{"as_of":"2026-08-10T22:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0d624be969d25d87b54bbff21f383205eae7f3c2987fb3ffee116f852c97c3e5","coverage":[{"denominator":88,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":88,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T16:56:27.480853Z","state":"measured"},{"denominator":90,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":90,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T13:44:46.515467Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-10T05:30:23.456663Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-10T05:30:23.456663Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"cited_work":{"arxiv_id":"2501.12734","doi":"10.48550/arxiv.2501.12734","metadata_source":"pith","pith_arxiv_id":"2501.12734","snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","venue":"astro-ph.GA","work_id":"62472d4e-132f-41c0-9521-98ef291ae55c","year":2025},"citing_paper":{"arxiv_id":"2505.21110","last_updated":"2025-05-27T12:31:55Z","snapshot_observed_at":"2026-08-08T02:34:18.304340Z","submitted_at":"2025-05-27T12:31:55Z","title":"Effect of Magnetic Field on the Accretion Phase of Population III Star Formation","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-07T13:44:46.515467Z"},"links":{"cited_paper":"/paper/2501.12734","citing_paper":"/paper/2505.21110"},"observation_digest":"sha256:695ea979a314c15f77f658efd79e40b45fda64c8a43fb9d889fdfcde6d95c45b","observation_id":"30c0421c-4804-4ba5-bd5c-1c30a96fedb4","resolution":{"observed_at":"2026-08-07T13:44:47.985467Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.12734","snapshot_observed_at":"2026-08-03T00:21:45.241141Z","title":"Sharda, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28713","last_updated":"2026-07-30T18:00:00Z","snapshot_observed_at":"2026-08-07T13:52:08.032780Z","submitted_at":"2026-07-30T18:00:00Z","title":"Searching for Population III stars with line intensity mapping cross-correlations","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T00:21:45.241141Z"},"links":{"cited_paper":"/paper/2501.12734","citing_paper":"/paper/2607.28713"},"observation_digest":"sha256:a77d52f737e9aa2823f5b702c5b0b5ebb3d7ad253788e172f899a5079f275ec6","observation_id":"20e82e14-425a-4ae9-915b-a0498b69794d","resolution":{"observed_at":"2026-08-03T00:21:45.241141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2501.12734/citation-record","integrity":"/paper/2501.12734/integrity","json":"/paper/2501.12734/citation-record.json","paper":"/paper/2501.12734"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.025417Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.025417Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:1b8c8a9f09c95f3b73defa3413ec878e60252963dc62c85b5f198bcb6c116a03","observation_id":"1880a62f-9043-49e9-b615-9b8766f1dd4f","resolution":{"observed_at":"2026-08-10T16:56:27.025417Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.031167Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.031167Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:18a2b26bb125f6ecf21541b8e3fd248fdd0e47df3537f6fe3960de31a2aece9d","observation_id":"c0d454f9-5494-4671-b938-cfd027f2ab00","resolution":{"observed_at":"2026-08-10T16:56:27.031167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.036221Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.036221Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:405013f406125fe8b510bfc300d351ff6e697ae9053d7bddbc84ac1158c5f48f","observation_id":"98830e41-3551-48e6-9f66-b6ee0a2569e1","resolution":{"observed_at":"2026-08-10T16:56:27.036221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.041291Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.041291Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:f56fad23d11e6f1111fe2103df54b11b624a8637044ccdbe6359a80feb979141","observation_id":"d59ac5bf-5e1a-41fa-8451-7497ba3c5b5b","resolution":{"observed_at":"2026-08-10T16:56:27.041291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.046084Z","title":"D., McInnes L","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.046084Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6ac9d2ed55da9b07c6f851d4e10d5db55818f079b87f91033fa08efc1a1c1bc9","observation_id":"dcb5d6ca-3a46-41f3-9d7f-2b96d2f61fd0","resolution":{"observed_at":"2026-08-10T16:56:27.046084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.051223Z","title":"S., Stiavelli M., Wiggins A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.051223Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6724f3440ad623411ec2306f9e7d95df2c6e4b31846dd3fa451ac12db348c8a6","observation_id":"feb45b5a-a5d0-4fe2-b06f-ffd8ebf83917","resolution":{"observed_at":"2026-08-10T16:56:27.051223Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.056316Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.056316Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:ec49a443cc81d394c91cdd3e9e8d9f4301567ecd610a739ffb97d10ef71ddbb3","observation_id":"56546ac8-8c17-40ad-a925-183a9f31c8d3","resolution":{"observed_at":"2026-08-10T16:56:27.056316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.061501Z","title":"P., Loeb