{"as_of":"2026-08-04T21:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:97c9f6b7f2182ecd7da31d9e6b0bc3b57ef762180da8abfd0970f67398a1ec46","coverage":[{"denominator":150,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-22T23:59:35.379178Z","state":"measured"},{"denominator":107,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":107,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T18:51:51.566041Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T12:15:01.137692Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-08-04T18:51:51.566041Z","title":"J., Jang I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.09665","last_updated":"2026-06-10T11:44:39Z","snapshot_observed_at":"2026-08-04T18:51:38.903465Z","submitted_at":"2025-09-11T17:57:56Z","title":"Two per cent measurement of $H_0$ from Cepheids alone","version":3},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-04T18:51:51.566041Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2509.09665"},"observation_digest":"sha256:1ba6bf78459639033367665941668d04014b91c835329ef1289855f94fb61269","observation_id":"af04e7be-5837-4c19-90b2-bc94f044e915","resolution":{"observed_at":"2026-08-04T18:51:51.566041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":"2503.11769","doi":"10.48550/arxiv.2503.11769","metadata_source":"pith","pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","venue":"astro-ph.GA","work_id":"087b4faa-e968-4462-a9f0-d360c559a108","year":2025},"citing_paper":{"arxiv_id":"2604.14145","last_updated":"2026-05-22T02:27:09Z","snapshot_observed_at":"2026-07-06T23:02:00.082783Z","submitted_at":"2026-04-15T17:59:19Z","title":"TDCOSMO XXV: A \"soup-to-nuts\" 6.5% $H_0$ measurement $-$ strong lensing and dynamics with a maximally flexible mass sheet","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-10T12:27:24.334046Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2604.14145"},"observation_digest":"sha256:2a7694942765f35bc132e40f0ffe6a2666e74f7e7acfa92617a8c9bc9d7a592f","observation_id":"757fb552-d931-4a1c-b5e1-1f99286c9aa0","resolution":{"observed_at":"2026-05-13T01:45:17.714796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":"2503.11769","doi":"10.48550/arxiv.2503.11769","metadata_source":"pith","pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","venue":"astro-ph.GA","work_id":"087b4faa-e968-4462-a9f0-d360c559a108","year":2025},"citing_paper":{"arxiv_id":"2604.14145","last_updated":"2026-05-22T02:27:09Z","snapshot_observed_at":"2026-07-06T23:02:00.082783Z","submitted_at":"2026-04-15T17:59:19Z","title":"TDCOSMO XXV: A \"soup-to-nuts\" 6.5% $H_0$ measurement $-$ strong lensing and dynamics with a maximally flexible mass sheet","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-25T06:56:40.117419Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2604.14145"},"observation_digest":"sha256:7d546e1b6d3a140a9edea0892ae518da51339d903212b1e5f7a99a63094cbbdf","observation_id":"d0dfca86-f53e-4977-b81f-0403ebbec129","resolution":{"observed_at":"2026-05-25T07:00:27.197198Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":"2503.11769","doi":"10.48550/arxiv.2503.11769","metadata_source":"pith","pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","venue":"astro-ph.GA","work_id":"087b4faa-e968-4462-a9f0-d360c559a108","year":2025},"citing_paper":{"arxiv_id":"2606.02499","last_updated":"2026-06-01T17:05:15Z","snapshot_observed_at":"2026-07-06T23:42:53.514946Z","submitted_at":"2026-06-01T17:05:15Z","title":"Evaluating Cepheid Metallicity Effect Determinations via IC1613 and Gaia-independent Parallaxes","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-28T12:28:47.378053Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2606.02499"},"observation_digest":"sha256:a48babc2b0a226988aabb7514265291c0f5c8c44eb5fa10b400162a2a9a8b8fb","observation_id":"4fb10d75-5ede-4b1b-9f9f-ddfe2b8e5dd4","resolution":{"observed_at":"2026-06-28T12:32:07.769919Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":"2503.11769","doi":"10.48550/arxiv.2503.11769","metadata_source":"pith","pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","venue":"astro-ph.GA","work_id":"087b4faa-e968-4462-a9f0-d360c559a108","year":2025},"citing_paper":{"arxiv_id":"2606.17136","last_updated":"2026-06-15T18:00:01Z","snapshot_observed_at":"2026-07-06T23:52:47.494791Z","submitted_at":"2026-06-15T18:00:01Z","title":"The Lazuli Space Observatory: Opportunities for time-domain and multi-messenger astronomy","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-06-27T02:54:09.792637Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2606.17136"},"observation_digest":"sha256:2623ee19866065ad02e4235a8c408c0e5132e9944ab317f7acdc66364e333430","observation_id":"dc258772-3a2f-40a9-8cd1-0308bfad1869","resolution":{"observed_at":"2026-06-27T03:00:24.320301Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-08-02T03:06:04.348765Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14007","last_updated":"2026-07-15T16:37:06Z","snapshot_observed_at":"2026-08-02T03:06:00.983798Z","submitted_at":"2026-07-15T16:37:06Z","title":"The potential broader complex linked to the key Cepheid SV Vul","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-02T03:06:04.348765Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2607.14007"},"observation_digest":"sha256:ef0e8104edf7db4ab785c85e347a2df36e2688b73b1dda947beb8e97b62fe446","observation_id":"7a00f393-859b-4c95-a789-97d87c3beded","resolution":{"observed_at":"2026-08-02T03:06:04.348765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.11769","snapshot_observed_at":"2026-08-03T11:58:34.602770Z","title":"The Chicago Carnegie Hubble Program: improving the calibration of Type Ia supernovae with JWST measurements of the tip of the red giant branch,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.29197","last_updated":"2026-07-31T09:16:30Z","snapshot_observed_at":"2026-08-04T21:14:09.145070Z","submitted_at":"2026-07-31T09:16:30Z","title":"A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T11:58:34.602770Z"},"links":{"cited_paper":"/paper/2503.11769","citing_paper":"/paper/2607.29197"},"observation_digest":"sha256:7aecc6c6bb50c2cfcebbb4245d10f338dc1d7065d7e967f46534600dc9e4024c","observation_id":"285ef10f-3295-4dab-b566-cc70a9e40385","resolution":{"observed_at":"2026-08-03T11:58:34.602770Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.11769/citation-record","integrity":"/paper/2503.11769/integrity","json":"/paper/2503.11769/citation-record.json","paper":"/paper/2503.11769"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.131.041002","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"collaboratiom, Physical Review Letters 131(4) (2023)","venue":null,"work_id":"8ae83475-bb4a-4513-bc1f-43a8f9add3ed","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:548db2bc937531fc062818f9c2fc3378f1d87f5421ec76224d813e1e82098bf9","observation_id":"bf20c0ee-2254-4ed4-8f1a-ab0c7b631613","resolution":{"observed_at":"2026-05-23T00:02:17.218734Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-07-11T04:03:02.952271+00:00","source":"paper_reference_links","state":"open"},"event_date":"2023-07-28","event_type":"correction","notice_doi":"10.1103/physrevlett.131.041002","provenance":{"observed_at":"2026-07-11T02:57:16.843555+00:00","source":"crossref","source_record_id":"10.1103/physrevlett.131.041002->10.1103/physrevlett.131.041002:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/308932","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2000, ApJ, 536, 438, doi: 10.1086/308932 