{"as_of":"2026-08-20T20:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:95d104eb52578cb6f3fe94325445fe05d778705a711a3011fff3a41c94ca5a12","coverage":[{"denominator":92,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":92,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T15:45:09.902947Z","state":"measured"},{"denominator":93,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":93,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T16:16:41.979750Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-06T16:16:43.643345Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"cited_work":{"arxiv_id":"1908.00655","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.00655","snapshot_observed_at":"2026-08-06T16:16:43.643345Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","venue":"gr-qc","work_id":"48f82535-21c6-4fdf-bed9-863201ecd0df","year":2019},"citing_paper":{"arxiv_id":"2507.14071","last_updated":"2025-07-18T16:49:25Z","snapshot_observed_at":"2026-08-17T19:52:27.348296Z","submitted_at":"2025-07-18T16:49:25Z","title":"Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T16:16:41.979750Z"},"links":{"cited_paper":"/paper/1908.00655","citing_paper":"/paper/2507.14071"},"observation_digest":"sha256:80d6082b175813ca3341b944c887f2fb64f5893d857119d69f5f2b77d02641a2","observation_id":"d78fcf4a-3c1e-4840-a833-6c08a39bae66","resolution":{"observed_at":"2026-08-06T16:16:43.648498Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1908.00655/citation-record","integrity":"/paper/1908.00655/integrity","json":"/paper/1908.00655/citation-record.json","paper":"/paper/1908.00655"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-14T15:45:09.447753Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.447753Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:2ae695747e30dfbdfa81d34230d50f2b27afe6dfdf1f6f61e352041f7c1679ec","observation_id":"b9b56f8a-c559-4382-b295-efe66ed151e6","resolution":{"observed_at":"2026-08-14T15:45:09.447753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05833","last_updated":"2017-10-24T12:03:18Z","snapshot_observed_at":"2026-08-19T15:24:12.152497Z","submitted_at":"2017-10-16T16:57:18Z","title":"Multi-messenger Observations of a Binary Neutron Star Merger","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05833","snapshot_observed_at":"2026-08-14T15:45:09.453489Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.453489Z"},"links":{"cited_paper":"/paper/1710.05833","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:83f284c232e99387e6aafcd93c368c8e924df8642d61571203154515dbd11c86","observation_id":"d77e382f-d4f0-4bd8-ad79-ed512660655d","resolution":{"observed_at":"2026-08-14T15:45:09.453489Z","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":"2026-08-15T21:57:31.832991Z","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":"2026-08-14T15:45:09.458790Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.458790Z"},"links":{"cited_paper":"/paper/1710.05834","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:6c466ebe076877425cb5b845fb451a0ec54c2cd7eed81db7d10e98fcab6b1e38","observation_id":"8f79f797-eddb-4738-9d03-b4857d532252","resolution":{"observed_at":"2026-08-14T15:45:09.458790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.463707Z","title":"Ajello, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.463707Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:d0176812207184103a4da1dabf8bc52937783b2fb99e70df5ea844f9b302c172","observation_id":"c1c82132-2250-46bf-8b21-d76c80f08aec","resolution":{"observed_at":"2026-08-14T15:45:09.463707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11579","last_updated":"2019-01-22T19:56:03Z","snapshot_observed_at":"2026-08-16T07:13:02.254304Z","submitted_at":"2018-05-29T16:55:48Z","title":"Properties of the binary neutron star merger GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11579","snapshot_observed_at":"2026-08-14T15:45:09.468563Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.468563Z"},"links":{"cited_paper":"/paper/1805.11579","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7ba2b325bd56462000d88d2c39588ca3111eca20f1b6488ca82ebc0415c7fbd8","observation_id":"1dbc3fe2-2997-4b78-85ce-67d34e1f192b","resolution":{"observed_at":"2026-08-14T15:45:09.468563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.473556Z","title":"Mochkovitch, M","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.473556Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:14b6eff86234ff4a7820ddf219de2a6a18edcf8508ffafe125cecc1cd098042e","observation_id":"359e8604-87df-4071-8454-b9d98e65cd61","resolution":{"observed_at":"2026-08-14T15:45:09.473556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.478600Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.478600Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:9d3b33856c3258a5dca99f9e9248f6ad71b028c7696bf4d9c767acee3e91379c","observation_id":"868688c8-1bbb-413b-badb-5646e02d888a","resolution":{"observed_at":"2026-08-14T15:45:09.478600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908290","last_updated":"1999-10-15T09:51:40Z","snapshot_observed_at":"2026-08-19T18:02:14.963831Z","submitted_at":"1999-08-26T19:31:48Z","title":"Black Hole - Neutron Star Mergers as Central Engines of Gamma-Ray Bursts","version":2},"cited_work":{"arxiv_id":"astro-ph/9908290","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9908290","snapshot_observed_at":"2026-08-14T15:45:10.973426Z","title":"Black Hole - Neutron Star Mergers as Central Engines of Gamma-Ray Bursts","venue":"astro-ph","work_id":"b93e1154-86b6-41ab-9040-f1caac36a802","year":1999},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.483336Z"},"links":{"cited_paper":"/paper/astro-ph/9908290","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:4adebf7b152610a9dfb0e16ffabd0882d2fb67c96f8ec0037487f9c9f1405d8b","observation_id":"a8db2242-046b-4751-a52e-72c2e3b4c998","resolution":{"observed_at":"2026-08-14T15:45:10.978538Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.09693","last_updated":"2018-10-30T18:31:23Z","snapshot_observed_at":"2026-08-14T18:59:23.805275Z","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":"2026-08-14T15:45:09.488676Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.488676Z"},"links":{"cited_paper":"/paper/1806.09693","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:c1ff127185b089554a8bf20e181668f6ff997b14be100811095bfb7551b3c2ab","observation_id":"4c9fa7c8-7bd8-44f3-b8b2-df033869097d","resolution":{"observed_at":"2026-08-14T15:45:09.488676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807272","last_updated":"1998-08-31T01:47:41Z","snapshot_observed_at":"2026-08-13T06:00:40.406877Z","submitted_at":"1998-07-27T17:06:14Z","title":"Transient Events from Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807272","snapshot_observed_at":"2026-08-14T15:45:09.493354Z","title":"Li and