A., 2001, @doi [ ] 10.1086/320549 , https://ui.adsabs.harvard.edu/abs/2001ApJ...552..464B 552, 464","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.061501Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2b048dc8501fafc45d014cb102bb253ea67850d637417c82092b0e4574ab3312","observation_id":"3256af34-3731-46d5-9135-ec1f7791b3c2","resolution":{"observed_at":"2026-08-10T16:56:27.061501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.066298Z","title":null,"venue":null,"work_id":null,"year":1948},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.066298Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:fda8735155bcb30aad47c6a87a4caaf0862a0e3751ffb0b3a1545b536177dd87","observation_id":"f7e24b91-b86a-469e-aa1c-df38859f9f88","resolution":{"observed_at":"2026-08-10T16:56:27.066298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.072045Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.072045Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2abe933692a4b3e8ae7e889a8e17a9ed8cb529762e1ede07961e81e6f5e7e4e9","observation_id":"b45e0cae-e291-403c-b8c7-2bf383efefb9","resolution":{"observed_at":"2026-08-10T16:56:27.072045Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.077385Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.077385Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2c0ab81bbf2d60648e6c82abf3b0e1a153a6c0b122bb405bb9404f5a1fe7e55c","observation_id":"b8f231b9-a9cf-4488-9fdf-7ce7c7a77e8b","resolution":{"observed_at":"2026-08-10T16:56:27.077385Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.084403Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.084403Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6c262afe96c315807cd510a35be4b18b35e702ce2f83e50f1b1aff1f79e43461","observation_id":"8a635425-e5e1-4d8c-8ab0-05860a0eaf39","resolution":{"observed_at":"2026-08-10T16:56:27.084403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.089580Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.089580Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:8101bb84474630bf71a208610502fb4e1883939aecbe202319f8d035bff4d106","observation_id":"de1664c0-c863-47f3-a49a-f60dbb380559","resolution":{"observed_at":"2026-08-10T16:56:27.089580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.094768Z","title":"V., Audit E., Zank G","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.094768Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2a453bb7839073a11971b6ea8333e97611fabe405de39b77068fbd2ffb02fa6e","observation_id":"a0f8f100-bdee-43c8-aaea-4745aef1947c","resolution":{"observed_at":"2026-08-10T16:56:27.094768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.099999Z","title":"pp 1--8, @doi 10.1109/SECSE.2013.6615093","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.099999Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:b2793d70fca6b0d82ec462426be90122037e5016da6ac2adcf89be818f2f40a6","observation_id":"d7ac282d-7b32-4861-9927-70e2bb5bf419","resolution":{"observed_at":"2026-08-10T16:56:27.099999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.105136Z","title":"S., Schmidt W., Mac Low M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.105136Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:3be84d07710cf779cc04a97898d475bce733ea5cf738d782ad26961322f164ac","observation_id":"2abdd808-41b2-4ae8-b4d0-5cda661ac8a8","resolution":{"observed_at":"2026-08-10T16:56:27.105136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.110495Z","title":"C., Klessen R","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.110495Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2609d1c8b16259d6a52761b1b6b28ec5692b9b5ebe83b0b6487850ee2b1a521b","observation_id":"fb1fb14a-a5cf-4829-b111-f13ad7495469","resolution":{"observed_at":"2026-08-10T16:56:27.110495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.2504","last_updated":"2010-09-21T08:18:44Z","snapshot_observed_at":"2026-07-06T02:12:56.089043Z","submitted_at":"2010-07-15T08:45:00Z","title":"Implementing and comparing sink particles in AMR and SPH","version":2},"cited_work":{"arxiv_id":"1007.2504","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.2504","snapshot_observed_at":"2026-08-10T16:56:29.113532Z","title":"Implementing and comparing sink particles in AMR and SPH","venue":"astro-ph.IM","work_id":"6f9c28ca-c4a3-4f53-8364-67236e1157dc","year":2010},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.116699Z"},"links":{"cited_paper":"/paper/1007.2504","citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:c08895e3823878605b30b020a45884de0f18e0e306a01a598799f9500eaac8b9","observation_id":"934442f3-7ec8-454c-816a-c5bbf94b0b79","resolution":{"observed_at":"2026-08-10T16:56:29.121219Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.124397Z","title":"E., 2015, @doi [ ] 10.1146/annurev-astro-082214-122423 , https://ui.adsabs.harvard.edu/abs/2015ARA&A..53..631F 53, 631","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.124397Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:ba6d87421396464a1dca465f6f341a1bcbe2341c6de80ae6386b093d9a804aa9","observation_id":"d9643d3b-ac0e-429b-be0c-ed650b3c09c5","resolution":{"observed_at":"2026-08-10T16:56:27.124397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.129822Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.129822Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:24ee0cca8921580d2a556a5190405ea163b8e6ff41aaabe5aac89952f24bc9fe","observation_id":"b8271f91-5b68-4fca-98ac-73778f5019c3","resolution":{"observed_at":"2026-08-10T16:56:27.129822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.11678","last_updated":"2025-01-23T18:24:10Z","snapshot_observed_at":"2026-08-10T18:33:24.256786Z","submitted_at":"2025-01-20T19:00:01Z","title":"GLIMPSE: An ultra-faint $\\simeq$ 10$^{5}$ $M_{\\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\\simeq6-7$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.11678","snapshot_observed_at":"2026-08-10T16:56:27.134460Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.134460Z"},"links":{"cited_paper":"/paper/2501.11678","citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:a616bc30d5ec10725b69d0b896222a40cfd52e6a4a8443cb79386a698d35d6d5","observation_id":"a93fbadb-f660-4cf8-91f6-761748c34664","resolution":{"observed_at":"2026-08-10T16:56:27.134460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/revmodphys.17.125","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:28.347209Z","title":null,"venue":null,"work_id":"a221f4db-37d7-4f12-839c-ecbd20c56dff","year":1945},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.139707Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:9f491588559f4a6a76cd95e102af9214f9ad447bfb1bff8ae126970adb86ca27","observation_id":"6ba5a423-e9f6-48e2-ba65-e6d2769a844c","resolution":{"observed_at":"2026-08-10T16:56:28.352161Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.146936Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.146936Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:f6a300547a69286360ef973407db58751e721e466115c3afc89fa0268edf769c","observation_id":"efe3c985-7c33-4528-9934-d1f3f1209693","resolution":{"observed_at":"2026-08-10T16:56:27.146936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/201527202","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:28.318167Z","title":null,"venue":null,"work_id":"0137e2c1-d543-43db-918a-c8319b8b87b7","year":2016},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.153120Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:55cc0434de7ab64d7fa1ef44d3f91318b8d23c0809b5304081c970dd2e257493","observation_id":"26796393-846d-4e1e-80fa-9684a25b1ecd","resolution":{"observed_at":"2026-08-10T16:56:28.322954Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.158175Z","title":"E., Klessen R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.158175Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:c55a53a867b946ac940fce392ce639b61863480d96b593050964e946c2920f0d","observation_id":"2bd2c785-898f-4ba4-8eb4-f0813e06eef2","resolution":{"observed_at":"2026-08-10T16:56:27.158175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.162836Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.162836Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:0cc8be366d8f32acccb9950b3a92c5ddc7bc9e8f2d8c69015fad487ad9a98692","observation_id":"7ec84dd8-2e05-4d91-86a4-78629071d26d","resolution":{"observed_at":"2026-08-10T16:56:27.162836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.167436Z","title":"R., et al., 2020, @doi [ ] 10.1038/s41586-020-2649-2 , https://ui.adsabs.harvard.edu/abs/2020arXiv200610256H 585, 357","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.167436Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:e529ecb531000c5983b9c73ecfebb60b8fdf4a8d8852e60d172078549f7e1aba","observation_id":"86902a86-08a6-4fbb-9535-47c2da5310dc","resolution":{"observed_at":"2026-08-10T16:56:27.167436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.172336Z","title":"E., 2010, @doi [ ] 10.1088/0004-637X/724/1/341 , https://ui.adsabs.harvard.edu/abs/2010ApJ...724..341H 724, 341","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.172336Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:ad2e6cdefe18720582652fe74ed4537164dcf578caecf1fc95a7cc1597e15b48","observation_id":"85efcd4d-b98d-46cb-bdd8-1abc3bdbf034","resolution":{"observed_at":"2026-08-10T16:56:27.172336Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.177073Z","title":"P., Whalen