{"as_of":"2026-08-08T21:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b9ef926e4f49528453787eecb93ea4baf98c7424e41f268b9b7328ec8aa4ad51","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T09:02:10.553457Z","state":"measured"},{"denominator":74,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":74,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+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/2607.10818/citation-record","integrity":"/paper/2607.10818/integrity","json":"/paper/2607.10818/citation-record.json","paper":"/paper/2607.10818"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":1,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:55438eebfe529f1fa80eacfa9d8dd640f1fa6dbdbb77d302071d533a746ec613","observation_id":"d7499e9f-7690-4dce-9830-61ce826badda","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":"1806.09693","last_updated":"2018-10-30T18:31:23Z","snapshot_observed_at":"2026-07-06T06:46:45.734215Z","submitted_at":"2018-06-25T20:34:21Z","title":"Superluminal motion of a relativistic jet in the neutron star merger GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.09693","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":2,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1806.09693","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:09430aaac9289a8ba3f4b0a77e0167974076bce0360d57ffa066c4013539c147","observation_id":"0fa2b5d5-efc6-4476-a7bc-72d35b6a1914","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":"2404.15027","last_updated":"2024-11-29T13:54:24Z","snapshot_observed_at":"2026-08-06T10:26:45.793138Z","submitted_at":"2024-04-23T13:33:53Z","title":"Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger","version":2},"cited_work":{"arxiv_id":"2404.15027","doi":"10.1093/mnras/stae2594","metadata_source":"pith","pith_arxiv_id":"2404.15027","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger","venue":"astro-ph.HE","work_id":"c1f612bb-aa9b-43d3-8d6d-d896fba6b79a","year":2024},"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":3,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2404.15027","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:11f64783c6287f515922b9057bbe9ec658be12c8d678442d3ae71f243f5fd73b","observation_id":"5e9c6957-4558-48bd-8828-4cdbcab4ddb6","resolution":{"observed_at":"2026-07-14T09:10:22.603410Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:00.846573+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:00.846573+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.14348","last_updated":"2023-01-30T15:26:12Z","snapshot_observed_at":"2026-08-08T18:51:05.346317Z","submitted_at":"2022-11-25T19:06:09Z","title":"The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.14348","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":4,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2211.14348","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:dec18134ecf01a54a37c85bae1f459bc1bba3e0a79a153794dddd35f143a9559","observation_id":"3049f7db-e3de-43e5-86cc-3f33e67bb6a2","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":"2105.11543","last_updated":"2021-05-24T21:13:17Z","snapshot_observed_at":"2026-08-08T16:02:20.807411Z","submitted_at":"2021-05-24T21:13:17Z","title":"A Broad Grid of 2D Kilonova Emission Models","version":1},"cited_work":{"arxiv_id":"2105.11543","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.11543","snapshot_observed_at":"2026-07-14T09:10:22.506870Z","title":"A Broad Grid of 2D Kilonova Emission Models","venue":"astro-ph.HE","work_id":"93768368-1f01-4f64-9e23-a6e39458e707","year":2021},"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":5,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2105.11543","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:2667146ba066e19443f6393c7fd3495a31a77bc4a34300c586a733e9b39dc09e","observation_id":"75d957f2-5603-4175-ba43-fa5e818753bd","resolution":{"observed_at":"2026-07-14T09:10:22.510269Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"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":6,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:c3afb69e1fee2c761b4161218bbb38602bb66a94fe278281d38f2f2f3dfc5bfd","observation_id":"bd051138-c4a2-4e1c-9eda-ed54246953b9","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":"2009.07279","last_updated":"2020-12-07T16:19:19Z","snapshot_observed_at":"2026-08-08T16:02:21.469072Z","submitted_at":"2020-09-15T18:00:01Z","title":"Polarized kilonovae from black hole-neutron star mergers","version":2},"cited_work":{"arxiv_id":"2009.07279","doi":"10.1093/mnras/staa3796","metadata_source":"pith","pith_arxiv_id":"2009.07279","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Polarized kilonovae from black hole-neutron star mergers","venue":"astro-ph.HE","work_id":"b8dc0bf2-03f5-4669-b006-efcbf4672006","year":2020},"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":7,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2009.07279","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:cf371860d2e52e96d38d8a34745b29a095b427d1490f49236e091f72e611b2de","observation_id":"a26ca83f-01de-4c42-a5b0-2a8797eaa93e","resolution":{"observed_at":"2026-07-14T09:10:22.430322Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:01.824576+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:01.824576+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.00299","last_updated":"2021-03-16T02:38:43Z","snapshot_observed_at":"2026-07-06T08:54:17.194727Z","submitted_at":"2020-02-02T01:41:07Z","title":"Inclination Dependence of Kilonova Light Curves from Globally Aspherical Geometries","version":2},"cited_work":{"arxiv_id":"2002.00299","doi":"10.3847/1538-4357/ab9a34","metadata_source":"pith","pith_arxiv_id":"2002.00299","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Inclination