{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LZMZECARDRRECUE52MYFBMK4YS","short_pith_number":"pith:LZMZECAR","schema_version":"1.0","canonical_sha256":"5e599208111c6241509dd33050b15cc4b04a6a7ecbc97cfa42a1bc513b9898e1","source":{"kind":"arxiv","id":"1604.05384","version":1},"attestation_state":"computed","paper":{"title":"Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. LaCluyz, D. P. Cruikshank, D. Reichart, F. Marchis, F. Vachier, J. Berthier, J.E. Enriquez, J. Haislip, J. P. Emery, J. Pollock, K. Ivarsen, L. Lim, M. Assafin, M. Baek, M. Mueller, R. Vieira Martins","submitted_at":"2016-04-19T00:02:15Z","abstract_excerpt":"Photometric lightcurves were also obtained for 14 of them during the Spitzer observations to provide the context of the observations and reliable estimates of their absolute magnitudes. The extracted mid-IR spectra were analyzed using a modified standard thermal model (STM) and a thermophysical model (TPM) that takes into account the shape and geometry of the large primary at the time of the Spitzer observation. We derived a reliable estimate of the size, albedo, and beaming factor for each of these asteroids, representing three main taxonomic groups: C, S, and X. For large (volume-equivalent "},"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":"1604.05384","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-04-19T00:02:15Z","cross_cats_sorted":[],"title_canon_sha256":"7d9cc1ec3d5cdba2e8b5d124edc934cca3e81c82bd699530dd0afc93eb724530","abstract_canon_sha256":"fef6c79d183c655746d5b89370e5d501550ae46b9187710d6a912c7c90807f9a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:54.081597Z","signature_b64":"JOT/zx3/KZCZeYU468YoreZ0h/5/zyW6pFa4219ARy4rjSh5OrG1hzwa9SOos7i+v/m+QRexe5F2AUza0o3fCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5e599208111c6241509dd33050b15cc4b04a6a7ecbc97cfa42a1bc513b9898e1","last_reissued_at":"2026-05-18T01:16:54.081020Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:54.081020Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. LaCluyz, D. P. Cruikshank, D. Reichart, F. Marchis, F. Vachier, J. Berthier, J.E. Enriquez, J. Haislip, J. P. Emery, J. Pollock, K. Ivarsen, L. Lim, M. Assafin, M. Baek, M. Mueller, R. Vieira Martins","submitted_at":"2016-04-19T00:02:15Z","abstract_excerpt":"Photometric lightcurves were also obtained for 14 of them during the Spitzer observations to provide the context of the observations and reliable estimates of their absolute magnitudes. The extracted mid-IR spectra were analyzed using a modified standard thermal model (STM) and a thermophysical model (TPM) that takes into account the shape and geometry of the large primary at the time of the Spitzer observation. We derived a reliable estimate of the size, albedo, and beaming factor for each of these asteroids, representing three main taxonomic groups: C, S, and X. For large (volume-equivalent "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.05384","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":"1604.05384","created_at":"2026-05-18T01:16:54.081116+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.05384v1","created_at":"2026-05-18T01:16:54.081116+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.05384","created_at":"2026-05-18T01:16:54.081116+00:00"},{"alias_kind":"pith_short_12","alias_value":"LZMZECARDRRE","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LZMZECARDRRECUE5","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LZMZECAR","created_at":"2026-05-18T12:30:29.479603+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22702","citing_title":"Follow the wobble: Statistical methods to detect astrometric binary asteroids in Gaia FPR","ref_index":77,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS","json":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS.json","graph_json":"https://pith.science/api/pith-number/LZMZECARDRRECUE52MYFBMK4YS/graph.json","events_json":"https://pith.science/api/pith-number/LZMZECARDRRECUE52MYFBMK4YS/events.json","paper":"https://pith.science/paper/LZMZECAR"},"agent_actions":{"view_html":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS","download_json":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS.json","view_paper":"https://pith.science/paper/LZMZECAR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.05384&json=true","fetch_graph":"https://pith.science/api/pith-number/LZMZECARDRRECUE52MYFBMK4YS/graph.json","fetch_events":"https://pith.science/api/pith-number/LZMZECARDRRECUE52MYFBMK4YS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS/action/storage_attestation","attest_author":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS/action/author_attestation","sign_citation":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS/action/citation_signature","submit_replication":"https://pith.science/pith/LZMZECARDRRECUE52MYFBMK4YS/action/replication_record"}},"created_at":"2026-05-18T01:16:54.081116+00:00","updated_at":"2026-05-18T01:16:54.081116+00:00"}