D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.177073Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2488eb8f902bf7920dd29690c61fd501a4c8588ab5ca7db0732f8908f21202cc","observation_id":"c51e187f-76de-448e-9774-87c17afb7c87","resolution":{"observed_at":"2026-08-10T16:56:27.177073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/sty487","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:28.239831Z","title":null,"venue":null,"work_id":"2749c5f6-3260-49aa-8c68-8bc8178bcb58","year":2018},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.181604Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:c7d4d03aed3e68f5e0d9cc6079bb688d2db3830c315b2749ce04d31b1cecbd8b","observation_id":"169adeb1-730a-4c74-b638-4f7fa25169c9","resolution":{"observed_at":"2026-08-10T16:56:28.244822Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.186217Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.186217Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:f7b6999bc32e2e015c622984818c27c7c9ed7ba9e74513c16cc18b6cb5752b5f","observation_id":"28acc6ce-44bf-4094-9d88-16e4b88966f9","resolution":{"observed_at":"2026-08-10T16:56:27.186217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.191234Z","title":"W., 2011, @doi [Science] 10.1126/science.1207433 , https://ui.adsabs.harvard.edu/abs/2011Sci...334.1250H 334, 1250","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.191234Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:94745d9aa0ff20d986a12180a46cea716da6dbd46df07cebc65aa4573db9eab3","observation_id":"11ddf204-687e-4386-995b-80fb4aaedf73","resolution":{"observed_at":"2026-08-10T16:56:27.191234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.196342Z","title":"W., Omukai K., Yoshida N., 2016, @doi [ ] 10.3847/0004-637X/824/2/119 , https://ui.adsabs.harvard.edu/abs/2016ApJ...824..119H 824, 119","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.196342Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:71e40cbaa78e030ccaec4ea4baf06001c9d0a4d45696a3f831a525d0b94735da","observation_id":"53554c53-1565-4d39-bf57-f38d4e38df12","resolution":{"observed_at":"2026-08-10T16:56:27.196342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.201544Z","title":"D., 2007, @doi [Computing in Science & Engineering] 10.1109/MCSE.2007.55 , 9, 90","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.201544Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:40e13015b4d07046792259ffc82d32150152335d6f81f860b9a5febb4c3df54f","observation_id":"d467cefb-9c45-44af-b3ef-cf44fe9070dd","resolution":{"observed_at":"2026-08-10T16:56:27.201544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.207961Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.207961Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:fc78c76e951aa0593fb8caca2068dda01a6bf5257634e751466f863f2f60a0b2","observation_id":"012e5877-c6f1-40b2-b5e6-f57f2afa1a3b","resolution":{"observed_at":"2026-08-10T16:56:27.207961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.213727Z","title":"L., Greif T","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.213727Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2abda6570aebcb160a8b96f4b27e9d6130997912916f7b6d68f0017790c3e2b5","observation_id":"075f44e3-fe10-4a90-9bad-95788ad912e0","resolution":{"observed_at":"2026-08-10T16:56:27.213727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.218837Z","title":"C., Filippova N., 2021, @doi [ ] 10.3847/1538-4357/abe934 , https://ui.adsabs.harvard.edu/abs/2021ApJ...911..128K 911, 128","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.218837Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:c2695777239dac50dad28599fd1ee82d686a2c7b6208dd6c89f83de20f83d649","observation_id":"45c1e284-3384-489b-9e5d-2136bf82d982","resolution":{"observed_at":"2026-08-10T16:56:27.218837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.224149Z","title":"S., Glover S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.224149Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:3fc4af0b8b979bf9158664a501ea83369507d53bb820b1ae35e2adfc7447119d","observation_id":"c46b4e8b-9f6e-4a76-83ab-58c17d7cdcaf","resolution":{"observed_at":"2026-08-10T16:56:27.224149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.230010Z","title":"N., 1941, Akademiia Nauk SSSR Doklady, https://ui.adsabs.harvard.edu/abs/1941DoSSR..32...16K 32, 16","venue":null,"work_id":null,"year":1941},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.230010Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:ac680ffb172dce3711e5bb5af2357f908e86db359a9385046bcbf652a2853c2c","observation_id":"68f41f25-9943-4416-837a-47b81e50a6c1","resolution":{"observed_at":"2026-08-10T16:56:27.230010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.235601Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.235601Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6f36c0e60d5cc14bebcdef7d4c1cfbbe91b75122fad4203678f0febe6f79bb1b","observation_id":"eb5b110d-d81e-41a0-ac39-ff63c0c92ea4","resolution":{"observed_at":"2026-08-10T16:56:27.235601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.242229Z","title":"M., Gerasimov R., Burgasser