B","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.493354Z"},"links":{"cited_paper":"/paper/astro-ph/9807272","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:dcc4088b9bdb1bb0b1b91e48d3a42951169d63b35a66ba9c988db55191945f0e","observation_id":"43897b16-34cb-4800-89f6-ddc806bbc38b","resolution":{"observed_at":"2026-08-14T15:45:09.493354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.497652Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.497652Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:a1ff8c123f85ca126f452dbb8edf11ea979dfbe348d1ff8c49b3ea4f4b7e4d88","observation_id":"c9a26545-9fd8-4b02-bbd7-4ced78d34f9c","resolution":{"observed_at":"2026-08-14T15:45:09.497652Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9811367","last_updated":"1998-11-23T16:56:15Z","snapshot_observed_at":"2026-08-16T20:05:46.218207Z","submitted_at":"1998-11-23T16:56:15Z","title":"Mass ejection in neutron star mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9811367","snapshot_observed_at":"2026-08-14T15:45:09.501829Z","title":"Rosswog, M","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.501829Z"},"links":{"cited_paper":"/paper/astro-ph/9811367","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:6ce6e09a46c3a9cdc8fd7b99dd31c125a0a8228c48c24a43c4f0e36e4ba638d2","observation_id":"709ad583-b779-4a27-80be-e343b9cf82f2","resolution":{"observed_at":"2026-08-14T15:45:09.501829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510256","last_updated":"2005-10-10T00:55:21Z","snapshot_observed_at":"2026-08-09T11:34:01.625126Z","submitted_at":"2005-10-10T00:55:21Z","title":"Modeling Supernova-like Explosions Associated with Gamma-ray Bursts with Short Durations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510256","snapshot_observed_at":"2026-08-14T15:45:09.506335Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.506335Z"},"links":{"cited_paper":"/paper/astro-ph/0510256","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:ddc8389fabf093d39424f460ca029ed5e4dd6c273dde7418b4c05951238d9762","observation_id":"19359d48-5eeb-4222-8e85-c3fac12df40b","resolution":{"observed_at":"2026-08-14T15:45:09.506335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.5029","last_updated":"2010-04-23T20:16:42Z","snapshot_observed_at":"2026-08-15T05:27:53.722753Z","submitted_at":"2010-01-28T17:17:53Z","title":"Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.5029","snapshot_observed_at":"2026-08-14T15:45:09.510566Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.510566Z"},"links":{"cited_paper":"/paper/1001.5029","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:0c20a4c705ec02cc91dea26530fcc9fe41f52e926cb0bef120a9d664d2cd18e7","observation_id":"c1d3c6a6-aa8f-47cc-b869-5e5e73720d36","resolution":{"observed_at":"2026-08-14T15:45:09.510566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.515284Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.515284Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7b7dac2d11cbfd7a4609b592b3e35d20b59274c3b86a424b7c69f46a47fd2d44","observation_id":"76e716d4-dad0-4a9b-ab3e-c8f5f38b1beb","resolution":{"observed_at":"2026-08-14T15:45:09.515284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05436","last_updated":"2017-10-16T16:57:43Z","snapshot_observed_at":"2026-08-20T20:21:54.365992Z","submitted_at":"2017-10-16T16:57:43Z","title":"Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05436","snapshot_observed_at":"2026-08-14T15:45:09.520089Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.520089Z"},"links":{"cited_paper":"/paper/1710.05436","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:5518e92e905ecfbdcce937f0b3d1bfd395babab00d241ba511704eaf788dec69","observation_id":"3780b067-5e65-4920-8263-2c23966d0c21","resolution":{"observed_at":"2026-08-14T15:45:09.520089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05452","last_updated":"2017-10-16T16:57:35Z","snapshot_observed_at":"2026-08-14T20:23:19.381034Z","submitted_at":"2017-10-16T16:57:35Z","title":"Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05452","snapshot_observed_at":"2026-08-14T15:45:09.525070Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.525070Z"},"links":{"cited_paper":"/paper/1710.05452","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7c6698daee5a63d5227272956c26a8342d839af1148827aee25ef19d0a21bc44","observation_id":"6a66156e-349a-4904-98b4-238393c6015b","resolution":{"observed_at":"2026-08-14T15:45:09.525070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05454","last_updated":"2017-10-16T16:57:30Z","snapshot_observed_at":"2026-08-19T17:11:11.610305Z","submitted_at":"2017-10-16T16:57:30Z","title":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05454","snapshot_observed_at":"2026-08-14T15:45:09.529744Z","title":"Chornock, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.529744Z"},"links":{"cited_paper":"/paper/1710.05454","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:c98d9e075afa9a42e80a27997a4b1f2234445d7d3dc681831a4a1cd2b5d299b5","observation_id":"657bb2d8-7984-4ed1-a884-c13bec405270","resolution":{"observed_at":"2026-08-14T15:45:09.529744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05840","last_updated":"2017-10-16T16:57:28Z","snapshot_observed_at":"2026-08-14T20:23:19.361123Z","submitted_at":"2017-10-16T16:57:28Z","title":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05840","snapshot_observed_at":"2026-08-14T15:45:09.534405Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.534405Z"},"links":{"cited_paper":"/paper/1710.05840","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:dc8d893a6c25f50afa94536f38e1eb4da32e1afd392b824d4b69f9fb5fb490da","observation_id":"d2b3781a-fc0d-4889-acfc-a95fd1d5a9b3","resolution":{"observed_at":"2026-08-14T15:45:09.534405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05463","last_updated":"2017-10-16T16:57:39Z","snapshot_observed_at":"2026-08-14T20:23:18.981067Z","submitted_at":"2017-10-16T16:57:39Z","title":"Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05463","snapshot_observed_at":"2026-08-14T15:45:09.538979Z","title":"Kasen, B","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.538979Z"},"links":{"cited_paper":"/paper/1710.05463","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:e09e080b0528f1cb87cfba96a24ecdea81822d91a38a006e1272ec5849b2d5fb","observation_id":"2ca1d7b3-9860-48e7-8e34-8c8eeef9cf40","resolution":{"observed_at":"2026-08-14T15:45:09.538979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05434","last_updated":"2017-10-16T16:57:41Z","snapshot_observed_at":"2026-08-18T08:10:27.997983Z","submitted_at":"2017-10-16T16:57:41Z","title":"Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05434","snapshot_observed_at":"2026-08-14T15:45:09.543657Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.543657Z"},"links":{"cited_paper":"/paper/1710.05434","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:cc6ce17c85196cba2de07d7b5b0a5278cdc1cc5d30ad68a38cd79c5fdc1452e6","observation_id":"3c1d4741-9f10-4ae4-adf7-902c84f20025","resolution":{"observed_at":"2026-08-14T15:45:09.543657Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05853","last_updated":"2017-10-16T16:58:10Z","snapshot_observed_at":"2026-08-14T20:23:17.560