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Paper Citation Record · LEDGER

Late-time emission-line profiles from kilonova models

As of 19 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 0 inbound Pith citation observations for arXiv:2607.10818.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2607.10818 v1

Coverage vector

measured 74 of 74 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-14T09:02:10.553457Z

measured 74 of 74 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

74 of 74 outbound references displayed

  • verified exact14
  • verified fuzzy0
  • unresolved56
  • parse uncertain4
  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation d7499e9f-7690-4dce-9830-61ce826badda · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 1

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:5b72e962a50ac009ad59ffb4aea29a508d3157772404009cba6b950d1ac65220

Observation 0fa2b5d5-efc6-4476-a7bc-72d35b6a1914 · outbound

This paper cites Superluminal motion of a relativistic jet in the neutron star merger GW170817.

Late-time emission-line profiles from kilonova models Superluminal motion of a relativistic jet in the neutron star merger GW170817

Reference 2

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:18ce3adc03dcf7336bd1a9c47e34e4392a4fffa69ea89a82fc2ddaa1a5e23b6e

Observation 5e9c6957-4558-48bd-8828-4cdbcab4ddb6 · outbound

This paper cites Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger.

Late-time emission-line profiles from kilonova models Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger

Reference 3

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local_arxiv, observed 2026-07-14T09:10:22.603410Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:fc1c6f3b6ddffde674930c2f39a99be277fad4616c2cd026e1e90d6ae274b6ea

Observation 3049f7db-e3de-43e5-86cc-3f33e67bb6a2 · outbound

This paper cites The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference.

Late-time emission-line profiles from kilonova models The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference

Reference 4

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:d1e1937f395acc0f84f3116a5d99367ba050393852b1dabb7239a6e41f8c1600

Observation 75d957f2-5603-4175-ba43-fa5e818753bd · outbound

This paper cites A Broad Grid of 2D Kilonova Emission Models.

Late-time emission-line profiles from kilonova models A Broad Grid of 2D Kilonova Emission Models

Reference 5

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local_arxiv, observed 2026-07-14T09:10:22.510269Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:11a3778c9567398cdb90e7cf4f6c14da640564bdce26609989dae15e550f42af

Observation bd051138-c4a2-4e1c-9eda-ed54246953b9 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 6

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:7a7437f89d1159e7e2c762ba8c1482f7dfae626c55493310c2fe785d967a7947

Observation a26ca83f-01de-4c42-a5b0-2a8797eaa93e · outbound

This paper cites Polarized kilonovae from black hole-neutron star mergers.

Late-time emission-line profiles from kilonova models Polarized kilonovae from black hole-neutron star mergers

Reference 7

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local_arxiv, observed 2026-07-14T09:10:22.430322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:86b35f37f7cf2bf57c93b947f44106d070a4041c522545b2f3f8137654efa195

Observation 2a8749e8-ece2-47c3-919c-dc687ea466cd · outbound

This paper cites Inclination Dependence of Kilonova Light Curves from Globally Aspherical Geometries.

Late-time emission-line profiles from kilonova models Inclination Dependence of Kilonova Light Curves from Globally Aspherical Geometries

Reference 8

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local_arxiv, observed 2026-07-14T09:10:22.437330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a0834ffb25f7d6b48b1e1e209ba91526c1e32b55c9229c63c04d403297ad5746

Observation b6d6c9ff-f4a8-4abe-bb28-a7f11ae3a0ae · outbound

This paper cites Radiative Transfer Simulations for Neutron Star Merger Ejecta.

Late-time emission-line profiles from kilonova models Radiative Transfer Simulations for Neutron Star Merger Ejecta

Reference 9

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:0817345ab34e7466119f3e984f52a8dfcd936406bab72448064de58f766d6f5c

Observation 74576fd8-f259-4f9f-9b39-3c10d8a01b68 · outbound

This paper cites Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer.

