{"as_of":"2026-08-07T19:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:798865da842578375c7a07dee70a15e5bf35b86520552c14900d24b986380b20","coverage":[{"denominator":113,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:28:34.261669Z","state":"measured"},{"denominator":102,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":102,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+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":"2026-08-02T07:32:04.668659Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08436","snapshot_observed_at":"2026-07-14T15:02:03.459139Z","title":"A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09858","last_updated":"2026-07-15T11:28:58Z","snapshot_observed_at":"2026-08-06T12:14:35.906039Z","submitted_at":"2026-07-10T18:00:03Z","title":"How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T15:02:03.459139Z"},"links":{"cited_paper":"/paper/2507.08436","citing_paper":"/paper/2607.09858"},"observation_digest":"sha256:c76fd3ce2037a07efa1bc09a08bca3e8a35b928dda42ab6a485c510a4783b18e","observation_id":"6afc834f-3a35-4923-9158-5e8a0b4e0f51","resolution":{"observed_at":"2026-07-14T15:02:03.459139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08436","snapshot_observed_at":"2026-08-02T07:32:04.668659Z","title":"A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09858","last_updated":"2026-07-15T11:28:58Z","snapshot_observed_at":"2026-08-06T12:14:35.906039Z","submitted_at":"2026-07-10T18:00:03Z","title":"How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-02T07:32:04.668659Z"},"links":{"cited_paper":"/paper/2507.08436","citing_paper":"/paper/2607.09858"},"observation_digest":"sha256:cf4e6bdaa0d07001c663062cda4f00171f35e6a9645e8aa7c465d4d846d6f40e","observation_id":"6f6962a6-426a-491e-af3e-131b7f15b5dd","resolution":{"observed_at":"2026-08-02T07:32:04.668659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2507.08436/citation-record","integrity":"/paper/2507.08436/integrity","json":"/paper/2507.08436/citation-record.json","paper":"/paper/2507.08436"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:25.131291Z","title":"2021, MNRAS, 503, 5826","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.131291Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:3503f4ac5bce5a33af4094e44c252fa54bd46355670710d552629f1893c2c3e4","observation_id":"d3ee008f-cad8-4289-90e4-f413f86887e3","resolution":{"observed_at":"2026-08-06T18:28:25.131291Z","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":"2026-08-06T18:28:25.259373Z","title":"2023, A&A, 680, A23","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.259373Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:cbb48dceaf5a589bc0f8bbaa32cffe579ad97f59f8e2530acbdfa7d3fd32d658","observation_id":"cec1c406-3284-4aa7-81d1-b860d0aced08","resolution":{"observed_at":"2026-08-06T18:28:25.259373Z","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":"2026-08-06T18:28:25.328678Z","title":"2024, A&A, 687, A90","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.328678Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f1bd02dcc9ed5857446231e731bd6561cf8247ab8989cfebacb7b95bfd1844ed","observation_id":"2294be30-67f9-4b03-a806-bb52ecf3294d","resolution":{"observed_at":"2026-08-06T18:28:25.328678Z","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":"2026-08-06T18:28:25.430388Z","title":"E., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.430388Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:962dfab735b720b8e755cd355e853742201f08ea6b2dc5bc96a85896ae6a6661","observation_id":"c7c0f6c0-1b48-4e7c-9067-c7474d74d6b9","resolution":{"observed_at":"2026-08-06T18:28:25.430388Z","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":"2026-08-06T18:28:25.532022Z","title":"2011, ApJS, 196, 22","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.532022Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:8746f06be63e5398635e9a43057c967c8cf81dced5dda9154dd0b13f029dfd3a","observation_id":"28dca9ba-575b-49b2-97b8-0cf07d50deef","resolution":{"observed_at":"2026-08-06T18:28:25.532022Z","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":"2026-08-06T18:28:25.663888Z","title":"2016, ARA&A, 54, 491","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.663888Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:08ef60320af0a730742d21a65f8f53bda9f4f209ffc2a9cb9d024737790d782d","observation_id":"a914b415-e659-4ae3-8d80-9c827b6ea86c","resolution":{"observed_at":"2026-08-06T18:28:25.663888Z","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":"2026-08-06T18:28:25.723545Z","title":"R., Bonnell, I","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.723545Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:4f303bdd1ecaa5736551df7877dd2a33e63716245acda6347da7eda6f70b57b9","observation_id":"61ab1e92-f1ea-4aca-8e31-32b0069df80e","resolution":{"observed_at":"2026-08-06T18:28:25.723545Z","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":"2026-08-06T18:28:25.788250Z","title":"2020, A&A, 