Dependence of Kilonova Light Curves from Globally Aspherical Geometries","venue":"astro-ph.HE","work_id":"e629c698-f6af-45d7-88df-ba6ebcf5e5e6","year":2020},"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":8,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2002.00299","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:68199d34f3f49d77bbf5558d3f6af9567a4dd04bbb2057e0e8b32109558df03d","observation_id":"2a8749e8-ece2-47c3-919c-dc687ea466cd","resolution":{"observed_at":"2026-07-14T09:10:22.437330Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:02.141955+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:02.141955+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1306.3742","last_updated":"2013-07-17T08:06:38Z","snapshot_observed_at":"2026-07-06T03:15:58.206519Z","submitted_at":"2013-06-17T05:50:45Z","title":"Radiative Transfer Simulations for Neutron Star Merger Ejecta","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.3742","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":9,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1306.3742","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:cf589d09d85f61ade50c5e032541c2a767f01fdd5323015b5c8e3f905346079c","observation_id":"b6d6c9ff-f4a8-4abe-bb28-a7f11ae3a0ae","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":"2204.00737","last_updated":"2022-04-02T01:48:02Z","snapshot_observed_at":"2026-07-06T12:55:57.209283Z","submitted_at":"2022-04-02T01:48:02Z","title":"Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.00737","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":10,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2204.00737","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:84e7e1f131f995c5d44560b393be83bff99ed3d71aef16a67149a3ac6a7f5017","observation_id":"74576fd8-f259-4f9f-9b39-3c10d8a01b68","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":"1710.05841","last_updated":"2017-10-17T15:25:29Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:57:47Z","title":"A kilonova as the electromagnetic counterpart to a gravitational-wave source","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05841","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":11,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1710.05841","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:975ec1a8e150f7e28f7837d3674b32ede4ed5580501db540dbc789201b60847e","observation_id":"679eab32-5d7f-4a7b-b63f-3d2fbff2fe28","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":"2026-07-14T09:02:10.553457Z","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":"1710.05834","last_updated":"2017-11-02T11:19:17Z","snapshot_observed_at":"2026-07-06T06:04:28.910951Z","submitted_at":"2017-10-16T16:57:19Z","title":"Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05834","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":13,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:2c54e7f2464c5bf63e366fc062185867431e3a96476716837e4f713e73f4fdd1","observation_id":"c480ecb7-6678-4dc1-b162-b9c170e0e84d","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"Monthly Notices of the Royal Astronomical Society , volume=","venue":null,"work_id":null,"year":2024},"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":14,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:1f493b986e85d7f12b670963b52fc575cbf25a6e08c565eaba3a7599dc10bf92","observation_id":"96993f88-f321-4d80-8208-dbfc7afd0ce3","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"Journal of Physics B: Atomic, Molecular and Optical Physics , volume=","venue":null,"work_id":null,"year":2024},"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":15,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:c28f55d6c11ada681e6727841208c3229e49ac460695f6165b93d1d986bac423","observation_id":"1a39db97-ccc6-457c-9fff-826b720d620e","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"2025 , eprint=","venue":null,"work_id":null,"year":2025},"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":16,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:5ccd2f872c2b0a4d38a28de63204f73d5503628ca9ee0c4b4a869126982797e3","observation_id":"9f167a86-d111-424e-abb7-287b6af895e3","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":"2302.06621","last_updated":"2023-02-13T19:00:00Z","snapshot_observed_at":"2026-08-07T08:36:16.174662Z","submitted_at":"2023-02-13T19:00:00Z","title":"Spherical symmetry in the kilonova AT2017gfo/GW170817","version":1},"cited_work":{"arxiv_id":"2302.06621","doi":null,"metadata_source":"pith","pith_arxiv_id":"2302.06621","snapshot_observed_at":"2026-07-14T09:10:22.391161Z","title":"Spherical symmetry in the kilonova AT2017gfo/GW170817","venue":"astro-ph.HE","work_id":"9418a3fb-5292-4710-91ea-d51160f0a491","year":2023},"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":17,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2302.06621","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:61ccba367ad516700dc438c69f17ff5a9d84881fbba364176e5c5f4c6b217236","observation_id":"e8a56f95-04dc-4f67-b665-e3b7b44871a9","resolution":{"observed_at":"2026-07-14T09:10:22.393800Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.05246","last_updated":"2023-02-23T11:46:40Z","snapshot_observed_at":"2026-07-06T13:51:12.442343Z","submitted_at":"2022-09-12T13:42:06Z","title":"3D radiative transfer kilonova modelling for binary neutron star merger simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.05246","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":18,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2209.05246","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:c423f43c4121e065c3553cbcb3252fe2196bf2089877f7a5ad5432b27bfbbda9","observation_id":"5b9d7026-6c24-4b85-89d9-f0d8c2c2f960","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":"2309.05579","last_updated":"2024-02-23T16:34:20Z","snapshot_observed_at":"2026-08-08T15:43:04.396654Z","submitted_at":"2023-09-11T16:08:43Z","title":"Towards