53","venue":null,"work_id":"7c36b0cb-745d-423b-94db-4d298569c6f9","year":2000},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:aec907c236fea637c9be493298db607b6f4d408867bcf9084b3559267fbf27fd","observation_id":"2babdd50-35c7-453f-9ce9-ecdc26318f1e","resolution":{"observed_at":"2026-05-23T00:02:17.288658Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/674875","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-01T02:45:17.849982Z","title":"G., & van Dokkum, P","venue":null,"work_id":"5c2b4044-b545-49bb-8672-7bfeccec65db","year":2014},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:95ce70f47215e052cb1a1e770fc2bbd6166f8b02100ff89289899d41b3e5d555","observation_id":"c70cc39d-ce45-44d3-982d-c1913c040470","resolution":{"observed_at":"2026-05-23T00:02:17.419962Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1117/12.458107","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T07:34:42.927047Z","title":"2002, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol","venue":null,"work_id":"87700020-e924-4e82-b4c4-6fd9bb508e84","year":1995},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:1084c40bb8c8493e95ae256c3d9ef7f50086d43451ca496a1305fa66284a9c5a","observation_id":"79698dd5-4996-4cf0-8a97-78bab0c828a7","resolution":{"observed_at":"2026-05-23T00:02:16.808990Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-10T21:18:55.015589+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T21:18:55.015589+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac68df","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T20:27:21.577948Z","title":"S., Tully, R","venue":null,"work_id":"1a49fd5b-dade-46d8-a1e3-bfd52d7c5477","year":2022},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:8b7ecaffcd3fd734553bd46da9b57931b83e8220f32f8800e40b2059ac09958d","observation_id":"e45c8272-8461-4c24-863d-ccb16e93c300","resolution":{"observed_at":"2026-05-23T00:02:17.139505Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/ac0440","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T12:32:07.655917Z","title":"S., Rizzi, L., Tully, R","venue":null,"work_id":"b67a67f6-5408-4c0b-90dd-0ba6006eb6a0","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:02ac9d1d1bc7952e9b1718db31609e00ee3b1a764b14f60a9baa8ca7eb3067c1","observation_id":"ce0e8242-5317-42ac-bb2a-37274c3e2716","resolution":{"observed_at":"2026-05-23T00:02:17.322718Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04776","last_updated":"2024-04-26T14:38:27Z","snapshot_observed_at":"2026-08-01T20:30:14.966409Z","submitted_at":"2024-01-09T19:05:00Z","title":"Tip of the Red Giant Branch Distances with JWST: An Absolute Calibration in NGC 4258 and First Applications to Type Ia Supernova Hosts","version":2},"cited_work":{"arxiv_id":"2401.04776","doi":"10.48550/arxiv.2401.04776","metadata_source":"arxiv_reference","pith_arxiv_id":"2401.04776","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"S., Riess, A","venue":null,"work_id":"a486b25b-5d86-4413-8b3e-3bd224055237","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/2401.04776","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:fde360b4e264a89b3c552aa244a656b574cfdb0f9cee67d3e213037750c08e97","observation_id":"890983f1-b9fd-4367-836b-03ac070de5c8","resolution":{"observed_at":"2026-05-23T00:02:17.193312Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad64c7","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T06:10:36.395623Z","title":"S., Tully, R","venue":null,"work_id":"819cac16-8c6d-4f08-bcf1-f5cd28cf18ef","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:e404edc78422d166a03c1b0049eb1c0cf645d98bfd35a0e6dd76b78b85976ecc","observation_id":"3e98994c-0ed1-414c-b937-f43f122ffb8f","resolution":{"observed_at":"2026-05-23T00:02:17.157458Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2016,, Astrophysics Source Code Library, record ascl:1611.017","venue":null,"work_id":"2298d4a3-22b4-49e7-a4fb-a8d150f334b8","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:f9e0fcb6cf926c8d9b74f33bc2709bb40cfbe841f570a67bb08b2bf55b6ccce3","observation_id":"ff556680-84c3-48bd-98e0-369a2298ff6f","resolution":{"observed_at":"2026-05-23T00:05:14.720446Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/0004-637x/832/2/210","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:44:16.646462Z","title":"L., Freedman, W","venue":null,"work_id":"b02f3052-11f9-4fb8-911a-95c033d9e099","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:0469d7c963fded2bdc5ab9cbfdc2c55b10b314f0bdf7c0a46ed5fe320a11252e","observation_id":"1512b3f3-1d4f-42db-9af0-110733656de8","resolution":{"observed_at":"2026-05-23T00:02:16.951039Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab4263","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T05:31:40.846955Z","title":"L., Seibert, M., Hatt, D., et al","venue":null,"work_id":"e69a1dff-9975-4b75-9038-e8b75a638b4e","year":2019},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d1bcc9c437781f0e46f1aed3d359121ce08ad7273fc16062368f12bf0e2201ca","observation_id":"aa54899f-7272-481a-8406-5a71c2275ba4","resolution":{"observed_at":"2026-05-23T00:02:17.281257Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2016","last_updated":"2007-11-13T16:02:35Z","snapshot_observed_at":"2026-07-06T01:35:43.677855Z","submitted_at":"2007-11-13T16:02:35Z","title":"The Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":"0711.2016","doi":"10.48550/arxiv.0711.2016","metadata_source":"pith","pith_arxiv_id":"0711.2016","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"The Tip of the Red Giant Branch","venue":"astro-ph","work_id":"e2664abe-e323-45b5-8dc2-817f4b43a1af","year":2007},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/0711.2016","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9b74ba89bc459a1bf9b00df6731e598b309f6dae7ce5ab5e76f99d0c48d4c274","observation_id":"6bf75d65-d41e-4db3-85d8-5fa7f0b7da10","resolution":{"observed_at":"2026-05-23T00:02:17.099289Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20035910","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2004, A&A, 424, 199, doi: 10.1051/0004-6361:20035910","venue":null,"work_id":"31c5ab7a-30b8-4a6f-8074-b14be1983f7c","year":2004},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:c61c376266c70e555391934116f8df7e9ff31c5acf18c98312d9bf0ff3908da7","observation_id":"5cb42ce8-a62f-4cbd-a7ec-a8e4b0f82648","resolution":{"observed_at":"2026-05-23T00:02:17.051298Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04781","last_updated":"2024-08-19T12:13:18Z","snapshot_observed_at":"2026-07-06T18:27:03.044022Z","submitted_at":"2024-06-07T09:28:58Z","title":"The red giant branch tip in the SDSS, PS1, JWST, NGRST and Euclid photometric systems. Calibration in optical passbands using Gaia DR3 synthetic photometry","version":3},"cited_work":{"arxiv_id":"2406.04781","doi":"10.48550/arxiv.2406.04781","metadata_source":"arxiv_reference","pith_arxiv_id":"2406.04781","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"2024, arXiv e-prints, arXiv:2406.04781, doi: 10.48550/arXiv.2406.04781","venue":null,"work_id":"35536cd1-04b2-4364-979b-e4daa65ade42","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/2406.04781","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:042332d2d7ccd1a87569e0ce36a7da2238b43b6a4a6e99c73d59250dcdba5d02","observation_id":"28fcb4c4-b677-4ef7-b9c2-fa8eeb41a540","resolution":{"observed_at":"2026-05-23T00:02:17.170721Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201423413","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T06:26:43.113566Z","title":"2014, A&A, 