{"as_of":"2026-08-13T05:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:126a7ad3c6aec1340eb2e516d4bc5d82e46a834e36f491a60c6b5430d158a479","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":32,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":32,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":32,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":32,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T13:00:55.478731Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T13:07:05.222050Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-12T13:00:55.478731Z","title":"Astrophys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.16606","last_updated":"2024-11-26T06:50:55Z","snapshot_observed_at":"2026-08-12T12:53:56.245542Z","submitted_at":"2024-11-25T17:41:54Z","title":"Detection of X-ray Emission from a Bright Long-Period Radio Transient","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T13:00:55.478731Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2411.16606"},"observation_digest":"sha256:cba89cc2860c0390eaf491b9d28a51c7cae010883cb6588c9cc383957afa7e07","observation_id":"dd1a4795-3e84-4d9b-a3f8-1d274117a375","resolution":{"observed_at":"2026-08-12T13:00:55.478731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-10T22:40:43.328450Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2501.01489","last_updated":"2025-01-02T19:00:01Z","snapshot_observed_at":"2026-08-11T00:53:00.340492Z","submitted_at":"2025-01-02T19:00:01Z","title":"Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T22:40:43.328450Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2501.01489"},"observation_digest":"sha256:e0ebba0180f1e4359e82502ce32f6039b0293b335154da5b150ab3b21bb7e06d","observation_id":"ce0d32cf-fca1-4c5e-be11-79e6c2c8e288","resolution":{"observed_at":"2026-08-10T22:40:43.328450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2504.02030","last_updated":"2026-05-09T04:00:38Z","snapshot_observed_at":"2026-08-03T04:21:58.102373Z","submitted_at":"2025-04-02T18:00:01Z","title":"Neutron Star Eclipses as Axion Laboratories","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-22T21:29:04.480897Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2504.02030"},"observation_digest":"sha256:0b4a89d78f539376eaa7a95db0a542aa1d7ed8167538428642e8a0ed332d4c1d","observation_id":"15af7799-2544-4a77-9a2c-3ca9cf59e9cb","resolution":{"observed_at":"2026-05-22T21:32:10.430131Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-07T11:09:35.345524Z","title":"Yao, R.N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.03536","last_updated":"2026-07-30T03:27:01Z","snapshot_observed_at":"2026-08-12T16:30:43.815468Z","submitted_at":"2025-06-04T03:34:29Z","title":"Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T11:09:35.345524Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2506.03536"},"observation_digest":"sha256:8726057feeb3635584d5342aa229238c41e3b942bf6c26aa61287e3f5880e27a","observation_id":"17aa384d-ce8a-4718-8599-8a9cef526b05","resolution":{"observed_at":"2026-08-07T11:09:35.345524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-06T17:41:22.806266Z","title":", Manchester , R.N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.10221","last_updated":"2025-07-14T12:39:06Z","snapshot_observed_at":"2026-08-12T22:45:37.637793Z","submitted_at":"2025-07-14T12:39:06Z","title":"Unlocking Gravity and Gravitational Waves with Radio Pulsars: Advances and Challenges","version":1},"reference_index":134,"source":"arxiv_source","source_observed_at":"2026-08-06T17:41:22.806266Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2507.10221"},"observation_digest":"sha256:658628c165f8d894e48f72c249c6f35dba0ca72d6386134d829f2a99f8d9c746","observation_id":"a1c71ac8-0170-4cea-9a64-e99748bf6957","resolution":{"observed_at":"2026-08-06T17:41:22.806266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-05T11:20:39.665646Z","title":", author Manchester , R.N","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.03001","last_updated":"2025-09-03T04:23:45Z","snapshot_observed_at":"2026-08-10T20:17:41.900143Z","submitted_at":"2025-09-03T04:23:45Z","title":"Low-frequency observations of low-mass binary systems with neutron star