{"as_of":"2026-08-11T01:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4efbccb895ea45842b05734295422a5d8982a353e31f9b59b32da15d415a4497","coverage":[{"denominator":72,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":72,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T10:54:11.187850Z","state":"measured"},{"denominator":72,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":72,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/2501.16770/citation-record","integrity":"/paper/2501.16770/integrity","json":"/paper/2501.16770/citation-record.json","paper":"/paper/2501.16770"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:10.999236Z","title":"A bright millisecond radio burst of extragalactic origin","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:10.999236Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:87d24e055afc6d9d66f2db3fcf07323491733ec31f0b89e66d5b78bcd2df60ce","observation_id":"3197aa65-6b3d-464a-959c-186ccdbe95a2","resolution":{"observed_at":"2026-08-10T10:54:10.999236Z","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":"2026-08-10T10:54:11.002725Z","title":"The baryon census in a multiphase intergalactic medium: 30% of the baryons may still be missing","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.002725Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:df31cf6b49bfbd2791d23174702df9f806147a55446349aa7f0192d59f324afa","observation_id":"e3ab2ad6-d10d-44ec-870a-b49e760cae07","resolution":{"observed_at":"2026-08-10T10:54:11.002725Z","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":"2026-08-10T10:54:11.005571Z","title":"A huge reservoir of ionized gas around the Milky Way: accounting for the missing mass? The Astrophysical Journal Letters 2012, 756, L8","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.005571Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:93fd84a0cad9808b60948e404046f94e2fdc8152165ce1e8541797d802676b10","observation_id":"5034bb61-10fa-477b-b3f9-97debaf65e4f","resolution":{"observed_at":"2026-08-10T10:54:11.005571Z","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":"2026-08-10T10:54:11.008636Z","title":"On the hot gas content of the Milky Way halo","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.008636Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:d4a4a08d8b641e589066a49d623731777d1638bf51eb4dca41414f9197894da3","observation_id":"f03a0f45-1f79-41be-88da-f010cbe3ead8","resolution":{"observed_at":"2026-08-10T10:54:11.008636Z","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":"2026-08-10T10:54:11.011135Z","title":"X-Ray Detection of the Galaxy’s Missing Baryons in the Circumgalactic Medium of L* Galaxies","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.011135Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:56686afbad61de91b49b555b66c77ee1ff56664e5e144be3e0558f595487d139","observation_id":"974d09aa-311d-413d-938b-f00bf71cc346","resolution":{"observed_at":"2026-08-10T10:54:11.011135Z","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":"2026-08-10T10:54:11.013341Z","title":"A census of baryons in the Universe from localized fast radio bursts","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.013341Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:b06e644d0d006ecade0b489cf01088eceb4dc407ded70a39c7c958e941c5c2a6","observation_id":"6a371a7a-78df-483f-952d-a559999433f3","resolution":{"observed_at":"2026-08-10T10:54:11.013341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207156","last_updated":"2003-01-28T16:07:00Z","snapshot_observed_at":"2026-07-07T00:27:17.742565Z","submitted_at":"2002-07-08T08:32:31Z","title":"NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207156","snapshot_observed_at":"2026-08-10T10:54:11.015549Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.015549Z"},"links":{"cited_paper":"/paper/astro-ph/0207156","citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:eccf36de2d9a09b0ac8662d34f15bd824f9dabfa96e23b240d4a5ba57631fb77","observation_id":"a3740e27-19b6-46ca-87a8-a81ba3647c11","resolution":{"observed_at":"2026-08-10T10:54:11.015549Z","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":"2026-08-10T10:54:11.017862Z","title":"A new electron-density model for estimation of pulsar and FRB distances","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.017862Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:ca057b3ba1964a61d57ff9ca4fe4456ab28d5261ee790581ac463dd96d5dc92f","observation_id":"9b15b2a6-5697-4049-b79b-23d23212bce9","resolution":{"observed_at":"2026-08-10T10:54:11.017862Z","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":"2026-08-10T10:54:11.019829Z","title":"A