568, A22, doi: 10.1051/0004-6361/201423413","venue":null,"work_id":"58386256-2707-4c5c-82c1-303755f61ebf","year":2014},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:776c46b447153cf3e19aab84ee0a28e3b6f1cc3bc5f3fc46a306d242c9e32bff","observation_id":"4d2a8fec-b20c-4856-8c7f-9370f6600f67","resolution":{"observed_at":"2026-05-23T00:02:17.306045Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:19.764757+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:19.764757+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abec3b","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T07:34:42.993952Z","title":"2021a, ApJ, 912, 71, doi: 10.3847/1538-4357/abec3b","venue":null,"work_id":"75c274ba-a786-4e9b-9623-2560349b97bc","year":2025},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:62e81b5cb2adf283ba3f5f4be538e1b1f1994d2312dea0e788e174b2242405cb","observation_id":"abe97409-22a1-4ce2-a790-3febc3e120dd","resolution":{"observed_at":"2026-05-23T00:02:17.398513Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-10T21:18:56.485626+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T21:18:56.485626+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abec3c","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T03:00:24.455551Z","title":"2021b, ApJ, 912, 70, doi: 10.3847/1538-4357/abec3c","venue":null,"work_id":"7001deb1-eabb-4700-88c8-1aa2f8e069a1","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9acfa039ed7e3a994b73dbe8553cf7a8b4fb808a0c9d60c1c5bf9cc27bbd2c23","observation_id":"07d1d46d-5de4-4a85-bcb2-e47ba98a269a","resolution":{"observed_at":"2026-05-23T00:02:17.417370Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-6256/141/1/19","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T03:10:24.808572Z","title":"R., Stritzinger, M., Phillips, M","venue":null,"work_id":"88e50682-5393-4140-91a5-48b472f1297e","year":2011},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:ddcee88eae55002fb6205f648d7e1dfcdab4407727283f46f4410f1448281e32","observation_id":"e626f5de-6530-4e4e-a85b-f1c3e3fa077e","resolution":{"observed_at":"2026-05-23T00:02:17.430930Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T14:19:32.643963+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T14:19:32.643963+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aae51c","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T06:10:36.308124Z","title":"R., Parent, E., Phillips, M","venue":null,"work_id":"5098d84f-c1b1-4166-8fac-f162e855b278","year":2018},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:c7bb0ba4eceae0c312cd114a41c3a36c1389d716eb5440775eefdc9b94181469","observation_id":"62b51766-ab2e-422b-bb1e-0b7558efd782","resolution":{"observed_at":"2026-05-23T00:02:17.069857Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T14:19:32.006815+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T14:19:32.006815+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"record/7038885","doi":"10.5281/zenodo.7038885","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"2023,, 1.9.6 doi: 10.5281/zenodo.7038885","venue":"Zenodo (CERN European Organization for Nuclear Research)","work_id":"11541b74-9f28-40fe-ad3e-5f5c2354f60e","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:2e669115cabef4ae28e4f725a814a03699f0d5ef6815d9c03ad3b29c807155e3","observation_id":"2889eda9-3b28-4b58-8386-79c8de433c2a","resolution":{"observed_at":"2026-05-23T00:02:17.206567Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-05-24T18:53:17.168958+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T18:53:17.168958+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/320383","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T08:01:46.763231Z","title":"year =","venue":null,"work_id":"864692cb-9ef1-48ce-afaa-a6e835c5b345","year":2001},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:43d7ebe2bf9f5d5fe36643a4b72b0e9ff89db9faf77e8af75234695d46271a5e","observation_id":"f968bec3-e4fd-47f0-b18c-5ea040c94109","resolution":{"observed_at":"2026-05-23T00:02:17.215811Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405087","last_updated":"2004-05-05T15:30:48Z","snapshot_observed_at":"2026-07-07T00:42:19.442022Z","submitted_at":"2004-05-05T15:30:48Z","title":"New Grids of ATLAS9 Model Atmospheres","version":1},"cited_work":{"arxiv_id":"astro-ph/0405087","doi":"10.48550/arxiv.astro-ph/0405087","metadata_source":"pith","pith_arxiv_id":"astro-ph/0405087","snapshot_observed_at":"2026-07-10T12:15:01.137692Z","title":"New Grids of ATLAS9 Model Atmospheres","venue":"astro-ph","work_id":"2d638a18-3a56-4884-b37a-036d42f2d39d","year":2004},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/astro-ph/0405087","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:0f5df9f6c777e8043f175b8df7b4c0fa85217836acc7b1772438dee57f8c485a","observation_id":"0d114704-01ee-4acf-8574-2eb36752ce7f","resolution":{"observed_at":"2026-05-23T00:02:17.135478Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-20T19:23:13.905165+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T19:23:13.905165+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/ab089d","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T19:27:32.160745Z","title":"J., Lang, D., et al","venue":"The Astronomical Journal","work_id":"41713e96-11a3-4f0a-9889-2c89056b9c78","year":2019},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:63720ed4be712d180a3183bedcd73cabfa90d54afc5780a0a1b7b64612490c54","observation_id":"c9d979be-5657-4ca8-8562-d52f22529045","resolution":{"observed_at":"2026-05-23T00:02:17.112433Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:08:41.270308+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:08:41.270308+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2016,, Astrophysics Source Code Library, record ascl:1608.013","venue":null,"work_id":"ece89be3-9014-4d5c-9607-16ddc1987560","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:934571e05818c3d102006c919ebd0d7e4df1b775fe97535f0ec4b63da6f55da1","observation_id":"8604ad1a-02e2-4f4a-ae16-3632e233a9ca","resolution":{"observed_at":"2026-05-23T00:05:14.717139Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/316630","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2016, Astrophysics Source Code Library","venue":"Publications of the Astronomical Society of the Pacific","work_id":"79b7277f-afc2-4d2a-b810-237c5751ae13","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:e4460b4c9b492e65570b01509245d1215c58eee904509577f530072ef5c21323","observation_id":"e120f7a5-ec54-4baa-91ff-0e32a0d28139","resolution":{"observed_at":"2026-05-23T00:02:16.994333Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-05-24T01:23:06.722212+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T01:23:06.722212+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab9cbb","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Beaton, R","venue":null,"work_id":"b95cf479-16b6-4d9f-b70f-eb0a65edb7e9","year":2020},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:85700825ec6e785c82a23849894d4c51a34772c7f858d4455fc3145ebe7c66ed","observation_id":"39176ef9-599e-4d7d-96f3-e9c196752d89","resolution":{"observed_at":"2026-05-23T00:02:17.093717Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/815/1/58","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:44:16.537817Z","title":"K., Boone, K., Aldering, G., et