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Paper Citation Record · LEDGER

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

As of 21 August 2026, this Paper Citation Record lists 100 of 155 outbound references and 1 inbound Pith citation observation for arXiv:2607.05208.

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

pith.paper-citation-record.v1
2607.05208 v1

Coverage vector

measured 100 of 155 reference resolution

Typed states for the displayed outbound observations.

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

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T00:39:49.564567Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-01T06:16:24.888925Z

Reference resolution

100 of 155 outbound references displayed

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External citation measurements

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Outbound references

Observation 7686baa8-87ba-46b1-a95e-bbb8af1e9e52 · outbound

This paper cites doi:10.3847/2041-8213/ace18b , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations doi:10.3847/2041-8213/ace18b , keywords =

Reference 1

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Observation 32eb11a6-ed40-444f-bfb3-6034d044bd43 · outbound

This paper cites doi:10.3847/2041-8213/acdac6 , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations doi:10.3847/2041-8213/acdac6 , keywords =

Reference 2

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Observation 45d0692c-b4cc-4883-97c3-5f12b708d27e · outbound

This paper cites good enough.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations good enough

Reference 3

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Observation a2c858c2-94d3-48be-8acb-30bb34aa6ed2 · outbound

This paper cites Arumugam, P.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Arumugam, P

Reference 4

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Observation 39c4dc70-3f4f-4c25-8711-2097283a3c84 · outbound

This paper cites Reardon and Andrew Zic and Ryan M.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Reardon and Andrew Zic and Ryan M

Reference 5

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Observation 859be1a8-84e8-404f-a7c9-369409fcc0ea · outbound

This paper cites Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I.Res.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I.Res

Reference 6

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Observation 3a50eda8-444b-4e83-8769-7951ea5d0e24 · outbound

This paper cites Premature supermassive black hole mergers in cosmological simulations of structure formation.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Premature supermassive black hole mergers in cosmological simulations of structure formation

Reference 7

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Observation fdcffbed-e996-49c7-9921-0d703879223e · outbound

This paper cites Nature , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Nature , keywords =

Reference 8

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Observation b56ba1fc-54bc-40f9-80d3-540954a4d171 · outbound

This paper cites Taylor , title =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Taylor , title =

Reference 9

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Observation efb05793-e1df-4894-b3a4-6d0ef243bf0b · outbound

This paper cites Z., Blecha, L., & Hernquist, L.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Z., Blecha, L., & Hernquist, L

Reference 10

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Observation 682c60f8-c06c-40ae-b02a-57434927676f · outbound

This paper cites The Gravitational Wave Background from Massive Black Holes in the ASTRID Simulation.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Gravitational Wave Background from Massive Black Holes in the ASTRID Simulation

Reference 11

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Observation 8b894468-c3b4-4b89-b4f7-e9b941fa25cc · outbound

This paper cites An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation

Reference 12

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Observation 0a598a3e-7da6-462f-a447-b338cb961ce8 · outbound

This paper cites The FABLE simulations: A feedback model for galaxies, groups and clusters.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The FABLE simulations: A feedback model for galaxies, groups and clusters

Reference 13

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Observation f4a7177f-3fe0-4279-8828-8b66c30d4c5c · outbound

This paper cites The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations

Reference 14

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Observation 5e49a0ef-1d83-40ef-a951-0d4a2566ff35 · outbound

This paper cites The baryon content of groups and clusters of galaxies in the FABLE simulations.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The baryon content of groups and clusters of galaxies in the FABLE simulations

Reference 15

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Observation 16bbc1bb-7ee7-43e8-9035-40e3f048eda4 · outbound

This paper cites Bigwood, M.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Bigwood, M

Reference 16

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Observation 8576f081-10fa-45c2-87ab-1148b8dbfa13 · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations H., Rantala, A., et al

Reference 17

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Observation e90735ed-5f29-4799-9aeb-df36072e3f51 · outbound

This paper cites Insights into the astrophysics of supermassive black hole binaries from pulsar timing observations , volume=.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Insights into the astrophysics of supermassive black hole binaries from pulsar timing observations , volume=

Reference 18

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Monthly Notices of the Royal Astronomical Society , volume =

Reference 19

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 20

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A., okas E

Reference 21

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Observation 47363478-fbd1-40ca-ad9e-202761cd26ea · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations M., Press W

Reference 22

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations and Shibahashi , H

Reference 23

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Observation 4177ae13-d891-4d19-adcc-746387743865 · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Simulating the joint evolution of quasars, galaxies and their large-scale distribution

Reference 24

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Observation 63c14bee-6959-4df1-90ca-78a4dbc8043a · outbound

