation","sign_citation":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4/action/citation_signature","submit_replication":"https://pith.science/pith/HW6XSDP5HLAEKM4PRIB2D5OKB4/action/replication_record"}},"created_at":"2026-05-18T02:03:24.752141+00:00","updated_at":"2026-05-18T02:03:24.752141+00:00"}