inferring the geometry of kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.05579","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":19,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2309.05579","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:a0cb8033d71476d413f7aef591a97c55d951b7745131f4380d20d34507965748","observation_id":"01691a40-12bd-4925-b93a-791d589c136d","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":"2306.17612","last_updated":"2026-05-18T15:47:07Z","snapshot_observed_at":"2026-08-07T14:22:32.434475Z","submitted_at":"2023-06-30T12:37:54Z","title":"Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.17612","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":20,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2306.17612","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:3465e0a5a83932766564a487e7eeae73dbf73baebf7bba392bc0d3c905100250","observation_id":"63f78488-c277-45d1-863d-15cb2c623e7b","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":"2507.06412","last_updated":"2025-07-08T21:29:48Z","snapshot_observed_at":"2026-08-06T19:03:01.708732Z","submitted_at":"2025-07-08T21:29:48Z","title":"Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles","version":1},"cited_work":{"arxiv_id":"2507.06412","doi":"10.3847/1538-4357/ae0734","metadata_source":"pith","pith_arxiv_id":"2507.06412","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles","venue":"astro-ph.HE","work_id":"2dcffd4e-d48e-4bdb-958e-94e61eeb4978","year":2025},"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":21,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2507.06412","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:f67049118e91406167e48a7665f904d51983066411b49d9608062b32b07a56b4","observation_id":"05ee7351-1220-4386-93fb-dc092ad7344f","resolution":{"observed_at":"2026-07-14T09:10:22.463573Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:04.371928+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:04.371928+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.16210","last_updated":"2025-01-06T11:31:25Z","snapshot_observed_at":"2026-07-06T19:21:16.524383Z","submitted_at":"2024-09-24T16:10:26Z","title":"Actinide signatures in low electron fraction kilonova ejecta","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.16210","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":22,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2409.16210","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:99ae69997d6df00e4cdc04e1d282b8de7aecad75483eeeee0808074e48326d3d","observation_id":"83f8d88b-2ff1-47c9-bb54-48d6238a7b06","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":23,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:e7b7e49895856ed15a8af162c4abf7161e06854981404d6f3c9a6ffabcb86745","observation_id":"57ffa23e-d538-4ade-a6f9-3db2d2c1b429","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":"2102.07879","last_updated":"2021-02-15T22:41:10Z","snapshot_observed_at":"2026-07-06T10:41:37.896766Z","submitted_at":"2021-02-15T22:41:10Z","title":"Nebular Emission from Lanthanide-rich Ejecta of Neutron Star Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.07879","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":24,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2102.07879","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:d771e8fa5fcbdbbd2c7bf14ea79c80c136c99b1d81590f1f3a15f4a66d8465e9","observation_id":"54f82fac-0408-4c13-b80f-d7da1251d385","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":"2309.01134","last_updated":"2023-10-16T11:45:01Z","snapshot_observed_at":"2026-07-06T16:13:42.284158Z","submitted_at":"2023-09-03T11:00:47Z","title":"NLTE Spectra of Kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.01134","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":25,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2309.01134","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:77fe060da8678e39cd29e2c180cd19caaa6543ff16fd922b22d158ce6f5ad870","observation_id":"1c65ca19-1ad4-4f31-af33-560f3342ae3b","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":26,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:72aa5f9ff2d8d8ea8732de4c7b7868737e1ff8873f5adec876c392c808fe8791","observation_id":"d8fb0d4b-ae84-4c47-b496-b96435403ab5","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"Living Reviews in Computational Astrophysics , 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":27,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:7a1aa155218bbedc6a496cd1d4da64c52110b9f26d793f176f0b376bcac788b5","observation_id":"e8fbd7a7-f6d9-40c1-b1dc-27343dc753ec","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":"2306.15055","last_updated":"2023-11-27T12:35:46Z","snapshot_observed_at":"2026-08-06T02:39:05.609072Z","submitted_at":"2023-06-26T20:36:02Z","title":"Modelling the spectra of the kilonova AT2017gfo -- II: Beyond the photospheric epochs","version":2},"cited_work":{"arxiv_id":"2306.15055","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.15055","snapshot_observed_at":"2026-07-14T09:10:22.443046Z","title":"Modelling the spectra of the kilonova AT2017gfo -- II: Beyond the photospheric