Late-time emission-line profiles from kilonova models Tungsten vs Selenium as a potential source of kilonova nebular emission observed by Spitzer

Reference 10

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:161e0a1e2b9921a43107042ab482436400eba1b2cd160776d8011afffe6b747e

Observation 679eab32-5d7f-4a7b-b63f-3d2fbff2fe28 · outbound

This paper cites A kilonova as the electromagnetic counterpart to a gravitational-wave source.

Late-time emission-line profiles from kilonova models A kilonova as the electromagnetic counterpart to a gravitational-wave source

Reference 11

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:4741e35317ca3efdf455b4cc7b164c2cc062f0836b2c1b285b4e0e975503d2a5

Observation 4ea592f4-feda-425b-8b67-0fcb0699a569 · outbound

This paper cites Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger.

Late-time emission-line profiles from kilonova models Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

Reference 12

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:dc78118f495c78825269cf809460c7b1bc92f69da1df5f559cf9cb2312dea15e

Observation c480ecb7-6678-4dc1-b162-b9c170e0e84d · outbound

This paper cites Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A.

Late-time emission-line profiles from kilonova models Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

Reference 13

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:7f1a7a3c1318d7dda77319e584f330ba995cd408fc5ca00d78cc83c953c8a3be

Observation 96993f88-f321-4d80-8208-dbfc7afd0ce3 · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , volume=.

Late-time emission-line profiles from kilonova models Monthly Notices of the Royal Astronomical Society , volume=

Reference 14

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:edecda2499b65bd7244a62999c53758469c93082dcef02edc87bd3937fe2efda

Observation 1a39db97-ccc6-457c-9fff-826b720d620e · outbound

This paper cites Journal of Physics B: Atomic, Molecular and Optical Physics , volume=.

Late-time emission-line profiles from kilonova models Journal of Physics B: Atomic, Molecular and Optical Physics , volume=

Reference 15

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:65d41e5a98912c7b64caca0843803b11ad5cf9c55ed58dacfd18c297cde23d96

Observation 9f167a86-d111-424e-abb7-287b6af895e3 · outbound

This paper cites 2025 , eprint=.

Late-time emission-line profiles from kilonova models 2025 , eprint=

Reference 16

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:1f54958549063d96b0c491ebac905090b36b8cfbba09d21d9d2bda5ccc663e62

Observation e8a56f95-04dc-4f67-b665-e3b7b44871a9 · outbound

This paper cites Spherical symmetry in the kilonova AT2017gfo/GW170817.

Late-time emission-line profiles from kilonova models Spherical symmetry in the kilonova AT2017gfo/GW170817

Reference 17

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verified exact
local_arxiv, observed 2026-07-14T09:10:22.393800Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:e907cc24a3c74af6d1daff410e9a5cb68d28d493115100662298b938ba65acb1

Observation 5b9d7026-6c24-4b85-89d9-f0d8c2c2f960 · outbound

This paper cites 3D radiative transfer kilonova modelling for binary neutron star merger simulations.

Late-time emission-line profiles from kilonova models 3D radiative transfer kilonova modelling for binary neutron star merger simulations

Reference 18

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a9a2d9bcb93be2daf75e558d9882fefc603bb245392b6613dae269a786677234

Observation 01691a40-12bd-4925-b93a-791d589c136d · outbound

This paper cites Towards inferring the geometry of kilonovae.

Late-time emission-line profiles from kilonova models Towards inferring the geometry of kilonovae

Reference 19

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:3fdc86ea107bb1a17f636e36324674f01c1d4d4570bd0ff9d6902df34c1c17a3

Observation 63f78488-c277-45d1-863d-15cb2c623e7b · outbound

This paper cites Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations.

Late-time emission-line profiles from kilonova models Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations

Reference 20

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a35242fdc8460b99e020e71756d1fd57c56472e19b7e0a07c62199622f869f28

Observation 05ee7351-1220-4386-93fb-dc092ad7344f · outbound

This paper cites Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles.