al","venue":null,"work_id":"9082466c-0f38-48af-9559-bbb71fd440d2","year":2015},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d48a3271c8543486717ab896f6aec74d2ceb9310c8f5bd4bd376fbf6f6d71471","observation_id":"9b455767-9fc0-4097-ba7e-0cf91ba41eb1","resolution":{"observed_at":"2026-05-23T00:02:16.802006Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stz3324","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Hoffmann, S","venue":null,"work_id":"92ea4dd9-ea20-4b63-8ee0-a8f88b6a6376","year":2020},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:5018380a43dc1ebca2c504d14251e95be1c5faeb0d61c8803591bca065c79778","observation_id":"9d4f6b97-4bdd-47e7-b441-df3f14813a36","resolution":{"observed_at":"2026-05-23T00:02:17.150876Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.21105/joss.00024","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T17:27:26.091123Z","title":"2016, The Journal of Open Source Software, 1, 24, doi: 10.21105/joss.00024","venue":"The Journal of Open Source Software","work_id":"f50776a9-00f0-49ad-a14d-ff9403d02d22","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:426cd725f578e1fbb025755443c47e895594c05b90639ded03abca98f7d52d66","observation_id":"fb19a84c-fa3d-44c2-9df3-ed7beb814b55","resolution":{"observed_at":"2026-05-23T00:02:17.310693Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:06.845354+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:06.845354+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/670067","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T01:57:46.492432Z","title":"W., Lang D., Goodman J., 2013, @doi [ ] 10.1086/670067 , http://adsabs.harvard.edu/abs/2013PASP..125..306F 125, 306","venue":"Publications of the Astronomical Society of the Pacific","work_id":"ba3f8533-f196-48e4-8e7b-fa5b168b7626","year":2013},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:5045d1d9ee0d2a6af476ccad9ab2e84ce50b552e190f6cab1f225454e4c4f8e3","observation_id":"b8711f57-662f-4fe5-9e26-ed8608df1c0c","resolution":{"observed_at":"2026-05-23T00:02:17.079245Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-01T04:38:19.479419+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-01T04:38:19.479419+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/166128","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-26T16:49:36.548665Z","title":null,"venue":null,"work_id":"ca20f6c2-0d9f-4e02-9418-e7a2bba60827","year":1988},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:99c83a83ad4efd1ea9c3b661af4d1ca0c878f33d87072264275a63ed2c36d1fc","observation_id":"07d84461-2733-4dbf-9b23-83a34c431791","resolution":{"observed_at":"2026-05-23T00:02:16.877579Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/115216","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"edf8181f-b863-4e5d-aa82-50024d994fb8","year":1989},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:fe823ce31fc4c1147efa7afed32733c9a84efdb85ebadf595392518b5f17e404","observation_id":"ca5a4135-ad4d-40de-9193-b603b9c4074d","resolution":{"observed_at":"2026-05-23T00:02:16.964417Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac0e95","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T06:56:43.617035Z","title":"keywords =","venue":null,"work_id":"41150e39-6228-49f6-bf42-957238d864dc","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:e901cd0180d1668da7b8155e7521f29735fcc4a68a3328b8c67e2661456ee2b0","observation_id":"ad10101d-6207-477c-ae56-896cf38063cb","resolution":{"observed_at":"2026-05-23T00:02:17.265410Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1146/annurev-astro-082708-101829","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T20:57:22.631432Z","title":"L., & Madore, B","venue":null,"work_id":"332acc62-b176-48ea-9024-9058f91ab656","year":2010},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:2437a6d2c7572df00a530825eaa40b31696631582b17764a12578184ff9b4832","observation_id":"7ea981dc-1fb2-4bcf-a5b8-b2f36f55e416","resolution":{"observed_at":"2026-05-23T00:02:16.938209Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2023/11/050","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"L., & Madore, B","venue":null,"work_id":"fa927195-08ca-4f88-a8ff-a89d5c812bf7","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:98c94e5a92d81cd470167d3a3ddf1fb7decde275c3c7f0fb9d4165ee2e59de82","observation_id":"f1d5439b-5ea2-4701-836c-0299fd2245ca","resolution":{"observed_at":"2026-05-23T00:02:17.302386Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.06153","last_updated":"2025-03-17T18:25:04Z","snapshot_observed_at":"2026-07-06T18:59:38.952273Z","submitted_at":"2024-08-12T13:48:33Z","title":"Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes","version":3},"cited_work":{"arxiv_id":"2408.06153","doi":"10.48550/arxiv.2408.06153","metadata_source":"arxiv_reference","pith_arxiv_id":"2408.06153","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"L., Madore, B","venue":null,"work_id":"c50ef59a-d8fa-44f3-834c-948c4da28d62","year":2025},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/2408.06153","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9c13398e3e059ab0a8beb06c02bd6404b6ff0499f7bd4021dd67c39fd183008a","observation_id":"2b5c3e12-2630-4dc8-a7b6-4cfdf69c6f2a","resolution":{"observed_at":"2026-05-23T00:02:17.294486Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/586701","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"L., Madore, B","venue":null,"work_id":"de75b628-f068-4a37-8a0a-9051c2ce9f33","year":2008},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:7fd901636f6db5a35e7f99c97066b295858efd765ef1bd0453c630e5976a6c57","observation_id":"eba5c5ce-03a4-4053-9375-2ba0dca1cf77","resolution":{"observed_at":"2026-05-23T00:02:17.262110Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/758/1/24","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:44:16.730673Z","title":"L., Madore, B","venue":null,"work_id":"8a2e84e4-11e9-4fcb-b9f2-156f09cd16c0","year":2012},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:6c891a5b3580f5c2c2ddbecd3f5b9a13e0e1237677cf2990f11d704cac4fd8ff","observation_id":"eca93328-75b1-4c46-8985-353ee9b89d87","resolution":{"observed_at":"2026-05-23T00:02:17.272710Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/371757a0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-26T17:59:41.484280Z","title":"L., Madore, B","venue":null,"work_id":"8d928c55-8814-4497-b643-6b16ca3d85f0","year":1994},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:74639358ff6ba4cdc1daaf70ec6ac248a493d7c1bd82c95486b117db275e61b9","observation_id":"11fac7ae-a513-41bc-9a83-9acea71773ed","resolution":{"observed_at":"2026-05-23T00:02:17.054654Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/320638","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T20:57:22.652090Z","title":"L., et al., 2001, @doi [ ] 10.1086/320638 , 553, 