{"as_of":"2026-08-10T23:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:072daf7f2718fcdfa98a817e00b1066ed730bca147187539ffd783f82c12d4e2","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T15:52:56.255810Z","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":"2026-07-09T20:06:29.571222Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"1912.02622","last_updated":"2020-03-24T17:57:53Z","snapshot_observed_at":"2026-08-02T17:41:15.064781Z","submitted_at":"2019-12-05T14:57:00Z","title":"Science Case for the Einstein Telescope","version":4},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-16T00:13:18.137293Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/1912.02622"},"observation_digest":"sha256:a6200d5a7035a115d6e0d69564f88dc5eb02abcbdce12a6bf13fb61269487f4c","observation_id":"5c34076c-86d2-4df4-a523-5ee92f5b315f","resolution":{"observed_at":"2026-05-16T00:13:18.348020Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-08-05T15:52:56.255810Z","title":"Pian et al., Nature (2017), 10.1038/nature24298, arXiv:1710.05858 [astro-ph.HE]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.19342","last_updated":"2025-08-26T18:00:29Z","snapshot_observed_at":"2026-08-06T22:36:44.913736Z","submitted_at":"2025-08-26T18:00:29Z","title":"Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-05T15:52:56.255810Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2508.19342"},"observation_digest":"sha256:ddfe21d7b23f1144cb680fb43c34407d10d55621cb9c74f1b9f7c7c56a3cba83","observation_id":"66ac215e-63e9-4e0c-bf57-9f018984e28a","resolution":{"observed_at":"2026-08-05T15:52:56.255810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2605.03947","last_updated":"2026-05-05T16:32:23Z","snapshot_observed_at":"2026-08-02T07:09:55.498496Z","submitted_at":"2026-05-05T16:32:23Z","title":"Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-07T14:05:21.961266Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2605.03947"},"observation_digest":"sha256:6c9181a46cb444d3fbed372c20fecb2b278a739fa1e2214ab63e6dd4f5a74fe6","observation_id":"0458462f-7681-4c36-a6b8-515e7ed64793","resolution":{"observed_at":"2026-05-12T08:41:25.305959Z","resolver_source":"arxiv_id","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":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2605.30548","last_updated":"2026-05-28T20:30:13Z","snapshot_observed_at":"2026-08-07T04:15:44.902066Z","submitted_at":"2026-05-28T20:30:13Z","title":"Magnetic Eruption and Nucleosynthesis in GR{\\nu}MHD Simulations of Spinning Neutron Star Mergers","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-29T05:38:27.204444Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2605.30548"},"observation_digest":"sha256:e7d02dff565e02609c6ae7a9084814be8b5c4c20b0e608e70b734a1c668a7f0a","observation_id":"4a60367b-fff8-4abc-a342-424bc4e25891","resolution":{"observed_at":"2026-06-29T05:43:08.371308Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2606.28210","last_updated":"2026-06-26T16:01:59Z","snapshot_observed_at":"2026-07-07T00:02:18.989389Z","submitted_at":"2026-06-26T16:01:59Z","title":"SKAO and Gamma-Ray Synergies","version":1},"reference_index":160,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2606.28210"},"observation_digest":"sha256:356b3b99e055a1aee19f1da9373df80aa0610069f4c789237ed6866d11a1c9db","observation_id":"84295acf-184c-4c82-ae3f-09d1825770bc","resolution":{"observed_at":"2026-06-29T03:03:03.512772Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2606.28267","last_updated":"2026-06-26T17:00:44Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-26T17:00:44Z","title":"Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes","version":1},"reference_index":244,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2606.28267"},"observation_digest":"sha256:6f88bc34e8003f68394a88c89aa8a1c602200c22d9c8f2abed56453c6a6592c6","observation_id":"3e6e33c1-ff23-4662-8986-4691abaab72d","resolution":{"observed_at":"2026-06-29T02:53:03.406155Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2607.01228","last_updated":"2026-07-27T16:29:36Z","snapshot_observed_at":"2026-08-02T09:02:31.743123Z","submitted_at":"2026-07-01T17:59:01Z","title":"Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics","version":1},"reference_index":168,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.01228"},"observation_digest":"sha256:1a66c02efd156446406fbd75c3496ef3a4670860f36bc1939e5fce0e8a9a4767","observation_id":"81e7c8b6-987f-49d0-b587-50ef56c658da","resolution":{"observed_at":"2026-07-02T07:16:43.962625Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2607.01337","last_updated":"2026-07-01T18:00:16Z","snapshot_observed_at":"2026-08-03T01:34:16.673968Z","submitted_at":"2026-07-01T18:00:16Z","title":"A