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Paper Citation Record · LEDGER

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

As of 6 August 2026, this Paper Citation Record lists 100 of 103 outbound references and 9 inbound Pith citation observations for arXiv:2604.05059.

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

pith.paper-citation-record.v1
2604.05059 v2

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measured 100 of 103 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-04T05:35:22.653964Z

measured 109 of 109 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:44:21.606559Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

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100 of 103 outbound references displayed

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Outbound references

Observation de7049d5-e986-41ac-98f6-1f4725ac1788 · outbound

This paper cites G., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars G., et al

Reference 1

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Observation 796196a1-79e8-47eb-965f-eb0b321c5220 · outbound

This paper cites GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 2

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Observation 11422f9d-47ea-46df-8dc6-75288069166a · outbound

This paper cites GWTC-4.0: Population Properties of Merging Compact Binaries.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars GWTC-4.0: Population Properties of Merging Compact Binaries

Reference 3

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Observation eb6822e9-7097-4c4a-9169-ff7a0e73998b · outbound

This paper cites GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients

Reference 4

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Observation 76d6cb41-acae-4a09-9937-6a524c545c3f · outbound

This paper cites P., Abbott, R., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., Abbott, R., et al

Reference 5

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Observation ccdd67cb-36ac-4f9f-bb5d-de3cf3e9a855 · outbound

This paper cites P., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., et al

Reference 6

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Observation 3a9dfaca-2195-465b-bd04-77c35848f879 · outbound

This paper cites P., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., et al

Reference 7

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Observation ffd004f4-1f35-4d69-bb25-0bd7f47fcdb4 · outbound

This paper cites P., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., et al

Reference 8

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Observation 6ecebf1d-1368-49ba-8707-a81486196aa4 · outbound

This paper cites P., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., et al

Reference 9

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Observation 3e122eb8-c4a7-42fc-a57d-674f93ee2b25 · outbound

This paper cites P., Abbott, R., Abbott, T.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., Abbott, R., Abbott, T

Reference 10

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Observation 9eae3d86-fe53-44c9-bfd0-3c11f9366a0f · outbound

This paper cites 2023, Phys.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2023, Phys

Reference 11

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Observation a3ccc645-453a-45eb-bbe0-9570f3e5b84e · outbound

This paper cites 2015, Classical and Quantum Gravity, 32, 024001, doi: 10.1088/0264-9381/32/2/024001.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2015, Classical and Quantum Gravity, 32, 024001, doi: 10.1088/0264-9381/32/2/024001

Reference 12

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Observation ad05851e-8914-44f7-8cad-413e2ab2ceab · outbound

This paper cites P., Anand, S., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars P., Anand, S., et al

Reference 13

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Observation 64be9c98-eea6-41e1-8295-4f948f0f9750 · outbound

This paper cites 2021, Progress of Theoretical and Experimental Physics, 2021, 05A101, doi: 10.1093/ptep/ptaa125.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2021, Progress of Theoretical and Experimental Physics, 2021, 05A101, doi: 10.1093/ptep/ptaa125

Reference 14

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Observation a3a34f8d-e5be-4e36-bda9-4af8234940d1 · outbound

This paper cites 1989, GeoCoA, 53, 197, doi: 10.1016/0016-7037(89)90286-X.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 1989, GeoCoA, 53, 197, doi: 10.1016/0016-7037(89)90286-X

Reference 15

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Observation 6e483166-4878-49be-a47f-c2858826cb9b · outbound

This paper cites C., Sagu´ es Carracedo, A., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars C., Sagu´ es Carracedo, A., et al

Reference 16

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Observation aa3deff2-e589-490e-aa0b-5367908aa444 · outbound

This paper cites W., Kool, E.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars W., Kool, E

Reference 17

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Observation 37833264-f67c-4c6d-9de7-12b5e353f22d · outbound

This paper cites 2020, Astrophys.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2020, Astrophys

Reference 18

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source=pdf_text observed=2026-08-04T05:35:14.307465Z digest=sha256:99c2c7e1829257c292ac4079b216399ba950d60251ba2e1c2acd27ae7d2d9d62

Observation d6f98fe4-7edf-4442-b94d-0ec7b59b1f1a · outbound

This paper cites 1999, ApJ, 525, 886, doi: 10.1086/307938.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 1999, ApJ, 525, 886, doi: 10.1086/307938

Reference 19

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Observation 3822daa5-d2f7-4442-afd9-dc37a59b13f2 · outbound