Late-time emission-line profiles from kilonova models Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles

Reference 21

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local_arxiv, observed 2026-07-14T09:10:22.463573Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:9513da648b20c3ba763725b65509e05920ed9ef5d013aa0a029175f9fa500b3e

Observation 83f8d88b-2ff1-47c9-bb54-48d6238a7b06 · outbound

This paper cites Actinide signatures in low electron fraction kilonova ejecta.

Late-time emission-line profiles from kilonova models Actinide signatures in low electron fraction kilonova ejecta

Reference 22

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f396e0988800bbb463fc21b2362e2a277f5762457d3e04030092707c5137e9eb

Observation 57ffa23e-d538-4ade-a6f9-3db2d2c1b429 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 23

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no resolver link, observed 2026-07-14T09:02:10.553457Z

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a26a8cc3391bbe362a8466017a60b037ef4d8dfa1ffcd23dfce17935558e2213

Observation 54f82fac-0408-4c13-b80f-d7da1251d385 · outbound

This paper cites Nebular Emission from Lanthanide-rich Ejecta of Neutron Star Merger.

Late-time emission-line profiles from kilonova models Nebular Emission from Lanthanide-rich Ejecta of Neutron Star Merger

Reference 24

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no resolver link, observed 2026-07-14T09:02:10.553457Z

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:5a338a01dcf401d24062e519b268b454907c82fd1d028bb92a83473fcc971631

Observation 1c65ca19-1ad4-4f31-af33-560f3342ae3b · outbound

This paper cites NLTE Spectra of Kilonovae.

Late-time emission-line profiles from kilonova models NLTE Spectra of Kilonovae

Reference 25

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:43bf59e5e5edcbc139ed90fade4ac3a30efea82b36eaeef774f6b9527b662674

Observation d8fb0d4b-ae84-4c47-b496-b96435403ab5 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 26

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no resolver link, observed 2026-07-14T09:02:10.553457Z

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:e1451114c0c8e442a639b986c1580d9a2f45c9a477831a1adbbf6b941a8eb294

Observation e8fbd7a7-f6d9-40c1-b1dc-27343dc753ec · outbound

This paper cites Living Reviews in Computational Astrophysics , keywords =.

Late-time emission-line profiles from kilonova models Living Reviews in Computational Astrophysics , keywords =

Reference 27

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no resolver link, observed 2026-07-14T09:02:10.553457Z

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:3d41a88f6eb3ef41094435e1400e90b21f533210355770bdb62abd8411a24c1f

Observation 56b91c27-d6d3-42db-b749-aeb7cb182639 · outbound

This paper cites Modelling the spectra of the kilonova AT2017gfo -- II: Beyond the photospheric epochs.

Late-time emission-line profiles from kilonova models Modelling the spectra of the kilonova AT2017gfo -- II: Beyond the photospheric epochs

Reference 28

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local_arxiv, observed 2026-07-14T09:10:22.444967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:9f67bfc5d3e98bb5449eeea12c77df0cc66fffa8aad53ac77188d3072853fe94

Observation 26521d77-7862-423e-a46b-4775a7ce73c0 · outbound

This paper cites Diagnostics of 3D explosion asymmetries of stripped-envelope supernovae by nebular line profiles.

Late-time emission-line profiles from kilonova models Diagnostics of 3D explosion asymmetries of stripped-envelope supernovae by nebular line profiles

Reference 29

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verified exact
local_arxiv, observed 2026-07-14T09:10:22.615630Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:52afaff84d28fae1946a628c5cc42047c014b6f8a5ddb78c45021fad59b71ff1

Observation 0f3e625f-6461-487d-928e-4919e33a397c · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 30

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:8848489bcb4d3e2da76a60b40206acdbac11a14dbfe74e1230d7b3a5344a480d

Observation 17565cf1-2d28-4848-b517-fe9994313fc5 · outbound

This paper cites Emission line models for the lowest mass core-collapse supernovae -- II. 3D NLTE radiative transfer modelling of a $9.0\,M_\odot$ neutrino-driven explosion.