comparison of Galactic electron density models using PyGEDM","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.019829Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:c253252cee07acc75ad0c2188ae1d0da0fd474a9a3d0871bfca3ec59f3319a13","observation_id":"8c81a081-e058-459b-81dc-78b8cad00c72","resolution":{"observed_at":"2026-08-10T10:54:11.019829Z","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":"2026-08-10T10:54:11.021814Z","title":"The vertical structure of warm ionised gas in the Milky Way","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.021814Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:eba702cb2541b182bd28580c19e1410d44fbf89e2e7cca7b5a8522634360ac95","observation_id":"c105bab4-296a-4283-bab5-99336aaed7bb","resolution":{"observed_at":"2026-08-10T10:54:11.021814Z","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":"2026-08-10T10:54:11.794461Z","title":"Binary pulsar distances and velocities from gaia data release","venue":null,"work_id":"480104cf-7928-4a94-ad1f-69fbb1f57879","year":null},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.024535Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:fc2dd34c617b96924f136e4241f863dc8f10c11dff56926d2f365628d88f735d","observation_id":"144a311a-35e4-43b2-9c3a-93d25c435ff9","resolution":{"observed_at":"2026-08-10T10:54:11.796527Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.027227Z","title":"https://doi.org/10.3847/1538-4357/aad084","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.027227Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:52737bab4c8f059fd08c3fac201e08168daf22e1f53a2988c63f87081a270351","observation_id":"acb3b6c9-66e3-4e8a-9352-016097180798","resolution":{"observed_at":"2026-08-10T10:54:11.027227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ab930a","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.444495Z","title":"A data-driven technique using millisecond transients to measure the milky way halo","venue":null,"work_id":"9c4e2aad-2cb2-4486-8ee9-12681eec520c","year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.030253Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4f71c3f8ba203301c5426ca1413cafd6d00ddebede96c2f953d858669c26b791","observation_id":"eb3cc7f8-d208-4017-a634-8239efa67bda","resolution":{"observed_at":"2026-08-10T10:54:11.447792Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.033334Z","title":"An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.033334Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:70b653293180f31e4e02d494743bfd60dab56e63a998b74d664d087a65d7382e","observation_id":"9a8d4dec-af2e-42f8-a4a9-3e1983f61c46","resolution":{"observed_at":"2026-08-10T10:54:11.033334Z","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":"2026-08-10T10:54:11.035941Z","title":"Investigating Cosmological Models and the Hubble Tension Using Localized Fast Radio Bursts.The Astrophysical Journal 2023, 955, 101","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.035941Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:39cc4901ada71a1db962e090696411f10acaf5dfe7fa89800ef5bdc408b9c0dc","observation_id":"44c337eb-f9f7-4184-8727-574fdde2864f","resolution":{"observed_at":"2026-08-10T10:54:11.035941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.22098","last_updated":"2024-10-30T07:17:21Z","snapshot_observed_at":"2026-07-06T19:41:32.754401Z","submitted_at":"2024-10-29T14:51:39Z","title":"Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.22098","snapshot_observed_at":"2026-08-10T10:54:11.038820Z","title":"Modeling the Cosmic Dispersion Measure in the D< 120 Mpc Local Universe","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.038820Z"},"links":{"cited_paper":"/paper/2410.22098","citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7127b1aefac8e2edeac19ae3a8ac0b332eadf15d54eabdb674d31bb3b0297d30","observation_id":"1485ca8c-3dd2-4638-8512-6471ce868cb6","resolution":{"observed_at":"2026-08-10T10:54:11.038820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/pasj/59.sp1.s141","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.423790Z","title":"Suzaku observations of the local and distant hot ISM","venue":null,"work_id":"4ffc2df1-80c2-4c7c-9783-f6ddd0e2069f","year":2007},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.042052Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:9b1d93c84ec3c28d3f68f4fb9fcac3bda321cccbcb221de81c2011a04a2f23b0","observation_id":"1aaf32dd-2daf-4373-9d3f-786074002bfd","resolution":{"observed_at":"2026-08-10T10:54:11.426699Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.044602Z","title":"An XMM-Newton survey of the soft X-ray