This paper cites 2007, PhR, 450, 97, doi: 10.1016/j.physrep.2007.06.002.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2007, PhR, 450, 97, doi: 10.1016/j.physrep.2007.06.002

Reference 20

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Observation 911ee549-356f-4bbd-9f90-f04ff8163148 · outbound

This paper cites J., & Scott, P.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars J., & Scott, P

Reference 21

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Observation 38943920-b75a-4d0a-a317-1f6715ed87c8 · outbound

This paper cites 2014, ARA&A, 52, 43, doi: 10.1146/annurev-astro-081913-035926.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2014, ARA&A, 52, 43, doi: 10.1146/annurev-astro-081913-035926

Reference 23

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Observation ca42cbf8-cdb0-49d3-88eb-299fb9477f96 · outbound

This paper cites 2023, Research Notes of the AAS, 7, 136, doi: 10.3847/2515-5172/ace258.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2023, Research Notes of the AAS, 7, 136, doi: 10.3847/2515-5172/ace258

Reference 24

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Observation ea5c580b-f1e2-47e5-9825-e09339432f5b · outbound

This paper cites 2022, Mon.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2022, Mon

Reference 25

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Observation fd4dd9bd-d183-42ec-80f8-c8cc68c90992 · outbound

This paper cites 2020, ApJ, 893, 38, doi: 10.3847/1538-4357/ab7eaf.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2020, ApJ, 893, 38, doi: 10.3847/1538-4357/ab7eaf

Reference 26

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Observation 813f6a3d-626a-4b5f-b117-e8728d3739c2 · outbound

This paper cites 2014, ApJ, 787, 10, doi: 10.1088/0004-637X/787/1/10.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2014, ApJ, 787, 10, doi: 10.1088/0004-637X/787/1/10

Reference 27

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Observation 9bbac650-4234-40d8-a4b7-e91694fb07e4 · outbound

This paper cites 2013, ApJ, 764, 179, doi: 10.1088/0004-637X/764/2/179.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2013, ApJ, 764, 179, doi: 10.1088/0004-637X/764/2/179

Reference 28

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Observation d8ebdaf9-00c4-4fd7-92a7-63d8b2d381b7 · outbound

This paper cites Inferring Neutron Star Nuclear Properties from Gravitational-Wave and Gamma-Ray Burst Observations.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars Inferring Neutron Star Nuclear Properties from Gravitational-Wave and Gamma-Ray Burst Observations

Reference 29

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Observation 243a6f4e-9f4b-4bfb-a277-f5a41ac407e3 · outbound

This paper cites an unresolved cited work.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars Unresolved cited work

Reference 30

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Observation 0f4cd3b5-670c-467d-82b3-ee5e45ec1a16 · outbound

This paper cites S., & Siegel, D.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars S., & Siegel, D

Reference 31

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Observation 72dc6d16-31f0-4896-b97c-ac6bd17212ff · outbound

This paper cites A., Kilpatrick, C.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars A., Kilpatrick, C

Reference 32

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Observation fc874838-ec77-4b6c-8dec-d6bf0ca6bc35 · outbound

This paper cites M., Howell, E.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars M., Howell, E

Reference 33

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Observation 00a87640-4fe8-47a9-957d-cc9a96dfff2d · outbound

This paper cites 2020, MNRAS, 492, 5011, doi: 10.1093/mnras/staa124.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars 2020, MNRAS, 492, 5011, doi: 10.1093/mnras/staa124

Reference 34

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Observation b3746b25-3778-46b0-b67b-75cab2f7bf66 · outbound

This paper cites W., Zevin, M., et al.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars W., Zevin, M., et al

Reference 35

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This paper cites an unresolved cited work.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars Unresolved cited work

Reference 36

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Observation 26614256-ff54-4cb7-bf54-f276108d8a18 · outbound

This paper cites an unresolved cited work.

Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars Unresolved cited work

Reference 37

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Observation cd9daba4-a187-448b-b888-644f963905b9 · outbound

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source=pdf_text observed=2026-08-04T05:35:16.430844Z digest=sha256:d727cf2eb154d925655776c4d1af3994b10552c05d46d15d81a8f0a25b0fa6cf

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Observation b51d4d8d-2b4a-40fe-af12-1025fdff944f · outbound

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source=pdf_text observed=2026-08-04T05:35:16.550851Z digest=sha256:2314c803769545d591688e230eea2c7665e2ced3e4fbc38f1fe805923c49ff4a

Observation 4313758d-af91-4189-8a24-4a191996ea36 · outbound

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source=pdf_text observed=2026-08-04T05:35:16.612012Z digest=sha256:fd8b840e3ab9ad4789a06ba9935ebfdfee4a1d7539c3c0d5d501b4cbe568a373

Observation 3cf268d3-ae06-4057-8574-46ebbed7dcdf · outbound

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source=pdf_text observed=2026-08-04T05:35:16.723423Z digest=sha256:fe3bbc6197b6d437a1a3b4fa5d805809bea77191d0dd3d0dc2973ac13d3c6bf3

Observation f41dec37-81f4-44fb-949a-d202260f5dca · outbound

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source=pdf_text observed=2026-08-04T05:35:16.853343Z digest=sha256:0c096e8c68f6c2d8a8f7aa1c4a32fe731da2e596e29e15c2b198e19c835e2b95

Observation e5d21fdd-9cf9-4a9c-8bd5-537b145e65d3 · outbound

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source=pdf_text observed=2026-08-04T05:35:17.016023Z digest=sha256:fde575f45880a20535694f0bb6808086b4d9dc0d0084293a1a73b84ce8b0ff74

Observation 73138bf0-a264-4112-94fc-bb7f938cb9ac · outbound

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source=pdf_text observed=2026-08-04T05:35:17.162424Z digest=sha256:b286b185f6cc3ede900fe6bd71f798a2c2878a7dea4307a1e46efe546b806f64

Observation 0a4d9f2c-f0f7-446d-843a-662c98e4a09c · outbound

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source=pdf_text observed=2026-08-04T05:35:17.257019Z digest=sha256:4faecb1e66ed2f70d5359cd8e0cbccf653b6e02ebc8b0c4359b29424ee109a59

Observation ca74e8d6-bc7d-4757-ae05-222b5cf5c091 · outbound

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source=pdf_text observed=2026-08-04T05:35:17.396967Z digest=sha256:e3a73f96c908f9e34522cd7ddfcfa0e9ad4b9e0ef66982a1b3e6c1be6bc1bca0

Observation 9c272469-779d-4301-bb29-c5ebf84fd9fb · outbound

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source=pdf_text observed=2026-08-04T05:35:17.523235Z digest=sha256:f9fea98aa65a4332d505c693641d937c87ab15737d728722ab5db87e826f8b63

Observation 7f636af2-847e-42f6-9682-3aa007518d17 · outbound

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source=pdf_text observed=2026-08-04T05:35:17.657863Z digest=sha256:49cf3bc6dcdd09cdc9a8df2a4f3fb5dc8f6c99ea27dcfd3efd20278e2731d7c0

Observation d16c9f9d-7ab7-4748-ae33-a8b2929d6cee · outbound

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source=pdf_text observed=2026-08-04T05:35:17.802378Z digest=sha256:424d14f4fa37ca4eef267b4cb8723e1e035dce239262310e872d861d3ffb3eee

Observation 350496a6-1aef-4f2f-8abf-7f5081aeff1d · outbound

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source=pdf_text observed=2026-08-04T05:35:17.971835Z digest=sha256:40274637c90da9b2f7a0c844f9f180f323b4d8d650c11d50954cd22e120b7e39

Observation 64138e73-f99f-4057-a2c1-efae5c320e02 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.088914Z digest=sha256:aeed7ba60736b3a0af42f5afa387bc59e3f982bfa9b742025085eb5fc2936e7c

Observation 66f8f95f-72b2-45de-9167-776600666520 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.145485Z digest=sha256:c78971dc9adcd47389ca981e1f86e6b9eaf0bf0f150eabbf7c494673bd3f1764

Observation 06e184d9-4df9-46e6-b3e0-2a3cee734847 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.211479Z digest=sha256:6612a9f7cac20bb2d90fea630e8cc3007e63e738bbf6ea4b34c99578e87a0756

Observation 3e370852-c730-4973-8d8d-658f95c7fe58 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.324922Z digest=sha256:35278509f64dd4d09e302a0d5481dc597b73164d72fc8d4fb4af055fb4b28cd3

Observation cad9191a-c4c9-45c7-92bf-5791dd0604f0 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.408221Z digest=sha256:7b08517c61925091a4a14b9d748160f03549f40a5ff6aeb83ecc15d39f257549