candidates","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-05T11:20:39.665646Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2509.03001"},"observation_digest":"sha256:294789f08800a0bef82f4abce4df82356828e3cb3ada8fb867c14556a40b15c0","observation_id":"6c64266f-e9e6-41c6-a5c1-6571360d8fc0","resolution":{"observed_at":"2026-08-05T11:20:39.665646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2512.17214","last_updated":"2026-04-27T01:51:04Z","snapshot_observed_at":"2026-08-13T00:09:31.155549Z","submitted_at":"2025-12-19T03:54:03Z","title":"Pulsed radio emission from a Central Compact Object","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-16T21:16:18.019954Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2512.17214"},"observation_digest":"sha256:f8652b1494b61410cd1857775ded4cd5065ea65c3c0b374122587c50077e03d9","observation_id":"8d48a8ab-00eb-4fa5-9ee5-31db9dcc8b6d","resolution":{"observed_at":"2026-05-16T21:18:32.485756Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2604.03769","last_updated":"2026-04-04T15:41:30Z","snapshot_observed_at":"2026-08-11T09:14:11.855136Z","submitted_at":"2026-04-04T15:41:30Z","title":"Dispersion Measure Distribution of Unlocalized Fast Radio Bursts as a Probe of the Hubble Constant","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-13T17:12:38.566382Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2604.03769"},"observation_digest":"sha256:b85b13cfade879eeb69e481d013860d486a28126a2bf813f86337f278b866c92","observation_id":"4e45a48e-e2fa-4c55-8d54-cd405fc8099b","resolution":{"observed_at":"2026-05-13T17:13:01.034675Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2605.02172","last_updated":"2026-05-04T03:05:51Z","snapshot_observed_at":"2026-08-12T02:15:12.500016Z","submitted_at":"2026-05-04T03:05:51Z","title":"Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-08T19:29:14.584013Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2605.02172"},"observation_digest":"sha256:0606c0c84df70a935d0db8585b65cbd199748759e63724504b1629a9ef280d0c","observation_id":"ffbef808-472b-4c36-99b0-9e1a38e88fcb","resolution":{"observed_at":"2026-05-09T05:50:27.298731Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2605.13605","last_updated":"2026-05-13T14:40:05Z","snapshot_observed_at":"2026-08-11T15:49:28.992765Z","submitted_at":"2026-05-13T14:40:05Z","title":"DEFROST: Detecting Excess in Faraday Rotation thrOugh Sophisticated analysis Techniques","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2605.13605"},"observation_digest":"sha256:e0efeb202f2763f1515769899b69d0dbff609c7a75d999df51ebae940ee96ad1","observation_id":"5fa74ab9-6164-4ab1-b5cc-9da613ce4cea","resolution":{"observed_at":"2026-05-14T17:57:31.902362Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2605.13697","last_updated":"2026-07-23T10:57:29Z","snapshot_observed_at":"2026-08-02T14:10:15.387815Z","submitted_at":"2026-05-13T15:49:07Z","title":"Guitar Nebula: extreme accelerator in extreme environment","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2605.13697"},"observation_digest":"sha256:0f76cd46b7a5f073e03f480733c54669b717a41436e8725fe00a5918be49ac82","observation_id":"70d540ed-2d09-46c2-b913-f072f0051dd2","resolution":{"observed_at":"2026-05-14T17:52:32.103486Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.07087","last_updated":"2026-06-05T09:34:11Z","snapshot_observed_at":"2026-08-02T12:20:54.646868Z","submitted_at":"2026-06-05T09:34:11Z","title":"A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.07087"},"observation_digest":"sha256:e67cf8b1e0bc158b63723bb927f0f67255c7cb777bd9706c4bbdcb446fb16fda","observation_id":"c2f2c7d4-8276-44c4-842e-3acb9b2d90a4","resolution":{"observed_at":"2026-06-27T21:51:19.055199Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.19701","last_updated":"2026-06-18T01:52:52Z","snapshot_observed_at":"2026-08-02T20:38:02.898818Z","submitted_at":"2026-06-18T01:52:52Z","title":"On the Contribution of Local Sources to the Galactic Cosmic-Ray Spectrum: An Exact Series Solution for Two-Zone