background","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.044602Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:860c391aa78fc8b862fcdffe3d2037a5bd909c263e1b29799f77a3d48e3bd107","observation_id":"33a016dd-cb43-4353-a759-4b3a608864e3","resolution":{"observed_at":"2026-08-10T10:54:11.044602Z","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":"2026-08-10T10:54:11.788307Z","title":"Observations of the missing baryons in the warm–hot intergalactic medium","venue":null,"work_id":"69711d0d-396c-44ca-bdde-9409fed78ecf","year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.047174Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4f33664a90810dd39a4af5a3b69b21fd9b6ae7e1ce6b98d4717a1fdd0ac38c93","observation_id":"e959d675-5c9c-42d7-a0a8-8a239c29a3e7","resolution":{"observed_at":"2026-08-10T10:54:11.790442Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.049628Z","title":"Blinkverse: a database of fast radio bursts","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.049628Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7e20474093f0a450c112c8489d4297aa3a08bcf26f562aec9d7173f4d08a7c98","observation_id":"9d7727d0-2817-4534-a1c6-a74c8a0bbb71","resolution":{"observed_at":"2026-08-10T10:54:11.049628Z","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":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.764680Z","title":"The NASA astrophysics data system: Overview","venue":null,"work_id":"e82f5934-370f-4480-b0c4-b3607147efb5","year":2000},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.052440Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:0647906d08122f26a47917c6ee55d65755d20cdf1d55aca0f99d5e37c11b78de","observation_id":"725dbabc-7642-4aaf-9c40-13d58b3e0e87","resolution":{"observed_at":"2026-08-10T10:54:11.768252Z","resolver_source":"arxiv_id_nonexistent","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.054944Z","title":"The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.054944Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:a986ac7453d9fca78045ab83312bbbe70e677a01f918252d3eb27fcee91928d8","observation_id":"fe585b9f-3cef-4902-8316-c224614bca1a","resolution":{"observed_at":"2026-08-10T10:54:11.054944Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-10T10:54:11.057544Z","title":"A repeating fast radio burst associated with a persistent radio source","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.057544Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:0ee353875ae62c7a97b3ab1bbda7e3925c93eed7f910638adf902c8fd8e88545","observation_id":"a704c4d6-222c-4eb1-b41c-9359623dd53c","resolution":{"observed_at":"2026-08-10T10:54:11.057544Z","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":"2026-08-10T10:54:11.782452Z","title":"A Nonrepeating Fast Radio Burst in a Dwarf Host Galaxy","venue":null,"work_id":"6ad16da5-486e-4b7c-9aad-ed79a9976a9d","year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.060021Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7c279a6b582d60c74648e8b608ea789fe55bbc98489384d16792ac444c06ef8a","observation_id":"e7c95fe6-b001-4447-9734-5be1c44f0c79","resolution":{"observed_at":"2026-08-10T10:54:11.784572Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.774444Z","title":"A luminous fast radio burst that probes the Universe at redshift 1","venue":null,"work_id":"46df40ff-92bc-4221-97b4-ec10b881c95f","year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.062419Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:e0afc9861bb38769234461c80ec59622fa0baeaa70325f895fdb76f349c9e8c6","observation_id":"e8e8c3da-4ab6-4137-9654-a13975e9e605","resolution":{"observed_at":"2026-08-10T10:54:11.777432Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.064956Z","title":"Deep Synoptic Array science: Two fast radio burst sources in massive galaxy clusters","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.064956Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:dffcfe789c3584901024ba21085edcafab0a4d074ed112f0f2be5a125391d32f","observation_id":"bb6744ab-e3e9-4286-b482-7d648a485b20","resolution":{"observed_at":"2026-08-10T10:54:11.064956Z","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":"2026-08-10T10:54:11.067721Z","title":"Redshift estimation and constraints on intergalactic and interstellar media from dispersion and scattering of fast radio bursts","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.067721Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:f18c897d647509f0d2aea285ad21d94a3f01aa641010a80cdad9564b8838dbf1","observation_id":"805eb5e6-2e11-43d7-9cf5-dd981d34d56c","resolution":{"observed_at":"2026-08-10T10:54:11.067721Z","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":"2026-08-10T10:54:11.071440Z","title":"The