Observation c7bc435e-a003-4467-8b12-2ad3184ecb7c · outbound

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source=pdf_text observed=2026-08-04T05:35:18.494472Z digest=sha256:85344ab01ed9190ea1ebfd099f38c33ade2ec1a4ee21b9ccf2c4112d039cb996

Observation 4d99144f-6d9c-49e1-849b-3ac195391cd5 · outbound

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Observation eb4050e3-1edf-46af-9fa2-6dc2b0f1da78 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.760267Z digest=sha256:41388a5f914725a94a64d4fd9461f78c5e841a5a93c3c322bd7c96a5c7189651

Observation 89b26842-83fa-4f2c-93c5-d714fad34a93 · outbound

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source=pdf_text observed=2026-08-04T05:35:18.883491Z digest=sha256:5856dcab3a74562f5952615b454f9505b091290bf82cf338ea426859d0a86a8f

Observation 0c50d649-8c18-482c-ab36-5c148e54e25d · outbound

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source=pdf_text observed=2026-08-04T05:35:19.004890Z digest=sha256:abc101e08afd4d52f21b35ea88d38add6d2e1740a07a75d1c7683a6c1a0648ba

Observation 94bbf857-1184-45af-9461-c6056cda0763 · outbound

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source=pdf_text observed=2026-08-04T05:35:19.173974Z digest=sha256:8bcd9ff353f63a5dc63f68f9f6585107e532d0f080fece3758e0ea279846849a

Observation 503f507c-40be-41a0-a7da-9916543ff8f2 · outbound

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source=pdf_text observed=2026-08-04T05:35:19.378391Z digest=sha256:0cc270fafce61c4c35391fa9326b7c5dd3689b27291aeae5aad5d82c87afae04

Observation acdf8265-8cb2-4e6c-8634-f3b3e8cdf4ec · outbound

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source=pdf_text observed=2026-08-04T05:35:19.471330Z digest=sha256:5c88646264cf06a5c20e96ecd63386b6a28b8208007582448befdb317e72d35f

Observation dca5caf8-75a2-4e48-8d3f-9d5f6e43d284 · outbound

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Observation 5154d140-f2dc-4b3c-a9d4-1e1ed1ef07f0 · outbound

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source=pdf_text observed=2026-08-04T05:35:19.644810Z digest=sha256:6308c8deb2bc94774dbaedfd143ba41d4862d16a6ba018134bb25a3d66d4097e

Observation c147f62c-1e65-4349-b12b-2acba5bd96a6 · outbound

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source=pdf_text observed=2026-08-04T05:35:19.745927Z digest=sha256:bc8a7ab48dc695d569ecb2a8c7c9a5c7773b5cd18ee46b5701f6771bc50e4f59

Observation 220e2b50-8b0d-4f2a-9dc5-30eecaec6491 · outbound

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source=pdf_text observed=2026-08-04T05:35:19.892820Z digest=sha256:e833e11a34414adcd1d8a1bc6dfe61a8aa8f1b0a23e3d928761dee614bfc2002

Observation 51d70c5f-44b6-4314-8781-849f3c64953b · outbound

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source=pdf_text observed=2026-08-04T05:35:20.027760Z digest=sha256:99680c4ddf7de676ce7f1de029c2c8f83b697d403fbbf88d3daec0e2c8ab0cb6

Observation f3705622-3034-4a96-a9a6-e77792609dbf · outbound

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Observation 780c2db8-ff25-4ec5-b0f9-4ea953f60fbd · outbound

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source=pdf_text observed=2026-08-04T05:35:20.159540Z digest=sha256:dda2f90d37c9cfd2d629fa373cc84cf9afb98f3d49fd5b0831c1cde4ea83f2c0

Observation 66bff8ea-8004-4965-b9cb-7c38a221a8f0 · outbound

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Observation ded3da3e-8f2f-472a-b082-4b8a6d46df85 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.453399Z digest=sha256:f86e091ea571513024907a01728ba9140588f75e0263a18bbd0ea31beffb1f7d

Observation 0a8f57cd-51a3-4aea-92fd-d1e6201c93f8 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.535961Z digest=sha256:a9f6bbac0b1848ec3859a4f1755524545fa5e23a6df915fc40b98070b833d30e

Observation 63f7d2de-b9e0-4dc5-88ab-e55d846d9293 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.601127Z digest=sha256:2883f1f48a07e15b351ee5331fa12b88c357e4506212cc890e3b4cee8e595058

Observation faa2e657-1538-4ec3-95db-3de867d95d30 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.708182Z digest=sha256:9ef4343549d6e296028c5d2ed20a2ef285b27b440912e5a4e14691bfdae4674d