638, A86","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.788250Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:bb3d247aaa1ced88305aeab1745a992e590c00d1450173b5515ea57bce46193e","observation_id":"58370f55-74f8-4f39-8943-d77bf63bc7e7","resolution":{"observed_at":"2026-08-06T18:28:25.788250Z","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":"2026-08-06T18:28:25.865629Z","title":"& Teyssier, R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.865629Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:9bac51430e0f08b3c974b288a49e4fb20cc961facfd4716418c8a714e4f2641a","observation_id":"07af9bde-e4c5-4b10-bfb0-5d6cccecc609","resolution":{"observed_at":"2026-08-06T18:28:25.865629Z","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":"2026-08-06T18:28:25.926379Z","title":"A., Bate, M","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.926379Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:857ce7e57fbd4a5006714d04f9b793e97988ff8602a3369c97892a4c0ad4ab94","observation_id":"0336027b-c1f2-4f0d-b312-3f354d95e215","resolution":{"observed_at":"2026-08-06T18:28:25.926379Z","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":"2026-08-06T18:28:25.997286Z","title":"A., Vine, S","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:25.997286Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:32c900c7c879a389d839815dc51ad6d428d6f5e77c68351c7acb6c8b7c90a9df","observation_id":"2119b84f-7125-405f-9d9b-567aebecc379","resolution":{"observed_at":"2026-08-06T18:28:25.997286Z","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":"2026-08-06T18:28:26.110440Z","title":"2020, ApJ, 896, L34","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.110440Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:277542cb4040bd11cb2ce48a4c273fb1022be12a34d0f6d95fb0bdff37702d7b","observation_id":"c53b4d0b-1fca-4691-a685-bb4d4a5cac8f","resolution":{"observed_at":"2026-08-06T18:28:26.110440Z","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":"2026-08-06T18:28:26.223119Z","title":"2023, A&A, 675, A144","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.223119Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:d7ea3714c3de6487a7a0defe86f1d1bbd7ca941d445f31fc622e49714c65ef72","observation_id":"aae7c807-1071-4bef-8820-f2ff90be6327","resolution":{"observed_at":"2026-08-06T18:28:26.223119Z","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":"2026-08-06T18:28:26.335045Z","title":"& Mocz, P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.335045Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:3b0ed3525dd8d58bc1983b539b7af6b3591c8cfb6ee49e88191a42726da327c5","observation_id":"3b7997f0-068b-4b1c-833d-e131f712f156","resolution":{"observed_at":"2026-08-06T18:28:26.335045Z","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":"2026-08-06T18:28:26.440797Z","title":"T., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.440797Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:23332326c2e805c883793703acfad1324184e25ca637892a1d93b2b06af65345","observation_id":"fc59b088-3689-46ab-9625-e18b5f147b26","resolution":{"observed_at":"2026-08-06T18:28:26.440797Z","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":"2026-08-06T18:28:26.546091Z","title":"2025, A&A, 696, A151","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.546091Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:35c66f178587394088a34350e6549d9dddae16ee6ea2d29297f2f03b79dc6ec1","observation_id":"465257f9-f9ec-4a8b-9131-9b7035a08417","resolution":{"observed_at":"2026-08-06T18:28:26.546091Z","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":"2026-08-06T18:28:26.626248Z","title":"2018, A&A, 620, A21","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.626248Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f40fb2eaeb786127437b0edf4bd530ebc6554af5fe6d09e100dbb05f409876cf","observation_id":"756631c6-0bba-4c55-8a2a-b6d857b96adc","resolution":{"observed_at":"2026-08-06T18:28:26.626248Z","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":"2026-08-06T18:28:26.743859Z","title":"& Teyssier, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.743859Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:c7670429fb4f1052700d2511384127a4217f93349808b85024728b50ff8441e8","observation_id":"b32a0a5d-ae64-4c7d-bf7c-13ba3134a20b","resolution":{"observed_at":"2026-08-06T18:28:26.743859Z","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":"2026-08-06T18:28:26.918287Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:26.918287Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:0acc16598c2f0d2964876c3f3148ef1e6657f3c7664b75456d6d853e35179e3b","observation_id":"210e1965-f82b-4db7-98c3-15de5caaae76","resolution":{"observed_at":"2026-08-06T18:28:26.918287Z","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":"2026-08-06T18:28:27.014338Z","title":"M., Wandelt, B., Heiles, C., Falgarone, E., & Troland, T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.014338Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:00725380a5bcad3741cab23957371a665b9426e1295787aeafadef038ae7188f","observation_id":"a0ec44cb-2137-4477-88f5-10788b45bd46","resolution":{"observed_at":"2026-08-06T18:28:27.014338Z","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":"2026-08-06T18:28:27.119252Z","title":"F., Testi, L., et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.119252Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:80e9f87113f351edf51a339b89bf7c3bea0fbcfcf90d35ea26348a244079678d","observation_id":"8d206d48-0a44-495f-b383-f562b09aaf20","resolution":{"observed_at":"2026-08-06T18:28:27.119252Z","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":"2026-08-06T18:28:27.313794Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.313794Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:4420daef10d43018bcd4bb776a52925669f30972f219150e9ed007fa3acd4dd9","observation_id":"8d30e101-6300-44ea-b0a9-49fee2bf8db2","resolution":{"observed_at":"2026-08-06T18:28:27.313794Z","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":"2026-08-06T18:28:27.447089Z","title":"E., Ngoumou, J., Ercolano, B., & Bonnell, I","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.447089Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:d185e037bf6327451410660d5140a80cf0a4943e83c6cf9f181c269a5007c120","observation_id":"7718f4d2-b7a4-4374-94ff-6d6a704326df","resolution":{"observed_at":"2026-08-06T18:28:27.447089Z","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":"2026-08-06T18:28:27.558141Z","title":"2015, MNRAS, 