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Paper Citation Record · LEDGER

Late-time emission-line profiles from kilonova models

As of 8 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 0 inbound Pith citation observations for arXiv:2607.10818.

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 2026-08-08T06:32:00.761636+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

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=sha256:55438eebfe529f1fa80eacfa9d8dd640f1fa6dbdbb77d302071d533a746ec613

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=sha256:09430aaac9289a8ba3f4b0a77e0167974076bce0360d57ffa066c4013539c147

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:11f64783c6287f515922b9057bbe9ec658be12c8d678442d3ae71f243f5fd73b

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:dec18134ecf01a54a37c85bae1f459bc1bba3e0a79a153794dddd35f143a9559

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

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:2667146ba066e19443f6393c7fd3495a31a77bc4a34300c586a733e9b39dc09e

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:c3afb69e1fee2c761b4161218bbb38602bb66a94fe278281d38f2f2f3dfc5bfd

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:cf371860d2e52e96d38d8a34745b29a095b427d1490f49236e091f72e611b2de

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:12a3b42c9a7cff9c8207809d80b8a347d9a43c75c5674a8b6def85cce70fedde

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:cf589d09d85f61ade50c5e032541c2a767f01fdd5323015b5c8e3f905346079c

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=sha256:84e7e1f131f995c5d44560b393be83bff99ed3d71aef16a67149a3ac6a7f5017

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=sha256:975ec1a8e150f7e28f7837d3674b32ede4ed5580501db540dbc789201b60847e

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=sha256:034f1dda33c7536acaa80ef5d5f6379861a2ec7f091d36b2673076a09ca9cc95

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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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=sha256:2c54e7f2464c5bf63e366fc062185867431e3a96476716837e4f713e73f4fdd1

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=sha256:1f493b986e85d7f12b670963b52fc575cbf25a6e08c565eaba3a7599dc10bf92

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:c28f55d6c11ada681e6727841208c3229e49ac460695f6165b93d1d986bac423

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=sha256:5ccd2f872c2b0a4d38a28de63204f73d5503628ca9ee0c4b4a869126982797e3

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:61ccba367ad516700dc438c69f17ff5a9d84881fbba364176e5c5f4c6b217236

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:c423f43c4121e065c3553cbcb3252fe2196bf2089877f7a5ad5432b27bfbbda9

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:a0cb8033d71476d413f7aef591a97c55d951b7745131f4380d20d34507965748

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=sha256:3465e0a5a83932766564a487e7eeae73dbf73baebf7bba392bc0d3c905100250

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:f67049118e91406167e48a7665f904d51983066411b49d9608062b32b07a56b4

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=sha256:99ae69997d6df00e4cdc04e1d282b8de7aecad75483eeeee0808074e48326d3d

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:e7b7e49895856ed15a8af162c4abf7161e06854981404d6f3c9a6ffabcb86745

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:d771e8fa5fcbdbbd2c7bf14ea79c80c136c99b1d81590f1f3a15f4a66d8465e9

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=sha256:77fe060da8678e39cd29e2c180cd19caaa6543ff16fd922b22d158ce6f5ad870

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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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:72aa5f9ff2d8d8ea8732de4c7b7868737e1ff8873f5adec876c392c808fe8791

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=sha256:7a1aa155218bbedc6a496cd1d4da64c52110b9f26d793f176f0b376bcac788b5

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:b1bec9929b93bba602b70ac2367f15724771e1266474d0ef506913c1f6568f4f

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:bfafd34b4549994726221ecf5dcabd152940206789420c20976b5ff056335ef9

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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unresolved
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=sha256:3fddfa5af82f08bfb761a011f63b8a92cda1ee92c1154d2b0ed8392774b5c8e9

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=sha256:74bd713424dc2bfe469fcf758c8df86dcbc54dce220df1b772b83f926737c0ba

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=sha256:3f28c3eb6897ecc742278bc9d7568993cf10fd7288c10ad339c4cf7245b658ff

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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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=sha256:7e9720c0db0b029bd71f6fdac5f3e8203d439d6471ef39db5791ea172a323243

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:fc26e611a3f72d84a645bb4cc477c35c7802378cb1631618764004fe93afd10a

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:094b9fd18cddbd35589e243259399be523f44d6b3dc9375ab2198c17d2b58bf4

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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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:a1d7b5a19d7d03617896e826a33360b73d57876cbd2dd211b9903746652c6ce3

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

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:e8f1ebb1ebd72af41ba22ace4c6162db7d4a1e530e3e29eb76f4d1f494d0742b