017Z","submitted_at":"2017-10-16T16:58:10Z","title":"The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05853","snapshot_observed_at":"2026-08-14T15:45:09.548408Z","title":"McCully, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.548408Z"},"links":{"cited_paper":"/paper/1710.05853","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:ad4feef4909b0811cbee02c47dceb945751b83a2de46325a8bfa8bd5deb6090a","observation_id":"7de3379c-5e5f-482c-a5c4-a713918fbbd4","resolution":{"observed_at":"2026-08-14T15:45:09.548408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05456","last_updated":"2017-10-16T16:57:29Z","snapshot_observed_at":"2026-08-19T19:14:59.780024Z","submitted_at":"2017-10-16T16:57:29Z","title":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05456","snapshot_observed_at":"2026-08-14T15:45:09.553181Z","title":"Nicholl, E","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.553181Z"},"links":{"cited_paper":"/paper/1710.05456","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:bc5d4ae52c018859277433459766d973e3f5ec256a189729dbf87b5968761db8","observation_id":"4edb453b-34ac-4a5a-b7bf-1bc5c78872e7","resolution":{"observed_at":"2026-08-14T15:45:09.553181Z","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":"2026-08-18T05:50:39.710683Z","submitted_at":"2017-10-16T16:58:15Z","title":"Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05858","snapshot_observed_at":"2026-08-14T15:45:09.558405Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.558405Z"},"links":{"cited_paper":"/paper/1710.05858","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:be3825676727e111688ea11cd0506bd94e26bfbe093b29f330a58b0a6ad4ce3e","observation_id":"f43f099c-0239-4889-98c0-a9bd06f1cfec","resolution":{"observed_at":"2026-08-14T15:45:09.558405Z","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":"2026-08-14T20:23:18.554582Z","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":"2026-08-14T15:45:09.563703Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.563703Z"},"links":{"cited_paper":"/paper/1710.05841","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:74765ad87cd3a58a8d8dd7e86f893ceffab0093cf258161e5492175283f423ac","observation_id":"44680909-8504-4b4d-ac95-796673df1c48","resolution":{"observed_at":"2026-08-14T15:45:09.563703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05459","last_updated":"2017-10-16T16:57:27Z","snapshot_observed_at":"2026-08-16T17:53:59.323643Z","submitted_at":"2017-10-16T16:57:27Z","title":"The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05459","snapshot_observed_at":"2026-08-14T15:45:09.568760Z","title":"Soares-Santos, D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.568760Z"},"links":{"cited_paper":"/paper/1710.05459","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:79b674336e4d87dc14d46c8bf1d8172054e3276d754b9704ca82a0a5a1bf337d","observation_id":"c2caef90-ded5-4e51-a6a5-5de3da6e92e6","resolution":{"observed_at":"2026-08-14T15:45:09.568760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05455","last_updated":"2017-10-16T16:57:52Z","snapshot_observed_at":"2026-08-14T20:23:18.337828Z","submitted_at":"2017-10-16T16:57:52Z","title":"The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05455","snapshot_observed_at":"2026-08-14T15:45:09.573590Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.573590Z"},"links":{"cited_paper":"/paper/1710.05455","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:b01dc185b680f5042282cdd53ecd75351f2c1bc08c54c46ef2294fecb1cd56de","observation_id":"06f77dbb-1586-458a-a736-13707b9d8f99","resolution":{"observed_at":"2026-08-14T15:45:09.573590Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05437","last_updated":"2017-10-16T16:57:45Z","snapshot_observed_at":"2026-08-19T15:08:07.452830Z","submitted_at":"2017-10-16T16:57:45Z","title":"Swift and NuSTAR observations of GW170817: detection of a blue kilonova","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05437","snapshot_observed_at":"2026-08-14T15:45:09.578548Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.578548Z"},"links":{"cited_paper":"/paper/1710.05437","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:cbcadb841e662d1f7f936bf259b2008a833567469899fb514996cf0d31424c96","observation_id":"7abaea14-1f7b-4b4e-adbb-469ae06e1093","resolution":{"observed_at":"2026-08-14T15:45:09.578548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-08-14T15:45:09.583435Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.583435Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:513b7fdf83fb1a2f5210458fbe10cd842d936c5648ba9d6178a661fbdba88880","observation_id":"3775a232-d433-4e43-919b-2ff1bc2a1a2a","resolution":{"observed_at":"2026-08-14T15:45:09.583435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00501","last_updated":"2016-03-01T21:44:59Z","snapshot_observed_at":"2026-08-14T22:07:58.076100Z","submitted_at":"2016-03-01T21:44:59Z","title":"Unequal mass binary neutron star mergers and multimessenger signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.00501","snapshot_observed_at":"2026-08-14T15:45:09.598291Z","title":"Lehner, S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.598291Z"},"links":{"cited_paper":"/paper/1603.00501","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:be0fec33f4ca1164053a063108e96d148f300b20da01890bb42ef3e9f77c6cdd","observation_id":"f795de09-787a-49b1-b1bc-5321b706d548","resolution":{"observed_at":"2026-08-14T15:45:09.598291Z","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":"2026-08-19T11:29:31.647749Z","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":"2026-08-14T15:45:09.603441Z","title":"Radice, F","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.603441Z"},"links":{"cited_paper":"/paper/1601.02426","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:0d3cd56da03d708f0bb8e212beb32b413318242647729364237558134e31005e","observation_id":"ff95dd63-e792-46a3-81f7-fbd0a2be4fdf","resolution":{"observed_at":"2026-08-14T15:45:09.603441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.2125","last_updated":"2011-06-24T03:23:51Z","snapshot_observed_at":"2026-08-15T04:47:08.722123Z","submitted_at":"2011-05-11T08:53:17Z","title":"Gravitational waves and neutrino emission from the merger of binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.2125","snapshot_observed_at":"2026-08-14T15:45:09.608268Z","title":"Sekiguchi, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.608268Z"},"links":{"cited_paper":"/paper/1105.2125","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:b6822b5091cb21a415f92c890d319417c66ef47bceca82f67382935eda217486","observation_id":"b0e89626-4760-4bd9-9352-1ab8b0bd99b5","resolution":{"observed_at":"2026-08-14T15:45:09.608268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9509006","last_updated":"1995-09-01T17:28:54Z","snapshot_observed_at":"2026-08-19T23:56:05.275318Z","submitted_at":"1995-09-01T17:28:54Z","title":"Coalescing Neutron Stars -- a Step Towards Physical Models. I. Hydrodynamic Evolution and Gravitational-Wave Emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9509006","snapshot_observed_at":"2026-08-14T15:45:09.612818Z","title":"Ruffert, H.