{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:GIB7WOXV3G537XXOTHO7XRLKX6","short_pith_number":"pith:GIB7WOXV","schema_version":"1.0","canonical_sha256":"3203fb3af5d9bbbfdeee99ddfbc56abf923ff808b4096d08fe4bb124a0e9df30","source":{"kind":"arxiv","id":"1312.3424","version":1},"attestation_state":"computed","paper":{"title":"3D Galactic dust extinction mapping with multi-band photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. A. L. Bailer-Jones, R. J. Hanson","submitted_at":"2013-12-12T09:33:28Z","abstract_excerpt":"We present a method to simultaneously infer the interstellar extinction parameters $A_0$ and $R_0$, stellar effective temperature $T_{\\rm eff}$, and distance modulus $\\mu$ in a Bayesian framework. Using multi-band photometry from SDSS and UKIDSS, we train a forward model to emulate the colour-change due to physical properties of stars and the interstellar medium for temperatures from 4000 to 9000 K and extinctions from 0 to 5 mag. We introduce a Hertzsprung-Russel diagram prior to account for physical constraints on the distribution of stars in the temperature-absolute magnitude plane. This al"},"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":"1312.3424","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-12-12T09:33:28Z","cross_cats_sorted":[],"title_canon_sha256":"ecaf603f4e68f23202f0ca1574f5c92930db379f462620eddef1cee584099d31","abstract_canon_sha256":"dc5793c73438f13b61a10fed580be531b3f5a785c71b70add7ad7ebcd7c5b977"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:51.323744Z","signature_b64":"3oFMUt3NgORjJs2KmyLz1sxbpi6301xsHGEZY0qO7pnoqin1XAYXd/mt1+5K2Nc0kMwwUBsTcVJ/39xaTZ8JBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3203fb3af5d9bbbfdeee99ddfbc56abf923ff808b4096d08fe4bb124a0e9df30","last_reissued_at":"2026-05-18T01:45:51.323293Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:51.323293Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"3D Galactic dust extinction mapping with multi-band photometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. A. L. Bailer-Jones, R. J. Hanson","submitted_at":"2013-12-12T09:33:28Z","abstract_excerpt":"We present a method to simultaneously infer the interstellar extinction parameters $A_0$ and $R_0$, stellar effective temperature $T_{\\rm eff}$, and distance modulus $\\mu$ in a Bayesian framework. Using multi-band photometry from SDSS and UKIDSS, we train a forward model to emulate the colour-change due to physical properties of stars and the interstellar medium for temperatures from 4000 to 9000 K and extinctions from 0 to 5 mag. We introduce a Hertzsprung-Russel diagram prior to account for physical constraints on the distribution of stars in the temperature-absolute magnitude plane. This al"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.3424","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":"1312.3424","created_at":"2026-05-18T01:45:51.323378+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.3424v1","created_at":"2026-05-18T01:45:51.323378+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.3424","created_at":"2026-05-18T01:45:51.323378+00:00"},{"alias_kind":"pith_short_12","alias_value":"GIB7WOXV3G53","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_16","alias_value":"GIB7WOXV3G537XXO","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_8","alias_value":"GIB7WOXV","created_at":"2026-05-18T12:27:45.050594+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/GIB7WOXV3G537XXOTHO7XRLKX6","json":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6.json","graph_json":"https://pith.science/api/pith-number/GIB7WOXV3G537XXOTHO7XRLKX6/graph.json","events_json":"https://pith.science/api/pith-number/GIB7WOXV3G537XXOTHO7XRLKX6/events.json","paper":"https://pith.science/paper/GIB7WOXV"},"agent_actions":{"view_html":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6","download_json":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6.json","view_paper":"https://pith.science/paper/GIB7WOXV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.3424&json=true","fetch_graph":"https://pith.science/api/pith-number/GIB7WOXV3G537XXOTHO7XRLKX6/graph.json","fetch_events":"https://pith.science/api/pith-number/GIB7WOXV3G537XXOTHO7XRLKX6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6/action/storage_attestation","attest_author":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6/action/author_attestation","sign_citation":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6/action/citation_signature","submit_replication":"https://pith.science/pith/GIB7WOXV3G537XXOTHO7XRLKX6/action/replication_record"}},"created_at":"2026-05-18T01:45:51.323378+00:00","updated_at":"2026-05-18T01:45:51.323378+00:00"}