{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XKHQHMSHFFAH352QUM3PYL6MCF","short_pith_number":"pith:XKHQHMSH","schema_version":"1.0","canonical_sha256":"ba8f03b24729407df750a336fc2fcc1155b2c2c90f8c4ef2c063efd81a87db4f","source":{"kind":"arxiv","id":"1402.0083","version":1},"attestation_state":"computed","paper":{"title":"Infrared extinction in the Inner Milky Way through the red clump giants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es Asensio Ramos, Antonio Cabrera-Lavers, Carlos Gonz\\'alez-Fern\\'andez, Francisco Garz\\'on, Peter L. Hammersley","submitted_at":"2014-02-01T12:50:10Z","abstract_excerpt":"While the shape of the extinction curve on the infrared is considered to be set and the extinction ratios between infrared bands are usually taken to be approximately constant, a recent number of studies point either to a spatially variable behavior on the exponent of the power law or to a different extinction law altogether. In this paper, we propose a method to analyze the overall behavior of the interstellar extinction by means of the red-clump population, and we apply it to those areas of the Milky Way where the presence of interstellar matter is heavily felt: areas located in 5 deg<l<30 d"},"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":"1402.0083","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-01T12:50:10Z","cross_cats_sorted":[],"title_canon_sha256":"93768922ed3314fd96b522514c4d9c2f509fd6d2e9cc533fb901715b808aee3e","abstract_canon_sha256":"e9ce2f49ce3e64d45648025c9c5af46e353e295a594c8011eb446a1ca679ef0f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:53.774065Z","signature_b64":"2CC64iN1uDmClDvO2rU+1k4HukPAT8meZUMZFaRgFlHt7vQDI632Y9/T34bIsnEUTuQhrV7rIbTNjjU0KCozAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ba8f03b24729407df750a336fc2fcc1155b2c2c90f8c4ef2c063efd81a87db4f","last_reissued_at":"2026-05-18T01:44:53.773586Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:53.773586Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Infrared extinction in the Inner Milky Way through the red clump giants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andr\\'es Asensio Ramos, Antonio Cabrera-Lavers, Carlos Gonz\\'alez-Fern\\'andez, Francisco Garz\\'on, Peter L. Hammersley","submitted_at":"2014-02-01T12:50:10Z","abstract_excerpt":"While the shape of the extinction curve on the infrared is considered to be set and the extinction ratios between infrared bands are usually taken to be approximately constant, a recent number of studies point either to a spatially variable behavior on the exponent of the power law or to a different extinction law altogether. In this paper, we propose a method to analyze the overall behavior of the interstellar extinction by means of the red-clump population, and we apply it to those areas of the Milky Way where the presence of interstellar matter is heavily felt: areas located in 5 deg<l<30 d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.0083","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":"1402.0083","created_at":"2026-05-18T01:44:53.773658+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.0083v1","created_at":"2026-05-18T01:44:53.773658+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.0083","created_at":"2026-05-18T01:44:53.773658+00:00"},{"alias_kind":"pith_short_12","alias_value":"XKHQHMSHFFAH","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XKHQHMSHFFAH352Q","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XKHQHMSH","created_at":"2026-05-18T12:28:57.508820+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/XKHQHMSHFFAH352QUM3PYL6MCF","json":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF.json","graph_json":"https://pith.science/api/pith-number/XKHQHMSHFFAH352QUM3PYL6MCF/graph.json","events_json":"https://pith.science/api/pith-number/XKHQHMSHFFAH352QUM3PYL6MCF/events.json","paper":"https://pith.science/paper/XKHQHMSH"},"agent_actions":{"view_html":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF","download_json":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF.json","view_paper":"https://pith.science/paper/XKHQHMSH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.0083&json=true","fetch_graph":"https://pith.science/api/pith-number/XKHQHMSHFFAH352QUM3PYL6MCF/graph.json","fetch_events":"https://pith.science/api/pith-number/XKHQHMSHFFAH352QUM3PYL6MCF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF/action/storage_attestation","attest_author":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF/action/author_attestation","sign_citation":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF/action/citation_signature","submit_replication":"https://pith.science/pith/XKHQHMSHFFAH352QUM3PYL6MCF/action/replication_record"}},"created_at":"2026-05-18T01:44:53.773658+00:00","updated_at":"2026-05-18T01:44:53.773658+00:00"}