453, L73","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.558141Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:fc09a637351dd3c420b6d60d066dc046033e736e9be3c91fcbd248e0f899fb99","observation_id":"eb9d2716-4d7f-4bfa-be08-8d573e6fffc5","resolution":{"observed_at":"2026-08-06T18:28:27.558141Z","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":"2026-08-06T18:28:27.693310Z","title":"C., Dittmann, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.693310Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:1b3c7d590d014a1d8c1aa8668f2dc0686cda3c1ad4115b1a83655a58bd640ddd","observation_id":"790b86bd-4a40-4024-ab0b-57df87477fd6","resolution":{"observed_at":"2026-08-06T18:28:27.693310Z","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":"2026-08-06T18:28:27.827337Z","title":"2021, MNRAS, 504, 2742","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.827337Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:8179998ec273be646d9e439198078417605a4151cc3bd1478b7a51446b1b8602","observation_id":"3e181bcc-fd5d-4fa1-9bea-64ee9c07a03e","resolution":{"observed_at":"2026-08-06T18:28:27.827337Z","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":"2026-08-06T18:28:27.964066Z","title":"2015, MNRAS, 450, 4035","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:27.964066Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:a53795d3332cad10a9f504c4ef2b8d7ab18b24c7fe4547c37af6b2ec46a82c97","observation_id":"b5bdf095-6c09-42e7-adb6-66cc9607da3e","resolution":{"observed_at":"2026-08-06T18:28:27.964066Z","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":"2026-08-06T18:28:28.070256Z","title":"C., & Klessen, R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.070256Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:2aadfe48728f6752ea4b50c5af667f06c5c44ede8e363d0359e9e7afc2ecdd23","observation_id":"8a44f3de-8c13-4d03-a722-be373206f1ab","resolution":{"observed_at":"2026-08-06T18:28:28.070256Z","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":"2026-08-06T18:28:28.147489Z","title":"& Klessen, R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.147489Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:adfa332b0be76ad59c3f01c9c995b35d259b985c4a82a1661deb332c6332068d","observation_id":"0b3d91bb-e633-492b-a05c-a85b2285fefa","resolution":{"observed_at":"2026-08-06T18:28:28.147489Z","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":"2026-08-06T18:28:28.213306Z","title":"S., Iapichino, L., & Beattie, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.213306Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f0002bf20e8812a8144b70f482b4bf4d7be618071f0e03ce975fbffc0301162b","observation_id":"fb47a43e-295b-4ddc-89af-6bc8966574bf","resolution":{"observed_at":"2026-08-06T18:28:28.213306Z","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":"2026-08-06T18:28:28.370698Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.370698Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:4ffc36323de5c70b5c7777a3810fda73ff171dd4570f688ca2534d72513e4632","observation_id":"918e627d-9764-45cd-a908-627e75b7dea6","resolution":{"observed_at":"2026-08-06T18:28:28.370698Z","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":"2026-08-06T18:28:28.549161Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.549161Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:ff080c1990392eb507fc070fa8b45e44588a5d9110d63be645cf466cdf054401","observation_id":"9b50aa0e-1e08-4945-90a5-a23b132133b9","resolution":{"observed_at":"2026-08-06T18:28:28.549161Z","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":"2026-08-06T18:28:28.637129Z","title":"2023, A&A, 672, A193","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.637129Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:aab493dcd813c32e1bd8bc034866eb79dc3ca45174fe5c50300442e9f5d2921a","observation_id":"14182347-96cf-4a94-aee5-7624b09fa774","resolution":{"observed_at":"2026-08-06T18:28:28.637129Z","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":"2026-08-06T18:28:28.752883Z","title":"2006, A&A, 457, 371","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.752883Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:6cb41859a06527a586c0bf4b3abd0a6ce9060c8632cbc2a9f7f3ae3f71c0f0a1","observation_id":"bd8e9f63-b91e-4728-ad16-0a5a8abf6da7","resolution":{"observed_at":"2026-08-06T18:28:28.752883Z","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":"2026-08-06T18:28:28.901463Z","title":"2000, ApJS, 131, 273","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:28.901463Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:25d9b3f6ca63c2d818dc922cfcbbe8441d27f4c507d5c1aa9fcef3c0682e1f20","observation_id":"acd00fe6-e4bc-4abf-b97c-a6c931cb56b4","resolution":{"observed_at":"2026-08-06T18:28:28.901463Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:44.696092Z","title":"2015, MNRAS, 454, 4484","venue":null,"work_id":"b0e7573e-a02e-4a03-a7c9-5c20b6889c3f","year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.016443Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:bd6d01b52f89d102b18c983fd0a67284ea204fd85c965e117ce1d70e7dc0bf17","observation_id":"ac0b1281-1aa6-4399-9adb-998c7e6e5525","resolution":{"observed_at":"2026-08-06T18:28:44.742541Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:29.123315Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.123315Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:4d0a266d27f342e1f7de5cc3192319c14291874ccc164c4cb98837797475d2c0","observation_id":"b0e81e17-fdd7-458f-b4c5-91f3461c66e5","resolution":{"observed_at":"2026-08-06T18:28:29.123315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.02646","last_updated":"2025-02-04T19:00:04Z","snapshot_observed_at":"2026-07-06T20:31:13.063382Z","submitted_at":"2025-02-04T19:00:04Z","title":"Introducing