host galaxy and redshift of the repeating fast radio burst FRB 121102","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.071440Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:75d56ad93466be1113e216aa7b97a9083c09b10256aeb5328574ef7a3da9f419","observation_id":"6b99d5f8-bf00-4df4-a8de-18c32d329061","resolution":{"observed_at":"2026-08-10T10:54:11.071440Z","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":"2026-08-10T10:54:11.074888Z","title":"The host galaxy of FRB 20171020A revisited","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.074888Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4553cb56d0cce59003204abf95a3ee3b837722b76960358b4ded58cac25e8df2","observation_id":"7a7aada8-8cf3-4fe1-8ae2-135f38f8c9b8","resolution":{"observed_at":"2026-08-10T10:54:11.074888Z","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":"2026-08-10T10:54:11.077518Z","title":"Characterizing the fast radio burst host galaxy population and its connection to transients in the local and extragalactic universe","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.077518Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:cdbe8c2835121d8676e1d25a329d1732759c13290eecace43f3a5e8f6f888faf","observation_id":"f0144607-0394-4861-8e45-27f1ffdb8f8c","resolution":{"observed_at":"2026-08-10T10:54:11.077518Z","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":"2026-08-10T10:54:11.080837Z","title":"A repeating fast radio burst source localized to a nearby spiral galaxy","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.080837Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7cbad5b3d13ea56fb35adbe690a1a844dc8345fc08c126e45bbccf2095daa668","observation_id":"70d7fef1-5c7a-4e7d-8ffe-774d373e94d8","resolution":{"observed_at":"2026-08-10T10:54:11.080837Z","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":"2026-08-10T10:54:11.084528Z","title":"A single fast radio burst localized to a massive galaxy at cosmological distance","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.084528Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:be8ccc7a117524672c14e8d0d4a8cc7d40c11e682b8d8336445a8786f010b37d","observation_id":"0e3f6455-f5b9-4eb7-8952-7427dafb8524","resolution":{"observed_at":"2026-08-10T10:54:11.084528Z","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":"2026-08-10T10:54:11.087389Z","title":"A local universe host for the repeating fast radio burst FRB 20181030A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.087389Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7063bdc1f0684f39aa36b76dba0431aeaa24367be2ac4ca9f9932e7edbc0dac5","observation_id":"971bf79f-16ed-425f-ad25-cbc8d009fec0","resolution":{"observed_at":"2026-08-10T10:54:11.087389Z","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":"2026-08-10T10:54:11.090428Z","title":"The low density and magnetization of a massive galaxy halo exposed by a fast radio burst","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.090428Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:32f6af4e9e33c8dd278cd5c4806c253324aeb9e67f638551e111e5a0b539ae81","observation_id":"0dbf5a3c-96be-4973-9daf-3695166d6b26","resolution":{"observed_at":"2026-08-10T10:54:11.090428Z","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":"2026-08-10T10:54:11.092378Z","title":"Host galaxies for four nearby CHIME/FRB sources and the local universe FRB host galaxy population","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.092378Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4aaa22edd0893a771699b95ace518a477bdcf37655d47fa5a80ff41935ad5e01","observation_id":"8440749f-ede9-417c-8836-cae06452d730","resolution":{"observed_at":"2026-08-10T10:54:11.092378Z","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":"2026-08-10T10:54:11.094447Z","title":"A fast radio burst localized to a massive galaxy","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.094447Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4f062aadd20361a7c4f4144a8787edb0a9afcd6722417b1ca19944e77c9a9e97","observation_id":"e1de9e7f-1e0f-464f-bd3c-89f025b5332c","resolution":{"observed_at":"2026-08-10T10:54:11.094447Z","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":"2026-08-10T10:54:11.096527Z","title":"Host galaxy properties and offset distributions of fast radio bursts: implications for their progenitors","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.096527Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:721056e88fe90e9daf5d82cbea62099c0b756b81a09d90aa26adc78dfe017a7b","observation_id":"1ae6eee3-8355-41f4-8381-0d639cdcef3d","resolution":{"observed_at":"2026-08-10T10:54:11.096527Z","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":"2026-08-10T10:54:11.098536Z","title":"A