A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.242229Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:62dbb1b06a7d1387c11ce4efe293b809035b42cfa055023afe46c04ba10269e5","observation_id":"b25978c1-5ecb-4d18-b186-0382408ecfcd","resolution":{"observed_at":"2026-08-10T16:56:27.242229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.247794Z","title":"A., Whalen D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.247794Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:01360c3fb8e1da2422b3d86c87c396532e2ced391b05b48eaa8c3b427d2a3caf","observation_id":"3d3d54b3-d6e7-4b78-a9e5-2d8b86adfac0","resolution":{"observed_at":"2026-08-10T16:56:27.247794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abd9b7","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:28.096310Z","title":null,"venue":null,"work_id":"60fbf087-0935-4cb8-aced-fe9c10f1b3c5","year":2021},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.252874Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:dbbe04aaf622eaacaa113bac9079af038240d6c01570f0c574d1969a179c373c","observation_id":"2616de75-0bee-4cae-accc-8079e55ffa06","resolution":{"observed_at":"2026-08-10T16:56:28.101841Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.258279Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.258279Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:f5cdb1b25e54dc835f4a5f94e77f18a0a722cd5760ff7aec44c677c6ab47af6b","observation_id":"2e6c088b-1cad-42f0-82f2-be62d92166c2","resolution":{"observed_at":"2026-08-10T16:56:27.258279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.263902Z","title":"N., Doi K., 2013, @doi [ ] 10.1093/mnras/stt1524 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.435.3283M 435, 3283","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.263902Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:2b1efbb5f6a0bc30c876e8453dd5da62e30923c2ffb4d28bedb31bea9c39aea3","observation_id":"1fc0e81e-14f0-48af-925b-746d667fcc9f","resolution":{"observed_at":"2026-08-10T16:56:27.263902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.269260Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.269260Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:7c8e8caeb4d3448d2891e21d432636c8c90247feb9a6cfd019541e1c86ca739e","observation_id":"08811c21-60c8-473a-930c-66f8149f5e69","resolution":{"observed_at":"2026-08-10T16:56:27.269260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.274136Z","title":"J., 2005, @doi [ ] 10.1111/j.1365-2966.2005.08826.x , https://ui.adsabs.harvard.edu/abs/2005MNRAS.358..614M 358, 614","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.274136Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:18036ae67d62bb206c1d938f1b66f10829a68b4d66dbd7cc4fc903272813bfa0","observation_id":"cd7f5a3b-22d1-44c0-a6e8-3291e44ead10","resolution":{"observed_at":"2026-08-10T16:56:27.274136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.278427Z","title":"H., Federrath C., Krumholz M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.278427Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:c87b90b50e16a8754b9de525eec51f22de0e4ae9626742f36575369730943601","observation_id":"4fc7680e-37de-4d3c-98ed-d65ca3dd8995","resolution":{"observed_at":"2026-08-10T16:56:27.278427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.282738Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.282738Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:d08716c81522ce9a9954455c3d6fbe4e10124fce0751b5e2564bb54f27dbc122","observation_id":"bd9e4973-c00f-4535-9815-95fd521f6347","resolution":{"observed_at":"2026-08-10T16:56:27.282738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.287450Z","title":"E., 2006, A guide to NumPy","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.287450Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:672efc0a83709d93a2b0b039020018b286ecc32eb3a504b30556393f6cca43bf","observation_id":"dd834e13-7b9a-458c-9936-32153ca112a9","resolution":{"observed_at":"2026-08-10T16:56:27.287450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.291869Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.291869Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:3c8a1219002f3acf44d0fe3198f7c0b93bc60adac271424ce9822788e92c403f","observation_id":"719a084a-9f54-4ab5-b86b-714643153c8b","resolution":{"observed_at":"2026-08-10T16:56:27.291869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.296504Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.296504Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:38cbfe71582c14994e3eede934f8f793d879200d18ebfcd7261eaa7c14e26ac6","observation_id":"fb3922f2-ace4-454d-83ab-63599135acb5","resolution":{"observed_at":"2026-08-10T16:56:27.296504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.301087Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.301087Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:8e560c56c5ca7cae9fc708727f741dae82c283270adc4ecfd49173826eb8cfaf","observation_id":"065e397d-8a48-4809-b4ba-6c2db90e4bdf","resolution":{"observed_at":"2026-08-10T16:56:27.301087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.305706Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