epochs","venue":"astro-ph.HE","work_id":"630b9178-76b4-4168-b731-d82630cfbdd9","year":2023},"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":28,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2306.15055","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:b1bec9929b93bba602b70ac2367f15724771e1266474d0ef506913c1f6568f4f","observation_id":"56b91c27-d6d3-42db-b749-aeb7cb182639","resolution":{"observed_at":"2026-07-14T09:10:22.444967Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01763","last_updated":"2024-04-02T09:27:30Z","snapshot_observed_at":"2026-08-03T13:45:04.318275Z","submitted_at":"2024-04-02T09:27:30Z","title":"Diagnostics of 3D explosion asymmetries of stripped-envelope supernovae by nebular line profiles","version":1},"cited_work":{"arxiv_id":"2404.01763","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.01763","snapshot_observed_at":"2026-07-14T09:10:22.614019Z","title":"Diagnostics of 3D explosion asymmetries of stripped-envelope supernovae by nebular line profiles","venue":"astro-ph.HE","work_id":"7d9a7cd1-c3b8-4652-bbfc-68a67a34f5cf","year":2024},"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":29,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2404.01763","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:bfafd34b4549994726221ecf5dcabd152940206789420c20976b5ff056335ef9","observation_id":"26521d77-7862-423e-a46b-4775a7ce73c0","resolution":{"observed_at":"2026-07-14T09:10:22.615630Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-07-14T09:02:10.553457Z","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":30,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:3fddfa5af82f08bfb761a011f63b8a92cda1ee92c1154d2b0ed8392774b5c8e9","observation_id":"0f3e625f-6461-487d-928e-4919e33a397c","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":"2511.07540","last_updated":"2026-05-04T09:54:26Z","snapshot_observed_at":"2026-07-06T22:35:27.050353Z","submitted_at":"2025-11-10T19:00:48Z","title":"Emission line models for the lowest mass core-collapse supernovae -- II. 3D NLTE radiative transfer modelling of a $9.0\\,M_\\odot$ neutrino-driven explosion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.07540","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"3D NLTE radiative transfer modelling of a 9.0 M _ neutrino-driven explosion","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":31,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2511.07540","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:74bd713424dc2bfe469fcf758c8df86dcbc54dce220df1b772b83f926737c0ba","observation_id":"17565cf1-2d28-4848-b517-fe9994313fc5","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":"2511.07539","last_updated":"2026-05-04T09:54:25Z","snapshot_observed_at":"2026-07-06T22:35:27.050353Z","submitted_at":"2025-11-10T19:00:47Z","title":"ExTraSS: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.07539","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"arXiv e-prints , 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":32,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2511.07539","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:3f28c3eb6897ecc742278bc9d7568993cf10fd7288c10ad339c4cf7245b658ff","observation_id":"f2a67d4b-8de9-4762-821f-12d643da2c87","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"Springer International Publishing","venue":null,"work_id":null,"year":2017},"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":33,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:7e9720c0db0b029bd71f6fdac5f3e8203d439d6471ef39db5791ea172a323243","observation_id":"388d91bf-8434-4f9a-952a-b6c4bfe1668b","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":"2411.16476","last_updated":"2025-02-17T16:42:15Z","snapshot_observed_at":"2026-08-07T07:21:22.015001Z","submitted_at":"2024-11-25T15:19:54Z","title":"Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova","version":2},"cited_work":{"arxiv_id":"2411.16476","doi":"10.1093/mnras/staf283","metadata_source":"pith","pith_arxiv_id":"2411.16476","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova","venue":"physics.atom-ph","work_id":"ea057956-fa22-4f9f-91cf-fe49cf0ffc41","year":2024},"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":34,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2411.16476","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:fc26e611a3f72d84a645bb4cc477c35c7802378cb1631618764004fe93afd10a","observation_id":"6ce15fb0-2fde-4f71-a9ef-6effed51475e","resolution":{"observed_at":"2026-07-14T09:10:22.597202Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:08.240661+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:08.240661+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05958","last_updated":"2024-10-08T12:12:20Z","snapshot_observed_at":"2026-08-03T22:21:35.404266Z","submitted_at":"2024-10-08T12:12:20Z","title":"Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks","version":1},"cited_work":{"arxiv_id":"2410.05958","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.05958","snapshot_observed_at":"2026-07-14T09:10:22.524102Z","title":"Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks","venue":"astro-ph.SR","work_id":"6b3be641-4a1f-46e1-a8a0-3d379f295cb6","year":2024},"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":35,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2410.05958","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:094b9fd18cddbd35589e243259399be523f44d6b3dc9375ab2198c17d2b58bf4","observation_id":"85a62f73-8978-41fe-ad5c-f93a864baf02","resolution":{"observed_at":"2026-07-14T09:10:22.526624Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10928","last_updated":"2023-06-02T10:52:24Z","snapshot_observed_at":"2026-07-06T14:54:19.013733Z","submitted_at":"2023-02-21T19:00:00Z","title":"End-to-end kilonova models of neutron-star mergers with delayed black-hole formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10928","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":36,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2302.10928","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:a1d7b5a19d7d03617896e826a33360b73d57876cbd2dd211b9903746652c6ce3","observation_id":"28d05afc-49ca-4351-8938-7d8ea0e57260","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":"2307.00988","last_updated":"2023-07-03T13:06:54Z","snapshot_observed_at":"2026-07-06T15:49:39.540157Z","submitted_at":"2023-07-03T13:06:54Z","title":"Tellurium emission line in kilonova AT 2017gfo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.00988","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":37,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2307.00988","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:e8f1ebb1ebd72af41ba22ace4c6162db7d4a1e530e3e29eb76f4d1f494d0742b","observation_id":"aa9dddef-7c57-4733-b920-bf769c7902aa","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":"2408.11093","last_updated":"2025-02-25T14:41:24Z","snapshot_observed_at":"2026-07-06T19:03:39.672411Z","submitted_at":"2024-08-20T18:00:01Z","title":"Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.11093","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":38,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2408.11093","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:1125ca517ae49be48c6d14b1032646cf25bc7bdf3a73ecf1e16fc7ccf77f4717","observation_id":"e9148b93-191c-4300-a05c-1778a4e8d920","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":"2307.02098","last_updated":"2023-07-05T08:19:23Z","snapshot_observed_at":"2026-07-06T15:50:26.113234Z","submitted_at":"2023-07-05T08:19:23Z","title":"JWST detection of heavy neutron capture elements in a compact object merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.02098","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":39,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2307.02098","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:11caaa3a1b28228c868c32e24cc05534fedf0ce2ad29105ec8c7055d7cc5bcc2","observation_id":"e01b136a-cd50-4cfa-b139-50d2319133fd","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":"2507.09040","last_updated":"2026-04-27T21:54:55Z","snapshot_observed_at":"2026-07-06T21:55:59.757729Z","submitted_at":"2025-07-11T21:36:15Z","title":"R-process heating implementation in hydrodynamic simulations with neural networks","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.09040","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":40,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2507.09040","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:a89da83ad2ebf8beb34a5f4e2af61280d0c081669774c0aba21b08ec6d08b925","observation_id":"c93b2a51-8cc2-4f60-afe3-8ef787ac1293","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":"1402.7317","last_updated":"2014-06-10T07:09:07Z","snapshot_observed_at":"2026-08-06T22:43:59.398491Z","submitted_at":"2014-02-28T16:51:22Z","title":"Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.7317","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":41,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1402.7317","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:258aa436a45a524ed616b20a33744827c1df9fd62526af559e70316612845b6b","observation_id":"55865e37-7ecc-48da-9f7d-cfb82cbadbfe","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":null,"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":42,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:1271ed62cce4e75f6d8255762725a8ae30d4e89232d3a32004fca54fb318df01","observation_id":"3b69a483-3a77-44f5-b8a4-05e6a00f06fc","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"parse_uncertain"},"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":"2026-07-14T09:02:10.553457Z","title":null,"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":43,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:142ecf998de243f7fcb471250abda092b2d42ee953a2af47f492164e0c4de1b2","observation_id":"eff4560b-07c0-4960-832b-5cc56c186c00","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":"2303.12284","last_updated":"2023-12-08T07:36:41Z","snapshot_observed_at":"2026-08-06T12:47:01.051292Z","submitted_at":"2023-03-22T03:23:27Z","title":"Jets from neutron-star merger remnants and massive blue kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12284","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":44,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2303.12284","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:bfe00637304c173af4f374774ad5c5e9bf94607dfc6ab65f3f4cc4f05ef58aec","observation_id":"62429f2e-04a7-41b7-86da-e095e45ffd01","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":"1406.2687","last_updated":"2015-01-07T17:51:39Z","snapshot_observed_at":"2026-08-02T05:38:11.057689Z","submitted_at":"2014-06-10T20:00:00Z","title":"Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.2687","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":45,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1406.2687","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:5e20ab8819c9cd9b166a1243b81e2b4867ab8cf29ac178742cb1d17352fe8946","observation_id":"7cda6569-030e-43a2-ad6e-547eb555a47a","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":"1412.5588","last_updated":"2015-02-04T02:43:47Z","snapshot_observed_at":"2026-07-06T04:03:58.110385Z","submitted_at":"2014-12-17T21:00:08Z","title":"The interplay of disk wind and dynamical ejecta in the aftermath of neutron star - black hole mergers","version":2},"cited_work":{"arxiv_id":"1412.5588","doi":"10.1093/mnras/stv238","metadata_source":"pith","pith_arxiv_id":"1412.5588","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The interplay of disk wind and dynamical ejecta in the aftermath of neutron star - black hole