-T","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.612818Z"},"links":{"cited_paper":"/paper/astro-ph/9509006","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:953be15d44f3adf1266653cff13e91009bb2b7fd9449d38a874af7d3ea4ed908","observation_id":"31e5b322-9c9b-4768-8699-2ddf1cecd0e6","resolution":{"observed_at":"2026-08-14T15:45:09.612818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302301","last_updated":"2003-02-15T11:53:53Z","snapshot_observed_at":"2026-08-17T11:51:46.872231Z","submitted_at":"2003-02-15T11:53:53Z","title":"High Resolution Calculations of Merging Neutron Stars II: Neutrino Emission","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302301","snapshot_observed_at":"2026-08-14T15:45:09.617233Z","title":"Rosswog and M","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.617233Z"},"links":{"cited_paper":"/paper/astro-ph/0302301","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:410d6752f36f03a607527741481f17ef296521c561595834ef15b219d028d526","observation_id":"0e30e231-95e7-4411-bf99-92077324718e","resolution":{"observed_at":"2026-08-14T15:45:09.617233Z","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":"2026-08-15T09:44:57.335615Z","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":"2026-08-14T15:45:09.621719Z","title":"Wanajo, Y","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.621719Z"},"links":{"cited_paper":"/paper/1402.7317","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:4cd3843f36e2f8c9f53179f36af027d9ac8edff3d053baba1b598c86c63e7b83","observation_id":"bde553ad-0c74-47c7-8902-4beafdb3e18d","resolution":{"observed_at":"2026-08-14T15:45:09.621719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.01607","last_updated":"2015-05-07T07:35:19Z","snapshot_observed_at":"2026-08-19T17:29:52.597988Z","submitted_at":"2015-05-07T07:35:19Z","title":"Effects of the microphysical Equation of State in the mergers of magnetized Neutron Stars With Neutrino Cooling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.01607","snapshot_observed_at":"2026-08-14T15:45:09.626688Z","title":"Palenzuela, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.626688Z"},"links":{"cited_paper":"/paper/1505.01607","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:ff74172b9b05260d871fb11cb70ca49996b34311a1381a6717d3d106a9d68471","observation_id":"848e3569-a056-49c3-989a-a058cbf7bf93","resolution":{"observed_at":"2026-08-14T15:45:09.626688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.631709Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.631709Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:1cb599901837d9939f0baccf132208bd24b6fc4fc6f399922dbe50f8ae456a5f","observation_id":"1d36209c-ee4f-4b45-acf6-aa7ffabf506d","resolution":{"observed_at":"2026-08-14T15:45:09.631709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.636325Z","title":"Foucart, M","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.636325Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:db210b2c4595e0234846ce008afd99596f64377f6d4302718116bd95635638ff","observation_id":"59cdb2ce-0ddd-4de0-84f6-4a7342522367","resolution":{"observed_at":"2026-08-14T15:45:09.636325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06398","last_updated":"2016-01-22T18:16:12Z","snapshot_observed_at":"2026-08-14T22:26:50.932522Z","submitted_at":"2015-10-21T20:04:14Z","title":"Low mass binary neutron star mergers : gravitational waves and neutrino emission","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06398","snapshot_observed_at":"2026-08-14T15:45:09.641401Z","title":"Foucart, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.641401Z"},"links":{"cited_paper":"/paper/1510.06398","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:ddba30535967fdb87de49d6fb6509c5ef8be83c6acd6b3edbbd676962f258916","observation_id":"4e15810d-30b9-4c5a-ac6d-535bad7d9048","resolution":{"observed_at":"2026-08-14T15:45:09.641401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.651109Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.651109Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:9a6092808f59bbadc40c159cf38390f8162c155be7e28a703ce2978b0f26052c","observation_id":"e31e1571-965a-4081-962a-f103558612c4","resolution":{"observed_at":"2026-08-14T15:45:09.651109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.3937","last_updated":"2011-04-20T04:24:29Z","snapshot_observed_at":"2026-08-15T04:48:51.556150Z","submitted_at":"2011-04-20T04:24:29Z","title":"Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.3937","snapshot_observed_at":"2026-08-14T15:45:09.655722Z","title":"Shibata, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.655722Z"},"links":{"cited_paper":"/paper/1104.3937","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:00c54f714dcb2a8bcb1d4dfc7bad1cf6eb56201704b9f3e897b87b6f79c96a64","observation_id":"436860e8-122d-4e4f-88bc-1fbbfba36f72","resolution":{"observed_at":"2026-08-14T15:45:09.655722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.660743Z","title":"Sekiguchi, K","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.660743Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:fc4436d67f2bb450ed0013bf33bd1b5e1707a9fc2713d515fd97d8a8b9a41cf8","observation_id":"9379817f-38f7-496d-8eca-15aa7f78bc5c","resolution":{"observed_at":"2026-08-14T15:45:09.660743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.665294Z","title":"Radice, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.665294Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:bb57f9837def00aa5eff49e24d1bc567d2f1a42d964a48e11fa4021425f87280","observation_id":"f20e171b-defa-4899-ad43-c70f0b3fa4d4","resolution":{"observed_at":"2026-08-14T15:45:09.665294Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.07450","last_updated":"2016-12-02T21:34:27Z","snapshot_observed_at":"2026-08-15T16:04:01.979770Z","submitted_at":"2016-07-25T20:00:05Z","title":"Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.07450","snapshot_observed_at":"2026-08-14T15:45:09.670041Z","title":"Foucart, E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.670041Z"},"links":{"cited_paper":"/paper/1607.07450","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:a99bcfbc210d2655e11e6bca88dd4dee070ab0436cd07b69ca6b580a231648dd","observation_id":"432edc64-f14f-41f6-b64f-94e379bfe808","resolution":{"observed_at":"2026-08-14T15:45:09.670041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.674809Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.674809Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:e488efc4ef0af635bdcb68d21e02ce4ca03462d3105569d5ad2424379ab97930","observation_id":"ac8c175a-a675-4bac-8a00-f86d46c14f96","resolution":{"observed_at":"2026-08-14T15:45:09.674809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.679953Z","title":"Lindblom, M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.679953Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:39b04bf19c3a5c33ed9bff7a0a45da1fc4e46ae7d89149dcad576607433c4636","observation_id":"0536d1e4-11cb-4280-ba58-621d2b1612ea","resolution":{"observed_at":"2026-08-14T15:45:09.679953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.684722Z","title":"Harten, P","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.684722Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:6c29b8c2183dd7a4dcf7fcf7e47bc7dcd668b7b52f60c0d3ddc207cbbf4c93d6","observation_id":"498703d0-7df8-4eeb-a185-24a6e458ab21","resolution":{"observed_at":"2026-08-14T15:45:09.684722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.346885Z","title":null,"venue":null,"work_id":"89554664-bb1a-4d37-bda2-6eabf0c89ac0","year":1994},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.689470Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:dc2ee2dca39401bdebce48b0a328d9b6b8383912f7df2ecdb44eb14279db6867","observation_id":"6d783205-607c-4242-99c8-ae1c1a8a550f","resolution":{"observed_at":"2026-08-14T15:45:11.352337Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.329287Z","title":"Jiang and C.