the Rhea simulations of Milky-Way-like galaxies I: Effect of gravitational potential on morphology and star formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.02646","snapshot_observed_at":"2026-08-06T18:28:29.187810Z","title":"2018, MNRAS, 480, 3511 Göller, J., Girichidis, P., Brucy, N., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.187810Z"},"links":{"cited_paper":"/paper/2502.02646","citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:566122b14bae5f5ae734a746dcb3e67fe57ed4f68a10207a9f91aff8436f90c7","observation_id":"a088dba7-db19-479f-aece-c69fd161a5ce","resolution":{"observed_at":"2026-08-06T18:28:29.187810Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:44.470932Z","title":"Y ., Hopkins, P","venue":null,"work_id":"a95008cf-4fde-46b1-a6ff-a21b8231ef82","year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.242774Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:4a653229bd85da7d7428d0f43ad4f2712fc9aba3eed1b6af57dc200f9db230aa","observation_id":"3c607609-3e90-44fc-86e1-751739980d6f","resolution":{"observed_at":"2026-08-06T18:28:44.577127Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:44.345855Z","title":"2018, A&A, 611, A24","venue":null,"work_id":"1e4f3f03-4d65-4628-bb03-d6849298bfb7","year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.359350Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:1f8111e93f103426bed70fcf398f43933da2963b20bf07d71089d7759330f46c","observation_id":"5af6b9b0-d665-45b4-8032-f0c2c383adb7","resolution":{"observed_at":"2026-08-06T18:28:44.410316Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:44.157264Z","title":"2020, ApJ, 904, 194","venue":null,"work_id":"8ef66167-9df0-46a3-abcb-757cdd2099ee","year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.507476Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:217cea8d44e7866a252191fccc5029d302a878f8898bc841ca3df9c6893779f7","observation_id":"744a910b-8816-48c2-a3c3-fd50a5ad3d0e","resolution":{"observed_at":"2026-08-06T18:28:44.234959Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.941606Z","title":"& Grudi´c, M","venue":null,"work_id":"ea4af4dc-7250-4998-8aa0-da7c59538957","year":2024},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.692179Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:1167df54b01ac992333e445e7788770baa8496e687440ecd04111ec3e5bacc0e","observation_id":"2277ca6a-d68a-4d02-8808-ed4195bbf902","resolution":{"observed_at":"2026-08-06T18:28:44.041662Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.729286Z","title":"2022, A&A, 668, A147","venue":null,"work_id":"3cc1acd6-69dd-42ed-8353-6243bd1f1c12","year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.779436Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:7bb198f1bdc0cb41c68e9f5859f0bc012b6b0920234c8e1d4f52e1dce9540b5c","observation_id":"eb67f425-fe62-4cb2-a025-ffca5d23abcf","resolution":{"observed_at":"2026-08-06T18:28:43.833087Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.569119Z","title":"2019, ApJ, 883, 140","venue":null,"work_id":"9cf4edb3-c5c6-4910-89fa-599a42b5985a","year":2019},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.857028Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f244663a3264edac05d0727bc4dbb6432dcb27358374793ce042b5ac79133cae","observation_id":"506c054e-37d3-4cd4-91d3-5d353e3eb450","resolution":{"observed_at":"2026-08-06T18:28:43.652775Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:29.916735Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.916735Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:60cb6e1c955fedf3f07b31abcb85362c87bd33a07786499df7fbbe350dfe9b4c","observation_id":"317553a1-2dcb-49f3-ad14-a1ab45c9d4ee","resolution":{"observed_at":"2026-08-06T18:28:29.916735Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.356312Z","title":null,"venue":null,"work_id":"c58eea8c-a1d8-4c1c-a1e4-7c4847d120e9","year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:29.991869Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:02ca2a14e9c5cb369fb519f7b1e91b4472a475a27d065ec70aac6a898ae4d2a2","observation_id":"9bca1b96-70eb-4876-90cf-70fe77d378b7","resolution":{"observed_at":"2026-08-06T18:28:43.438345Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.205273Z","title":null,"venue":null,"work_id":"b5992db8-1fec-4612-b75c-f8fbfb9f4939","year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.104594Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:3559995ae1fc8a0ef44e3ca1877bbe0bdc72cd51dc41013fb2f584104d7a52d7","observation_id":"8e3062da-b93e-4e81-a274-f6ae732e97c9","resolution":{"observed_at":"2026-08-06T18:28:43.277764Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:30.195496Z","title":"& Ostriker, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.195496Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:09bcb0620ac8f02619833efcc6c0346f2d68f331ba70af1482403f67c011d121","observation_id":"b765fa0e-02c3-4eae-8110-319c7c0afd64","resolution":{"observed_at":"2026-08-06T18:28:30.195496Z","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":"2026-08-06T18:28:30.244793Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.244793Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:722c24f2ad0a03e312467995f49f2f068e73723332ea329345d72bd5ae0bdf4d","observation_id":"f7671414-7bf3-48b8-b3e1-35ba241a900f","resolution":{"observed_at":"2026-08-06T18:28:30.244793Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