Observation 1b170977-b30c-40e9-8483-079db9142824 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.826796Z digest=sha256:ccdaad6c39a7e12157455c1b19e6d4a05c70b2a4b1b5f84acd6d21c9f4b9cc64

Observation faad2f8b-e28f-4e94-8b71-c0625f841008 · outbound

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source=pdf_text observed=2026-08-04T05:35:20.974212Z digest=sha256:075f2dafa89c775a9ecfee5c515f3ca5893230776d220e0e250d7f27cdf00ac2

Observation 6d3cdf6d-be89-4aea-b057-eab2e4ed60f2 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.088982Z digest=sha256:29421a6379bfc89f88e91e00efe74933a6a7025f2c287d5a82d19eae3f64ba95

Observation 3fe119ef-6d5f-43fd-ba38-d502de2f772f · outbound

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source=pdf_text observed=2026-08-04T05:35:21.210187Z digest=sha256:6af5d7d219090a727999a773e325d0d2458ee2f1932a2b359b121036cd001e62

Observation 1bc89aab-a48e-464a-bb4b-e2a747089938 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.405407Z digest=sha256:e29395e9854551cf2a4f4a9a4fa7908d19e190d36fa298e3b62ce0d1aa52de13

Observation 99b0b071-697f-4818-b187-6399bf94e714 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.512255Z digest=sha256:f7b735b83a60632fe5162ccff4894baec402cec54c591e778ec8a85af8ec1866

Observation f8459a3a-14c1-44a1-aedd-ef840bf99db3 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.606941Z digest=sha256:f1ab9415af8fe37f09a7551e75976cbb33a2ee32ee1f34a4939def5ae90d3c0b

Observation 5cfed2e1-3ef5-4cf5-ba3a-807091d780a6 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.688579Z digest=sha256:b751b0651d0aa5de8b0b409c1ee17129743318ca57a16e6ccd15e8edf662de59

Observation 2ec62a99-6526-4521-b35b-63597ea9a677 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.765134Z digest=sha256:a7c9f71ed52804d1f3c667cd2bfc723634a535ae64b073ada879c176932718a3

Observation 758f2a05-200e-49e1-8d74-9833e2651237 · outbound

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Observation dd03c283-d46a-425c-813d-dce8c0484dbf · outbound

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source=pdf_text observed=2026-08-04T05:35:21.868792Z digest=sha256:f8f2ab6c6e6a5bc6c8141062d2193933c131518c37eaf87b01bd206a6196d678

Observation 90e7bb65-1896-4341-ab3e-d0c8f3669677 · outbound

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source=pdf_text observed=2026-08-04T05:35:21.939214Z digest=sha256:78b03842807033ed04df8c9cebd7cdd06d3ff92f9d995622caf6583a5180cdb6

Observation f158d2d7-6b5b-4aa4-be24-169faa553c7d · outbound

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source=pdf_text observed=2026-08-04T05:35:22.011689Z digest=sha256:4c656d6cb7a736631af76661700094ee93e66c0371bbb67e534032d376031afc

Observation d8dc7b5e-ec33-445c-a1c6-1026e3d9254c · outbound

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source=pdf_text observed=2026-08-04T05:35:22.122029Z digest=sha256:8a3b9b6a69e5940b87b681d154f5f3a73703a8d8c49f344ff5cf3e25f016f6e2

Observation 9154be66-6dce-4e08-a17c-49ded55e1272 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.189611Z digest=sha256:94475ddde00eee56a13b1fc76b0361fbf1090675d56432f40a9496daa68b80e7

Observation 13b83a58-b497-48bc-bcd0-06972d2626bd · outbound

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source=pdf_text observed=2026-08-04T05:35:22.282522Z digest=sha256:1035fe6498bddea7c5a613b7f99140784190f09a4b061e887c582867510b7be0

Observation 1b5ace2b-c107-44d5-aba5-098cfcf23301 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.321817Z digest=sha256:431b43b182f8855d75fff3b80abe594d1fec06b4770a21f1147a884b2288d863

Observation 0afa9985-f204-4144-95ad-6cd067dd49c8 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.394804Z digest=sha256:6b8a1241a63abded96a6a19485b6f0c48f949eb329e2cd822cd70fdf9d3d6795

Observation 5f7f131c-9868-4cb6-850c-86a933269848 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.458581Z digest=sha256:d2045a0d746aeabf874caabe502469a44b86c70f1ef89fd9f822922afd156fba

