Paper Citation Record · LEDGER

Can current models predict the local black hole merger rate?

As of 7 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 4 inbound Pith citation observations for arXiv:2606.02725.

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

pith.paper-citation-record.v1
2606.02725 v1

Coverage vector

measured 100 of 300 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 104 of 104 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T08:18:36.381451Z

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

Reference resolution

100 of 300 outbound references displayed

verified exact83
verified fuzzy0
unresolved5
parse uncertain0
malformed identifier0
metadata mismatch12

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation b80a7a59-0186-4e1b-8602-7eabc2ebe807 · outbound

This paper cites Array Programming with NumPy.

Can current models predict the local black hole merger rate? Array Programming with NumPy

Reference 1

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.985628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ad4e3d17-0b69-4467-921f-2876f86e3338 · outbound

This paper cites SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python.

Can current models predict the local black hole merger rate? SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

Reference 2

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T13:02:10.691310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation eaa0866b-2d25-47cd-8956-c4962389935a · outbound

This paper cites doi:10.5281/zenodo.10697587 , version =.

Can current models predict the local black hole merger rate? doi:10.5281/zenodo.10697587 , version =

Reference 3

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.946367Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3f0d6297-8e64-451e-8722-8802790c6fe7 · outbound

This paper cites D., 2007, @doi [Computing in Science and Engineering] 10.1109/MCSE.2007.55 , 9, 90.

Can current models predict the local black hole merger rate? D., 2007, @doi [Computing in Science and Engineering] 10.1109/MCSE.2007.55 , 9, 90

Reference 4

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.971972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e1cdc0f5-2303-448d-ad46-7a45c4604880 · outbound

This paper cites 2013, Stellar Structure and Evolution, doi: 10.1007/978-3-642-30304-3.

Can current models predict the local black hole merger rate? 2013, Stellar Structure and Evolution, doi: 10.1007/978-3-642-30304-3

Reference 5

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.979708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 24fca909-640f-41a9-bf04-707425507191 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA).

Can current models predict the local black hole merger rate? Modules for Experiments in Stellar Astrophysics (MESA)

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.991851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2b14969b-68f0-44cb-8ec1-b988d3657b73 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars.

Can current models predict the local black hole merger rate? Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.697915Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 645ecdfd-23ec-40c2-8213-caeddf42954c · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions.

Can current models predict the local black hole merger rate? Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.913912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f9d3f3fa-ec63-4c60-b251-d3a78d8cac59 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions.

Can current models predict the local black hole merger rate? Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.893027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8e58df35-f487-438d-9a24-77ea8b4564ef · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation.

Can current models predict the local black hole merger rate? Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.989477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 1155f2e9-b0b3-49e1-9dd7-1418ea197ac4 · outbound

This paper cites Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code.

Can current models predict the local black hole merger rate? Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.942173Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6e0fdefd-25a1-4bc6-8818-d8d3f75ea134 · outbound

This paper cites Merging black hole binaries with the SEVN code.

Can current models predict the local black hole merger rate? Merging black hole binaries with the SEVN code

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.979062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 79d5d942-d459-4778-b626-ee48c3ac6e0e · outbound

This paper cites 2020, http://dx.doi.org/10.3847/1538-4357/ab584d , 888, 76 , arXiv: 1909.01371.

Can current models predict the local black hole merger rate? 2020, http://dx.doi.org/10.3847/1538-4357/ab584d , 888, 76 , arXiv: 1909.01371

Reference 13

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.939865Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f238ee8a-c7c5-4191-b060-485f1d6fc5d4 · outbound

This paper cites 2020, Frontiers in Astronomy and Space Sciences, 7, 38, doi: 10.3389/fspas.2020.00038.

Can current models predict the local black hole merger rate? 2020, Frontiers in Astronomy and Space Sciences, 7, 38, doi: 10.3389/fspas.2020.00038

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-06-28T13:02:10.954196Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 88396746-c0b3-43a6-b55c-3a9a3e82bd90 · outbound

This paper cites 2023, Mon.

Can current models predict the local black hole merger rate? 2023, Mon

Reference 15

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.916237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2583568a-9f62-40b8-8421-fc3cf2a680af · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 16

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.642951Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 13f22aae-8994-4814-8b09-38ab95e6de8b · outbound

This paper cites , keywords =.

Can current models predict the local black hole merger rate? , keywords =

Reference 17

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.981366Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d63d9557-3abc-4396-87db-c2fa9e053f49 · outbound

This paper cites an unresolved cited work.