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=sha256:1125ca517ae49be48c6d14b1032646cf25bc7bdf3a73ecf1e16fc7ccf77f4717

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=sha256:11caaa3a1b28228c868c32e24cc05534fedf0ce2ad29105ec8c7055d7cc5bcc2

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:a89da83ad2ebf8beb34a5f4e2af61280d0c081669774c0aba21b08ec6d08b925

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=sha256:258aa436a45a524ed616b20a33744827c1df9fd62526af559e70316612845b6b

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=sha256:1271ed62cce4e75f6d8255762725a8ae30d4e89232d3a32004fca54fb318df01

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=sha256:142ecf998de243f7fcb471250abda092b2d42ee953a2af47f492164e0c4de1b2

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:bfe00637304c173af4f374774ad5c5e9bf94607dfc6ab65f3f4cc4f05ef58aec

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=sha256:5e20ab8819c9cd9b166a1243b81e2b4867ab8cf29ac178742cb1d17352fe8946

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:a391de09b7cdedb2a271c68adbc0b26a6ccfc13109b237ce4e7137d44123ba1d

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=sha256:00ef52d704497b5d7456cd3a4eb2f79ae854add7835ff287bb37938f24a9bf5f

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:ce593a81796dc11e76b55ca7f39d99085030c579acbd0dcaf56d9a6cbd5ae638

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:af572511defb63831c2c0b390acd489c132babd79a3017e778a7053a9c0d6a8b

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:4dcef5cb3b59948c0117a8dbcd2688d11ac3cfc9f647acac8af7e2891509be48

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=sha256:52f4b2dae53fcaf66ff749301b0cc273dc9da0d65900bc8e62d05fc8285a7bf1

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=sha256:2fafc9fafb410e193817557d76304645f546b351bd1c74ac9f59ae877e1de5dc

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=sha256:6c43157cadcdca8c5b6e5dd5d6d9bafcc15468d860d38751df09fffd4a4cf145

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=sha256:40a4ec4a8400353209d191537e2e976262e13e365c423e0a4f4bcc2a0d4fce84

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=sha256:7217b0a9d9aabf00aabc61c4911e820b37531b51e5516852fe90fbf90b23c9f8

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=sha256:2b769df5d97bc3c0716126fe5a44b2b4cde33caed4a7ab476d928212c958e60d

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=sha256:2040384b0eac15af1a66d22661791ffeeb5569a0615fa2f02fedbf00ad21faa0

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=sha256:86326d17c1e9bafac9aaf543d99eb7357f7d9d3575f4b08794ce997f945af0dd

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=sha256:26d70b484b3d7d41d2ac1cd53d7bd409db8ac640571747e760f6c36aa462b77f

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=sha256:3613b11a1ad5767d28e39b3c2584d330b95428acab22357ad3f471be215a59a8

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=sha256:8e4f1d8c52bad35fe2ea92ee3e6fc15eaae24f608356479a6a9b3378220dce8d

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:c5b76f3f55857aabc6b3812350465df66da08902a512cbbe2c7164b6295f13f8

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:4ecbc6e8f777bbf7ad7189674fc007032c04a30bd1f36c5ed2da2bc574f389a7

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=sha256:45ef4c93f33e644f662ab949444a44c5841597d5e82318828b354356d13b92a3

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=sha256:5785349d2491f9b81bddcac02760c371972bf2f05da34cc22073de45c50cd321

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:e4e83b022236fe5832b100f30bd1d9fac4ea4762ca9ec85b6e33cee8d7fc09da

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=sha256:5ac787f66de5019c82e4c5b049ecd41c851a2ef25e08655cd6eeb890e718808c

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=sha256:004cbf86e70aa59bdbaddaa9f3e196bc521517cee387312cf6614e4fd6f9c6e9

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:f7c5f79715b3497fd9f75ed062e02f5c3f00482f20286c25f97e80a2f768be4a

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=sha256:448340a71e0966468c230eee092e529564e11fd610a48dfe392d6c9243e2baa3

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=sha256:4105684767f6fc4c5a4e943f9979ebd60736340661401a696aa74a6047e1b3d7

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=sha256:1d465c647e7ee950fd09211b8947f210c3b8ac322f1ee3dc5bec913f58af3276

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-14T09:02:10.553457Z digest=sha256:bc0fa204354901f5e3918cc77cf85c1444ad00b98dc0d73e6800beba0ad3284a

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:bbf8e4c5aac0a50d1aa34a03fccc62f46599e8a70de5ab03c7978e65786ef285

Pith citing papers

No inbound Pith citation observations are available.