Diffusion","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-06-26T16:43:02.409335Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.19701"},"observation_digest":"sha256:fb4c63ec4cfbaec5711919801cc6fe04d6a07f0c4ed399f4b8605c75432487b8","observation_id":"dc1adeee-90f1-494b-b319-5345286751a1","resolution":{"observed_at":"2026-07-04T04:49:35.715389Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.20201","last_updated":"2026-07-29T07:31:01Z","snapshot_observed_at":"2026-08-13T04:12:51.612482Z","submitted_at":"2026-06-18T13:15:54Z","title":"Dependences of radio pulsar parameters on the bimodal kick mode","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.20201"},"observation_digest":"sha256:8d43238f991dd133a6a28ca12d50fcd198dd46c24ce9fabe7fa4d474ce2fbebe","observation_id":"56a8110e-5e6d-4dcd-8f24-605143c5baa4","resolution":{"observed_at":"2026-06-26T16:39:36.111896Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.20471","last_updated":"2026-06-18T16:52:06Z","snapshot_observed_at":"2026-07-06T23:55:38.979306Z","submitted_at":"2026-06-18T16:52:06Z","title":"The impact of FRB dispersion measure probability distribution functions on cosmographic estimates","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-06-26T16:01:06.661486Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.20471"},"observation_digest":"sha256:d8da0abfe2b2ed3cee85f7aea3205e191b6088c9feabf639b3a78df0bd69b4de","observation_id":"ea174264-4909-4036-ba7e-fabf79faaed2","resolution":{"observed_at":"2026-07-04T05:29:35.294903Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.23926","last_updated":"2026-06-22T20:44:51Z","snapshot_observed_at":"2026-08-12T22:58:06.120246Z","submitted_at":"2026-06-22T20:44:51Z","title":"Detection of relativistic orbital deformation from improved timing of PSR J1757$-$1854","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.23926"},"observation_digest":"sha256:e5e3e596b009eab83c0ab532837f92ef377ed8571e0c8456e3628738fb05d2d7","observation_id":"344c210e-1ee4-411f-9d99-074f089f7653","resolution":{"observed_at":"2026-06-26T06:59:07.826626Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.25077","last_updated":"2026-06-23T18:35:44Z","snapshot_observed_at":"2026-08-08T14:52:38.897535Z","submitted_at":"2026-06-23T18:35:44Z","title":"Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.25077"},"observation_digest":"sha256:713bd7e55fc467151ca276e8f94282035fd45689031070064a454dd5d5613efc","observation_id":"fbd3064b-2a9f-40a2-895a-14c589958ec4","resolution":{"observed_at":"2026-06-26T00:48:45.505461Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.27225","last_updated":"2026-06-25T16:13:28Z","snapshot_observed_at":"2026-08-02T09:31:06.532764Z","submitted_at":"2026-06-25T16:13:28Z","title":"A search for Fast Radio Bursts from globular clusters in M49 with FAST","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.27225"},"observation_digest":"sha256:38832646ee3017305fab35d85f6c9314aabf8594074690e8a80f87c83e8a12b9","observation_id":"d4f149f9-f818-404b-8eda-ea0116f2afd8","resolution":{"observed_at":"2026-06-26T03:18:57.679435Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.27714","last_updated":"2026-06-26T04:44:56Z","snapshot_observed_at":"2026-08-01T17:32:21.309572Z","submitted_at":"2026-06-26T04:44:56Z","title":"Fast Radio Bursts as Cosmological Probes","version":1},"reference_index":260,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.27714"},"observation_digest":"sha256:54cc3d1fd8c73b62cd5b9a7e30095f376e27dc91b92cea4bf8f6f4fcd779ecd5","observation_id":"6713bcd9-a9ed-4d11-b7af-e43c2abefff2","resolution":{"observed_at":"2026-06-29T03:53:04.960457Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.29300","last_updated":"2026-06-28T09:40:18Z","snapshot_observed_at":"2026-08-12T02:14:50.906526Z","submitted_at":"2026-06-28T09:40:18Z","title":"SPICE: Scintillation Pipeline for Interferometric Candidate Extraction","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.29300"},"observation_digest":"sha256:74fc0bb7a122e570276c224dc9ef64df8c94812719ba84d401625d9c704389ec","observation_id":"545ff76d-8901-42d2-9f2b-4d33b848a2dd","resolution":{"observed_at":"2026-06-30T02:44:10.655259Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2606.31042","last_updated":"2026-06-30T02:23:39Z","snapshot_observed_at":"2026-07-31T02:20:06.641037Z","submitted_at":"2026-06-30T02:23:39Z","title":"An Acceleration is Worth a Hundred Thousand Phase Space