Can current models predict the local black hole merger rate? Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-06-28T13:01:54.102298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b36fb036-9f8d-47e9-a5dd-b3b077a383c2 · outbound

This paper cites year = 1947, month = mar, volume =.

Can current models predict the local black hole merger rate? year = 1947, month = mar, volume =

Reference 19

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.721957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3c5d8385-8bc5-4fc0-9831-ab54d469dc59 · outbound

This paper cites N., Vink J.

Can current models predict the local black hole merger rate? N., Vink J

Reference 20

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.910613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f2a892f3-06f2-493d-a5f0-c074ef830989 · outbound

This paper cites The evolution of AGB stars with convective overshoot.

Can current models predict the local black hole merger rate? The evolution of AGB stars with convective overshoot

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.898261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f2e27bab-feae-41a5-b09b-a2aa19ab792e · outbound

This paper cites A., De Marco O., Barlow M.

Can current models predict the local black hole merger rate? A., De Marco O., Barlow M

Reference 22

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.540820Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8b681ae8-71d1-4eb0-a398-736b86c69512 · outbound

This paper cites Bulletin d'Information du Centre de Donnees Stellaires , year = 1988, month = dec, volume =.

Can current models predict the local black hole merger rate? Bulletin d'Information du Centre de Donnees Stellaires , year = 1988, month = dec, volume =

Reference 23

Resolution: unresolved; no resolver link, observed 2026-06-28T13:01:54.102298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6efb30ee-07e7-44ef-a780-3e6034668d7a · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 24

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.688101Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e80278d2-8fc1-4f24-84c0-70c87d9f1bb8 · outbound

This paper cites Massive Stars Near and Far , year = 2024, editor =.

Can current models predict the local black hole merger rate? Massive Stars Near and Far , year = 2024, editor =

Reference 25

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.654578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f76cd607-e772-4d7c-a228-639d8d13fd51 · outbound

This paper cites Hot Star Winds.

Can current models predict the local black hole merger rate? Hot Star Winds

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-06-28T13:02:10.888096Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 15dc0bae-1554-42f0-806e-99c2de43adef · outbound

This paper cites I., 2001, @doi [ ] 10.1046/j.1365-8711.2001.04416.x , http://adsabs.harvard.edu/abs/2001MNRAS.325..231O 325, 231.

Can current models predict the local black hole merger rate? I., 2001, @doi [ ] 10.1046/j.1365-8711.2001.04416.x , http://adsabs.harvard.edu/abs/2001MNRAS.325..231O 325, 231

Reference 27

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.916352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation de761f3b-be70-4e17-bad2-b4aca6ffb33b · outbound

This paper cites Pulsational Pair-Instability Supernovae.

Can current models predict the local black hole merger rate? Pulsational Pair-Instability Supernovae

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.938193Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f78eae83-50a5-487f-bef2-4353b6a13d81 · outbound

This paper cites Mass-loss predictions for O and B stars as a function of metallicity.

Can current models predict the local black hole merger rate? Mass-loss predictions for O and B stars as a function of metallicity

Reference 29

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.877668Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8af5f0d2-288a-4ec6-a552-84002ac57bde · outbound

This paper cites Mixing by overshooting and rotation in intermediate mass stars.

Can current models predict the local black hole merger rate? Mixing by overshooting and rotation in intermediate mass stars

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.929652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d3c3d13b-91ed-4140-a109-9a186d11c019 · outbound

This paper cites Astronomy and Astrophysics , author =.

Can current models predict the local black hole merger rate? Astronomy and Astrophysics , author =

Reference 31

Resolution: metadata mismatch; doi, observed 2026-06-28T13:02:10.678649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation fe5ae42a-d623-4fb9-a26f-7ae2774010b1 · outbound

This paper cites 2022 , pages =.

Can current models predict the local black hole merger rate? 2022 , pages =

Reference 32

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.858892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 5a2f73db-e96c-43c6-b28d-ec66ebcc96a7 · outbound

This paper cites and Shibahashi , H.

Can current models predict the local black hole merger rate? and Shibahashi , H

Reference 33

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:11.002136Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3baf52a2-6e88-4cb3-99e9-15ac4decc5b8 · outbound

This paper cites 2022, ApJS, 259, 20, doi: 10.3847/1538-4365/ac3dfc.

