{"as_of":"2026-08-05T15:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3f1c54200305cf553c0d3dffc07038a74352ab66f791e78040aadcf08c0218cb","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T09:55:42.904006Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":"1711.03982","doi":"10.48550/arxiv.1711.03982","metadata_source":"pith","pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","venue":"astro-ph.HE","work_id":"9b45146d-9b68-4234-b944-1ad78bcd1da2","year":2017},"citing_paper":{"arxiv_id":"2303.15923","last_updated":"2023-06-17T10:49:26Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-03-28T12:29:33Z","title":"Science with the Einstein Telescope: a comparison of different designs","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-17T21:43:29.760310Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2303.15923"},"observation_digest":"sha256:a48b38f2e8816872ab14fb49fbff248e51717b01cce7441274710b8f4b18f301","observation_id":"878a09b9-3dc6-4904-a015-6319610ff0cd","resolution":{"observed_at":"2026-05-17T21:43:30.230578Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":"1711.03982","doi":"10.48550/arxiv.1711.03982","metadata_source":"pith","pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","venue":"astro-ph.HE","work_id":"9b45146d-9b68-4234-b944-1ad78bcd1da2","year":2017},"citing_paper":{"arxiv_id":"2605.29187","last_updated":"2026-05-27T23:52:21Z","snapshot_observed_at":"2026-08-04T14:14:53.187077Z","submitted_at":"2026-05-27T23:52:21Z","title":"Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-29T10:03:39.187375Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2605.29187"},"observation_digest":"sha256:c6adb6afcc718e760b982f2280ad02aef32810d6f7c4ff07307146464c0611a5","observation_id":"4950c553-c037-47f5-a899-e79b3ac7c3bf","resolution":{"observed_at":"2026-06-29T13:53:29.279496Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":"1711.03982","doi":"10.48550/arxiv.1711.03982","metadata_source":"pith","pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","venue":"astro-ph.HE","work_id":"9b45146d-9b68-4234-b944-1ad78bcd1da2","year":2017},"citing_paper":{"arxiv_id":"2606.11299","last_updated":"2026-06-09T18:00:02Z","snapshot_observed_at":"2026-07-06T23:50:25.158108Z","submitted_at":"2026-06-09T18:00:02Z","title":"A magnetar formation in binary neutron star merger","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-06-27T12:03:16.536504Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2606.11299"},"observation_digest":"sha256:017ebb1c2b9c32dcf0273509e1cd0eda3b87428afc242985dc1d3abd25197ffc","observation_id":"6afd9020-73fa-495c-b0d4-898e7b5dd104","resolution":{"observed_at":"2026-07-03T07:37:45.154765Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-07-12T05:14:58.841553Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2607.03045","last_updated":"2026-07-03T07:34:46Z","snapshot_observed_at":"2026-08-03T21:49:18.542361Z","submitted_at":"2026-07-03T07:34:46Z","title":"nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors","version":1},"reference_index":149,"source":"arxiv_source","source_observed_at":"2026-07-12T05:14:58.841553Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2607.03045"},"observation_digest":"sha256:2d6ce9944e38cb8a08c9467ca2dff4f53b2af9970adab35964a84182a67a65dc","observation_id":"46a6869a-62ff-410d-95ae-952c2ff143c8","resolution":{"observed_at":"2026-07-12T05:14:58.841553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":"1711.03982","doi":"10.48550/arxiv.1711.03982","metadata_source":"pith","pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","venue":"astro-ph.HE","work_id":"9b45146d-9b68-4234-b944-1ad78bcd1da2","year":2017},"citing_paper":{"arxiv_id":"2607.07120","last_updated":"2026-07-08T08:02:30Z","snapshot_observed_at":"2026-08-04T05:36:48.322349Z","submitted_at":"2026-07-08T08:02:30Z","title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","version":1},"reference_index":134,"source":"arxiv_source","source_observed_at":"2026-07-09T19:57:37.088370Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2607.07120"},"observation_digest":"sha256:081d58acc0886835554a52e5b5cd4755fff0a881b9c4dfee6987d9496b516c3c","observation_id":"b6e4640c-0b5c-4c9b-b7bb-4ace1da31550","resolution":{"observed_at":"2026-07-09T20:06:29.569761Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":"1711.03982","doi":"10.48550/arxiv.1711.03982","metadata_source":"pith","pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","venue":"astro-ph.HE","work_id":"9b45146d-9b68-4234-b944-1ad78bcd1da2","year":2017},"citing_paper":{"arxiv_id":"2607.07120","last_updated":"2026-07-08T08:02:30Z","snapshot_observed_at":"2026-08-04T05:36:48.322349Z","submitted_at":"2026-07-08T08:02:30Z","title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","version":1},"reference_index":163,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2607.07120"},"observation_digest":"sha256:993a876fea0c141ee2d745ffa591113b568264905357ecce6be456fc686835fe","observation_id":"f93e353d-7eee-4e17-91ba-9ea03862233a","resolution":{"observed_at":"2026-07-09T20:06:29.646504Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03982","snapshot_observed_at":"2026-08-01T09:55:42.904006Z","title":"Perego, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.20609","last_updated":"2026-07-22T18:00:00Z","snapshot_observed_at":"2026-08-04T15:52:22.544739Z","submitted_at":"2026-07-22T18:00:00Z","title":"Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-01T09:55:42.904006Z"},"links":{"cited_paper":"/paper/1711.03982","citing_paper":"/paper/2607.20609"},"observation_digest":"sha256:4209ccf1b292d39432c353706e5105ace198188345da04da22aebbf08a153067","observation_id":"af2eee1f-688e-450a-8380-1d88ed0526bc","resolution":{"observed_at":"2026-08-01T09:55:42.904006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1711.03982/citation-record","integrity":"/paper/1711.03982/integrity","json":"/paper/1711.03982/citation-record.json","paper":"/paper/1711.03982"},"outbound":[],"paper":{"arxiv_id":"1711.03982","last_updated":"2017-11-10T19:00:39Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-04T13:12:37.616541Z","submitted_at":"2017-11-10T19:00:39Z","title":"AT2017gfo: an anisotropic and three-component kilonova counterpart of GW170817"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1711.03982."}