Observation 8cf8f983-74e4-414e-9ea8-dcd4f8b81f13 · outbound

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no resolver link, observed 2026-08-04T05:35:22.515667Z

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source=pdf_text observed=2026-08-04T05:35:22.515667Z digest=sha256:9b55d579326267b09e3847999a4ec975f679aee0dfd8887018fd71a8c17619f2

Observation 6b0a44b5-63ba-4916-b847-dca441f73124 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.578696Z digest=sha256:adb70a9c1230fa30c143fca4f77be89cece2f66ca7ddf71a89a886a9b6e3b619

Observation ed77a086-4efc-47a8-850f-fa3e9cb16c78 · outbound

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source=pdf_text observed=2026-08-04T05:35:22.618525Z digest=sha256:541cdfd5f773bcc3c5d047d5b9bba0c95d15e7b32370c56f0d6201b1f0fde56a

Observation 48899c31-972e-4d5e-a3c5-c3f1b27a8ffd · outbound

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source=pdf_text observed=2026-08-04T05:35:22.653964Z digest=sha256:64427370d74f003b60294f73d5b706598ec5a2fd5baaec49f69d99a353d78ee0

Pith citing papers

Observation d4ffd863-8f4e-4cc9-b673-b85d47f29bf9 · inbound

Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates cites this paper.

Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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local_arxiv, observed 2026-05-10T22:45:48.232502Z

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No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-10T19:36:48.497341Z digest=sha256:8f2873161d71f05685924795feaa7c745c62ed4d8793a0797ac6438100659f15

Observation 6c508373-f9f8-46e1-b64b-e791cf5a8ada · inbound

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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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local_arxiv, observed 2026-05-10T07:31:59.370340Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-05-10T07:31:20.205636Z digest=sha256:5eabf3ffa04ac0813f50b903ca247429d3b278cefb253e70baaed094304c66b4

Observation 65f9985f-5707-408d-b765-f212e75f94c6 · inbound

Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors cites this paper.

Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-08T17:29:32.083922Z digest=sha256:2af99390edf1380803040df16e64cc3f12a98194e35c222aa3a0b3632f416332

Observation f4eb47e2-104a-411a-8f5d-3202173c584b · inbound

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Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-07-01T00:00:28.796229Z digest=sha256:01dc0902cdc998c86c7f12dad7ff627f2ea9f0ee79bf019a73a0e816328c0de7

Observation b1ff5c01-19b7-423e-be4f-c8afda51976a · inbound

Binary Neutron Star Merger Evolution and r-Process Enrichment in the Milky Way Disk cites this paper.

Binary Neutron Star Merger Evolution and r-Process Enrichment in the Milky Way Disk Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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local_arxiv, observed 2026-05-21T04:29:34.617327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-21T04:26:53.781342Z digest=sha256:f020363463195083cccbf8a519a2d8353f2a05412ab3e5a8d828dc192b5d4868

Observation b673356e-0796-4a1a-9a6c-279cfd06587b · inbound

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Binary Neutron Star Merger Evolution and r-Process Enrichment in the Milky Way Disk Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

Reference 20

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local_arxiv, observed 2026-05-21T04:29:34.134569Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-21T04:26:53.781342Z digest=sha256:9c3b6cc12e448a4b275f7a1393d7bd0cd299dc519b99929f1836c8bddc44d151

Observation e245ac6b-ed03-4e6a-8de0-2d66b50a6415 · inbound

Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences cites this paper.

Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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verified exact
local_arxiv, observed 2026-07-02T00:36:25.335426Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-06-28T13:18:38.984279Z digest=sha256:2f35f306bc8d74854fa72878f7b5573648d2fa53aab211a9c0dff072b1bfc738

Observation 46b75a7d-502e-45a7-a4f4-10d326630ae3 · inbound

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Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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unresolved
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source=pdf_text observed=2026-07-31T05:12:16.712241Z digest=sha256:6a0232fcf27aa2ed9554591f91fa10229d45156258a85e5a791ba8c9a2c47e0d

Observation 65865ffb-72ca-43fa-89bb-ee90f55ae5cd · inbound

Gamma-ray burst progenitors revisited cites this paper.

Gamma-ray burst progenitors revisited Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars

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Source-reported events for the cited work

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source=arxiv_source observed=2026-08-01T00:44:21.606559Z digest=sha256:5aec344d0d5e98e64df57162e59599ea5c20598f1d2891b5bcdc5193361e176e