{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:EDGTCBXH4AC6GOJ3HUVLYVX7MP","short_pith_number":"pith:EDGTCBXH","schema_version":"1.0","canonical_sha256":"20cd3106e7e005e3393b3d2abc56ff63f016ae908d3b1e33455b7c0a4b15ee81","source":{"kind":"arxiv","id":"2406.03532","version":2},"attestation_state":"computed","paper":{"title":"An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. II. JWST NIRCam Wide Filters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrew E. Dolphin, Evan D. Skillman, Kristen B. W. McQuinn, Martha L. Boyer, Max J. B. Newman, O. Grace Telford, Roger E. Cohen","submitted_at":"2024-06-05T18:00:01Z","abstract_excerpt":"The tip of the red giant (TRGB) is a standardizable candle and is identifiable as the discontinuity at the bright extreme of the red giant branch (RGB) stars in color-magnitude diagram (CMD) space. The TRGB-based distance method has been calibrated and used to measured distances to galaxies out to $D\\leq20$ Mpc with the $I$-band equivalent Hubble Space Telescope ($HST$) $F814W$ filter, and as an important rung in the distance ladder to measure the Hubble constant, $H_0$. In the infrared (IR), the TRGB apparent magnitude ranges from $1-2$ magnitudes brighter than in the optical, and now with th"},"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":"2406.03532","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-06-05T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"11c3687def40e2d39e9b685dd570feca185849a70606a0760d1212d54292dace","abstract_canon_sha256":"8b8eb7231225c8184f97887dff97db47f68328fdb1d51051c7c036eb55968f05"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:30:13.518452Z","signature_b64":"bqP2kTvFQcc04xQzXXCAiMxfhWdSgXOP/av8/RP1+/n4EuPnJq0u8vhENJw4QaQl9CJobfPhKrhbIuJnZh3mAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"20cd3106e7e005e3393b3d2abc56ff63f016ae908d3b1e33455b7c0a4b15ee81","last_reissued_at":"2026-07-05T08:30:13.517964Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:30:13.517964Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. II. JWST NIRCam Wide Filters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Andrew E. Dolphin, Evan D. Skillman, Kristen B. W. McQuinn, Martha L. Boyer, Max J. B. Newman, O. Grace Telford, Roger E. Cohen","submitted_at":"2024-06-05T18:00:01Z","abstract_excerpt":"The tip of the red giant (TRGB) is a standardizable candle and is identifiable as the discontinuity at the bright extreme of the red giant branch (RGB) stars in color-magnitude diagram (CMD) space. The TRGB-based distance method has been calibrated and used to measured distances to galaxies out to $D\\leq20$ Mpc with the $I$-band equivalent Hubble Space Telescope ($HST$) $F814W$ filter, and as an important rung in the distance ladder to measure the Hubble constant, $H_0$. In the infrared (IR), the TRGB apparent magnitude ranges from $1-2$ magnitudes brighter than in the optical, and now with th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.03532","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/2406.03532/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":"2406.03532","created_at":"2026-07-05T08:30:13.518018+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.03532v2","created_at":"2026-07-05T08:30:13.518018+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.03532","created_at":"2026-07-05T08:30:13.518018+00:00"},{"alias_kind":"pith_short_12","alias_value":"EDGTCBXH4AC6","created_at":"2026-07-05T08:30:13.518018+00:00"},{"alias_kind":"pith_short_16","alias_value":"EDGTCBXH4AC6GOJ3","created_at":"2026-07-05T08:30:13.518018+00:00"},{"alias_kind":"pith_short_8","alias_value":"EDGTCBXH","created_at":"2026-07-05T08:30:13.518018+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.04801","citing_title":"Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics","ref_index":163,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP","json":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP.json","graph_json":"https://pith.science/api/pith-number/EDGTCBXH4AC6GOJ3HUVLYVX7MP/graph.json","events_json":"https://pith.science/api/pith-number/EDGTCBXH4AC6GOJ3HUVLYVX7MP/events.json","paper":"https://pith.science/paper/EDGTCBXH"},"agent_actions":{"view_html":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP","download_json":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP.json","view_paper":"https://pith.science/paper/EDGTCBXH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.03532&json=true","fetch_graph":"https://pith.science/api/pith-number/EDGTCBXH4AC6GOJ3HUVLYVX7MP/graph.json","fetch_events":"https://pith.science/api/pith-number/EDGTCBXH4AC6GOJ3HUVLYVX7MP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP/action/storage_attestation","attest_author":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP/action/author_attestation","sign_citation":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP/action/citation_signature","submit_replication":"https://pith.science/pith/EDGTCBXH4AC6GOJ3HUVLYVX7MP/action/replication_record"}},"created_at":"2026-07-05T08:30:13.518018+00:00","updated_at":"2026-07-05T08:30:13.518018+00:00"}