{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:P4N2IXAU44EJTNDYHGUCWSCQLL","short_pith_number":"pith:P4N2IXAU","schema_version":"1.0","canonical_sha256":"7f1ba45c14e70899b47839a82b48505ac0c6ff8726b08d68c86a17a52039562e","source":{"kind":"arxiv","id":"1310.4832","version":1},"attestation_state":"computed","paper":{"title":"The Andromeda Optical and Infrared Disk Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jean-Charles Cuillandre, Jonathan Sick, St\\'ephane Courteau","submitted_at":"2013-10-17T20:06:47Z","abstract_excerpt":"The Andromeda Optical and Infrared Disk Survey has mapped M31 in $u^* g^\\prime r^\\prime i^\\prime J K_s$ wavelengths out to R=40 kpc using the MegaCam and WIRCam wide-field cameras on the Canada-France-Hawaii Telescope. Our survey is uniquely designed to simultaneously resolve stars while also carefully reproducing the surface brightness of M31, allowing us to study M31's global structure in the context of both resolved stellar populations and spectral energy distributions. We use the Elixir-LSB method to calibrate the optical $u^* g^\\prime r^\\prime i^\\prime$ images by building real-time maps o"},"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":"1310.4832","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-17T20:06:47Z","cross_cats_sorted":[],"title_canon_sha256":"6dc09696e89515a64ae544242dbf8de9d7a7f95c93279d33cf796b4c3330bcb3","abstract_canon_sha256":"f78d69969b40bc539e59c2ca24d73924bbc9a845c4d542b4b1222ff4e8ba3ccc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:10:02.742245Z","signature_b64":"N2PXQ8yMla1rWM63N5Z7nRmh2Z1kTSqJrbY9a/HBQ49dLLexS3XCtVqRkEsVg9hdjKwJUeQa1wYktNvsef8+Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7f1ba45c14e70899b47839a82b48505ac0c6ff8726b08d68c86a17a52039562e","last_reissued_at":"2026-05-18T03:10:02.741678Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:10:02.741678Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Andromeda Optical and Infrared Disk Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Jean-Charles Cuillandre, Jonathan Sick, St\\'ephane Courteau","submitted_at":"2013-10-17T20:06:47Z","abstract_excerpt":"The Andromeda Optical and Infrared Disk Survey has mapped M31 in $u^* g^\\prime r^\\prime i^\\prime J K_s$ wavelengths out to R=40 kpc using the MegaCam and WIRCam wide-field cameras on the Canada-France-Hawaii Telescope. Our survey is uniquely designed to simultaneously resolve stars while also carefully reproducing the surface brightness of M31, allowing us to study M31's global structure in the context of both resolved stellar populations and spectral energy distributions. We use the Elixir-LSB method to calibrate the optical $u^* g^\\prime r^\\prime i^\\prime$ images by building real-time maps o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.4832","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":"1310.4832","created_at":"2026-05-18T03:10:02.741753+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.4832v1","created_at":"2026-05-18T03:10:02.741753+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.4832","created_at":"2026-05-18T03:10:02.741753+00:00"},{"alias_kind":"pith_short_12","alias_value":"P4N2IXAU44EJ","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"P4N2IXAU44EJTNDY","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"P4N2IXAU","created_at":"2026-05-18T12:27:54.935989+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/P4N2IXAU44EJTNDYHGUCWSCQLL","json":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL.json","graph_json":"https://pith.science/api/pith-number/P4N2IXAU44EJTNDYHGUCWSCQLL/graph.json","events_json":"https://pith.science/api/pith-number/P4N2IXAU44EJTNDYHGUCWSCQLL/events.json","paper":"https://pith.science/paper/P4N2IXAU"},"agent_actions":{"view_html":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL","download_json":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL.json","view_paper":"https://pith.science/paper/P4N2IXAU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.4832&json=true","fetch_graph":"https://pith.science/api/pith-number/P4N2IXAU44EJTNDYHGUCWSCQLL/graph.json","fetch_events":"https://pith.science/api/pith-number/P4N2IXAU44EJTNDYHGUCWSCQLL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL/action/storage_attestation","attest_author":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL/action/author_attestation","sign_citation":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL/action/citation_signature","submit_replication":"https://pith.science/pith/P4N2IXAU44EJTNDYHGUCWSCQLL/action/replication_record"}},"created_at":"2026-05-18T03:10:02.741753+00:00","updated_at":"2026-05-18T03:10:02.741753+00:00"}