repeating fast radio burst source in a globular cluster","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.098536Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:475fc990e8a563b61353749dc6071e465557a323db25e1bee08541a68d35d823","observation_id":"056dcb21-2993-4393-a585-08511c984966","resolution":{"observed_at":"2026-08-10T10:54:11.098536Z","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":"2026-08-10T10:54:11.100559Z","title":"First discoveries and localizations of Fast Radio Bursts with MeerTRAP: real-time, commensal MeerKAT survey","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.100559Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:468b50497187ab41c27fc8c210cd4968c9467dd559a0b6de47d5ada34a699758","observation_id":"eb6e08dc-6e91-4193-a47e-016bf0ddd3ce","resolution":{"observed_at":"2026-08-10T10:54:11.100559Z","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":"2026-08-10T10:54:11.102439Z","title":"Chronicling the host galaxy properties of the remarkable repeating FRB 20201124A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.102439Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:a2243aeb061108f70cc2e2ee32d4d930ad956dd9945daac15bb532bcaa1c6e36","observation_id":"f4f0888f-935b-40e7-9886-39e98800ebd7","resolution":{"observed_at":"2026-08-10T10:54:11.102439Z","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":"2026-08-10T10:54:11.104266Z","title":"The Demographics, Stellar Populations, and Star Formation Histories of Fast Radio Burst Host Galaxies: Implications for the Progenitors","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.104266Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:94b3d04d461b8aae903fbf367520d40dc021a8603a8b8d30ffd3985964999096","observation_id":"b9d04ad4-2fc0-4866-b46b-e8727f554d9a","resolution":{"observed_at":"2026-08-10T10:54:11.104266Z","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":"2026-08-10T10:54:11.107674Z","title":"FRB 20210405I: a nearby Fast Radio Burst localized to sub-arcsecond precision with MeerKAT","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.107674Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4b55d9506061626244709dbc2232b6d49a070b9a5aa4db171e2ae1e178650eff","observation_id":"04b81927-ab17-4eb9-af57-37457dc11699","resolution":{"observed_at":"2026-08-10T10:54:11.107674Z","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":"2026-08-10T10:54:11.110543Z","title":"A subarcsec localized fast radio burst with a significant host galaxy dispersion measure contribution","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.110543Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:6e5e55ec69cc87095119d19256b56ecc9633a6cd8afad5b5bc9bd7bbcd9363eb","observation_id":"456df331-7f99-44d7-a447-78cf69aa6f3a","resolution":{"observed_at":"2026-08-10T10:54:11.110543Z","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":"2026-08-10T10:54:11.113129Z","title":"WALLABY Pilot Survey: H i in the Host Galaxy of a Fast Radio Burst","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.113129Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:c3bb8d1f917fc9283330c19984b0372fe5eb8db3ffe12bb91b70dee0cf955b9b","observation_id":"9d018519-d116-4b5c-8646-72660f8f5768","resolution":{"observed_at":"2026-08-10T10:54:11.113129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03344","last_updated":"2024-01-24T20:19:49Z","snapshot_observed_at":"2026-08-09T18:02:52.367638Z","submitted_at":"2023-07-07T01:19:46Z","title":"Deep Synoptic Array Science: First FRB and Host Galaxy Catalog","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03344","snapshot_observed_at":"2026-08-10T10:54:11.115818Z","title":"Deep Synoptic Array Science: First FRB and Host Galaxy Catalog","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.115818Z"},"links":{"cited_paper":"/paper/2307.03344","citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:37ec21d8da7f01c59c96a26bc4ef6a4be93708b5d5c27e601d7973e35667e7df","observation_id":"3d79c687-44b3-47a9-9b0a-4a02c5e2c3c1","resolution":{"observed_at":"2026-08-10T10:54:11.115818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.01000","last_updated":"2023-01-03T08:23:40Z","snapshot_observed_at":"2026-07-06T14:36:57.323236Z","submitted_at":"2023-01-03T08:23:40Z","title":"Deep Synoptic Array science: a 50 Mpc fast radio burst constrains the mass of the Milky Way circumgalactic medium","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.01000","snapshot_observed_at":"2026-08-10T10:54:11.119288Z","title":"Deep