mergers","venue":"astro-ph.HE","work_id":"4c9c98db-e04b-4a87-bab5-fbaf750e32e1","year":2014},"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":46,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1412.5588","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:a391de09b7cdedb2a271c68adbc0b26a6ccfc13109b237ce4e7137d44123ba1d","observation_id":"8fbd5e5f-6a30-4b26-bdf0-c9212d9b22a0","resolution":{"observed_at":"2026-07-14T09:10:22.558253Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-07-14T19:20:10.770307+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T19:20:10.770307+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04146","last_updated":"2015-02-13T22:47:44Z","snapshot_observed_at":"2026-07-06T04:09:12.373040Z","submitted_at":"2015-02-13T22:47:44Z","title":"Post-merger evolution of a neutron star-black hole binary with neutrino transport","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.04146","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":47,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1502.04146","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:00ef52d704497b5d7456cd3a4eb2f79ae854add7835ff287bb37938f24a9bf5f","observation_id":"b30277d0-2505-4e35-ba1e-51316a9d8f68","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":"2007.00474","last_updated":"2020-07-01T13:24:57Z","snapshot_observed_at":"2026-07-06T09:34:27.720277Z","submitted_at":"2020-07-01T13:24:57Z","title":"Post-merger Mass Ejection of Low-mass Binary Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.00474","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"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":48,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2007.00474","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:ce593a81796dc11e76b55ca7f39d99085030c579acbd0dcaf56d9a6cbd5ae638","observation_id":"80c1d1b5-0951-47fd-9dcc-df0a2813d712","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":null,"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":49,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:af572511defb63831c2c0b390acd489c132babd79a3017e778a7053a9c0d6a8b","observation_id":"ceb60e2f-3348-4b1c-adc8-9eff305f42f5","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6720","last_updated":"2013-07-16T17:25:04Z","snapshot_observed_at":"2026-07-06T03:11:57.623498Z","submitted_at":"2013-04-24T20:00:01Z","title":"Delayed outflows from black hole accretion tori following neutron star binary coalescence","version":2},"cited_work":{"arxiv_id":"1304.6720","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.6720","snapshot_observed_at":"2026-07-14T09:10:22.465686Z","title":"Delayed outflows from black hole accretion tori following neutron star binary coalescence","venue":"astro-ph.HE","work_id":"143c7d25-c2b3-42e5-b9e8-82edc0130914","year":2013},"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":50,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1304.6720","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:4dcef5cb3b59948c0117a8dbcd2688d11ac3cfc9f647acac8af7e2891509be48","observation_id":"11aa6471-7bb1-4b9a-a80a-9cb6fe614430","resolution":{"observed_at":"2026-07-14T09:10:22.468244Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05473","last_updated":"2017-11-02T18:07:50Z","snapshot_observed_at":"2026-07-06T05:42:46.786223Z","submitted_at":"2017-05-15T22:40:35Z","title":"Three-dimensional GRMHD simulations of the remnant accretion disks from neutron star mergers: outflows and r-process nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.05473","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":51,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1705.05473","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:52f4b2dae53fcaf66ff749301b0cc273dc9da0d65900bc8e62d05fc8285a7bf1","observation_id":"d0f1728f-35cd-4030-a467-a5a3511d5ef2","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":"2403.13883","last_updated":"2024-10-03T13:47:27Z","snapshot_observed_at":"2026-08-05T12:36:58.857278Z","submitted_at":"2024-03-20T18:00:02Z","title":"Element formation in radiation-hydrodynamics simulations of kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.13883","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":52,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2403.13883","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:2fafc9fafb410e193817557d76304645f546b351bd1c74ac9f59ae877e1de5dc","observation_id":"433a93bf-c34f-40d3-b41c-6e700d28bffe","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":53,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:6c43157cadcdca8c5b6e5dd5d6d9bafcc15468d860d38751df09fffd4a4cf145","observation_id":"031ef0aa-6fef-49de-96ce-ee60bb0d8034","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":"2012.14711","last_updated":"2022-08-30T01:37:14Z","snapshot_observed_at":"2026-07-06T10:28:28.378332Z","submitted_at":"2020-12-29T11:40:07Z","title":"A low-mass binary neutron star: long-term ejecta evolution and kilonovae with weak blue emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.14711","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"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":54,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2012.14711","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:40a4ec4a8400353209d191537e2e976262e13e365c423e0a4f4bcc2a0d4fce84","observation_id":"17cc2826-583e-4b72-906c-69243d3bfe88","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":"1705.07084","last_updated":"2017-05-19T16:46:15Z","snapshot_observed_at":"2026-07-06T05:43:25.911696Z","submitted_at":"2017-05-19T16:46:15Z","title":"Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.07084","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":55,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1705.07084","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:7217b0a9d9aabf00aabc61c4911e820b37531b51e5516852fe90fbf90b23c9f8","observation_id":"7719b4e9-40ed-4e1d-8c54-9e030873ebb3","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":56,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:2b769df5d97bc3c0716126fe5a44b2b4cde33caed4a7ab476d928212c958e60d","observation_id":"7e21520e-453d-47d3-8eb0-6d57b86da571","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":null,"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":57,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:2040384b0eac15af1a66d22661791ffeeb5569a0615fa2f02fedbf00ad21faa0","observation_id":"eebefc32-d22c-496f-afb0-c37cc0fe118a","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.3726","last_updated":"2014-11-13T21:00:07Z","snapshot_observed_at":"2026-08-01T15:58:06.080805Z","submitted_at":"2014-11-13T21:00:07Z","title":"Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.3726","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":58,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1411.3726","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:86326d17c1e9bafac9aaf543d99eb7357f7d9d3575f4b08794ce997f945af0dd","observation_id":"c50968cf-76e5-4bd3-8960-1c702169445f","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":"0705.4512","last_updated":"2007-05-31T13:46:30Z","snapshot_observed_at":"2026-07-06T01:27:52.334995Z","submitted_at":"2007-05-31T13:46:30Z","title":"The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.4512","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2007},"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":59,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/0705.4512","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:26d70b484b3d7d41d2ac1cd53d7bd409db8ac640571747e760f6c36aa462b77f","observation_id":"33dcc84d-37e1-4ed9-9bab-ddf8df3dedd7","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":"1901.01410","last_updated":"2021-02-01T18:05:27Z","snapshot_observed_at":"2026-07-06T07:25:04.099406Z","submitted_at":"2019-01-05T13:08:05Z","title":"Origin of the Heaviest Elements: the Rapid Neutron-Capture Process","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.01410","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":"Reviews of Modern Physics , keywords =","venue":null,"work_id":null,"year":1901},"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":60,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1901.01410","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:3613b11a1ad5767d28e39b3c2584d330b95428acab22357ad3f471be215a59a8","observation_id":"5eb30fea-c66d-44e0-88e6-617ec336936d","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"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":61,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:8e4f1d8c52bad35fe2ea92ee3e6fc15eaae24f608356479a6a9b3378220dce8d","observation_id":"84f33e34-8638-4359-a982-34989f4d3ed6","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2008},"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":62,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:c5b76f3f55857aabc6b3812350465df66da08902a512cbbe2c7164b6295f13f8","observation_id":"6d160492-3b53-40fa-a918-429912bd019a","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":"astro-ph/0611047","last_updated":"2007-03-12T12:50:21Z","snapshot_observed_at":"2026-07-07T01:04:18.735176Z","submitted_at":"2006-11-02T11:10:14Z","title":"Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state","version":2},"cited_work":{"arxiv_id":"astro-ph/0611047","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0611047","snapshot_observed_at":"2026-07-14T09:10:22.397630Z","title":"Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state","venue":"astro-ph","work_id":"517fbb33-c964-4018-a0e2-1bf8dd1e2193","year":2006},"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":63,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/astro-ph/0611047","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:4ecbc6e8f777bbf7ad7189674fc007032c04a30bd1f36c5ed2da2bc574f389a7","observation_id":"d524acd3-1ae5-4766-965e-d2f413a7e536","resolution":{"observed_at":"2026-07-14T09:10:22.399894Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-07-14T09:02:10.553457Z","title":null,"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":64,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:45ef4c93f33e644f662ab949444a44c5841597d5e82318828b354356d13b92a3","observation_id":"c7851f03-e980-4158-8f09-788acf0dadbc","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":"1905.07477","last_updated":"2019-05-17T21:00:36Z","snapshot_observed_at":"2026-07-06T07:53:51.699343Z","submitted_at":"2019-05-17T21:00:36Z","title":"Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.07477","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":1905},"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":65,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1905.07477","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:5785349d2491f9b81bddcac02760c371972bf2f05da34cc22073de45c50cd321","observation_id":"0ad59a2d-7a1d-4ba4-9c83-a93f58306e24","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":"2410.02380","last_updated":"2024-11-29T14:03:13Z","snapshot_observed_at":"2026-07-06T19:26:54.335667Z","submitted_at":"2024-10-03T10:57:02Z","title":"Long-term Monte Carlo-based neutrino-radiation hydrodynamics simulations for a black hole-torus