{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:Z5ZDUPIQCHQVSCDB6UL5RCA2L6","short_pith_number":"pith:Z5ZDUPIQ","schema_version":"1.0","canonical_sha256":"cf723a3d1011e1590861f517d8881a5f97b6d898a378b0b2b04875329a6b03ca","source":{"kind":"arxiv","id":"0710.5938","version":2},"attestation_state":"computed","paper":{"title":"SPITZER SAGE Observations of Large Magellanic Cloud Planetary Nebulae","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. A. Whitney, B. L. Babler, B.-Q. For, C. Leitherer, C. W. Engelbracht, J. L. Hora, K. Gordon, K. Misselt, M. Block, M. Cohen, M. Meixner, M. R. Meade, R. D. Blum, R. G. Ellis, R. Indebetouw, U. Vijh, W. B. Latter","submitted_at":"2007-10-31T19:37:22Z","abstract_excerpt":"We present IRAC and MIPS images and photometry of a sample of previously known planetary nebulae (PNe) from the SAGE survey of the Large Magellanic Cloud (LMC) performed with the Spitzer Space Telescope. Of the 233 known PNe in the survey field, 185 objects were detected in at least two of the IRAC bands, and 161 detected in the MIPS 24 micron images. Color-color and color-magnitude diagrams are presented using several combinations of IRAC, MIPS, and 2MASS magnitudes. The location of an individual PN in the color-color diagrams is seen to depend on the relative contributions of the spectral co"},"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":"0710.5938","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-10-31T19:37:22Z","cross_cats_sorted":[],"title_canon_sha256":"015bf1c28830195a62b63bf312bc5c5332a04160e47466d6719d5b123701511c","abstract_canon_sha256":"537fec6eac94f12e2bc5ae088efa275a2b275450336477fec2a72a469f68e091"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:44:34.357193Z","signature_b64":"WLvszfL5z9g7N3DzZ9PEFdJ42piEOldWTfsMTnVRIMm6HMWHkQ4t6hN8vAf1E3gonW1iyU4XUUuWFu6T7rtuDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf723a3d1011e1590861f517d8881a5f97b6d898a378b0b2b04875329a6b03ca","last_reissued_at":"2026-07-04T15:44:34.356653Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:44:34.356653Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SPITZER SAGE Observations of Large Magellanic Cloud Planetary Nebulae","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. A. Whitney, B. L. Babler, B.-Q. For, C. Leitherer, C. W. Engelbracht, J. L. Hora, K. Gordon, K. Misselt, M. Block, M. Cohen, M. Meixner, M. R. Meade, R. D. Blum, R. G. Ellis, R. Indebetouw, U. Vijh, W. B. Latter","submitted_at":"2007-10-31T19:37:22Z","abstract_excerpt":"We present IRAC and MIPS images and photometry of a sample of previously known planetary nebulae (PNe) from the SAGE survey of the Large Magellanic Cloud (LMC) performed with the Spitzer Space Telescope. Of the 233 known PNe in the survey field, 185 objects were detected in at least two of the IRAC bands, and 161 detected in the MIPS 24 micron images. Color-color and color-magnitude diagrams are presented using several combinations of IRAC, MIPS, and 2MASS magnitudes. The location of an individual PN in the color-color diagrams is seen to depend on the relative contributions of the spectral co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0710.5938","kind":"arxiv","version":2},"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/0710.5938/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":"0710.5938","created_at":"2026-07-04T15:44:34.356715+00:00"},{"alias_kind":"arxiv_version","alias_value":"0710.5938v2","created_at":"2026-07-04T15:44:34.356715+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0710.5938","created_at":"2026-07-04T15:44:34.356715+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z5ZDUPIQCHQV","created_at":"2026-07-04T15:44:34.356715+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z5ZDUPIQCHQVSCDB","created_at":"2026-07-04T15:44:34.356715+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z5ZDUPIQ","created_at":"2026-07-04T15:44:34.356715+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/Z5ZDUPIQCHQVSCDB6UL5RCA2L6","json":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6.json","graph_json":"https://pith.science/api/pith-number/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/graph.json","events_json":"https://pith.science/api/pith-number/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/events.json","paper":"https://pith.science/paper/Z5ZDUPIQ"},"agent_actions":{"view_html":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6","download_json":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6.json","view_paper":"https://pith.science/paper/Z5ZDUPIQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0710.5938&json=true","fetch_graph":"https://pith.science/api/pith-number/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/graph.json","fetch_events":"https://pith.science/api/pith-number/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/action/storage_attestation","attest_author":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/action/author_attestation","sign_citation":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/action/citation_signature","submit_replication":"https://pith.science/pith/Z5ZDUPIQCHQVSCDB6UL5RCA2L6/action/replication_record"}},"created_at":"2026-07-04T15:44:34.356715+00:00","updated_at":"2026-07-04T15:44:34.356715+00:00"}