Late-time emission-line profiles from kilonova models Emission line models for the lowest mass core-collapse supernovae -- II. 3D NLTE radiative transfer modelling of a $9.0\,M_\odot$ neutrino-driven explosion

Reference 31

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:96be93ca2ea28b60c1cb558852a3e1c9596eddc11644fedd623f599605f858aa

Observation f2a67d4b-8de9-4762-821f-12d643da2c87 · outbound

This paper cites ExTraSS: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients.

Late-time emission-line profiles from kilonova models ExTraSS: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients

Reference 32

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:64484e62b1155d8bdc52766a4a458d48146afa54b7250a4bde8e3d2cdfda95ff

Observation 388d91bf-8434-4f9a-952a-b6c4bfe1668b · outbound

This paper cites Springer International Publishing.

Late-time emission-line profiles from kilonova models Springer International Publishing

Reference 33

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f14cf6bd6bd207a6f680390f91ca48e1ede64710d2fcfb0cd2a718b717e2bbe2

Observation 6ce15fb0-2fde-4f71-a9ef-6effed51475e · outbound

This paper cites Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova.

Late-time emission-line profiles from kilonova models Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova

Reference 34

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verified exact
local_arxiv, observed 2026-07-14T09:10:22.597202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:5e5a9d4968437abfa41552e37b72cc9b774600fd77ff714abfd42174d79fa0b4

Observation 85a62f73-8978-41fe-ad5c-f93a864baf02 · outbound

This paper cites Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks.

Late-time emission-line profiles from kilonova models Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks

Reference 35

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verified exact
local_arxiv, observed 2026-07-14T09:10:22.526624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:1b8cdc535cceec75456a1166efce87848826821297f37534fd93dfdf78587d7c

Observation 28d05afc-49ca-4351-8938-7d8ea0e57260 · outbound

This paper cites End-to-end kilonova models of neutron-star mergers with delayed black-hole formation.

Late-time emission-line profiles from kilonova models End-to-end kilonova models of neutron-star mergers with delayed black-hole formation

Reference 36

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source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:acd30d2efc3b578de6c02414b7a89ac20fca5551c4035a2ef2866e064723112f

Observation aa9dddef-7c57-4733-b920-bf769c7902aa · outbound

This paper cites Tellurium emission line in kilonova AT 2017gfo.

Late-time emission-line profiles from kilonova models Tellurium emission line in kilonova AT 2017gfo

Reference 37

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unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:41d0addf46dbc9c03d6c4a6a235e67a364cdced72b2b0a6c4fc42a937430bb1a

Observation e9148b93-191c-4300-a05c-1778a4e8d920 · outbound

This paper cites Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A.

Late-time emission-line profiles from kilonova models Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A

Reference 38

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:5a277766191ef2f06545dd04c8a390bfcb1c543b6de6e11b9ba1c022e3e9d9ef

Observation e01b136a-cd50-4cfa-b139-50d2319133fd · outbound

This paper cites JWST detection of heavy neutron capture elements in a compact object merger.

Late-time emission-line profiles from kilonova models JWST detection of heavy neutron capture elements in a compact object merger

Reference 39

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f2ad6805320dfa9d6a8ed1d444e82d1ab7dfacb62bb02191c2eac02961f57c3a

Observation c93b2a51-8cc2-4f60-afe3-8ef787ac1293 · outbound

This paper cites R-process heating implementation in hydrodynamic simulations with neural networks.

Late-time emission-line profiles from kilonova models R-process heating implementation in hydrodynamic simulations with neural networks

Reference 40

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:36e5c3909853b7a228bdcf000b4469c703951df862bbc9ffccc130791ca59238

Observation 55865e37-7ecc-48da-9f7d-cfb82cbadbfe · outbound

This paper cites Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers.