-W","venue":null,"work_id":"169fee40-ceb2-4d53-a8d3-b78100a74a2f","year":1996},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.694275Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:14d089520da3335f0ddf6e476d8c12e55b2d97f416b95f9654c276000ba44e58","observation_id":"1028dd16-c0c8-4108-a409-cc20969907f0","resolution":{"observed_at":"2026-08-14T15:45:11.334895Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.311530Z","title":"Foucart, L","venue":null,"work_id":"42000493-3b2f-4ce7-88ef-14b373f6d613","year":2008},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.698942Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:fda9b8bf43710f9adc17b50d7c13c687ba2726114ee315d65977a3f3342ba37f","observation_id":"265d91ef-239a-4c8c-b724-5ac0033d52ea","resolution":{"observed_at":"2026-08-14T15:45:11.316969Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0202096","last_updated":"2002-02-27T14:59:18Z","snapshot_observed_at":"2026-07-07T03:15:29.974825Z","submitted_at":"2002-02-27T14:59:18Z","title":"A multidomain spectral method for solving elliptic equations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0202096","snapshot_observed_at":"2026-08-14T15:45:09.703524Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.703524Z"},"links":{"cited_paper":"/paper/gr-qc/0202096","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:a5c18e6e4889c56680c3b81bada4229de02d3721fc2c86d0b4b0fdded1104799","observation_id":"6cb09230-5712-4ef2-bc14-734d6e9da811","resolution":{"observed_at":"2026-08-14T15:45:09.703524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.293722Z","title":"Tacik, F","venue":null,"work_id":"b0092e8d-d171-4d89-b4df-2008b37442c3","year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.708576Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:d5081addbaf23c90bc7f4aa9cebf95e6425848dd6ca730edf34a6085a10c649d","observation_id":"d5431482-e866-4287-b01b-bf1ca4383dc4","resolution":{"observed_at":"2026-08-14T15:45:11.299077Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.00782","last_updated":"2016-06-25T18:55:01Z","snapshot_observed_at":"2026-08-15T07:43:34.319366Z","submitted_at":"2016-04-04T09:22:40Z","title":"Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.00782","snapshot_observed_at":"2026-08-14T15:45:09.713251Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.713251Z"},"links":{"cited_paper":"/paper/1604.00782","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:1a87d394e8a691f76f3461cc9394adb3e6fff46239c0c26c45d247590fe4ee80","observation_id":"f938be85-ab66-46a3-829a-63ee4830d391","resolution":{"observed_at":"2026-08-14T15:45:09.713251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.276019Z","title":null,"venue":null,"work_id":"99eb04b0-4489-473a-8a16-69d41fc37011","year":2003},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.718164Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:e3492bca37d9575eea9b7677ee13e4eb3ef2d47f32f03f0a06fe79ca1c0fe90f","observation_id":"8d18e086-08ef-48ab-9d16-da273a38b182","resolution":{"observed_at":"2026-08-14T15:45:11.281580Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.258545Z","title":null,"venue":null,"work_id":"282b68a3-ba49-4b4f-9599-fa4a600ffcc2","year":2007},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.722981Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:164f16f552bbe5004fffd63630e200ddf218d8787b55538ba739e56a1256def0","observation_id":"8eb0af7e-2263-47b5-9d67-62aa71e50098","resolution":{"observed_at":"2026-08-14T15:45:11.263800Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.240754Z","title":"Pretorius, Classical and Quantum Gravity 22, 425 (2005)","venue":null,"work_id":"e00feb90-cdde-460a-bc70-57c57a81b743","year":2005},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.727736Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7253d4f9b703f93f53beb8fe29bdf418a0b94acae11b806cc16d04517007b5fa","observation_id":"0a02db8b-79c3-4267-92cd-0c5fdafbf6be","resolution":{"observed_at":"2026-08-14T15:45:11.246490Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.220967Z","title":"Szil´ agyi, International Journal of Modern Physics D 23, 1430014 (2014)","venue":null,"work_id":"0214abf9-d6f4-44a2-9961-f624bf70e91a","year":2014},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.732340Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:e94a278d9818521fa7e1968c60f94d69dc1b9d6e38cda35f23b725a127e0b1ea","observation_id":"62d227b4-bf06-4af1-bfc0-828d75d87399","resolution":{"observed_at":"2026-08-14T15:45:11.227465Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.201320Z","title":"Foucart, E","venue":null,"work_id":"68a9587b-d94b-41ae-86cf-b6686abec5a9","year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.736875Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:c95e9133372edab1995396724ecbf3aaa585ef7506b033c025e963f91086ff4e","observation_id":"68daa163-7b79-460e-851f-db864f261285","resolution":{"observed_at":"2026-08-14T15:45:11.205644Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.185825Z","title":null,"venue":null,"work_id":"7bd77e6c-f3b9-45e5-bcaf-4a8c750546a0","year":1978},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.741170Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:fe9fefff476c143a3aba4c050add9f73f9e02ea388d90dcbac22cbd618ed2f59","observation_id":"4c860641-b701-45d3-a4f2-3976b89a1d62","resolution":{"observed_at":"2026-08-14T15:45:11.190645Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04146","last_updated":"2015-02-13T22:47:44Z","snapshot_observed_at":"2026-08-15T20:50:47.001446Z","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":"2026-08-14T15:45:09.745543Z","title":"Foucart, E","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.745543Z"},"links":{"cited_paper":"/paper/1502.04146","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:39358d0c73a10b57b5e782fb38240773ae27e6370bdbf2c4aa4c47e92c6abbc5","observation_id":"c941e1bd-d784-442d-a83e-883a7b74fcc8","resolution":{"observed_at":"2026-08-14T15:45:09.745543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.171347Z","title":"Shibata, K","venue":null,"work_id":"538cbd1a-3121-4c18-afda-d65154e8124b","year":2011},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.749359Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:fc4010f7ef939cffbae20e95b2ca56223e46a6c7d138c3a2c7a3c43bf4f34426","observation_id":"93969f7b-427a-484b-8262-f0dba1073fab","resolution":{"observed_at":"2026-08-14T15:45:11.175644Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404432","last_updated":"2004-04-21T21:27:30Z","snapshot_observed_at":"2026-08-20T01:10:29.959641Z","submitted_at":"2004-04-21T21:27:30Z","title":"Neutrino