Can current models predict the local black hole merger rate? 2022, ApJS, 259, 20, doi: 10.3847/1538-4365/ac3dfc

Reference 34

Resolution: verified exact; doi, observed 2026-06-28T13:02:11.005999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 256705ac-c1f9-401c-a7cb-1cad1c425ea7 · outbound

This paper cites The Hyper Suprime-Cam SSP Survey: Overview and Survey Design.

Can current models predict the local black hole merger rate? The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:11.001140Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c8186c6a-d98d-4a80-a8c5-7609221f45cc · outbound

This paper cites 2019, MNRAS, 489, 5202, doi: 10.1093/mnras/stz2522.

Can current models predict the local black hole merger rate? 2019, MNRAS, 489, 5202, doi: 10.1093/mnras/stz2522

Reference 36

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.400385Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7116b763-1b66-459f-8ef5-e59b740a553f · outbound

This paper cites Cosmic Star Formation History.

Can current models predict the local black hole merger rate? Cosmic Star Formation History

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.677815Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f1e818be-959f-4196-930b-68dea27fdd3c · outbound

This paper cites Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries.

Can current models predict the local black hole merger rate? Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:11.009936Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 770f6aee-bfdb-4cbc-bb2a-b59b84db8a23 · outbound

This paper cites The FMOS-Cosmos Survey of Star-Forming Galaxies at z~1.6 II. The Mass-Metallicity Relation and the Dependence on Star Formation Rate and Dust Extinction.

Can current models predict the local black hole merger rate? The FMOS-Cosmos Survey of Star-Forming Galaxies at z~1.6 II. The Mass-Metallicity Relation and the Dependence on Star Formation Rate and Dust Extinction

Reference 39

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.988529Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6a7e1e7a-b2c4-4e4e-8c45-86531d9ad630 · outbound

This paper cites and Shibahashi , H.

Can current models predict the local black hole merger rate? and Shibahashi , H

Reference 40

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.987027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e69a6ec6-e618-40b3-8889-13065e415919 · outbound

This paper cites MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3.

Can current models predict the local black hole merger rate? MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.621461Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4f0cd375-efec-4599-841e-dafe7db52468 · outbound

This paper cites How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?.

Can current models predict the local black hole merger rate? How Do Star-Forming Galaxies at Z>3 Assemble Their Masses?

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.474805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 1bb16654-238c-4e38-ad9e-c1b7db7fdf19 · outbound

This paper cites The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields.

Can current models predict the local black hole merger rate? The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.997398Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 68dcb05c-2397-4941-a08c-4a682289fb3d · outbound

This paper cites Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity.

Can current models predict the local black hole merger rate? Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.901494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 1fe566e5-0611-4b54-82e4-ddf165375bba · outbound

This paper cites 2024, , 683, A223, 10.1051/0004-6361/202346855.

Can current models predict the local black hole merger rate? 2024, , 683, A223, 10.1051/0004-6361/202346855

Reference 45

Resolution: metadata mismatch; doi, observed 2026-06-28T13:02:10.613715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e0e08218-831d-487f-957a-eafd6ae0f7bb · outbound

This paper cites The Nucleosynthetic Signature of Population III.

Can current models predict the local black hole merger rate? The Nucleosynthetic Signature of Population III

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.708433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7665e0db-a0a0-44cd-b645-56c53a53de50 · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 47

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.464474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 59a1b618-1849-43b6-a49a-bfeeee9bad4b · outbound

This paper cites The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers.

Can current models predict the local black hole merger rate? The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-06-28T13:02:10.456453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6c4136aa-4689-41fc-8cd2-8c975f49155e · outbound

This paper cites The transition mass-loss rate: Calibrating the role of line-driven winds in massive star evolution.

Can current models predict the local black hole merger rate? The transition mass-loss rate: Calibrating the role of line-driven winds in massive star evolution

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.713547Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 894f4be9-f1fe-407a-828b-3f1a0052faa5 · outbound

This paper cites The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Gamma-dependence of Wolf-Rayet type mass loss.

Can current models predict the local black hole merger rate? The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Gamma-dependence of Wolf-Rayet type mass loss

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.512955Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 6a6387d7-5f30-4a32-9aa7-740beed10f75 · outbound

This paper cites The VLT-FLAMES Tarantula Survey XVII. Physical and wind properties of massive stars at the top of the main sequence.

Can current models predict the local black hole merger rate? The VLT-FLAMES Tarantula Survey XVII. Physical and wind properties of massive stars at the top of the main sequence

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.451854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b0f51751-ae39-4801-bbdf-48016f7ffaaf · outbound

This paper cites J., Reeves J.