Late-time emission-line profiles from kilonova models Production of all the r-process nuclides in the dynamical ejecta of neutron star mergers

Reference 41

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:84028716030c60f84459e06f2bc363c862c6420b4cf3c931268ffe756d042197

Observation 3b69a483-3a77-44f5-b8a4-05e6a00f06fc · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 42

Resolution
parse uncertain
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:3a96a7b0df73d09cf1ff524562a06e305abcc7e4f0177199bbf924f74d88da70

Observation eff4560b-07c0-4960-832b-5cc56c186c00 · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 43

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:bc1d08b2d64551d8706b3faa1a3c8bfda985019f176ca31586b9882899f72912

Observation 62429f2e-04a7-41b7-86da-e095e45ffd01 · outbound

This paper cites Jets from neutron-star merger remnants and massive blue kilonovae.

Late-time emission-line profiles from kilonova models Jets from neutron-star merger remnants and massive blue kilonovae

Reference 44

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a51b3f8edc7dbad6fe2c93c2a8dfb0b44d34eb646cf79a02f64795805e215842

Observation 7cda6569-030e-43a2-ad6e-547eb555a47a · outbound

This paper cites Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers.

Late-time emission-line profiles from kilonova models Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers

Reference 45

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:d82fa35d224895f58e0e4b7e76cab9fe963821c36b00d3a4ea1bcede1adaa9ae

Observation 8fbd5e5f-6a30-4b26-bdf0-c9212d9b22a0 · outbound

This paper cites The interplay of disk wind and dynamical ejecta in the aftermath of neutron star - black hole mergers.

Late-time emission-line profiles from kilonova models The interplay of disk wind and dynamical ejecta in the aftermath of neutron star - black hole mergers

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:10:22.558253Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:ab07f79ba92dc929b0e4de36323ad54b5387cc17005faafa89c88067f80f851b

Observation b30277d0-2505-4e35-ba1e-51316a9d8f68 · outbound

This paper cites Post-merger evolution of a neutron star-black hole binary with neutrino transport.

Late-time emission-line profiles from kilonova models Post-merger evolution of a neutron star-black hole binary with neutrino transport

Reference 47

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:fd7644f81edf9472ce633c2ed91c4ba690d2c0cb5961cced1eacb269b574482d

Observation 80c1d1b5-0951-47fd-9dcc-df0a2813d712 · outbound

This paper cites Post-merger Mass Ejection of Low-mass Binary Neutron Stars.

Late-time emission-line profiles from kilonova models Post-merger Mass Ejection of Low-mass Binary Neutron Stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:471929ae0b3199de9e5436736904e3b34bde4d0b456f19622da88203ad6ea1ec

Observation ceb60e2f-3348-4b1c-adc8-9eff305f42f5 · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 49

Resolution
parse uncertain
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:2413e885c75dd81dd86d13cad1c23bde90ec2e642825b7974844344a97d6cc25

Observation 11aa6471-7bb1-4b9a-a80a-9cb6fe614430 · outbound

This paper cites Delayed outflows from black hole accretion tori following neutron star binary coalescence.

Late-time emission-line profiles from kilonova models Delayed outflows from black hole accretion tori following neutron star binary coalescence

Reference 50

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:10:22.468244Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:c767f244437750fc98b408f0fd6341ee135dc2cf1b4fa529d6b66ab627f209d9

Observation d0f1728f-35cd-4030-a467-a5a3511d5ef2 · outbound

This paper cites Three-dimensional GRMHD simulations of the remnant accretion disks from neutron star mergers: outflows and r-process nucleosynthesis.