Measurements","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2606.31042"},"observation_digest":"sha256:c008d7464ddb3b4a95559d4b85cae633e1bb4f2a77be3e39f4263132f6c4de55","observation_id":"73862be4-c296-4b7d-acf0-e26c06cfd44d","resolution":{"observed_at":"2026-07-01T05:25:25.610994Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-12T05:03:41.498841Z","title":"doi:10.3847/1538-4357/835/1/29 , adsurl =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03078","last_updated":"2026-07-03T08:11:20Z","snapshot_observed_at":"2026-08-11T15:16:24.063431Z","submitted_at":"2026-07-03T08:11:20Z","title":"Galactic Centre Pulsars with the SKAO","version":1},"reference_index":132,"source":"arxiv_source","source_observed_at":"2026-07-12T05:03:41.498841Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.03078"},"observation_digest":"sha256:da8a46191a02e24f47c069944e01f3a909ed56bdc0ab7926ce74e575e0d20df8","observation_id":"5defb305-5ce2-4007-9c22-7a178efd04cc","resolution":{"observed_at":"2026-07-12T05:03:41.498841Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-12T05:00:29.237939Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03087","last_updated":"2026-07-03T08:20:29Z","snapshot_observed_at":"2026-08-13T00:30:03.085636Z","submitted_at":"2026-07-03T08:20:29Z","title":"Understanding the Neutron Star Population with the SKAO Telescopes","version":1},"reference_index":252,"source":"arxiv_source","source_observed_at":"2026-07-12T05:00:29.237939Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.03087"},"observation_digest":"sha256:eb2e7fd1b81ce92d54f28eb6054f1b2953091d91d090081321212ad9085aa95c","observation_id":"530e60d4-a39d-4961-bc83-056279871218","resolution":{"observed_at":"2026-07-12T05:00:29.237939Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-12T04:59:26.773930Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.03090","last_updated":"2026-07-03T08:22:09Z","snapshot_observed_at":"2026-08-06T07:01:52.527883Z","submitted_at":"2026-07-03T08:22:09Z","title":"A Square Kilometre Array Pulsar Census","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-12T04:59:26.773930Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.03090"},"observation_digest":"sha256:d973051323e7bd507015819f8c214c2f9e589beb3f065b0a795870207482a122","observation_id":"87586131-15b8-4760-a1f9-5140f4961333","resolution":{"observed_at":"2026-07-12T04:59:26.773930Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-12T08:30:18.472851Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.06096","last_updated":"2026-07-13T13:38:29Z","snapshot_observed_at":"2026-08-13T01:18:44.178708Z","submitted_at":"2026-07-02T10:28:38Z","title":"Exploring the Galactic plasma with pulsars in the SKA Era","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-12T08:30:18.472851Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.06096"},"observation_digest":"sha256:3417217c1bcb74b2bbe081827f4ffd1b92fcec2a8dcbb8ac2af10873abdde64e","observation_id":"40f664e6-c3d2-4471-ada5-4b26eb970a47","resolution":{"observed_at":"2026-07-12T08:30:18.472851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-14T16:43:10.179035Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.06096","last_updated":"2026-07-13T13:38:29Z","snapshot_observed_at":"2026-08-13T01:18:44.178708Z","submitted_at":"2026-07-02T10:28:38Z","title":"Exploring the Galactic plasma with pulsars in the SKA Era","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T16:43:10.179035Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.06096"},"observation_digest":"sha256:131f49fe13890d5e3d9f9e0d66e7d0c5798d4961e3122b4a6b9491b6dae0a602","observation_id":"4d5f4834-9f9b-472c-b45b-5f83e6a5e24b","resolution":{"observed_at":"2026-07-14T16:43:10.179035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2607.08106","last_updated":"2026-07-09T04:46:17Z","snapshot_observed_at":"2026-08-06T08:59:39.684459Z","submitted_at":"2026-07-09T04:46:17Z","title":"The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars","version":1},"reference_index":142,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.08106"},"observation_digest":"sha256:81ab18fe8aaf88f824b4734a186718b66713d2124c41b279d0489724ba9cef54","observation_id":"2587434e-8321-458e-b7ba-ba122188649f","resolution":{"observed_at":"2026-07-10T13:07:05.223725Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":"1610.09448","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-10T13:07:05.222050Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","venue":"astro-ph.GA","work_id":"52c2cf9d-a657-4440-aa39-38cebad7b7e8","year":2016},"citing_paper":{"arxiv_id":"2607.08542","last_updated":"2026-07-09T14:36:04Z","snapshot_observed_at":"2026-08-07T14:04:07.639758Z","submitted_at":"2026-07-09T14:36:04Z","title":"Constraints