47","venue":null,"work_id":"eb64f134-0d93-46f8-98b4-3977b7f36b74","year":2001},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:307c1edef92b56a5f14b95b6498d9f80a7d5ee37d6ebe401caf2809f2371858a","observation_id":"1d77ed86-38fa-45bc-b3f6-a35b94d66820","resolution":{"observed_at":"2026-05-23T00:02:17.090201Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab2f73","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:44:16.728932Z","title":"L., Madore, B","venue":null,"work_id":"980dc601-c08b-46a7-be4a-d0bb75a30199","year":1907},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:c741c88417a635481a23775623503568cb7a2bd46eaafd5577acf70fb8a96998","observation_id":"95f524ec-3d64-4eec-a8a2-23be929b9063","resolution":{"observed_at":"2026-05-23T00:02:17.355395Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab7339","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:44:16.748400Z","title":"L., Madore, B","venue":null,"work_id":"ffad4f63-4ef6-4bf6-825d-650275ac20f8","year":2002},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:1c057d7ba5c38dea1f6d77a1b6e76b9b902f45aa3d083f4fcc1928a964567635","observation_id":"8e901e87-b563-48d9-bdea-92be3721e07d","resolution":{"observed_at":"2026-05-23T00:02:17.126025Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/161573","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"A., Cohen, J","venue":null,"work_id":"abf45b8c-fd61-40a7-b1e2-846de09bb3a8","year":1983},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:ae20bb355c94b46d3f2e97fc023acdae0d62334ea96cc039ec4ad10b8606a7b7","observation_id":"db20d351-42b1-4230-bffc-44db955bf971","resolution":{"observed_at":"2026-05-23T00:02:17.057637Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:50:59.136643+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T06:50:59.136643+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-94-009-8492-9","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"A., Persson, S","venue":null,"work_id":"d61eb465-f221-4968-84eb-b27fa7a76a64","year":1981},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:a17358c99b9e75ee3ebfa53164787370640ddcab4a8fec622c46b306f8171c1c","observation_id":"749fd3df-e5b1-4873-a967-60be62cab094","resolution":{"observed_at":"2026-05-23T00:02:17.367017Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20066930","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T18:07:15.986954Z","title":"2007, A&A, 466, 11, doi: 10.1051/0004-6361:20066930","venue":null,"work_id":"fd32d4d1-9a04-4d15-87be-f1f70ed4a1c5","year":2007},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:a6463ce0827891c053531c716691742f9b71eb29bdcf1887154fdaad51f4fe9a","observation_id":"f9e3146a-0413-4e70-98bc-932de4eb360b","resolution":{"observed_at":"2026-05-23T00:02:17.245511Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T12:49:59.291289+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T12:49:59.291289+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/118193","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"M., Suntzeff, N","venue":null,"work_id":"dc7e633f-f343-4ec8-8c9f-879a793a18f6","year":1996},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:914475ce54af22d67edffc5e4b2985dc1a386a1305bc70c19beebf36e7ddc57a","observation_id":"534485b7-1dee-4be5-8c5f-4d101be95be2","resolution":{"observed_at":"2026-05-23T00:02:17.373645Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/301527","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T03:00:24.549949Z","title":"C., Pinto, P","venue":null,"work_id":"5c819183-78e3-4c34-b34f-f75f7014af26","year":2000},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:82fc6f2605c9e3bc1b3bbec0d06f16a28592b5db6498baf58d23b1ad49dc0367","observation_id":"e2b0ac76-7f6b-4917-a3a0-49bbb3826487","resolution":{"observed_at":"2026-05-23T00:02:17.002070Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/500228","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T04:54:15.942182Z","title":"I., et al","venue":null,"work_id":"22d73f30-5f64-41e0-a5a4-648a6e6d4d42","year":2006},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9c0c147fcd75467780781a0b09bad1d0ec417309e2550aaf8b577876601d79c0","observation_id":"8f6b35a2-e218-4482-a85e-376d91a1a6ad","resolution":{"observed_at":"2026-05-23T00:02:17.231656Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T14:19:39.427326+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T14:19:39.427326+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/22972","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"R., Moran, J","venue":null,"work_id":"52784ba3-6e0b-43d1-aaff-575f84c1591d","year":1999},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:bd3ea3b4b6730a48d9c0c4df076a1e67665c9838dece77bbd093317d75b9d689","observation_id":"1841182f-4d0c-4742-b465-2cdb562dfc31","resolution":{"observed_at":"2026-05-23T00:02:17.389389Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/700/1/331","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T04:21:38.915808Z","title":"2009, ApJ, 700, 331, doi: 10.1088/0004-637X/700/1/331","venue":null,"work_id":"f29bfbed-27c2-4fdc-ad15-cfdb9e12da53","year":2009},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:f1188039a336288e1d87eadecbf2ae6ad9bfb4dff4d8c40d200844cbbee1589a","observation_id":"af2ef602-b027-4cb7-9baf-abea7c73fa44","resolution":{"observed_at":"2026-05-23T00:02:16.979744Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T14:19:39.739049+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T14:19:39.739049+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aab158","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T00:20:16.412807Z","title":"L., Pietrinferni, A., Cassisi, S., et al","venue":null,"work_id":"d07312d3-696e-45de-b1eb-17d8ef4d4591","year":2018},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:50c87b9093aa3d8183b67941b304d9797bfe1051da243e3fe0c92944d415a8b4","observation_id":"38f92888-cec7-4a6d-9f8f-e01e13310cf2","resolution":{"observed_at":"2026-05-23T00:02:17.359688Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-18T10:21:12.193457+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-18T10:21:12.193457+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/0004-637x/830/1/10","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T12:32:07.772732Z","title":"L., Macri, L","venue":null,"work_id":"98db1c76-f46f-4b37-bd6b-bac67ccb7d60","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:bb9f3789cd3aa876a7d70ef5ad4b7c16b4eae108b25aa548ef84380622cf3fe0","observation_id":"da723a4f-c8ec-450c-bba1-dab4aff98b23","resolution":{"observed_at":"2026-05-23T00:02:17.106940Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"L., Beaton, R","venue":null,"work_id":"45eb4295-e4b7-4148-bb34-e56541219051","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:e274d5df1a610c8faaa984b3ee7d9bccad8239f9b600467bda9801272fa96b1d","observation_id":"b725d9f5-2a43-49c9-b8d9-680e59f89f70","resolution":{"observed_at":"2026-05-23T00:05:14.713721Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/s41550-023-01913-1","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5ddefab5-b58e-4c4a-8fa7-1f6e4d60fe18","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:c4634dba33d08257ecbdfe07bcae65fa35fac23b45548c02c62a329264fbb57f","observation_id":"3834b367-d35e-470c-88b1-fa7331a17064","resolution":{"observed_at":"2026-05-23T00:02:17.044998Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07309","last_updated":"2024-07-10T02:09:37Z","snapshot_observed_at":"2026-08-04T06:41:48.614004Z","submitted_at":"2024-07-10T02:09:37Z","title":"Coordinated JWST Imaging of Three Distance Indicators in a SN Host Galaxy and an Estimate of the TRGB Color