:43.037068Z","title":"R., Bate, M","venue":null,"work_id":"6bb2eb3e-e5c5-4fbe-ab38-df35b3c9e245","year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.310509Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:d779de48e15020d5cb7085a371d5440e9ab48ee433ed3dd87b5f445cc22d4104","observation_id":"8900f091-71f5-4fe9-bd55-722bb78edb8f","resolution":{"observed_at":"2026-08-06T18:28:43.128208Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:42.852852Z","title":null,"venue":null,"work_id":"b470705b-4c67-4192-a6b1-3f81301c8d7a","year":2019},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.376463Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:7dd2a5007d89e4c59c7346ed4ce8069672aea69eff47accfba3fecba372119d1","observation_id":"fde4e494-b1bd-4fe5-a47b-a443b0ea7019","resolution":{"observed_at":"2026-08-06T18:28:42.933815Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:30.438021Z","title":"2017, ApJ, 846, 7","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.438021Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:3c1c4076f505bd114bdf76ff24119f43c0efef79b0e05e5592deb2d43e31f2d0","observation_id":"80c327f2-8cd8-40c0-8968-2620639870e0","resolution":{"observed_at":"2026-08-06T18:28:30.438021Z","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":"2026-08-06T18:28:30.515214Z","title":"& Yorke, H","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.515214Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:0105707e5a554656c19ac760348cfe31357a2ee71c36aa0fa4eb8343ad995b60","observation_id":"1f5f2a5a-b3aa-42b7-bbd5-d97c1d452b08","resolution":{"observed_at":"2026-08-06T18:28:30.515214Z","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":"2026-08-06T18:28:30.653965Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.653965Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:5ea471476e6985ff1003ad5053652e6bf149a880e3b7a65e1f6ccde313721d79","observation_id":"c9369ca8-7827-4c03-8921-fffdf426c999","resolution":{"observed_at":"2026-08-06T18:28:30.653965Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:42.603855Z","title":"B., Grudi´c, M","venue":null,"work_id":"be2b0e92-6fa0-4fcc-a256-1d438cec612e","year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.709078Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:d2211eccdc779eb04e0efcf6154e1a370ca9feb7b1681f9d824ea0cfd69a2615","observation_id":"4a616184-9ab7-4daa-aef8-ba0b28689c55","resolution":{"observed_at":"2026-08-06T18:28:42.722272Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:30.801504Z","title":null,"venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.801504Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:88ce5d8bf584c6d0228bc8a8c82be0b82c9a89f885a975f95921925fbff2dc96","observation_id":"01ba4e61-7326-4a59-8199-9cf5211d051b","resolution":{"observed_at":"2026-08-06T18:28:30.801504Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:42.476109Z","title":"2021, ApJ, 917, L10","venue":null,"work_id":"3d6939e7-e360-40a1-91cc-43c521724423","year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.892678Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:827b78a4ced3107d423d77bbbd833f1abc770e2f23ce0ab76a9a65ea572c6add","observation_id":"95078a85-fb85-42b4-9bd7-5cd0fd5cb631","resolution":{"observed_at":"2026-08-06T18:28:42.532450Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:30.956709Z","title":"2023, MNRAS, 518, 3326","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:30.956709Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:fc88263baeb958be6567707fc71622880bbbe6a9c65dd0231eba50b37f74d0b8","observation_id":"00834946-b473-4fa3-8e6f-599a5077d8ad","resolution":{"observed_at":"2026-08-06T18:28:30.956709Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:42.255049Z","title":"& Hennebelle, P","venue":null,"work_id":"9d9074e4-d7de-4be0-866f-6e4638a37a01","year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.054907Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f69731e2378999be3c50eeb775e9ad2950927b312a2dfe153e6d50b33c06f5b1","observation_id":"9da1607b-7070-47ce-bd46-f09f2507b9c9","resolution":{"observed_at":"2026-08-06T18:28:42.361556Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:42.105108Z","title":"2010, ApJ, 720, L26","venue":null,"work_id":"0d927cb6-b566-4cda-b849-1e1e6a403b9f","year":2010},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.105372Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:f33a677f28093c117502f3184702a0c66b5fb465f5d93d84f16d4f7139fb8e58","observation_id":"fd7d94b5-a96f-47db-97a6-5a5303d1ac10","resolution":{"observed_at":"2026-08-06T18:28:42.184062Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.939894Z","title":"2021, A&A, 653, A157 Article number, page 16 of 18 Lebreuilly et al: Rosetta Stone","venue":null,"work_id":"e74bcfd3-d3df-4e15-af5f-4aa62f09cc99","year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.185728Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:57227cd87ef1201190fc0ec709a07988976afd58bec6607073d4c932bd1ea28e","observation_id":"0fa686fe-ea1b-4b95-b2f3-0db59fc1b0ad","resolution":{"observed_at":"2026-08-06T18:28:42.024891Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.728032Z","title":null,"venue":null,"work_id":"d81c7cdd-8898-4f92-8c3b-40a884f32f87","year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.273274Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:965b72b362984a2cb2d2d02bae1771cfa4ea30c7c7774e3f2debe7f0ea582c2f","observation_id":"7c0e8f16-fa93-4865-a2b0-a1851b0d5652","resolution":{"observed_at":"2026-08-06T18:28:41.809833Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.589133Z","title":"S., Federrath, C., & Seta, A","venue":null,"work