Opacities in Nuclear Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0404432","snapshot_observed_at":"2026-08-14T15:45:09.754021Z","title":"Burrows, S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.754021Z"},"links":{"cited_paper":"/paper/astro-ph/0404432","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:ef4795b7254991272bbf9788a5f74f2f1f3541ff5bc30ca820d7e3bce0382f18","observation_id":"019d980f-0fff-4c3e-b1a4-5a82d8ba5bb4","resolution":{"observed_at":"2026-08-14T15:45:09.754021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.155845Z","title":"Borges, M","venue":null,"work_id":"12e9fbbb-f132-4f82-af04-f7d2665776be","year":2008},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.758180Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:35252c2e8229e49ad08a93ca3d49687c79bd0f93fd64c76fc170c31304ba5a42","observation_id":"2d65bcbf-3240-4027-8110-c611a27cadb8","resolution":{"observed_at":"2026-08-14T15:45:11.160527Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:09.762216Z","title":"Walecka, Annals of Physics 83, 491 (1974)","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.762216Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:13032aa4b00c53ed1a268fb86d041aa6885cda9aa1722ce9c8a1f59bd373791a","observation_id":"627e0beb-1e74-47d3-b390-3977d9e1f963","resolution":{"observed_at":"2026-08-14T15:45:09.762216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.130079Z","title":null,"venue":null,"work_id":"eedcc3be-f86f-43c3-b20b-7e3a1f4ec194","year":1991},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.766323Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7f9aab79cf14a9566ce268224271536bb9d7711b743f0bd8c13079e798c4abf7","observation_id":"35bb7608-cba5-48c4-be0b-181f2e36a3d3","resolution":{"observed_at":"2026-08-14T15:45:11.135174Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0848","last_updated":"2012-11-22T15:11:18Z","snapshot_observed_at":"2026-08-18T13:49:02.027374Z","submitted_at":"2011-08-03T14:08:54Z","title":"New Equations of State in Simulations of Core-Collapse Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0848","snapshot_observed_at":"2026-08-14T15:45:09.770219Z","title":"Hempel, T","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.770219Z"},"links":{"cited_paper":"/paper/1108.0848","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:2cdfcf201d7e36660140657ad919ba601fe110e5a89e10d507d561d58aacd120","observation_id":"9e2f447b-15c6-4eac-a3c0-1f8c794c9ff1","resolution":{"observed_at":"2026-08-14T15:45:09.770219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.03772","last_updated":"2017-03-10T17:30:39Z","snapshot_observed_at":"2026-08-16T22:15:17.089586Z","submitted_at":"2017-03-10T17:30:39Z","title":"How Well Do We Know The Supernova Equation of State?","version":1},"cited_work":{"arxiv_id":"1703.03772","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.03772","snapshot_observed_at":"2026-08-14T15:45:10.254463Z","title":"How Well Do We Know The Supernova Equation of State?","venue":"nucl-th","work_id":"5fb20f0d-be20-4f49-b37f-b1970b88dd3d","year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.774519Z"},"links":{"cited_paper":"/paper/1703.03772","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:8a8a86d8d5a881d15bb2e05ad68711d4d986253504520141a4fbf5fcf02dfe90","observation_id":"c26c9e09-78a0-4e90-a955-2b721727263d","resolution":{"observed_at":"2026-08-14T15:45:10.261865Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.6871","last_updated":"2012-05-31T02:15:12Z","snapshot_observed_at":"2026-08-17T21:53:14.974409Z","submitted_at":"2012-05-31T02:15:12Z","title":"The Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.6871","snapshot_observed_at":"2026-08-14T15:45:09.778749Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.778749Z"},"links":{"cited_paper":"/paper/1205.6871","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:5a45dd886787946f3f33935aa32d657376c5fce7ce2fafa8580ed61ad74a3d66","observation_id":"f1c75dc9-9b7d-40b8-b982-b94782eddf73","resolution":{"observed_at":"2026-08-14T15:45:09.778749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.5788","last_updated":"2010-10-27T20:00:10Z","snapshot_observed_at":"2026-08-15T05:04:38.827864Z","submitted_at":"2010-10-27T20:00:10Z","title":"Shapiro delay measurement of a two solar mass neutron star","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.5788","snapshot_observed_at":"2026-08-14T15:45:09.783019Z","title":"Demorest, T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.783019Z"},"links":{"cited_paper":"/paper/1010.5788","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:980edf0e5cddb9067336e6b6d06e6768818d9de910a6014857ca1a802c79763d","observation_id":"02d827af-3c08-41d5-a4e2-976b3bf217a6","resolution":{"observed_at":"2026-08-14T15:45:09.783019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.11581","last_updated":"2018-10-15T17:59:04Z","snapshot_observed_at":"2026-08-20T05:33:33.272209Z","submitted_at":"2018-05-29T16:56:13Z","title":"GW170817: Measurements of Neutron Star Radii and Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.11581","snapshot_observed_at":"2026-08-14T15:45:09.788154Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.788154Z"},"links":{"cited_paper":"/paper/1805.11581","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:55cf81170d31f8e138632dff3fb9eedb615d42e794b41b47b49411a59c4a46e1","observation_id":"4e507c97-cdd0-4def-aae2-c612126bae2d","resolution":{"observed_at":"2026-08-14T15:45:09.788154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.114127Z","title":"Bauswein, T","venue":null,"work_id":"b0bbcd0a-bfba-4c9b-af56-104b9764fd68","year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.793640Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:6ec97f4eaf3f5419544d7d8b9a361c59a0b69fef94f015d534a619432f27d94e","observation_id":"96b8b0bb-8fbc-4901-8a33-7863ae0a5c22","resolution":{"observed_at":"2026-08-14T15:45:11.119120Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3510","last_updated":"2013-05-15T14:59:02Z","snapshot_observed_at":"2026-08-17T22:35:56.062775Z","submitted_at":"2013-05-15T14:59:02Z","title":"The Nuclear Equation of State and Neutron