Can current models predict the local black hole merger rate? J., Reeves J

Reference 52

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.570256Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 16417658-eaa4-4cfe-982b-7e8a56d0a89c · outbound

This paper cites Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones.

Can current models predict the local black hole merger rate? Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.467223Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 917f488c-cf01-4c4d-bfc4-e202980855a1 · outbound

This paper cites A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417.

Can current models predict the local black hole merger rate? A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417

Reference 54

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.963483Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ee7b9c54-e49b-4fdf-a8eb-fb99a6d8c79a · outbound

This paper cites Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002.

Can current models predict the local black hole merger rate? Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.540036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a1425c8a-cba6-4def-ab38-da10607873a3 · outbound

This paper cites Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0.

Can current models predict the local black hole merger rate? Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.839012Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a42630a7-6f74-4511-b601-c3908e652f8f · outbound

This paper cites Pulsational pair instability as an explanation for the most luminous supernovae.

Can current models predict the local black hole merger rate? Pulsational pair instability as an explanation for the most luminous supernovae

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.547323Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ddc9577f-22fb-4ded-a919-6ed0d39828de · outbound

This paper cites Supernova 2007bi as a pair-instability explosion.

Can current models predict the local black hole merger rate? Supernova 2007bi as a pair-instability explosion

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.925945Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4f175e95-31e7-4257-8d81-268217f85518 · outbound

This paper cites The Astronomer's Telegram , keywords =.

Can current models predict the local black hole merger rate? The Astronomer's Telegram , keywords =

Reference 59

Resolution: unresolved; no resolver link, observed 2026-06-28T13:01:54.102298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 544e76c5-c1d7-4e2b-a712-357b19de8ba1 · outbound

This paper cites Super-luminous supernovae at redshifts of 2.05 and 3.90.

Can current models predict the local black hole merger rate? Super-luminous supernovae at redshifts of 2.05 and 3.90

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.846847Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c2b6151e-6be4-4d8a-864a-1556efc5f284 · outbound

This paper cites Can pair-instability supernova models match the observations of superluminous supernovae?.

Can current models predict the local black hole merger rate? Can pair-instability supernova models match the observations of superluminous supernovae?

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.861497Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b6a08ed4-96cc-47f0-a28a-62229d47b390 · outbound

This paper cites OGLE14-073 - a promising pair-instability supernova candidate.

Can current models predict the local black hole merger rate? OGLE14-073 - a promising pair-instability supernova candidate

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.747463Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8da9ffb6-1e72-4850-bb71-fd277ae69447 · outbound

This paper cites The nature of PISN candidates: clues from nebular spectra.

Can current models predict the local black hole merger rate? The nature of PISN candidates: clues from nebular spectra

Reference 63

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.575005Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation cb54533f-f1c9-4cd5-a0c5-ef82f6cac258 · outbound

This paper cites Evolution and fate of very massive stars.

Can current models predict the local black hole merger rate? Evolution and fate of very massive stars

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.633855Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 912de4c8-dfcf-4227-ac09-8b777710a4c1 · outbound

This paper cites Evolution and Nucleosynthesis of Very Massive Stars.

Can current models predict the local black hole merger rate? Evolution and Nucleosynthesis of Very Massive Stars

Reference 65

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T13:02:10.638946Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 09cfffd3-a128-49a3-b9fb-10d638b3e440 · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 66

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.781914Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation aced3b86-9044-484d-9647-46ad04b7dea1 · outbound

This paper cites Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way , year = 2012, editor =.

Can current models predict the local black hole merger rate? Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way , year = 2012, editor =

Reference 67

Resolution: unresolved; no resolver link, observed 2026-06-28T13:01:54.102298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d868f56-abc7-4b40-a54b-78369aa1883e · outbound

This paper cites Goswami and L.

Can current models predict the local black hole merger rate? Goswami and L

Reference 68

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.609532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 989edd5c-5e45-4dcd-aa66-78e7bf1a275f · outbound

This paper cites Core-Collapse Very Massive Stars: Evolution, Explosion, and Nucleosynthesis of Population III 500 -- 1000 $M_{\odot}$ Stars.

Can current models predict the local black hole merger rate? Core-Collapse Very Massive Stars: Evolution, Explosion, and Nucleosynthesis of Population III 500 -- 1000 $M_{\odot}$ Stars

Reference 69

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.891591Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2df289cb-ef02-4343-b235-a997536b0352 · outbound

This paper cites an unresolved cited work.