_id":"9b29ecda-e062-491f-889d-3e056f0fef0a","year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.327335Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:c749eee7b94df94937829e849fc3575cf2ef3ba50c0220dd24d6bd7eb35cef53","observation_id":"b4945a5f-1162-4191-864d-538870957b45","resolution":{"observed_at":"2026-08-06T18:28:41.664580Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.452307Z","title":"J., Girart, J","venue":null,"work_id":"88d9deb3-76e6-4754-a3c5-ddfcda210f38","year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.415920Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:c2533e5ea5a6d5c2b08ed6d908c77f82ba1af358ed49bd6c25c3c4011bd16ca9","observation_id":"3bc2c1c1-ff4b-45a3-b26d-fcf5f362b643","resolution":{"observed_at":"2026-08-06T18:28:41.516779Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:31.512273Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.512273Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:5942c5cc6adc6e205939283288cd7349d23ad74ce3c3221d94b057d390f67ec8","observation_id":"aca97b1e-52a9-48f1-af0d-ee197ba6abdc","resolution":{"observed_at":"2026-08-06T18:28:31.512273Z","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":"2026-08-06T18:28:31.570392Z","title":"P., Waters, B., Schiebel, D., Young, W., & Golap, K","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.570392Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:026d61b2b21741d0ec155726287785dccc715c1a39ef2743aece93b1affd9d08","observation_id":"ab671f59-48e6-4729-8962-a175ce8e3160","resolution":{"observed_at":"2026-08-06T18:28:31.570392Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.287465Z","title":"1966, MNRAS, 133, 265","venue":null,"work_id":"c1d2808c-517a-42aa-b972-780a4551d22e","year":1966},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.649664Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:ad58e04bf764edb0caaf5c0ddea43c83709033d1be710ecdd24520694b1d3eda","observation_id":"0cc1174c-3273-4244-bf7d-4c08b91d6c69","resolution":{"observed_at":"2026-08-06T18:28:41.364980Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:31.694109Z","title":"2007, ApJS, 170, 228","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.694109Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:8a384adbdd7217bc1606a6b275ca4fd63fa9a92af96fd1fe9cb0f4f5651a1a46","observation_id":"fab61d88-e390-4385-90ce-3b899f487883","resolution":{"observed_at":"2026-08-06T18:28:31.694109Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:41.145671Z","title":"F., & Springel, V","venue":null,"work_id":"83f1d5e3-28af-4447-bd34-b823e4ebde99","year":2017},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.764074Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:5bf23f38ae26a01489298956743a0804d31d361ab8db062300ddb546f7f920f5","observation_id":"2e3858f3-6968-4b94-a13d-8300f6fa20fd","resolution":{"observed_at":"2026-08-06T18:28:41.218023Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:31.836023Z","title":"2016, ApJ, 826, L8","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.836023Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:0d3c88db971a7b844d73d7576f1f5663cf72aea8931570aedafa7b363f0691cb","observation_id":"4329f597-e508-48bc-a2f4-f6bb3ac5239a","resolution":{"observed_at":"2026-08-06T18:28:31.836023Z","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":"2026-08-06T18:28:31.930186Z","title":"2025, A&A, 696, A149","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:31.930186Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:70a6d7677693cb88ae492f64dd52fd586af2ef86060928205bc84791a2895a63","observation_id":"d426de7e-83d8-4ed0-9df8-6ae912f08a26","resolution":{"observed_at":"2026-08-06T18:28:31.930186Z","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":"2026-08-06T18:28:32.000356Z","title":"2022, A&A, 662, A8","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.000356Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:808bce7fec04e46fd64967b945c4018deaa3843be6634112c0e4e3f3c4fe389c","observation_id":"e584307e-7461-462f-aaa2-03303b7553ff","resolution":{"observed_at":"2026-08-06T18:28:32.000356Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.978452Z","title":"2018, ARA&A, 56, 41","venue":null,"work_id":"2cbc2157-7a63-4d2d-9389-b394d1f3ec9c","year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.062112Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:ea92640eb7007c07835e08c94b24373260ee58852f1c562b1b1dfe1e083cb4cc","observation_id":"bf97a241-7412-46e6-9cfa-b2befb3e4904","resolution":{"observed_at":"2026-08-06T18:28:41.060195Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.750802Z","title":"G., Federrath, C., & Krumholz, M","venue":null,"work_id":"d66faec7-f360-4538-96cd-89ad4d1a3753","year":2021},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.123418Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:d201386d5254bea56ca6182d1b02b41ad0c917838d1a203d402bf1ca6ff6fe37","observation_id":"c0d3938b-3048-4620-82a6-dec1dfee7a59","resolution":{"observed_at":"2026-08-06T18:28:40.874315Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.605938Z","title":null,"venue":null,"work_id":"60f9fdd9-3ea5-4e4e-a3b6-263a6c066815","year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.195152Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:414b6590ffff2c5cd75a9b053892859d6ed4b9d0f55a382403626bb9c4dc14e7","observation_id":"97c5ff89-ee60-412b-a6b9-933d219dc944","resolution":{"observed_at":"2026-08-06T18:28:40.678156Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.471413Z","title":null,"venue":null,"work_id":"6d499794-e62e-4b18-8e57-d435f125e181","year":2008},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.257131Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:0c64aed19a17f5b590f32032e17af821a261b6ca5bc7a8f48955c6fd84c3ef5c","observation_id":"15aa609f-aa43-446c-85c4-f51ea513f2df","resolution":{"observed_at":"2026-08-06T18:28:40.545994Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.288188Z","title":"& Kuiper, R","venue":null,"work_id":"ac22c823-3cb7-4720-837d-b6652d1628b7","year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.341504Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:56e3d1031410e32357a10940c6e018857114639892d65c1fb1a536a1839daec1","observation_id":"8248e3b8-477c-4556-9ef1-2cd0c137d25b","resolution":{"observed_at":"2026-08-06T18:28:40.363367Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:40.042089Z","title":"2020, ApJ, 