Late-time emission-line profiles from kilonova models Three-dimensional GRMHD simulations of the remnant accretion disks from neutron star mergers: outflows and r-process nucleosynthesis

Reference 51

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:ebefee32279d8780e36c8f5dd3de4832b58408670596a6b5425e51005b3384ee

Observation 433a93bf-c34f-40d3-b41c-6e700d28bffe · outbound

This paper cites Element formation in radiation-hydrodynamics simulations of kilonovae.

Late-time emission-line profiles from kilonova models Element formation in radiation-hydrodynamics simulations of kilonovae

Reference 52

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:830469dcb792d5ff09ab409737b70cfe5edfcb1c1574eeffc2623f183f47f4f8

Observation 031ef0aa-6fef-49de-96ce-ee60bb0d8034 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 53

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:9e1c8c4852cef51088c3f2aedc667c4d374be3442b620818e88039ce295f89b0

Observation 17cc2826-583e-4b72-906c-69243d3bfe88 · outbound

This paper cites A low-mass binary neutron star: long-term ejecta evolution and kilonovae with weak blue emission.

Late-time emission-line profiles from kilonova models A low-mass binary neutron star: long-term ejecta evolution and kilonovae with weak blue emission

Reference 54

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:3de7c7a3380788a74327566c5a9235ef45aaf82dc79b19e71db64f3becdec2cc

Observation 7719b4e9-40ed-4e1d-8c54-9e030873ebb3 · outbound

This paper cites Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers.

Late-time emission-line profiles from kilonova models Impact of ejecta morphology and composition on the electromagnetic signatures of neutron star mergers

Reference 55

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f8709771d589cdd56bf7a479b9f7c09b4d5a7003b1878cc13acc015122c3ad32

Observation 7e21520e-453d-47d3-8eb0-6d57b86da571 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 56

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:acc23ec8dd2fcf1e9863d0b9eb9546ec3db418b55ee14d6da03dea8dd8d203fc

Observation eebefc32-d22c-496f-afb0-c37cc0fe118a · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 57

Resolution
parse uncertain
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:277eabe5b5f089b1802bdef4bc9af210546cca592e49eccdb35be4831e9c0ff3

Observation c50968cf-76e5-4bd3-8960-1c702169445f · outbound

This paper cites Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers.

Late-time emission-line profiles from kilonova models Kilonova Light Curves from the Disk Wind Outflows of Compact Object Mergers

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:61364e74336140c1b9ba693686f93a9c9368d2cb180d64516109f063e97ee69e

Observation 33dcc84d-37e1-4ed9-9bab-ddf8df3dedd7 · outbound

This paper cites The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries.

Late-time emission-line profiles from kilonova models The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries

Reference 59

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:6b685e16fe60a5b41eb80ebf3e0f6e5dd6f3aee1de0452d75c8682b6de58bcf4

Observation 5eb30fea-c66d-44e0-88e6-617ec336936d · outbound

This paper cites Origin of the Heaviest Elements: the Rapid Neutron-Capture Process.

Late-time emission-line profiles from kilonova models Origin of the Heaviest Elements: the Rapid Neutron-Capture Process

Reference 60

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:b3be40752994d264e6b674a6a5e0a3346bf893d908e3613bffad2a8d152e8340

Observation 84f33e34-8638-4359-a982-34989f4d3ed6 · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 61

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:c32dc7974ae5de02bf8bfada939137ab0ddc9e638b8ba74079164972379d9184

Observation 6d160492-3b53-40fa-a918-429912bd019a · outbound

This paper cites , keywords =.

Late-time emission-line profiles from kilonova models , keywords =

Reference 62

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:d5cd00a69da82b438d874494c9a485a1f3bdfde09cdb7288e872ffa844f21ca6

Observation d524acd3-1ae5-4766-965e-d2f413a7e536 · outbound

This paper cites Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state.