This paper cites Comparing recent PTA results on the nanohertz stochastic gravitational wave background.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Comparing recent PTA results on the nanohertz stochastic gravitational wave background

Reference 25

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Observation 5b4fd1da-3010-4fbe-b762-c694a719655a · outbound

This paper cites R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607

Reference 26

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 27

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Observation 289d74e8-1d76-4946-b0b5-56d5796de234 · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Nature , keywords =

Reference 28

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astronomical Journal , keywords =

Reference 29

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Observation 78a01efc-2b9f-47ae-90b4-9238c0ceee8a · outbound

This paper cites Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

Reference 30

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 31

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Source-reported events for the cited work

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Observation 7d31d8d7-2cf7-471f-9bc1-e1e659f1667f · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations 2002, ApJ, 578, 90, doi: 10.1086/342308

Reference 32

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doi, observed 2026-07-07T23:34:19.167374Z

Source-reported events for the cited work

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Observation f34387a9-297a-4639-b28d-f0719eacceea · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 33

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Source-reported events for the cited work

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Observation 25a06598-d2d3-4229-b015-80984acecc87 · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 34

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Source-reported events for the cited work

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Observation bcc61745-d40c-438e-ae24-c2edf4c18336 · outbound

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Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 35

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:557db8042cae544df26b4615beddec27acdca9191a6fabb95d868cf9edce0915

Observation 3c94dca8-bbc2-4fae-a928-e0aa451f8a54 · outbound

This paper cites The Astrophysical Journal , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 36

Resolution
verified fuzzy
raw_fallback, observed 2026-07-07T23:34:19.713141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:8877d6982e58a49cdf99109245ed6ba825f6e0e3629fc39ff77c7d97c23541a4

Observation 7a34aa6a-80d2-41e8-bda0-fb80b75ebe42 · outbound

This paper cites The Astrophysical Journal , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-07-07T23:34:19.733769Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:6691fc14e55a12adb5e1efa56424f853590214c188cd4864bf8587eda1eae5b5

Observation 1e755172-54dd-4a55-9f38-4a5f7369be8c · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 38

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.195705Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:e8ec00cd36a0e89382df072581c0b9d93c85ca87ec92a2b8b3419dc4d083a247

Observation 643f28e3-91ea-40b2-9f05-09a1e55c22d2 · outbound

This paper cites The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.299205Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7df0fc3df4548a8c2d09fc32429eca5f6b4425f6c6f4c1b1097aa33fefda57a5

Observation 8d8cb14a-d8b6-44f7-add2-70ba0e5ecbcf · outbound

This paper cites Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive Galaxies

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.277465Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:467e071e08c47e9872d624eeb78f355d854c84493bd38f2e01e1d3f321f2ef05

Observation 2bdd45b3-8081-42eb-868a-4bd83915149f · outbound

This paper cites Observational constraints on the merger history of galaxies since $z\approx6$: Probabilistic galaxy pair counts in the CANDELS fields.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Observational constraints on the merger history of galaxies since $z\approx6$: Probabilistic galaxy pair counts in the CANDELS fields

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.365242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2afb666aced6f3ae16cb249c7778c6545c367935044996d23c95980b619cbf3a

Observation 04e04212-82ac-4ef4-b705-e7db20d748ff · outbound

This paper cites GA-NIFS: High number of dual active galactic nuclei at z~3.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations GA-NIFS: High number of dual active galactic nuclei at z~3

Reference 42

Resolution
metadata mismatch
local_arxiv, observed 2026-07-07T23:34:19.382254Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7e926d15e5bbf970888c5f661a2b9350298b69ee928973c6073bf287569eadac

Observation 69cb4f10-debb-4e5e-beba-aefeaace0553 · outbound

This paper cites GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang

Reference 43

Resolution
metadata mismatch
local_arxiv, observed 2026-07-07T23:34:19.489547Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:879079d9f26afda2a4c07fd6b28a0f9ac3b7be50b620fe40521218635728f56b

Observation d82c39b0-7e90-4147-a5ed-5c644eee01bd · outbound

This paper cites GA-NIFS: A massive black hole in a low-metallicity AGN at $z\sim5.55$ revealed by JWST/NIRSpec IFS.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations GA-NIFS: A massive black hole in a low-metallicity AGN at $z\sim5.55$ revealed by JWST/NIRSpec IFS

Reference 44

Resolution
metadata mismatch
local_arxiv, observed 2026-07-07T23:34:19.499470Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:592da072cc493981903fd6175ee25f144ae9da3054be4006f4d2f865235fd99c

Observation dc9f5cea-060f-45b2-a8e3-9b383e2e291a · outbound

This paper cites Comerford and Kyle Schluns and Jenny E.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Comerford and Kyle Schluns and Jenny E