.305706Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:e0e72c0d53b7bf3706c18609955e60852cde41155d284ba63086b62436a06565","observation_id":"19cefe18-9bc9-4acf-aae6-2a9d030564b4","resolution":{"observed_at":"2026-08-10T16:56:27.305706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.310273Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.310273Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:a51bb3ca27a1e8505e4c6c8a641b11646fcd95785ada5996f9eabb571d5335e9","observation_id":"b8245340-383e-4042-a09d-f6fb9b9512bc","resolution":{"observed_at":"2026-08-10T16:56:27.310273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.315012Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.315012Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6500452e05fee8d9c807a40cd5e43d293d89e6c877d0ba0755a6c52a353cff6f","observation_id":"38f4fe7d-ac17-4690-9326-6ce0a9bbde9c","resolution":{"observed_at":"2026-08-10T16:56:27.315012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.319820Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.319820Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:d5f1f2c8a9acabd589ec2cd01d78551bbefbaab84f764b08255f9be9c8bf7efa","observation_id":"96672138-9d59-4b65-a4b9-80c9bfd56f83","resolution":{"observed_at":"2026-08-10T16:56:27.319820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.324422Z","title":"R., Clark P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.324422Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:23f2b9cc1b292ec791f53926d3c8880f4b7b3dc7cf6bd47c6da2edc67ffe6eee","observation_id":"dcdd633e-e04a-4fc0-b5a1-862ba8679249","resolution":{"observed_at":"2026-08-10T16:56:27.324422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.329171Z","title":"L., Krumholz M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.329171Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:aa90bbb316b36e7078d6fa7b840e334c31981e5dd7879cab10933d8a9ff19994","observation_id":"95a668a7-0bf9-47c4-b3c5-fc20dfb754b2","resolution":{"observed_at":"2026-08-10T16:56:27.329171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.334151Z","title":"R., Bromm V., El Eid M., 2022, @doi [ ] 10.1093/mnras/stac2479 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.516.3130S 516, 3130","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.334151Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:84e0b4c9451aa5db740afa24ef6582026d6b7a292944e323085058e6c8907188","observation_id":"79708e82-e16d-467a-8d36-d0c2041a8b74","resolution":{"observed_at":"2026-08-10T16:56:27.334151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.338999Z","title":"E., Omukai K., Sugimura K., Matsumoto T., Tomida K., 2023, @doi [ ] 10.1093/mnras/stac3724 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.3076S 519, 3076","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.338999Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:a2015b0e2792cfc9bd75d451a47bf8086ab50c770b0ab8a315f41aab03658fca","observation_id":"f237beaa-fa46-4953-95eb-8d1ac353c93f","resolution":{"observed_at":"2026-08-10T16:56:27.338999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.344133Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.344133Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:e5efcb29e9d2e68764727df9f600fa816d9b20fa5e325394ded098a68e5be8cc","observation_id":"b9f2f811-ece0-46e6-a14c-c2f5fb7cd74c","resolution":{"observed_at":"2026-08-10T16:56:27.344133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.349596Z","title":"S., Banerjee R., 2012, @doi [ ] 10.1088/0004-637X/754/2/99 , https://ui.adsabs.harvard.edu/abs/2012ApJ...754...99S 754, 99","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.349596Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:bbd5bb1ebdfaae1b0fcab801b7c3fde1d64af869dfb54eda4345e4a41f646ae7","observation_id":"3c2f68ae-58ce-4847-ba41-4b0754b9a991","resolution":{"observed_at":"2026-08-10T16:56:27.349596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physreve.92.023010","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.747027Z","title":null,"venue":null,"work_id":"a8e4c4bb-4382-4716-9ae3-ee76fcedd5f4","year":2015},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.354736Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:b000e71bbe48269dbe8570a41b3c2730cb7e4cee70356e1f15cb26c48fe8ede9","observation_id":"f9865b73-2c90-4fa4-9a82-185f9113abe1","resolution":{"observed_at":"2026-08-10T16:56:27.751928Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.359983Z","title":"R., 2022, @doi [ ] 10.1093/mnras/stab2921 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.1959S 509, 1959","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.359983Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:53e6258a5e9ee11d8801e61dc9fa257072b325591f72d26b96db184a1c1e7385","observation_id":"cc437d69-fc9d-4d53-9169-cac07ecba065","resolution":{"observed_at":"2026-08-10T16:56:27.359983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18265","last_updated":"2025-05-16T09:24:45Z","snapshot_observed_at":"2026-07-06T18:21:22.569625Z","submitted_at":"2024-05-28T15:17:03Z","title":"Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18265","snapshot_observed_at":"2026-08-10T16:56:27.365026Z","title":"H., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2405.18265 , https://ui.adsabs.harvard.edu/abs/2024arXiv240518265S p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.365026Z"},"links":{"cited_paper":"/paper/2405.18265","citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:4eb0f0dcea68c1a4cb03fab90b3cc0c251ac732f1d70f598646b10dfde1ddb2c","observation_id":"b2f8a887-0c98-4ffa-9643-dddca724671e","resolution":{"observed_at":"2026-08-10T16:56:27.365026Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.370563Z","title":"R., 2020, @doi [ ] 10.1093/mnras/staa1926 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.497..336S 497, 336","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.370563Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:b3b987d98a30419cbeefaee123b3c6881b104a3c958d82762cacedd4d4d3af7e","observation_id":"4aa0a79b-acfc-479e-8542-c48be0b52798","resolution":{"observed_at":"2026-08-10T16:56:27.370563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.376133Z","title":"R., Schleicher D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.376133Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:255b05613f50e02810af25bd4b21bb5ef564a40e93c65dda279a9d538b43db73","observation_id":"a3a2f8b0-0b77-42da-a23f-f2b448516f78","resolution":{"observed_at":"2026-08-10T16:56:27.376133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.381552Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.381552Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:7169dbd01805665ffaf583052cab8c07e2cb9df0a31fa25c40d9d9c4893ea0cc","observation_id":"97449187-0a7f-4336-a0e9-03758a4dd84a","resolution":{"observed_at":"2026-08-10T16:56:27.381552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.391847Z","title":"H., Bromm V., 2012, @doi [ ] 10.1111/j.1365-2966.2012.20605.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.422..290S 422, 290","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.391847Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:9d19752894dd2b531e6653c1f4ffdb7377c827efed2ab120bbcde5ef42dfb310","observation_id":"eba3bc80-9531-4b18-9d7a-1346a4f655b5","resolution":{"observed_at":"2026-08-10T16:56:27.391847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.396862Z","title":"T., 2016, @doi [ ] 10.1093/mnras/stw1728 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1307S 462, 1307","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.396862Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:26a1c4aff91a693f39cd5f22703de600daf1f2bd18023d36925d05efbfaf20bb","observation_id":"21faea34-93d1-4fa0-ac24-c03da1c06dae","resolution":{"observed_at":"2026-08-10T16:56:27.396862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.402155Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.402155Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:bd0413d463ee4be2d70c004bc577ec964745f27ea8cc85f21e8deeafd22f0345","observation_id":"5c78a3c3-e02f-4ef4-b637-63fe47090bf6","resolution":{"observed_at":"2026-08-10T16:56:27.402155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aac892","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.641854Z","title":null,"venue":null,"work_id":"4c6bb41d-dec4-4ffe-b00c-afdf7fd8364a","year":2018},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.407931Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:21653735868e2b4329aa8393eb1597e0528456671fb31f7932650267f0b3669a","observation_id":"df585cb3-b2eb-456d-886f-3b75875c6f63","resolution":{"observed_at":"2026-08-10T16:56:27.648482Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.412916Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.412916Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:a10bca804ec6c70aca39cf290e88183177fdffbbb8cdac98fdb38dfa8604f611","observation_id":"5a0cec54-4dc8-42a2-bb90-94bd2dfc45a4","resolution":{"observed_at":"2026-08-10T16:56:27.412916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.417667Z","title":"J., Smith B","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.417667Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:9335edc692029e3f94e305ffdbebed7fdbd46859928dcc23530bdc790178362a","observation_id":"b35a49d4-a48d-49cc-885a-6ad20e66d3ed","resolution":{"observed_at":"2026-08-10T16:56:27.417667Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.422137Z","title":"J., Oishi