possible high-redshift origin for the short GRB 061201: implications of a compact binary merger beyond cosmic noon","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.01337"},"observation_digest":"sha256:5f60da1d89c4aa27417c0b00aae5836b6dccc7b7a52f479f973d6b1553dd1073","observation_id":"1c439b7e-3dbf-4904-add0-58bd2fa698c0","resolution":{"observed_at":"2026-07-03T19:48:53.217558Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":"1710.05858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-09T20:06:29.571222Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","venue":"astro-ph.HE","work_id":"23930e9e-e038-474b-9fe0-866623bdbd3a","year":2017},"citing_paper":{"arxiv_id":"2607.07120","last_updated":"2026-07-08T08:02:30Z","snapshot_observed_at":"2026-08-08T06:28:48.615790Z","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":210,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.07120"},"observation_digest":"sha256:a7cf60234d1ec1d26de3be84d7673c069d6d72613d2a562d0b970c1404a2afb7","observation_id":"32dd9ea3-b9ac-4858-b697-544ab557aca8","resolution":{"observed_at":"2026-07-09T20:06:29.572668Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.10818","last_updated":"2026-07-12T16:08:28Z","snapshot_observed_at":"2026-08-08T16:02:02.874872Z","submitted_at":"2026-07-12T16:08:28Z","title":"Late-time emission-line profiles from kilonova models","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:034f1dda33c7536acaa80ef5d5f6379861a2ec7f091d36b2673076a09ca9cc95","observation_id":"4ea592f4-feda-425b-8b67-0fcb0699a569","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-08-01T22:19:57.605077Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15803","last_updated":"2026-07-17T10:13:52Z","snapshot_observed_at":"2026-08-06T08:52:24.513248Z","submitted_at":"2026-07-17T10:13:52Z","title":"Chemical Evolution of Galaxies: Past, Present and Future","version":1},"reference_index":106,"source":"arxiv_source","source_observed_at":"2026-08-01T22:19:57.605077Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.15803"},"observation_digest":"sha256:dafc7771d83b91d581d18b43352031a39ccf728ed310e81300d0b577df4d3c23","observation_id":"012b5503-be0d-47c4-9ba2-e2c48f983087","resolution":{"observed_at":"2026-08-01T22:19:57.605077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-08-01T10:52:08.417342Z","title":"Nature , keywords =","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.20091","last_updated":"2026-07-22T12:47:13Z","snapshot_observed_at":"2026-08-09T19:16:07.780577Z","submitted_at":"2026-07-22T12:47:13Z","title":"A universal chromosome map for globular clusters: chemical calibration and environmental regulation of the multiple populations","version":1},"reference_index":151,"source":"arxiv_source","source_observed_at":"2026-08-01T10:52:08.417342Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.20091"},"observation_digest":"sha256:f62286f157c21531e51932855ea21348df9115c2ca3a446f6660e83f8520a037","observation_id":"cd1f462f-e45b-48f0-94fc-e6645be85414","resolution":{"observed_at":"2026-08-01T10:52:08.417342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-08-01T09:55:36.936093Z","title":"Pianet al., Nature551, 67 (2017), arXiv:1710.05858 [astro- ph.HE]","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.20609","last_updated":"2026-07-22T18:00:00Z","snapshot_observed_at":"2026-08-09T04:37:08.877289Z","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":9,"source":"pdf_text","source_observed_at":"2026-08-01T09:55:36.936093Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/2607.20609"},"observation_digest":"sha256:537655ff642b7334fe18bf6a38a127a8eec0b240c9a91e85d4a9c0a3c3027581","observation_id":"f242006b-b950-4005-b19c-ead198b5e41b","resolution":{"observed_at":"2026-08-01T09:55:36.936093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1710.05858/citation-record","integrity":"/paper/1710.05858/integrity","json":"/paper/1710.05858/citation-record.json","paper":"/paper/1710.05858"},"outbound":[],"paper":{"arxiv_id":"1710.05858","last_updated":"2017-10-16T16:58:15Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:1710.05858."}