system","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.02380","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":66,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2410.02380","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:e4e83b022236fe5832b100f30bd1d9fac4ea4762ca9ec85b6e33cee8d7fc09da","observation_id":"a7fe57dd-6380-4f0c-8cce-ff875037a148","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":"2307.04572","last_updated":"2023-07-10T14:06:59Z","snapshot_observed_at":"2026-08-06T13:15:40.127683Z","submitted_at":"2023-07-10T14:06:59Z","title":"M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04572","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":67,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2307.04572","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:5ac787f66de5019c82e4c5b049ecd41c851a2ef25e08655cd6eeb890e718808c","observation_id":"92d3730c-527d-4c2f-a1c4-d54a530ef196","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":"1402.4803","last_updated":"2014-05-02T04:29:13Z","snapshot_observed_at":"2026-07-06T03:36:27.214082Z","submitted_at":"2014-02-19T21:00:01Z","title":"Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.4803","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":68,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1402.4803","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:004cbf86e70aa59bdbaddaa9f3e196bc521517cee387312cf6614e4fd6f9c6e9","observation_id":"1839438c-e1af-4458-aa32-15fd7239e851","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":"1405.6730","last_updated":"2014-05-26T20:02:56Z","snapshot_observed_at":"2026-08-01T16:29:37.820781Z","submitted_at":"2014-05-26T20:02:56Z","title":"Neutrino-driven winds from neutron star merger remnants","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.6730","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":69,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1405.6730","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:f7c5f79715b3497fd9f75ed062e02f5c3f00482f20286c25f97e80a2f768be4a","observation_id":"5d81e522-66c9-45aa-9d31-f145b127b965","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":"1601.02426","last_updated":"2016-05-12T22:50:16Z","snapshot_observed_at":"2026-08-03T19:32:03.280725Z","submitted_at":"2016-01-11T12:51:45Z","title":"Dynamical Mass Ejection from Binary Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.02426","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":70,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/1601.02426","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:448340a71e0966468c230eee092e529564e11fd610a48dfe392d6c9243e2baa3","observation_id":"dca89052-ca3c-455a-85a2-cb167eff9d47","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":"2410.06253","last_updated":"2024-10-08T18:00:02Z","snapshot_observed_at":"2026-07-06T19:29:55.838200Z","submitted_at":"2024-10-08T18:00:02Z","title":"On the impact of neutrinos on the launching of relativistic jets from \"magnetars\" produced in neutron-star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.06253","snapshot_observed_at":"2026-07-14T09:02:10.553457Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":71,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2410.06253","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:4105684767f6fc4c5a4e943f9979ebd60736340661401a696aa74a6047e1b3d7","observation_id":"89dfd147-d69d-4ff0-accc-8e5b00e54f40","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":"2410.20681","last_updated":"2025-01-30T07:10:16Z","snapshot_observed_at":"2026-08-07T16:01:04.252107Z","submitted_at":"2024-10-28T02:41:22Z","title":"Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20681","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":72,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2410.20681","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:1d465c647e7ee950fd09211b8947f210c3b8ac322f1ee3dc5bec913f58af3276","observation_id":"9e34c78c-7665-4411-bd07-ff991d887117","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":"2409.18185","last_updated":"2025-07-11T12:52:43Z","snapshot_observed_at":"2026-08-01T23:29:05.874114Z","submitted_at":"2024-09-26T18:00:13Z","title":"Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves","version":2},"cited_work":{"arxiv_id":"2409.18185","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.18185","snapshot_observed_at":"2026-07-14T09:10:22.429689Z","title":"Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves","venue":"astro-ph.HE","work_id":"80b57ba8-ce7f-4203-bb3e-df3974129061","year":2024},"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":73,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"cited_paper":"/paper/2409.18185","citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:bc0fa204354901f5e3918cc77cf85c1444ad00b98dc0d73e6800beba0ad3284a","observation_id":"218371db-fd62-4bd7-b91c-691096c0f994","resolution":{"observed_at":"2026-07-14T09:10:22.432135Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+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":"2026-07-14T09:02:10.553457Z","title":null,"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":74,"source":"arxiv_source","source_observed_at":"2026-07-14T09:02:10.553457Z"},"links":{"citing_paper":"/paper/2607.10818"},"observation_digest":"sha256:bbf8e4c5aac0a50d1aa34a03fccc62f46599e8a70de5ab03c7978e65786ef285","observation_id":"e38c1ec9-e5e0-4cc0-8724-2e198fda1200","resolution":{"observed_at":"2026-07-14T09:02:10.553457Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.10818","last_updated":"2026-07-12T16:08:28Z","latest_version":1,"primary_category":"astro-ph.HE","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"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":4,"unresolved":56,"verified_exact":14,"verified_fuzzy":0},"total_outbound_references":74},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 0 inbound Pith citation observations for arXiv:2607.10818."}