J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.422137Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:5a580491cad2466c7b3c9478ffb5eb658064e337f6619935e377e2e6fc23a09c","observation_id":"75696a7d-aeda-4e33-8632-e091bd500b23","resolution":{"observed_at":"2026-08-10T16:56:27.422137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.426692Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.426692Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:76b2f930d25650a2a1c319cabb35233dcf5024863d727b357a5240b84e37675c","observation_id":"cc376dda-15b9-466c-bb34-8279f250a3d1","resolution":{"observed_at":"2026-08-10T16:56:27.426692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.431355Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.431355Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:71dfd362629d12574092428a5eb5fc755187aed743a40c8a433296fc4d917b23","observation_id":"3652a899-c6a3-41cb-8dd0-36591867e592","resolution":{"observed_at":"2026-08-10T16:56:27.431355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.436532Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.436532Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:4c33b313cf07222c7b3fae3c00ac08c910afd1ad0a78cfef34b9e7b8e487c556","observation_id":"a4380f37-ca4d-4da7-a588-9bba1011320d","resolution":{"observed_at":"2026-08-10T16:56:27.436532Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.441619Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.441619Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:3af4bbe1d08613b90c56a2f2f27f0eda761734d656bcf1b21f20a8e8370d38db","observation_id":"22c7c439-b65b-4198-8aa7-f4dd11dc183d","resolution":{"observed_at":"2026-08-10T16:56:27.441619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.447089Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.447089Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:55b71b1bb6cee3991623a630d8829fda58ccfde1c11e086c2667bf81979136bb","observation_id":"1204cbf6-1675-4aea-b07e-4a7490e46098","resolution":{"observed_at":"2026-08-10T16:56:27.447089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.452360Z","title":"L., 2011, @doi [ ] 10.1111/j.1365-2966.2011.19538.x , https://ui.adsabs.harvard.edu/abs/2011MNRAS.418..838W 418, 838","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.452360Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:059987cb4065a4f85715bc8aa7ee940d3312f738cb5abbff935805e85843d1cf","observation_id":"ced59e54-be8a-448f-a41f-263c75b579bb","resolution":{"observed_at":"2026-08-10T16:56:27.452360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.457144Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.457144Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:6caa6aab5689b70ca95ca386405f8796335cd3892f0802f8fa8b5f4613de1d13","observation_id":"561d7fb6-694c-4ad2-9606-c5b64bc3be19","resolution":{"observed_at":"2026-08-10T16:56:27.457144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.461833Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.461833Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:a9a4aab7f66bc2ae717529080f8221d7477ce4aa8330845d7f3e20da46846a54","observation_id":"960f1fbb-cae9-4717-9785-fac0f1d17e41","resolution":{"observed_at":"2026-08-10T16:56:27.461833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.466147Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.466147Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:325e9e400d0326f06a4d91d95ce503889011b0b046c423f8fa02b8235709a033","observation_id":"d3d0d859-cd6a-4a98-a875-c74a3a625346","resolution":{"observed_at":"2026-08-10T16:56:27.466147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.470683Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.470683Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:66df0495cdf2dd2eb65435b55fd79190fd2716963113e8bbacf1096ee64f978c","observation_id":"97d77d4a-97ac-4391-9d94-3594302a4ccd","resolution":{"observed_at":"2026-08-10T16:56:27.470683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.475814Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.475814Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:decff42676d5fec52f253dde45e8f587bc5a312ea4e4ac9f3d0a28e42f3eba0c","observation_id":"302ca7fe-b11a-451d-a5ba-e3a67c20daf4","resolution":{"observed_at":"2026-08-10T16:56:27.475814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T16:56:27.480853Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback","version":2},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-10T16:56:27.480853Z"},"links":{"citing_paper":"/paper/2501.12734"},"observation_digest":"sha256:8baacaef14f5c47f44c30b5ad247e09131d257287be52bbf54e0e5af75016f31","observation_id":"7d13a3b3-ba78-41f4-822d-9555261e08bc","resolution":{"observed_at":"2026-08-10T16:56:27.480853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.12734","last_updated":"2025-04-30T15:43:08Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T18:19:34.477652Z","submitted_at":"2025-01-22T09:10:22Z","title":"Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback"},"reference_resolution":{"displayed":88,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":81,"verified_exact":7,"verified_fuzzy":0},"total_outbound_references":88},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 88 of 88 outbound references and 2 inbound Pith citation observations for arXiv:2501.12734."}