Synoptic Array science: a 50 Mpc fast radio burst constrains the mass of the Milky Way circumgalactic medium","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.119288Z"},"links":{"cited_paper":"/paper/2301.01000","citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:e233c3804a46e23571e7c8e6d59dac85a563e6dc17204346e68fff45226eccf0","observation_id":"656f910f-c139-4cc9-8f6f-f1680f6a3a4b","resolution":{"observed_at":"2026-08-10T10:54:11.119288Z","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":"2026-08-10T10:54:11.122195Z","title":"Deep Synoptic Array Science: Discovery of the Host Galaxy of FRB 20220912A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.122195Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:3b80ad51030913a0e84b78cc19f91b014b5314ac915f73c8bb692c5420d38cfa","observation_id":"6d1ab5f3-e6a3-4b86-8ba0-adb64d5d3444","resolution":{"observed_at":"2026-08-10T10:54:11.122195Z","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":"2026-08-10T10:54:11.125360Z","title":"H i, FRB, What’s Your z: The First FRB Host Galaxy Redshift from Radio Observations","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.125360Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:01581b454967d19e96bd4a05f326595ddcfc2acc292e294fca5ed5f5b97f9d98","observation_id":"aa678ff7-1c9f-4a59-97a4-2016be29b276","resolution":{"observed_at":"2026-08-10T10:54:11.125360Z","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":"2026-08-10T10:54:11.128248Z","title":"XMM-NEWTON SURVEY OF LOCAL ABSORPTION LINES IN THE SPECTRA OF ACTIVE GALACTIC NUCLEI","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.128248Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:6609dae246e7a6ad374e2d95f2e46c7f2a22945b7f3b8cdc2cadcba9e477dd18","observation_id":"ea0d92ba-af04-4d7f-82ca-6c3699c8af2c","resolution":{"observed_at":"2026-08-10T10:54:11.128248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/200912925","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.308655Z","title":"High- resolution X-ray spectroscopy of the Seyfert 1 Mrk 841: insights into the warm absorber and warm emitter","venue":null,"work_id":"9e76d80d-4775-45d0-aa94-84ef9eed7b40","year":2010},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.131212Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:c3e39d97bf9b6172db7992fd02f043c9cd5b240a54e0f008faa115c949e5c562","observation_id":"d4cb42d7-f17d-40eb-973e-7551b8bd0e93","resolution":{"observed_at":"2026-08-10T10:54:11.311650Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.133844Z","title":"Empirical estimates of the Galactic halo contribution to the dispersion measures of extragalactic fast radio bursts using X-ray absorption","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.133844Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:a0c0c64fd6085c6e748a102749bb45976080c36f4fc9ec2c55e2729f80660f77","observation_id":"cbdf062b-635e-4b0d-bdec-e12ccde5b1f8","resolution":{"observed_at":"2026-08-10T10:54:11.133844Z","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":"2026-08-10T10:54:11.136497Z","title":"Fast radio burst energetics and detectability from high redshifts","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.136497Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4d1d2fd03b3178926d92c94fadc7311bcc5431de12f1cee40a7ce8317b08c93a","observation_id":"af3e6487-16c5-4bfe-801c-72d5f6986cef","resolution":{"observed_at":"2026-08-10T10:54:11.136497Z","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":"2026-08-10T10:54:11.140173Z","title":"Studying the WHIM content of large-scale structures along the line of sight to H 2356-309","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.140173Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:d073a48879461a4751c3debf48ffcc133eef0cf5d5833185e4706e215e4dcb4b","observation_id":"7a812791-9420-4072-b4c6-271cb9ab0ade","resolution":{"observed_at":"2026-08-10T10:54:11.140173Z","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":"2026-08-10T10:54:11.142850Z","title":"High resolution X-ray spectroscopy of the local hot gas along the 3C 273 sightline","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.142850Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:ee0173427890b464db6af4d3558d658a16e2e8ee5309fc1a231ae9136501b3fc","observation_id":"1b5460c1-d1c5-4e97-9d9a-66239b966c99","resolution":{"observed_at":"2026-08-10T10:54:11.142850Z","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":"2026-08-10T10:54:11.145390Z","title":"A possible Chandra and Hubble Space Telescope detection of extragalactic WHIM towards PG 1116+ 