Reference 45

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.334403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:ca62736076678d71c497393c455ec2a617fc01a921f5ea41b557aec538521931

Observation 9f028dc0-241e-40eb-8676-f47f7a4e1152 · outbound

This paper cites Rodriguez and G.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Rodriguez and G

Reference 46

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.237764Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:03e1b25f167c46d75953571c27331215b8582f07f6fb9707e8a3def9a0f498d3

Observation 5e74f127-25f9-49e5-8adb-c09bf3b42f43 · outbound

This paper cites D., Greene, J.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations D., Greene, J

Reference 47

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.210107Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:eb2c7e00198d84c3c64b49ac704dba34abb342dd5b5c391caa9d439b65c7678a

Observation e5e21a94-72a0-460f-b648-1897899625f2 · outbound

This paper cites GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCI.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCI

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.374632Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4502ba31a3cc11a17a26882a6aa113ba603e22738a1d3b30b2504b10a2c07cd6

Observation 2508f600-e8a7-4b25-8dc6-e7956a662b63 · outbound

This paper cites Where are NANOGrav's big black holes?.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Where are NANOGrav's big black holes?

Reference 49

Resolution
metadata mismatch
local_arxiv, observed 2026-07-07T23:34:19.337826Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a6715ae049c400335a6344cbb62a4a456d7a3607ab6fd0aaa10aedad7367ebb5

Observation 5fb2ad43-9a54-47b4-b139-088db6baba86 · outbound

This paper cites an unresolved cited work.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Unresolved cited work

Reference 50

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.200544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:ba6ec50f58e0b0492b527f59a23542c6b2875a6600f033daa7f2c85d405f063e

Observation 3400aa85-76e2-4366-ae88-c70c373abdd5 · outbound

This paper cites Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background

Reference 51

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.343272Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:362a1d9b6a01a25f625237df5009acc1a3dfbbf4719b3e9a1c3e5fe430aecf06

Observation 773eac71-ae44-4294-9bc0-dfdac92f15a4 · outbound

This paper cites T., Ogilvie G.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations T., Ogilvie G

Reference 52

Resolution
metadata mismatch
arxiv_id, observed 2026-07-07T23:34:19.441894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:72e4fed7b6124b45fec07bf34ae86eb4b6ad76f2700b9ce24c7f28abe288c4e3

Observation ec916d8a-79a9-4c4a-b54a-42ead130652d · outbound

This paper cites R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations R., 2009, @doi [ ] 10.1111/j.1365-2966.2009.15167.x , http://adsabs.harvard.edu/abs/2009MNRAS.398..607V 398, 607

Reference 53

Resolution
metadata mismatch
arxiv_id, observed 2026-07-07T23:34:19.450053Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:be9ff8287a5ecbe7e64472b3c4cb4f1561b254c5e0a4783d26f349b147126f15

Observation 52d75cf6-3ead-4b67-8c67-215563853503 · outbound

This paper cites The Astrophysical Journal Letters , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal Letters , keywords =

Reference 54

Resolution
verified fuzzy
raw_fallback, observed 2026-07-07T23:34:19.727324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:008ad0b79a1096118890ee7cded0e424d11da634643b194e0c23f6f03d0c2199

Observation 23f80233-8bd2-4303-901f-bc170f636c00 · outbound

This paper cites A black-hole mass measurement from molecular gas kinematics in NGC4526.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A black-hole mass measurement from molecular gas kinematics in NGC4526

Reference 55

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.509744Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:188ccc6507f1fbb1d5900dcc8c117515074bf89d5a08662956c7412ec4f891bc

Observation 5ff5cdda-37ee-49d4-b09e-c0153cac1dae · outbound

This paper cites A Stellar Dynamical Mass Measurement of the Black Hole in NGC 3998 from Keck Adaptive Optics Observations.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A Stellar Dynamical Mass Measurement of the Black Hole in NGC 3998 from Keck Adaptive Optics Observations

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.220300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3fa9020d70cfee39680cdfc17ccc4efac17bf38e88ed140c3eeb3524ac4bcd03

Observation 1a178fcd-fd65-4381-a3bd-b002588cefd5 · outbound

This paper cites A Measurement of the Black-Hole Mass in NGC 1097 using ALMA.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A Measurement of the Black-Hole Mass in NGC 1097 using ALMA

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.141713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:855e38b2791f84c344073e81d1390d06c49d8d21facd11778ceae32abb26da3a

Observation 1140719a-4ac0-4f49-a971-e68a054a94e0 · outbound

This paper cites and Yang , J.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations and Yang , J

Reference 58

Resolution
metadata mismatch
arxiv_id, observed 2026-07-07T23:34:19.330174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:4f1f79a8c5fc99ef717fad904acb669fce2698c654e381271aaaa5a599cb02d4