900, 82 Pencil Code Collaboration, Brandenburg, A., Johansen, A., et al","venue":null,"work_id":"fdd2c227-b0d5-4068-9ca5-76d54ac7726f","year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.407357Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:56ea7b9d36a0116bd790b621283b448324c9f74d3fe3f60b65dc1776427b5022","observation_id":"6e8180a2-8b71-490a-a37c-3bc12543d8a9","resolution":{"observed_at":"2026-08-06T18:28:40.154156Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:39.844039Z","title":"2006, A&A, 459, 797 Portegies Zwart, S","venue":null,"work_id":"90d7cab9-a839-4208-a2d9-17b764d63cbc","year":2006},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.479401Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:8c1ff789477e68f4ba19f98d026179db4d735e36d30a59293daa15bfc15c50ab","observation_id":"ed03b57f-1a2a-4bd1-a9c0-6823de395b72","resolution":{"observed_at":"2026-08-06T18:28:39.940609Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:32.530466Z","title":"J., Wurster, J., Tricco, T","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.530466Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:7251e31ca81821d6169cea3b6daceb407093b4efa00af5b973ace73340a53d24","observation_id":"e5b965d9-f57b-49b1-999f-eab89cab9769","resolution":{"observed_at":"2026-08-06T18:28:32.530466Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:39.661792Z","title":"2016, A&A, 593, A87","venue":null,"work_id":"eb69fa96-2360-498f-8170-08f4be82d540","year":2016},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.584308Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:ee40b86c8740568f21e658480cd41ecb1a89244aea113e4efe172f1c163fb2dd","observation_id":"f8331b75-b056-4c6f-b559-cd06f0ac3af1","resolution":{"observed_at":"2026-08-06T18:28:39.750229Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:39.450222Z","title":"2013, MNRAS, 436, 1836","venue":null,"work_id":"2f839a64-dc98-4ac2-8dd7-6993d57e8404","year":2013},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.636141Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:ed660df67d928fd9eb3c8fbf8062559930f642a7ab8e3163bbe46d490847c2d0","observation_id":"0be0bec0-172f-4012-92a3-503ed6aca295","resolution":{"observed_at":"2026-08-06T18:28:39.563690Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:39.288417Z","title":null,"venue":null,"work_id":"f45e14b4-cec8-4d19-b68b-8dee82e52bf6","year":2022},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.695249Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:e183c845c51b04fd428673829ea071120678e3b15fca0241f5b523b7a398b062","observation_id":"23377de3-1210-4bb9-808e-92b47a6ffb2a","resolution":{"observed_at":"2026-08-06T18:28:39.376466Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:39.115393Z","title":"2019, ApJ, 886, 102","venue":null,"work_id":"eb50ea15-c0b0-4ad0-8187-5d29d17b1581","year":2019},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.779143Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:affeb1fcfe908e6441b0a4acb302ad386857d69059d916e17c2216a6e5301e47","observation_id":"b963f4f1-77e4-4f29-a34f-0e09596fe9e0","resolution":{"observed_at":"2026-08-06T18:28:39.204225Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.952676Z","title":"2017, MNRAS, 472, 4797","venue":null,"work_id":"ddeaa8ce-1cdc-4e8b-88c3-051f25b9c8ac","year":2017},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:32.902840Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:a672fbc358822ea8b7ee077beb93853fb2077be004be70db3b520a86f17f5711","observation_id":"e2091211-8e14-4a71-b79b-7dfee4c92fa7","resolution":{"observed_at":"2026-08-06T18:28:39.057928Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.777561Z","title":"J., Treß, R","venue":null,"work_id":"35295f3b-3925-406c-a016-4dd21e7de546","year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.006117Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:64aedda96e0c19c0b25efd04f782c08b042b2d8d01fe9532513f2c92a9ed367e","observation_id":"99055009-8e11-471c-8e5f-aefe27ede914","resolution":{"observed_at":"2026-08-06T18:28:38.852837Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:33.079520Z","title":"2010, MNRAS, 401, 791","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.079520Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:0c03040df7543d51aadae22bd4b49597ea43f72854f58208ac43dd1fc8db44cb","observation_id":"d62237cc-3f02-4885-a43e-e20e6467d7fd","resolution":{"observed_at":"2026-08-06T18:28:33.079520Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.612436Z","title":"2024, A&A, 