215","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.145390Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:3df385f0ff65c899740006ce3dbb87eb00955b5c8ec062f64654980ab9f976bc","observation_id":"3980352b-18e2-4894-a8ef-78481ca935a1","resolution":{"observed_at":"2026-08-10T10:54:11.145390Z","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":"2026-08-10T10:54:11.148076Z","title":"Discovery of a very hot phase of the Milky Way circumgalactic medium with non-solar abundance ratios","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.148076Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:a30a1f05d805ee660035032d7f5d0f578fca162cca88e2a5f8538165a390ba25","observation_id":"8669220d-d85e-427e-974d-45605da3a00c","resolution":{"observed_at":"2026-08-10T10:54:11.148076Z","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":"2026-08-10T10:54:11.150717Z","title":"The XMM-Newton Line Emission Analysis Program (X-LEAP)","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.150717Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7802c7819a9b7e54bcef831e4b5b6d1dc12f5f874cf7f0ea384740813d81dca7","observation_id":"0ef15137-84ae-44c3-b53e-9cac77d3858f","resolution":{"observed_at":"2026-08-10T10:54:11.150717Z","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":"2026-08-10T10:54:11.153320Z","title":"A disk-dominated and clumpy circumgalactic medium of the Milky Way seen in X-ray emission","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.153320Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:4bfc1448f61318a23d9acb3c572d2e9573f6a101a1b3ced83f8df426f39ca576","observation_id":"fc62476b-7fd3-4b02-b722-579038aac5ab","resolution":{"observed_at":"2026-08-10T10:54:11.153320Z","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":"2026-08-10T10:54:11.155978Z","title":"The mass of the missing baryons in the X-ray forest of the warm–hot intergalactic medium","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.155978Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:a599feb869085cf46da2a0b00a960d1ea1a95ef3b2d92ebeccd9c38f97aba5f5","observation_id":"f51168a2-e1f7-4179-a09c-61a3dc22840a","resolution":{"observed_at":"2026-08-10T10:54:11.155978Z","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":"2026-08-10T10:54:11.158826Z","title":"X-Ray absorption from the Milky Way halo and the local group","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.158826Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:0b7b0287bee00cc39b37afa1a7486bd53c944048ecd99924f2947beb35a6798e","observation_id":"c864ef7a-892b-4f21-b215-326e304e55d5","resolution":{"observed_at":"2026-08-10T10:54:11.158826Z","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":"2026-08-10T10:54:11.161829Z","title":"The Dispersion of Fast Radio Bursts from a Structured Intergalactic Medium at Redshifts z < 1.5","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.161829Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:babd6510c7299e3a014a53aa50353cd3d115eafa9d451548d0c343a9e51e2957","observation_id":"8d2f1f7c-0ac8-4de8-b156-0ce2582bb51b","resolution":{"observed_at":"2026-08-10T10:54:11.161829Z","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":"2026-08-10T10:54:11.164574Z","title":"Probing Galactic haloes with fast radio bursts","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.164574Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:1eebe58d99588a2a46497438f5e61a226842f0a8267d1ad1734cb82ec5040ab0","observation_id":"4307244c-c9e5-451f-a17f-414c8af7d9e0","resolution":{"observed_at":"2026-08-10T10:54:11.164574Z","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":"2026-08-10T10:54:11.166527Z","title":"The galactic halo contribution to the dispersion measure of extragalactic fast radio bursts.The Astrophysical Journal 2020, 888, 105","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.166527Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:360da0898a5fcfb4d5371e871c46ca468cc81c413783970ef0c205a698e669cc","observation_id":"bf61cea0-72ed-491c-a3da-cef056f7cd5c","resolution":{"observed_at":"2026-08-10T10:54:11.166527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/344509","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.252857Z","title":"Tracing the warm-hot intergalactic medium at low redshift: X-ray forest observations toward H1821+ 643","venue":null,"work_id":"0ff508cc-ccda-4bb9-bc3f-c189ad9428b1","year":2003},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.168469Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:5fe18e93036189889d09a6f3edbe3f13bbda713d4a0d02b003c8829a9630a622","observation_id":"b5a6ea8f-5b14-439c-84f9-6db226f66dbe","resolution":{"observed_at":"2026-08-10T10:54:11.255721Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.170473Z","title":"Probing