Dependence","version":1},"cited_work":{"arxiv_id":"2407.07309","doi":"10.48550/arxiv.2407.07309","metadata_source":"arxiv_reference","pith_arxiv_id":"2407.07309","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"J., Jang, I","venue":null,"work_id":"0b75a800-0785-4b98-a0bb-a029e143fb08","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"cited_paper":"/paper/2407.07309","citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:900592ee0532b37b8bfcdad1f282e49454a1f7a6f1744aad92000f7b99fd8300","observation_id":"e368f34e-c1d6-4da3-a310-98dd3dac8b28","resolution":{"observed_at":"2026-05-23T00:02:17.144266Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aab7ed","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Freedman, W","venue":null,"work_id":"c9d18d47-e42e-42de-b843-176bec03085d","year":2018},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:48dc27acfe8811fd6111bc33ef24d5a85645a276cd9526ff88c78b29340e412d","observation_id":"759a516e-2017-498a-bd05-e96477f78821","resolution":{"observed_at":"2026-05-23T00:02:16.825390Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abfe5a","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"J., Beaton, R","venue":null,"work_id":"9a9944cd-6bc7-4c68-aeb3-78f1417958d3","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:1205a6f8fa1b3514fb90c3b7a7e5d4a8e08d38b0b9303dea17a63e2ccd8a6ed0","observation_id":"6a84a7fd-66e2-474f-97ee-40a191d146eb","resolution":{"observed_at":"2026-05-23T00:02:16.814220Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1073/pnas.15.3.168","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T05:46:50.134361Z","title":"1929, Proceedings of the National Academy of Science, 15, 168, doi: 10.1073/pnas.15.3.168","venue":null,"work_id":"aac71667-1f47-4639-9660-b08bbb6f2678","year":1929},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:fba17f17bc4afb67d2e99d73ef46ccb575a61e99100253cb6f34a6ec13b17589","observation_id":"74174843-3e19-47d9-b57c-7798b9571bb8","resolution":{"observed_at":"2026-05-23T00:02:17.179934Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-12T23:50:55.994882+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T23:50:55.994882+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/523637","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"211eadb6-acac-43b1-a56e-59f6384eeb6e","year":2008},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:68da580de1a91a62f9e2e0848442eacd7c2186ddbdd4454b498693c4e5dba29d","observation_id":"bf4ada7d-e477-4381-ab88-63b5b8108cfe","resolution":{"observed_at":"2026-05-23T00:02:16.976232Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/775/1/13","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"c1caaae5-6c89-448e-b729-13284b735ae2","year":2013},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b312a54c5de011d26ec371a9966d353f4ac353432c5f9769371677be82f292b8","observation_id":"17800026-e69e-4d02-bcec-d5aa23152378","resolution":{"observed_at":"2026-05-23T00:02:16.983036Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-6256/138/2/332","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-25T21:48:32.711855Z","title":"A., Rizzi, L., Tully, R","venue":null,"work_id":"7235536f-1417-4b5c-b6b7-b7068910efae","year":2009},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:a128e1103304a2955dc9a8550049a3ae67908142b98811b381af61afe72a727f","observation_id":"3a5225d4-3b31-4def-b379-dab61968ca86","resolution":{"observed_at":"2026-05-23T00:02:16.869726Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201936994","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"S., de Jong, R","venue":null,"work_id":"df4908f6-8444-4af5-8157-528a466a2f54","year":2020},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:34570cce009ec947effbb04194a198cb49b56a3ff6410a0b3af9631f5fb20821","observation_id":"4b4ebf9a-c0af-4946-9da0-efd95e361393","resolution":{"observed_at":"2026-05-23T00:02:17.318472Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/807/2/133","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"S., & Lee, M","venue":null,"work_id":"482213fb-dda6-40df-b8a5-69a74e775eef","year":2015},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:56f898a04039c44afc77df932be76a8e5d1455b0eda1149fe6cb644c8ba72dee","observation_id":"3f3b6cf6-7d90-4762-92cb-31a22bf796e7","resolution":{"observed_at":"2026-05-23T00:02:16.972433Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/836/1/74","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T05:31:40.802895Z","title":"S., & Lee, M","venue":null,"work_id":"6de90a1b-3b0d-4d87-bb74-7b1c07a86547","year":2017},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:a0e5fbf4be9ac9f4937f5919b51a8d0b2b92199816baf61e7e160e3861e430e1","observation_id":"f789cdb8-48b4-432a-942a-bb59127eb243","resolution":{"observed_at":"2026-05-23T00:02:17.030660Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/835/1/28","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"S., & Lee, M","venue":null,"work_id":"ef186edc-723c-40d3-a84b-2c72f1f7acba","year":null},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:7f1d3d61042ede05a78ef98a632794b267eabd64955281b2a47146045e459241","observation_id":"61b019a8-9537-48d2-a0eb-d7d004c1e5be","resolution":{"observed_at":"2026-05-23T00:02:17.009620Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abc8e9","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"S., Hoyt, T","venue":null,"work_id":"c986553f-7b30-4cd7-9416-29882d06f7c2","year":2021},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:3024ca7845875bfb2a75019376bc96f6d47362c6839fe484106cadf144463366","observation_id":"5e40ec43-c76e-4c0a-b794-087f1b05b588","resolution":{"observed_at":"2026-05-23T00:02:17.298236Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/497989","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"P., Challis, P., et al","venue":null,"work_id":"52037c2c-c815-4200-a9b4-64f282c7cfa7","year":2006},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:dcf99c5c7975893fa215dca7ef85790b78b4476d4c05c2f231f17000964f48cc","observation_id":"23e9a8d0-d43d-4497-8238-3e6b0daa2f51","resolution":{"observed_at":"2026-05-23T00:02:17.060600Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:15.373667+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:15.373667+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/500013","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T01:11:28.768105Z","title":"D., Dolphin, A., Tully, R","venue":null,"work_id":"a152939e-3f67-4058-b41e-550bea28ca64","year":2006},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b51638639f51d80654970528e11291946164b0a37b0532160df3f6429693dba4","observation_id":"4ef1c75a-bf34-431f-be75-d52e16d953b1","resolution":{"observed_at":"2026-05-23T00:02:17.249294Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"1990, Stellar Structure and Evolution","venue":null,"work_id":"d01b900e-1f80-4a9a-b9ed-bd1ba3e05516","year":1990},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:3f098c874b4a19f314815ffad6055d96b6743a46a37e5dacb9adc58541bd28f7","observation_id":"886c37b5-85a7-430d-b661-631455e0e378","resolution":{"observed_at":"2026-05-23T00:05:14.710452Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"record/1493272","doi":"10.1007/978-3-642-30304-3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"2013, Stellar Structure and Evolution, doi: 10.1007/978-3-642-30304-3","venue":"Astronomy and Astrophysics Library","work_id":"c8b38109-f594-4c23-bcf9-170004ed1835","year":2012},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:dd089159611a39ffab7004708dde7fa89384bd31b20ff08e8310093eec5f1ddf","observation_id":"45e55e9e-c72f-45bc-86bc-76fb3e866802","resolution":{"observed_at":"2026-05-23T00:02:16.931934Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T13:19:23.610439+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:19:23.610439+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T21:37:43.212331Z","title":"2016, in Positioning and Power in Academic Publishing: Players, Agents and