Can current models predict the local black hole merger rate? Unresolved cited work

Reference 70

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.662361Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d3411db1-9e2c-4a84-af64-67e8e74db4f3 · outbound

This paper cites , keywords =.

Can current models predict the local black hole merger rate? , keywords =

Reference 71

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.926923Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d3f3f4f0-068f-4c64-9a05-edc3bf70d705 · outbound

This paper cites Missing Link Found? --- The ``runaway'' path to supermassive black holes.

Can current models predict the local black hole merger rate? Missing Link Found? --- The ``runaway'' path to supermassive black holes

Reference 72

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.766445Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3e0150e0-7057-416d-829a-77c5ae5c539a · outbound

This paper cites , keywords =.

Can current models predict the local black hole merger rate? , keywords =

Reference 73

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.636514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4971c456-146f-4479-938b-c4cd4df0acf0 · outbound

This paper cites Merging black holes in young star clusters.

Can current models predict the local black hole merger rate? Merging black holes in young star clusters

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.938554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c09bf2b6-f4d0-4944-9af4-98d04f9ab38a · outbound

This paper cites Formation of black holes in the pair-instability mass gap: Evolution of a post-collision star.

Can current models predict the local black hole merger rate? Formation of black holes in the pair-instability mass gap: Evolution of a post-collision star

Reference 75

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.529899Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 887264dd-9346-42e5-a1ad-a8bcc519d911 · outbound

This paper cites The runaway growth of intermediate-mass black holes in dense star clusters.

Can current models predict the local black hole merger rate? The runaway growth of intermediate-mass black holes in dense star clusters

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.477278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 27004fe8-69c8-4121-bd6c-9cbac69a09d8 · outbound

This paper cites The formation of massive black holes through collision runaway in dense young star clusters.

Can current models predict the local black hole merger rate? The formation of massive black holes through collision runaway in dense young star clusters

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.756902Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a71a5a6e-3b74-4dfb-9ac6-e150c5f9d08e · outbound

This paper cites 1967", month =.

Can current models predict the local black hole merger rate? 1967", month =

Reference 78

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.918186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8bc5589d-de6b-4159-8b76-6f3b4afaf769 · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 79

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.874719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2a829a89-309e-4519-bdea-817ef11d6702 · outbound

This paper cites 1968", month =.

Can current models predict the local black hole merger rate? 1968", month =

Reference 80

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.752245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 0ced43ff-fa30-4b9e-a3e1-ab8cfbfa64c1 · outbound

This paper cites E., Heger A., Weaver T.

Can current models predict the local black hole merger rate? E., Heger A., Weaver T

Reference 81

Resolution: metadata mismatch; doi, observed 2026-06-28T13:02:10.572236Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 9f59108e-c8a7-4b48-bea5-2a362ecdb41c · outbound

This paper cites Two-Dimensional Simulations of Pulsational Pair-Instability Supernovae.

Can current models predict the local black hole merger rate? Two-Dimensional Simulations of Pulsational Pair-Instability Supernovae

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.754429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation bf69ec74-435e-47c5-b5c9-baad60d45cfb · outbound

This paper cites Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae.

Can current models predict the local black hole merger rate? Mass ejection by pulsational pair instability in very massive stars and implications for luminous supernovae

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.782597Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4db58375-e372-43a7-afef-4d7e81e9e469 · outbound

This paper cites Pair creation supernovae at low and high redshift.

Can current models predict the local black hole merger rate? Pair creation supernovae at low and high redshift

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.870940Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation eb64f891-5a67-4b92-a811-e648f7dd95a1 · outbound

This paper cites doi:10.1093/mnras/stac1100 , url =.

Can current models predict the local black hole merger rate? doi:10.1093/mnras/stac1100 , url =

Reference 85

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.847157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation cf6a7195-9c62-4a24-8345-7f6a7d2da046 · outbound

This paper cites 2020, ApJL, 902, L36, doi: 10.3847/2041-8213/abbadd.

Can current models predict the local black hole merger rate? 2020, ApJL, 902, L36, doi: 10.3847/2041-8213/abbadd

Reference 86

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.409069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3a2590ac-25de-467b-bacb-b4459c482b05 · outbound

This paper cites The Low Detection Rate of Pair Instability Supernovae and the Effect of the Core Carbon Fraction.