on the properties of warm ionized gas from low-frequency hydrogen radio recombination lines","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.08542"},"observation_digest":"sha256:a62cc59cc1a75825d2b9862c2688f95f85715695f453e0d7b86a658c160de942","observation_id":"85f64e67-8a62-4cf6-88ac-99d15c9997a6","resolution":{"observed_at":"2026-07-10T05:46:49.669225Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-07-13T05:21:16.491609Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.09109","last_updated":"2026-07-10T05:45:41Z","snapshot_observed_at":"2026-08-13T05:10:21.052897Z","submitted_at":"2026-07-10T05:45:41Z","title":"Fast Radio Bursts Trace Cosmic Star Formation with Little Delay","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-13T05:21:16.491609Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.09109"},"observation_digest":"sha256:d13d4b347b836cc386e548978834d07b646484e382ac4f1c19d8f11d336178dc","observation_id":"ffeeaf18-b622-471e-9217-7bd661803b9c","resolution":{"observed_at":"2026-07-13T05:21:16.491609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-01T08:50:53.638780Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.20985","last_updated":"2026-07-23T07:07:54Z","snapshot_observed_at":"2026-08-08T14:39:32.764255Z","submitted_at":"2026-07-23T07:07:54Z","title":"Accurate Extragalactic Magnetic Fields from Faraday Rotation with Optimal Dispersion Measure Estimators","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-01T08:50:53.638780Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.20985"},"observation_digest":"sha256:34d24ed8d5a4101084f421a0c079d83abc4e93ab97fa524dfedab53ecbdb8354","observation_id":"6346e152-409a-4130-886a-afe903a170c5","resolution":{"observed_at":"2026-08-01T08:50:53.638780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-01T09:26:45.859307Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.27333","last_updated":"2026-07-29T18:00:06Z","snapshot_observed_at":"2026-08-03T23:18:43.786661Z","submitted_at":"2026-07-29T18:00:06Z","title":"Relativistic effects of PSR~J1856--0039 double neutron star system in a 2.36-hour compact orbit","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T09:26:45.859307Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2607.27333"},"observation_digest":"sha256:1e47147f177043619ee158f2ecc387ab4482137194f920e72eea97b3627380de","observation_id":"25c64f6a-dcaa-47b7-8324-46555d855a8c","resolution":{"observed_at":"2026-08-01T09:26:45.859307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.09448","snapshot_observed_at":"2026-08-05T00:40:16.197199Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2608.00589","last_updated":"2026-08-01T10:57:38Z","snapshot_observed_at":"2026-08-12T00:47:53.652987Z","submitted_at":"2026-08-01T10:57:38Z","title":"Gamma Rays from ALP-Photon Conversion and Inverse Compton Reprocessing in Neutron Star Magnetospheres","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-05T00:40:16.197199Z"},"links":{"cited_paper":"/paper/1610.09448","citing_paper":"/paper/2608.00589"},"observation_digest":"sha256:c3644c5652fe1ff8fed399ba29f2648c8b65d5769b889859eb5e3ba01ad7bbd6","observation_id":"6c9193c0-585e-4f01-ac3e-377e4ab105a0","resolution":{"observed_at":"2026-08-05T00:40:16.197199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1610.09448/citation-record","integrity":"/paper/1610.09448/integrity","json":"/paper/1610.09448/citation-record.json","paper":"/paper/1610.09448"},"outbound":[],"paper":{"arxiv_id":"1610.09448","last_updated":"2016-11-03T09:39:51Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T05:16:37.188435Z","submitted_at":"2016-10-29T03:41:27Z","title":"A New Electron Density Model for Estimation of Pulsar and FRB Distances"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 32 inbound Pith citation observations for arXiv:1610.09448."}