Agendas, ed","venue":null,"work_id":"d3096eaa-4bd5-42fb-8865-b52b37f04bbb","year":2016},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b0f01eacf276ff46168879dac36eb2f61f92f9d18ac8414a958873fd0b7d7e0a","observation_id":"85d4f33e-c5b4-4d20-86ff-0b34a774ee20","resolution":{"observed_at":"2026-05-23T00:05:14.707579Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/589937","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-26T23:20:14.979672Z","title":"2008, ApJ, 686, 749, doi: 10.1086/589937","venue":null,"work_id":"79738121-71bc-4e85-a374-c2742cc58b29","year":2008},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b1b234dd826a0d7f4626224dcd8d07d345b1db1a194924e7038226c36751fd44","observation_id":"5d5d9870-e5cc-45f3-8f52-9d80dba616f0","resolution":{"observed_at":"2026-05-23T00:02:17.363097Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/425629","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"B., Phillips, M","venue":null,"work_id":"52fa9985-ab4c-4c5f-9672-bfa13ac2651a","year":2004},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:633d36a66859b4b885ce45370b9efab181e40103dd240c02b7715a40cbedd3dd","observation_id":"37ff5169-1cac-4b0f-8b76-b439e10fc0b2","resolution":{"observed_at":"2026-05-23T00:02:17.410312Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T14:19:44.080091+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T14:19:44.080091+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/173334","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T05:31:40.782447Z","title":"G., Freedman, W","venue":null,"work_id":"e2cc57aa-c59f-4b32-bbae-3458854e36ee","year":1993},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d97858862d9da7941c5194a70d54f824ee598bf034b7909ee58aaa61d06b647d","observation_id":"db993f42-6b93-40dc-b334-76b7a5235517","resolution":{"observed_at":"2026-05-23T00:02:17.187647Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-14T05:50:25.520265+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T05:50:25.520265+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac7559","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"23d3291b-676e-4883-8f63-d32e8ef19410","year":2022},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:10faa204ab1f9ce591230b352e24db3f2226a6c71409ef0a33678fe2cf500990","observation_id":"be2d5122-3b7b-4091-ba4c-318f6576f271","resolution":{"observed_at":"2026-05-23T00:02:17.184209Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[{"edge_observation":{"observed_at":"2026-07-11T03:18:56.379957+00:00","source":"paper_reference_links","state":"open"},"event_date":"2025-06-20","event_type":"correction","notice_doi":"10.3847/1538-4357/add2fb","provenance":{"observed_at":"2026-07-11T03:00:18.704642+00:00","source":"crossref","source_record_id":"10.3847/1538-4357/add2fb->10.3847/1538-4357/ac7559:correction"}}],"reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/acf4fb","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"G., Scolnic, D., et al","venue":null,"work_id":"b1394b96-8555-41bc-9d73-0a96b189b5a4","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:8d01fb1508af80ec8184b23635b03049d0dfd2b6e3eddee3c33f794541d05eb8","observation_id":"903eb758-9b1c-4a31-93b5-5ded29d7d329","resolution":{"observed_at":"2026-05-23T00:02:17.268982Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad84f3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"S., Riess, A","venue":null,"work_id":"f6bcd545-1f73-4640-ab32-57a8dd983107","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:3da0d2c73daa1191dd366926374d82ee5dad473139496cee8edcaa35e8427191","observation_id":"e6ff6f81-3a2c-409f-9015-2e73e3cb3da9","resolution":{"observed_at":"2026-05-23T00:02:17.285214Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202039709","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T20:27:21.590173Z","title":"The astrometric solution","venue":null,"work_id":"9e4c0797-4018-42db-8b81-8eb863f1ac46","year":2012},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b6af53081a91747cddbda70775de6a99e0c85367c13a6f53fe80f88ec67184fa","observation_id":"0ee10ab1-adb5-4b52-92b3-d2a383933438","resolution":{"observed_at":"2026-05-23T00:02:16.888674Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-01T05:08:11.565587+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-01T05:08:11.565587+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/319465","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T12:32:07.783121Z","title":"M., Calzetti, D., Freedman, W","venue":null,"work_id":"ed404a2e-745b-446b-84c6-d5feb8944eb0","year":2001},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d5451544fa1df139c35d7c7928e2b48e44992cd319f8805b45eaa7a213d69bb6","observation_id":"48e3df1a-bfcd-4688-bfe3-a2ec5747a3a5","resolution":{"observed_at":"2026-05-23T00:02:17.163268Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"19a4fff7-91bd-4560-a9e8-e46bab3fa8b0","year":1976},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:5ff3ee6ed265daf2c631dc98e16bebc4493c5595721ea07e15b94fdd40ef26e3","observation_id":"871bd7a9-f3bf-4e8e-b94b-39a25210276b","resolution":{"observed_at":"2026-05-23T00:05:14.704352Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/159659","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T06:10:36.372121Z","title":"The period-luminosity relation","venue":null,"work_id":"034e42b7-a671-4eb4-90e3-25d4f92d594f","year":1982},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:2e2b8c920ce30edb2aa7a3e183a312ebfe93544270d5933d4721b9853253661f","observation_id":"9c1fcf1b-c3b3-4468-acce-e89aceaa3e4c","resolution":{"observed_at":"2026-05-23T00:02:16.896392Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F., & Freedman, W","venue":null,"work_id":"85264121-8468-4b8c-873f-31210d1633ea","year":1999},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:5a8dcd3b10e071fbfd2fca206df393e78cc1c1f6a7430349dc8af9b219f2beac","observation_id":"e3b48a37-04d5-4e39-bd5a-bd3ba04b692e","resolution":{"observed_at":"2026-05-23T00:05:14.701306Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/690/1/389","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F., Mager, V., & Freedman, W","venue":null,"work_id":"c9b557b7-c9dc-49fd-885c-1f149fada0a2","year":2009},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:14085efc43187dcc681b2089bfda8d5ff5e84febee41e460639464dfe9e93e95","observation_id":"7072af26-138d-47a7-9508-aabbf6254a64","resolution":{"observed_at":"2026-05-23T00:02:17.066576Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aab7f4","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"F., Freedman, W","venue":null,"work_id":"d256068d-8328-407a-af1f-19fb2de286e8","year":2018},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d6fd01006801a4da80ea38f993584fcb1beed39b38b6fbe8f25f183a962d16f2","observation_id":"74af2d0b-9426-4e46-b33c-24cd3f02a8a1","resolution":{"observed_at":"2026-05-23T00:02:17.072607Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"1d3e7cca-350e-4305-b93f-a7705b962afe","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:0a10b3dae888971d9e84a007e89bbe229a6909cf78308d1741f8756fc9a35d98","observation_id":"0f74703c-2672-46e6-9ec2-74237cb179d9","resolution":{"observed_at":"2026-05-23T00:05:14.697251Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/508925","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T05:31:40.780648Z","title":"2006, AJ, 132, 2729, doi: 10.1086/508925","venue":null,"work_id":"03d9d281-9cef-4cf7-87e5-81816376cc72","year":2006},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d0b8d56fb11bcf31dcb88036fe4731436df7ab255eae1c6e1d0d275f1a390263","observation_id":"7b9c7e48-99fb-4aff-bea6-a4e033446bf5","resolution":{"observed_at":"2026-05-23T00:02:16.990360Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201423496","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T08:56:48.963748Z","title":"2014, A&A, 