Star Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3510","snapshot_observed_at":"2026-08-14T15:45:09.798031Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.798031Z"},"links":{"cited_paper":"/paper/1305.3510","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:c297e4fb92fe75097a99c8ef66ef19c659e09df7e63e3eca03e173ae1e22a8c6","observation_id":"4e88eeb4-1238-49e5-82de-4285d6fbbd0e","resolution":{"observed_at":"2026-08-14T15:45:09.798031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.097951Z","title":"Rezzolla and O","venue":null,"work_id":"ab6b5911-e5f0-4aa2-8bcc-23b5f3ae7718","year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.803500Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:dd12ebc615c5163e358e5ed37953c6a95f869ab1d0525c36fe56e05c7304cec8","observation_id":"b9378376-caf1-4f77-81b8-a6223e464314","resolution":{"observed_at":"2026-08-14T15:45:11.102698Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1411.7975","last_updated":"2015-04-08T17:03:35Z","snapshot_observed_at":"2026-08-18T06:49:21.359156Z","submitted_at":"2014-11-28T19:03:43Z","title":"Properties of hypermassive neutron stars formed in mergers of spinning binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.7975","snapshot_observed_at":"2026-08-14T15:45:09.812997Z","title":"Kastaun and F","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.812997Z"},"links":{"cited_paper":"/paper/1411.7975","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:7eaf7d88972c7aa624b6da85206a5ce4d84f2a1cb87bf7c459206c4b79a4f5d4","observation_id":"c8562f99-ce38-4912-8301-c4d805b1df78","resolution":{"observed_at":"2026-08-14T15:45:09.812997Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0905","last_updated":"2013-01-31T04:35:00Z","snapshot_observed_at":"2026-08-15T00:37:07.133067Z","submitted_at":"2012-12-04T23:47:33Z","title":"The mass ejection from the merger of binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.0905","snapshot_observed_at":"2026-08-14T15:45:09.817893Z","title":"Hotokezaka, K","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.817893Z"},"links":{"cited_paper":"/paper/1212.0905","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:36522443789efa7f231edffae3966d0be98b7cda6f613419fb8d7a39dc48473d","observation_id":"b5f7d579-17ec-407e-921b-a6a4b0b16c1c","resolution":{"observed_at":"2026-08-14T15:45:09.817893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2660","last_updated":"2014-07-14T17:56:17Z","snapshot_observed_at":"2026-08-19T13:56:16.581856Z","submitted_at":"2014-07-10T00:50:27Z","title":"High resolution numerical-relativity simulations for the merger of binary magnetized neutron stars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2660","snapshot_observed_at":"2026-08-14T15:45:09.823834Z","title":"Kiuchi, K","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.823834Z"},"links":{"cited_paper":"/paper/1407.2660","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:a00a452a99334f21f33d32b4d65ec224f4e4d0ee61471d60fc0190bbf26a62fc","observation_id":"8ca37265-a8f2-409c-9542-ca25b8f1cb3a","resolution":{"observed_at":"2026-08-14T15:45:09.823834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.082863Z","title":"Neilsen, S","venue":null,"work_id":"049e088a-a6b3-477d-ac45-847543bbfbad","year":2014},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.829382Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:89f20cf39ad6a01eb7a7d56ede15adf1c652e4f411fccf1264d7458fa168fea5","observation_id":"4b4a2b43-ba0a-4c7b-99b8-655d51491f7e","resolution":{"observed_at":"2026-08-14T15:45:11.087608Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1808.00461","last_updated":"2018-10-27T22:02:39Z","snapshot_observed_at":"2026-08-14T18:45:24.720722Z","submitted_at":"2018-08-01T18:00:01Z","title":"Long-term GRMHD Simulations of Neutron Star Merger Accretion Disks: Implications for Electromagnetic Counterparts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.00461","snapshot_observed_at":"2026-08-14T15:45:09.834286Z","title":"Fernandez, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.834286Z"},"links":{"cited_paper":"/paper/1808.00461","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:a121bb467adc48188e437fe9e49dbec8147d844585a68e389392a04bb8814b85","observation_id":"de733871-d32c-4fe0-ae15-d62867d163b7","resolution":{"observed_at":"2026-08-14T15:45:09.834286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03665","last_updated":"2016-12-12T13:24:28Z","snapshot_observed_at":"2026-08-14T21:26:00.313156Z","submitted_at":"2016-12-12T13:24:28Z","title":"Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03665","snapshot_observed_at":"2026-08-14T15:45:09.839105Z","title":"Dietrich and M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.839105Z"},"links":{"cited_paper":"/paper/1612.03665","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:d00c7422ea375de53b2e8747d7104052d793fd36cecf8b6182755d23e609d523","observation_id":"8392831f-8407-4e47-8e3d-92f379e7b0a3","resolution":{"observed_at":"2026-08-14T15:45:09.839105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5787","last_updated":"2013-03-22T22:18:44Z","snapshot_observed_at":"2026-08-16T00:39:59.643857Z","submitted_at":"2013-03-22T22:18:44Z","title":"Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5787","snapshot_observed_at":"2026-08-14T15:45:09.843704Z","title":"Barnes and D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.843704Z"},"links":{"cited_paper":"/paper/1303.5787","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:5ffa9c210e03b4201e164c6b7fd6a52c6ae2fb0d1b762f8d8a120fce3c191e30","observation_id":"5b496203-3699-4216-9876-a1257b9eaed8","resolution":{"observed_at":"2026-08-14T15:45:09.843704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.03133","last_updated":"2015-11-02T21:48:41Z","snapshot_observed_at":"2026-08-14T22:36:41.466167Z","submitted_at":"2015-08-13T07:13:19Z","title":"r-Process Lanthanide Production and Heating Rates in Kilonovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.03133","snapshot_observed_at":"2026-08-14T15:45:09.848438Z","title":"Lippuner and L","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.848438Z"},"links":{"cited_paper":"/paper/1508.03133","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:99e4c94d20ef5914cddec698caa2cdf841015313aac21d22031a0c014fb330df","observation_id":"95b361dc-643c-4e92-ba05-9bb5eb47b51e","resolution":{"observed_at":"2026-08-14T15:45:09.848438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5788","last_updated":"2013-03-22T22:24:13Z","snapshot_observed_at":"2026-08-15T00:24:08.344186Z","submitted_at":"2013-03-22T22:24:13Z","title":"Opacities and Spectra of the r-process Ejecta from Neutron Star Mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5788","snapshot_observed_at":"2026-08-14T15:45:09.853365Z","title":"Kasen, N","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.853365Z"},"links":{"cited_paper":"/paper/1303.5788","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:b51829d25799799610377f5b6b0bb12249847d9afcd299f53d6076ae1945074f","observation_id":"9c8096cc-0b20-4db9-bc38-a4c88e9400c7","resolution":{"observed_at":"2026-08-14T15:45:09.853365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.07711","last_updated":"2016-09-02T06:35:35Z","snapshot_observed_at":"2026-08-14T22:12:44.342389Z","submitted_at":"2016-01-28T10:12:21Z","title":"Models