Late-time emission-line profiles from kilonova models Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state

Reference 63

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:10:22.399894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:bc1aa54d702f585d06c7e8bdb1e3d20df91afb1ec28fa769f551e51508c1f023

Observation c7851f03-e980-4158-8f09-788acf0dadbc · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 64

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a46b4e7a6ae051577fc86bc968b3d175515dcef3c62b573e9f3ac9ec82f87f93

Observation 0ad59a2d-7a1d-4ba4-9c83-a93f58306e24 · outbound

This paper cites Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova.

Late-time emission-line profiles from kilonova models Full Transport Model of GW170817-Like Disk Produces a Blue Kilonova

Reference 65

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:fee724ae6a1cba5c527d035e409621f90487de6b3b34778c2cdf5b569397a1c7

Observation a7fe57dd-6380-4f0c-8cce-ff875037a148 · outbound

This paper cites Long-term Monte Carlo-based neutrino-radiation hydrodynamics simulations for a black hole-torus system.

Late-time emission-line profiles from kilonova models Long-term Monte Carlo-based neutrino-radiation hydrodynamics simulations for a black hole-torus system

Reference 66

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a2f686fb9f78206b8995e0bbe8c2325465c9e10a1ca64245b928e7dd55b435ea

Observation 92d3730c-527d-4c2f-a1c4-d54a530ef196 · outbound

This paper cites M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers.

Late-time emission-line profiles from kilonova models M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers

Reference 67

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:59d256754d1c2f8952320890bc3ddbecb9cbcf7094fe0a1816d683163ac6da8b

Observation 1839438c-e1af-4458-aa32-15fd7239e851 · outbound

This paper cites Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger.

Late-time emission-line profiles from kilonova models Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

Reference 68

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:12a21e48365ce28d05f4a650c0c3986213b3e2cf251c8bd100e19eb7c974e15d

Observation 5d81e522-66c9-45aa-9d31-f145b127b965 · outbound

This paper cites Neutrino-driven winds from neutron star merger remnants.

Late-time emission-line profiles from kilonova models Neutrino-driven winds from neutron star merger remnants

Reference 69

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:e01b88d0532ac08c72621c42d85e9b1f59015363db12413c29e3077d9cbaf969

Observation dca89052-ca3c-455a-85a2-cb167eff9d47 · outbound

This paper cites Dynamical Mass Ejection from Binary Neutron Star Mergers.

Late-time emission-line profiles from kilonova models Dynamical Mass Ejection from Binary Neutron Star Mergers

Reference 70

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:d246e909ac58f23f44e421d100c467d10c3fb0a3fa074bb9ea17a9d24aa2a342

Observation 89dfd147-d69d-4ff0-accc-8e5b00e54f40 · outbound

This paper cites On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers.

Late-time emission-line profiles from kilonova models On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers

Reference 71

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:17d337e29356ad5a9d5a3c74bf18eae0c9155997541e05800077df6b2a745cd3

Observation 9e34c78c-7665-4411-bd07-ff991d887117 · outbound

This paper cites Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star.

Late-time emission-line profiles from kilonova models Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star

Reference 72

Resolution
unresolved
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f9a3cbff862e2a0d3d12dc9c9ef3abda062e8b9ca7e942c31fecfabd59e92f22

Observation 218371db-fd62-4bd7-b91c-691096c0f994 · outbound

This paper cites Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves.

Late-time emission-line profiles from kilonova models Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves

Reference 73

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:10:22.432135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:b16a02509f8fc7b489adf235150c72f7efe9d55237171d6f7e3a4d06627bbd5f

Observation e38c1ec9-e5e0-4cc0-8724-2e198fda1200 · outbound

This paper cites an unresolved cited work.

Late-time emission-line profiles from kilonova models Unresolved cited work

Reference 74

Resolution
parse uncertain
no resolver link, observed 2026-07-14T09:02:10.553457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f05ce8a83b54e66488a70527cb3e8e0f98213c3bc81d10ca2d5f5f4bfd44ace9

Pith citing papers

No inbound Pith citation observations are available.