570, A13, doi: 10.1051/0004-6361/201423496","venue":"Astronomy &amp; Astrophysics","work_id":"5603e92d-6182-4a59-9567-3bc5d9bee17b","year":2014},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:e143e2f75383a2205374c90d69c882372ff48ac005a7133002d562e30457a3c7","observation_id":"171240c4-1761-4992-9745-a2c1e47e7ad8","resolution":{"observed_at":"2026-05-23T00:02:17.212961Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/183803","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"2659cd51-9a2d-4638-96ce-9c3adcccb829","year":1982},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:58920d5c9bcd7ac9f8d2404df9c29b1647189468c4dd61b13a7e2908a981ed50","observation_id":"bd98c473-711a-4413-bf69-429415076f31","resolution":{"observed_at":"2026-05-23T00:02:16.904351Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab2627","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"McQuinn, M","venue":null,"work_id":"3846f897-73eb-46d3-8bcf-fcb5a34c6af8","year":2019},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9bb6c1548a3a8c27d20dc01df9ecde25d2023aff0fca58a9296be2ba97129a68","observation_id":"5f5b8f09-6399-4f02-b3e9-ba1d91ebe647","resolution":{"observed_at":"2026-05-23T00:02:17.034484Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/762/2/82","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"96aa00e3-1d06-47e8-a245-7985e1c87b3e","year":2013},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:a7e1406a552b027bd22b3cfb363d8183a2e551000ccdaee9674fe9e2886b4cc6","observation_id":"b57e8972-f025-488f-8a2c-2d0a1164fbb2","resolution":{"observed_at":"2026-05-23T00:02:17.255917Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"8711.2003","doi":"10.1046/j.1365-8711.2003","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Jiang, F","venue":null,"work_id":"7159653d-74d0-44ca-b473-c338d9a8cd44","year":2003},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d7b05626df4887facea31abe2f40e317eea987add54fb5bd528964c540f6ed6b","observation_id":"10cff387-b7ca-4da3-99d2-55df0f88d94f","resolution":{"observed_at":"2026-05-23T00:02:16.860088Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/697/2/996","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"2009, ApJ, 697, 996, doi: 10.1088/0004-637X/697/2/996","venue":null,"work_id":"e1ecefc9-f777-438c-8097-8c20ecb5997b","year":2009},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:d2fc3de8a055ae0075013cc1d563f7b87aae5ba6ace8f7455da1a209180a7fa0","observation_id":"fe0a40b0-cea8-47b4-8e70-bcdfae5071d4","resolution":{"observed_at":"2026-05-23T00:02:17.407233Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/308304","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T17:57:14.995733Z","title":"R., Huchra, J","venue":null,"work_id":"0e00d9f6-c31d-45ff-b135-dca1c77c9bfb","year":2000},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:021d0ad7c7b05f62efb616e5ea862d20c7a8a48dc165d8ce94111aede4d0e587","observation_id":"b5cb7151-0146-403c-8128-99d152e65c53","resolution":{"observed_at":"2026-05-23T00:02:17.395662Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4365/acfaa2","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T06:00:36.873837Z","title":"2023, ApJS, 269, 3, doi: 10.3847/1538-4365/acfaa2","venue":null,"work_id":"f7a53873-1c84-40b7-a493-522d8528a176","year":2023},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:b36b27c814d210357e0180aab9ae2b98dcd4e5a18fe5cb42e26cc24e23067c57","observation_id":"f313d290-168b-4298-a1ba-7787296a1e9e","resolution":{"observed_at":"2026-05-23T00:02:17.027276Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-11T15:21:43.234481+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T15:21:43.234481+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/707/2/1449","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T01:11:28.800945Z","title":"D., Sullivan, M., Howell, D","venue":null,"work_id":"df27d4ba-2a68-486c-a4d7-dcf4be521dc1","year":2009},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:0d88055c5c42d5dc683de7803f90001ccdb684656bf75d680c3533be499b7199","observation_id":"ce92d979-fad3-4ccb-a0b9-f09f02c4479a","resolution":{"observed_at":"2026-05-23T00:02:16.986708Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad79f8","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T01:52:58.760018Z","title":null,"venue":null,"work_id":"6f628eb3-4e8e-40b8-9849-2ff9c7b54081","year":2024},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:fae373fe1037a7c71a5144745e458875af73c3a887beafd806ffb3208c726687","observation_id":"79f9ae34-03f3-49c7-a70d-1248fe294fef","resolution":{"observed_at":"2026-05-23T00:02:17.370044Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab7305","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-25T22:48:38.365570Z","title":"L., Hasselquist, S., Hayes, C","venue":null,"work_id":"53c66bbc-87ff-43c7-88d5-73fd3cf42f17","year":2020},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:52545a012afa93517a00dca268050f65a857980534e9dcafb29d4242a24ffd8b","observation_id":"b200ebb6-90d4-4a5a-a98c-79b7077375b6","resolution":{"observed_at":"2026-05-23T00:02:16.818933Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-01T04:39:39.873398+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-01T04:39:39.873398+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/317048","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"4e6486a7-4c1d-430e-a33d-1431dd35cb4c","year":2000},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:f3c8cf8d28bb0167f48c8b88eb954a79ee4ad37ac0e7e7c157363c72eaa8ca2f","observation_id":"0493fa54-1e3f-4e60-a22d-23520adc277c","resolution":{"observed_at":"2026-05-23T00:02:17.019955Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac479e","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T12:32:07.798110Z","title":"A., Freedman, W","venue":null,"work_id":"6f3f7e78-e237-456b-b3f8-77a21023e0b3","year":2022},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:841ae7b02ed1bc05f459afc31802be9bf947dc5b38adab6d82d10d71183ad7c9","observation_id":"8d6637d6-bf1b-4fe1-9e76-9a15d76e43ff","resolution":{"observed_at":"2026-05-23T00:02:16.961034Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/186970","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T09:44:49.089470Z","title":"M., 1993, @doi [ ] 10.1086/186970 , https://ui.adsabs.harvard.edu/abs/1993ApJ...413L.105P 413, L105","venue":null,"work_id":"51308d42-0c6c-47ce-90c3-3d347991371b","year":1993},"citing_paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-22T23:59:35.379178Z"},"links":{"citing_paper":"/paper/2503.11769"},"observation_digest":"sha256:9f8b70e6ef8e9bf564c19ef4fe176718d143eb59d31b3b2b1601bff2dff4ae7f","observation_id":"c02224d1-d151-4595-a21a-a0a5b2d8291f","resolution":{"observed_at":"2026-05-23T00:02:17.403873Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T16:38:14.197629+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T16:38:14.197629+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2503.11769","last_updated":"2025-03-14T18:03:15Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T20:52:59.928598Z","submitted_at":"2025-03-14T18:03:15Z","title":"The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":2,"verified_exact":88,"verified_fuzzy":6},"total_outbound_references":150},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 100 of 150 outbound references and 7 inbound Pith citation observations for arXiv:2503.11769."}