of Kilonova/macronova emission from black hole-neutron star mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.07711","snapshot_observed_at":"2026-08-14T15:45:09.858220Z","title":"Kawaguchi, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.858220Z"},"links":{"cited_paper":"/paper/1601.07711","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:1b5d23a2e0229d19d15d79416f854aa4ca0d6c5b74b3e8ac473ef547e48ea747","observation_id":"af86a129-68c3-4b63-af15-a5d071d30964","resolution":{"observed_at":"2026-08-14T15:45:09.858220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.01159","last_updated":"2016-11-03T20:00:02Z","snapshot_observed_at":"2026-08-14T21:32:04.489059Z","submitted_at":"2016-11-03T20:00:02Z","title":"Dynamical ejecta from precessing neutron star-black hole mergers with a hot, nuclear-theory based equation of state","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.01159","snapshot_observed_at":"2026-08-14T15:45:09.863263Z","title":"Foucart, D","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.863263Z"},"links":{"cited_paper":"/paper/1611.01159","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:6c803da7ac5b5339d35e0b24c45d1a9009d286549f87815cf3ff69eca3279f87","observation_id":"2bf3c6e1-2206-45dc-bd43-9dfda8333922","resolution":{"observed_at":"2026-08-14T15:45:09.863263Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05931","last_updated":"2017-10-16T18:00:12Z","snapshot_observed_at":"2026-08-20T19:30:18.188478Z","submitted_at":"2017-10-16T18:00:12Z","title":"Welcome to the Multi-Messenger Era! Lessons from a Neutron Star Merger and the Landscape Ahead","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05931","snapshot_observed_at":"2026-08-14T15:45:09.868274Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.868274Z"},"links":{"cited_paper":"/paper/1710.05931","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:40b8702ef8b3be153f0d86c125fb8859ff4934499d391a14d8154d2d8d849d40","observation_id":"7df99d63-f773-4e8c-8d99-26e7a47112d7","resolution":{"observed_at":"2026-08-14T15:45:09.868274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.07579","last_updated":"2017-12-04T10:54:24Z","snapshot_observed_at":"2026-08-18T09:14:32.098559Z","submitted_at":"2017-10-20T15:43:00Z","title":"Modeling GW170817 based on numerical relativity and its implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.07579","snapshot_observed_at":"2026-08-14T15:45:09.873300Z","title":"Shibata, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.873300Z"},"links":{"cited_paper":"/paper/1710.07579","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:772177261d1d51ec4b005dc605e8ff649bbd0251a70ae515238a92002c0d5bc8","observation_id":"5d3b7cc2-9ebd-42fd-9e27-dc3081428556","resolution":{"observed_at":"2026-08-14T15:45:09.873300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05473","last_updated":"2017-11-02T18:07:50Z","snapshot_observed_at":"2026-08-14T21:00:32.952589Z","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":"2026-08-14T15:45:09.877715Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.877715Z"},"links":{"cited_paper":"/paper/1705.05473","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:e536ada84f5e4b9779cd89e754db38373d1b6761664bf7d9d96c4c89d167f006","observation_id":"431b1203-110d-42bf-a26c-7d69729e3dc0","resolution":{"observed_at":"2026-08-14T15:45:09.877715Z","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":"2026-08-14T23:30:51.448456Z","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":"2026-08-14T15:45:09.882560Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.882560Z"},"links":{"cited_paper":"/paper/1406.2687","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:30457381cff189478e1f862634c0c1b2603e4d6e8750d01b3e30ceb9e52e6c5b","observation_id":"44d83b2a-eff3-4e9e-9029-9788ee6a7c0e","resolution":{"observed_at":"2026-08-14T15:45:09.882560Z","resolver_source":null,"status":"unresolved"},"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":"2026-08-15T00:20:03.334607Z","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":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6720","snapshot_observed_at":"2026-08-14T15:45:09.888234Z","title":"Fern´ andez and B","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.888234Z"},"links":{"cited_paper":"/paper/1304.6720","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:2efef558a45825facf3864cf372d77b2e672e786084c0ae7429f9e8e91f2486c","observation_id":"1a83ea94-7d14-49cb-aadd-552840450170","resolution":{"observed_at":"2026-08-14T15:45:09.888234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.066311Z","title":"Hanauske, K","venue":null,"work_id":"6278b465-c344-462c-830f-1b6af85036ca","year":2017},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.892608Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:f5b8b1dc264e772dcad7856d8899314d7bf0d1939df4c15b3a30ffb2a8f4dec6","observation_id":"96b3f572-ac6a-4b97-9192-8504ffaef9c1","resolution":{"observed_at":"2026-08-14T15:45:11.071446Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.01918","last_updated":"2016-03-07T02:26:25Z","snapshot_observed_at":"2026-08-14T22:07:17.593082Z","submitted_at":"2016-03-07T02:26:25Z","title":"Dynamical mass ejection from the merger of asymmetric binary neutron stars: Radiation-hydrodynamics study in general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.01918","snapshot_observed_at":"2026-08-14T15:45:09.898057Z","title":"Sekiguchi, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.898057Z"},"links":{"cited_paper":"/paper/1603.01918","citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:c0cccdd34086e81c89e2984568d5702ae643858e399d04c119375a5024b27012","observation_id":"08848d93-0430-4197-bee5-ffbd5bcd9e9e","resolution":{"observed_at":"2026-08-14T15:45:09.898057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T15:45:11.051106Z","title":"Loken, D","venue":null,"work_id":"ad9d7ae5-8f45-494a-a1ad-573fac24dbc4","year":2010},"citing_paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-14T15:45:09.902947Z"},"links":{"citing_paper":"/paper/1908.00655"},"observation_digest":"sha256:cfe2b1fd377d5891da340c92a6ba13223860ac12e8d8d4c8f5e57a725e918f9f","observation_id":"40c24683-b7f5-4f74-bce3-fef0a4bce27a","resolution":{"observed_at":"2026-08-14T15:45:11.055769Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.00655","last_updated":"2019-08-01T23:03:45Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-18T10:34:31.114570Z","submitted_at":"2019-08-01T23:03:45Z","title":"Unequal Mass Binary Neutron Star Simulations with Neutrino Transport: Ejecta and Neutrino Emission"},"reference_resolution":{"displayed":92,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":77,"verified_exact":2,"verified_fuzzy":13},"total_outbound_references":92},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 92 of 92 outbound references and 1 inbound Pith citation observation for arXiv:1908.00655."}