682, A76","venue":null,"work_id":"8ca039e1-52b0-4db9-9cb9-4273413faeab","year":2024},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.171528Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:a8e9ec77f56b2efd15dcae5f42b16075e4c609eee5c9356a6990865a7d79b37d","observation_id":"d09c1783-9e43-44f2-9d8f-bf7070b13332","resolution":{"observed_at":"2026-08-06T18:28:38.672917Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:33.290076Z","title":"E., Shirley, Y","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.290076Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:7ab63c94ead35c0afccdb3467c18f2d7c8323a5bb71a10d29214afc16f62e4da","observation_id":"20e8d162-3bbe-4072-a630-315dd0fded88","resolution":{"observed_at":"2026-08-06T18:28:33.290076Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.463867Z","title":"C., Beltrán, M","venue":null,"work_id":"a99d87ed-65f2-4e15-8aeb-009242208f0a","year":2014},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.391015Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:3da5a8bd25b51177d426d69f4d79631b000b19234c9684d8d0636c41d3fd4bb3","observation_id":"4c592b99-37cd-4354-807f-cb6c2ad11ee1","resolution":{"observed_at":"2026-08-06T18:28:38.553478Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:33.485651Z","title":"2002, A&A, 385, 337","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.485651Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:c8c6a92e8049391124f6a5d2b1cfc5db75e0d705a63c5cf25639bc9175db55bf","observation_id":"1e73376d-7370-4011-89b7-c09cd1231a00","resolution":{"observed_at":"2026-08-06T18:28:33.485651Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.227352Z","title":"& Galli, D","venue":null,"work_id":"51b8e6c7-c24e-4580-801f-e6b43fb0c4a2","year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.560025Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:fa050b3bdedf5b4d02ab1c9c59aa4d96faffa363a8a9b55f486471767fda6b98","observation_id":"bc4802aa-d90f-48fc-b62d-dccaaa33e1ab","resolution":{"observed_at":"2026-08-06T18:28:38.332309Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:38.081920Z","title":"2020, ApJ, 888, L4","venue":null,"work_id":"ba9d981c-6dd9-4698-a6f6-3a7e9a7838c5","year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.630145Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:65825f84b2df9c93b46f84bc7a8ded56971b99f5282c7dffa9089cd3537e197c","observation_id":"2baa30c0-6df9-4e6b-9ab1-e14b25e709bc","resolution":{"observed_at":"2026-08-06T18:28:38.160754Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:33.706152Z","title":"2013, ApJ, 763, 6","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.706152Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:25a74935f4ecc8efec3bd872980807b4556735c056f2b74340622ad586a7ddb6","observation_id":"96dc3fe0-47d1-4e26-934e-18f51cefa7eb","resolution":{"observed_at":"2026-08-06T18:28:33.706152Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:37.906845Z","title":"2018, MNRAS, 477, 2220","venue":null,"work_id":"8aeb03c1-5dba-4926-882e-e556d23052fd","year":2018},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.819699Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:1a7520eab97ac2ade2d95179444683999cbe81d8f912f3429be61ef03ee467e9","observation_id":"08c0bf08-d4cd-4fc2-9c10-217986a15d04","resolution":{"observed_at":"2026-08-06T18:28:38.013921Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:37.689757Z","title":"A., Billot, N., et al","venue":null,"work_id":"8a517b0d-57e3-49f8-897b-f80b85fb464f","year":2017},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:33.945758Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:56c3161f78626ff57ed9cf9c69a863d968e90eae5cfa3def75c33925e2cfb373","observation_id":"bc63c34a-37c2-4348-b080-133cf5ced5ae","resolution":{"observed_at":"2026-08-06T18:28:37.784100Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:28:37.521141Z","title":"A., Peretto, N., Pineda, J","venue":null,"work_id":"feebdb44-d67b-4548-b309-954069d1fa79","year":2015},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:34.035268Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:350257a5e77c4d53dc25a09ab39528b8b022a5d4fcb72d9ec822d1ec35b94c93","observation_id":"dfbad3f7-99d8-4295-8323-4e8c129ed279","resolution":{"observed_at":"2026-08-06T18:28:37.576547Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T18:28:34.084178Z","title":"M., Avison, A., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:34.084178Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:efe871e621df62796a0a4823fd225c93a4bc0369ffd6a7647160c45ea2d2d1b5","observation_id":"b80e2e3c-6ada-4c6c-a790-fe96a3417859","resolution":{"observed_at":"2026-08-06T18:28:34.084178Z","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":"2026-08-06T18:28:34.166334Z","title":"G., Sormani, M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:34.166334Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:aa3ead3c83985cdee5091aa263939bd05ed9f7a1e9ab4d9cfbc7d8e0d86b712c","observation_id":"f051633a-e6a2-4fbc-bb30-d80e4c528753","resolution":{"observed_at":"2026-08-06T18:28:34.166334Z","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":"2026-08-06T18:28:34.261669Z","title":"K., Klein, R","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T18:28:34.261669Z"},"links":{"citing_paper":"/paper/2507.08436"},"observation_digest":"sha256:66c9f40197b8d22fd76119520411e67a5866d9237239b3cd9cb3bc84b06d3a33","observation_id":"9695b603-3196-476b-ae88-f14ffc627840","resolution":{"observed_at":"2026-08-06T18:28:34.261669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.08436","last_updated":"2025-07-17T07:50:15Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-06T18:16:27.541551Z","submitted_at":"2025-07-11T09:28:57Z","title":"The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":66,"verified_exact":0,"verified_fuzzy":34},"total_outbound_references":113},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 100 of 113 outbound references and 2 inbound Pith citation observations for arXiv:2507.08436."}