the local group medium toward Markarian 421 with Chandra and the far ultraviolet spectroscopic explorer","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.170473Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:f95837f2353d521eb7ac8ee7f5c99fc5f3c6be8086247941ba4167246c06eb56","observation_id":"9ef1d8f2-1fda-48b8-90a5-490c720ac65a","resolution":{"observed_at":"2026-08-10T10:54:11.170473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0067-0049/202/2/14","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.241069Z","title":"An XMM-Newton survey of the soft X-ray background","venue":null,"work_id":"1212aef6-a9f7-4761-b946-d7906bb9122c","year":2012},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.172473Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:184332405414a6a86f52c4d09ea880c92e80a93f0e78805559a49e2db36f29cb","observation_id":"e23af73d-668f-45ab-a399-7004d84ec53c","resolution":{"observed_at":"2026-08-10T10:54:11.244119Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.174357Z","title":"The CHIME fast radio burst project: system overview","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.174357Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:5729d2333cbc2f421bc7dce6caf13a0b065c58d88e7b19d33c2b75a41c40ff60","observation_id":"d7ea422b-e451-4450-9456-d62414878301","resolution":{"observed_at":"2026-08-10T10:54:11.174357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnrasl/slx022","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.226241Z","title":"Density and metallicity of the Milky Way circumgalactic gas","venue":null,"work_id":"dd48568e-3150-4dba-ab8b-3002288f0f03","year":2017},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.176327Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:7aa1408064be2e9ff6e7d734ac08a53f7eb0c6590bdb1ebb02808224066e222b","observation_id":"1f97ee9b-3d16-45f1-9636-5b1f5b874c12","resolution":{"observed_at":"2026-08-10T10:54:11.231759Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T10:54:11.178781Z","title":"Constraining density and metallicity of the Milky Way’s hot gas halo from O vii spectra and ram-pressure stripping","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.178781Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:851600c6cce862481b6ceb48f43a4ce8f51cda0c91c55247441b30b2e8e6c287","observation_id":"9dc4af2e-a89e-4bcf-a593-6395be0098ff","resolution":{"observed_at":"2026-08-10T10:54:11.178781Z","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":"2026-08-10T10:54:11.182103Z","title":"Electron density structure of the local galactic disk","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.182103Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:54f88a4af6fa312506b1d0e2ac3108ab226a899cfd7dcf91f59f19c3f7629273","observation_id":"15495211-3064-47c9-8aea-3a20e0ff0b36","resolution":{"observed_at":"2026-08-10T10:54:11.182103Z","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":"2026-08-10T10:54:11.185048Z","title":"Spatial distribution of the Milky Way hot gaseous halo constrained by Suzaku X-ray observations","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.185048Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:1c18e2adaecf98b134395fc70337aa84f58079c1d538fafaa9051ef236e5757f","observation_id":"ba9ee8ba-f575-45a5-874f-4c4babf2d96a","resolution":{"observed_at":"2026-08-10T10:54:11.185048Z","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":"2026-08-10T10:54:11.187850Z","title":"Cosmological implications of fast radio burst/gamma-ray burst associations","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-10T10:54:11.187850Z"},"links":{"citing_paper":"/paper/2501.16770"},"observation_digest":"sha256:56d28c3532a6d80461367421d94bb65e602fe2f7238ffc19059305dbbbc12204","observation_id":"e105eea1-4090-450d-930c-712135e5851e","resolution":{"observed_at":"2026-08-10T10:54:11.187850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2501.16770","last_updated":"2025-01-28T07:50:05Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-10T10:48:25.015317Z","submitted_at":"2025-01-28T07:50:05Z","title":"Constraining the Milky Way's Dispersion Measure Using FRB and X-ray Data"},"reference_resolution":{"displayed":72,"state_counts":{"malformed_identifier":4,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":60,"verified_exact":7,"verified_fuzzy":1},"total_outbound_references":72},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 72 of 72 outbound references and 0 inbound Pith citation observations for arXiv:2501.16770."}