Can current models predict the local black hole merger rate? The Low Detection Rate of Pair Instability Supernovae and the Effect of the Core Carbon Fraction

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.525767Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c30743e4-3498-497a-9769-80402e76a99e · outbound

This paper cites keywords =.

Can current models predict the local black hole merger rate? keywords =

Reference 88

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.718233Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 9d408e8b-ab10-4d27-aefe-15c27b1be8d1 · outbound

This paper cites The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO.

Can current models predict the local black hole merger rate? The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO

Reference 89

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.688810Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a1e2cd88-db9e-4f33-9b36-bf753ef062cf · outbound

This paper cites Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries.

Can current models predict the local black hole merger rate? Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries

Reference 90

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.700522Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 087abe88-3989-4f96-b5a5-4d80eeae3c43 · outbound

This paper cites An upper limit on the spins of merging binary black holes formed through binary evolution.

Can current models predict the local black hole merger rate? An upper limit on the spins of merging binary black holes formed through binary evolution

Reference 91

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T13:02:10.698657Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 850e876d-4587-49c9-aafe-a5b1c6fd4229 · outbound

This paper cites Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity.

Can current models predict the local black hole merger rate? Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity

Reference 92

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.521782Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation befba1a8-e729-4f7b-99d0-42131f5b04c1 · outbound

This paper cites 2021, MNRAS, 505, 663, doi: 10.1093/mnras/stab1291.

Can current models predict the local black hole merger rate? 2021, MNRAS, 505, 663, doi: 10.1093/mnras/stab1291

Reference 93

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.523501Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 623c5e52-dc9f-4b7a-9320-406dca902ab8 · outbound

This paper cites 2023, A&A, 671, A62, doi: 10.1051/0004-6361/202244712.

Can current models predict the local black hole merger rate? 2023, A&A, 671, A62, doi: 10.1051/0004-6361/202244712

Reference 94

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.417091Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a9ef672c-46ce-4830-8002-e8a3a0b46aba · outbound

This paper cites arXiv e-prints , keywords =.

Can current models predict the local black hole merger rate? arXiv e-prints , keywords =

Reference 95

Resolution: unresolved; no resolver link, observed 2026-06-28T13:01:54.102298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd86b8bd-8330-4f61-b774-a23ef37778a5 · outbound

This paper cites , keywords =.

Can current models predict the local black hole merger rate? , keywords =

Reference 96

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.700378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 400ee337-0848-4309-9e3d-932ad21b554c · outbound

This paper cites 2024, MNRAS, 534, 151, doi: 10.1093/mnras/stae2048.

Can current models predict the local black hole merger rate? 2024, MNRAS, 534, 151, doi: 10.1093/mnras/stae2048

Reference 97

Resolution: verified exact; doi, observed 2026-06-28T13:02:10.724464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 3279a0c7-52f3-414f-b604-f1cc8cdcfffb · outbound

This paper cites Wind modelling of very massive stars up to 300 solar masses.

Can current models predict the local black hole merger rate? Wind modelling of very massive stars up to 300 solar masses

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.596292Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a442aa61-ec39-4ff2-a606-a55ab565bf49 · outbound

This paper cites The evolution of very massive stars.

Can current models predict the local black hole merger rate? The evolution of very massive stars

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.485021Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation eafdfaca-7a43-454d-a571-55d017391825 · outbound

This paper cites On the evolution and fate of supermassive stars.

Can current models predict the local black hole merger rate? On the evolution and fate of supermassive stars

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.898065Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Pith citing papers

Observation 27c2f311-538d-4675-a594-322d447f3eb2 · inbound

Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis cites this paper.

Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis Can current models predict the local black hole merger rate?

Reference 17

Resolution: metadata mismatch; local_arxiv, observed 2026-06-30T01:14:08.150701Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 24d21dea-d14a-4191-8674-1bb6af26bb89 · inbound

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation Can current models predict the local black hole merger rate?

Reference 150

Resolution: verified exact; local_arxiv, observed 2026-06-30T14:34:46.115446Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b74834ea-fa46-4f4c-91b3-c3d728a0a22f · inbound

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity cites this paper.

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity Can current models predict the local black hole merger rate?

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T00:42:17.115593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1063aa2b-e604-476e-bf85-f8a6a88c9cdc · inbound

Binary neutron star populations across cosmic time: the impact of binary stellar evolution uncertainties cites this paper.

Binary neutron star populations across cosmic time: the impact of binary stellar evolution uncertainties Can current models predict the local black hole merger rate?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T08:18:36.381451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.