Observation 341eb5cd-433f-4eda-8b70-a6f99e5d2a95 · outbound

This paper cites A Search for "Dwarf" Seyfert Nuclei. IV. Nuclei with Broad H-alpha Emission.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A Search for "Dwarf" Seyfert Nuclei. IV. Nuclei with Broad H-alpha Emission

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.574254Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0cd1cd2bd47099afc8a60d3b50bda1cd839dce0ed271473a7823c62f55d0af8d

Observation 1f5abc90-be81-418c-9add-71e877e40175 · outbound

This paper cites Radio Sources in Low-Luminosity Active Galactic Nuclei.IV. Radio Luminosity Function, Importance of Jet Power, and Radio Properties of the Complete Palomar Sample.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Radio Sources in Low-Luminosity Active Galactic Nuclei.IV. Radio Luminosity Function, Importance of Jet Power, and Radio Properties of the Complete Palomar Sample

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.346276Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e15531dcf42add4bf241cd69045270f13f18ad896e3e848a609e62da4e67df33

Observation c0067d96-6e15-4b62-9f60-ddd26f448a94 · outbound

This paper cites The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.155202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:22206124e18f12edf723cfba63363342357073741b16660302ec714a1c2da162

Observation 6b415b81-45c1-4ee1-afe3-cc78e955b711 · outbound

This paper cites Chandra Snapshot Observations of Low-Luminosity AGNs with a Compact Radio Source.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Chandra Snapshot Observations of Low-Luminosity AGNs with a Compact Radio Source

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.464128Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f28b8efa1b08736272e13c6842dee31ade9e4587f7d3eefcb443855fc79b6920

Observation 75ffb8e4-3c0f-4c33-a3bc-f32daf0a0bfa · outbound

This paper cites M., Papadakis I.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations M., Papadakis I

Reference 63

Resolution
metadata mismatch
arxiv_id, observed 2026-07-07T23:34:19.431199Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:4ae91ac542e9cf618b8574708eba5c6c5365fce6a43301e145aa98689ae80ab7

Observation 442d99a1-b8d5-403a-986a-101345099086 · outbound

This paper cites Mignone and Jonathan C.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Mignone and Jonathan C

Reference 64

Resolution
metadata mismatch
arxiv_id, observed 2026-07-07T23:34:19.305023Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:3dc7190cd9c0d8c34c30d6ada4cf5e7c54a1e11acddf5d6f23a9b6d3fcbeb570

Observation c2c67bc3-66ba-45c4-8e1e-05c6896c15e1 · outbound

This paper cites The Mass Function of Active Black Holes in the Local Universe.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Mass Function of Active Black Holes in the Local Universe

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.292979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5c95fa2533fcca06f123098bce0010b3b75e1faf3e8ce1e290dfcef9befed152

Observation df959d60-b132-47fe-8dbe-758ec6b39ebb · outbound

This paper cites Annual Review of Astronomy and Astrophysics , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Annual Review of Astronomy and Astrophysics , keywords =

Reference 66

Resolution
verified fuzzy
raw_fallback, observed 2026-07-07T23:34:19.737719Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:2fa4d086a0a12772bfb79310148ed257b3d306663e538e9bf8103e5623ff0cb5

Observation 165f216a-5d38-46dd-92da-1b872973c790 · outbound

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

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Monthly Notices of the Royal Astronomical Society , keywords =

Reference 67

Resolution
verified fuzzy
raw_fallback, observed 2026-07-07T23:34:19.719147Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:2e35429c5103533480f81b53851891435ad619f84518e00b28d53e8d56233b3c

Observation 7ac554b2-fdcb-4d4e-9a30-fc02bd8bb82f · outbound

This paper cites A dormant, overmassive black hole in the early Universe.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A dormant, overmassive black hole in the early Universe

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.452822Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f87d05ed37192463fb472395edb18db38d3f57f63e76645e2e0c4aaf3dcbeb51

Observation cb8e9a23-5441-402d-8b06-61cd24673350 · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 69

Resolution
metadata mismatch
doi, observed 2026-07-07T23:34:19.180033Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:adb2db2c5e029ac24434d3b9c201786ee93ed651237911e6d136ca60abd281ef

Observation 4c3f46d6-febb-41ce-b8a4-a3205d8550f0 · outbound

This paper cites 2024, Nature Astron., 8, 126, 10.1038/s41550-023-02111-9.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations 2024, Nature Astron., 8, 126, 10.1038/s41550-023-02111-9

Reference 70

Resolution
metadata mismatch
doi, observed 2026-07-07T23:34:19.536085Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation da68087f-afc5-4c47-8ce9-e33ea5b36e11 · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 71

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation e7d47e99-68df-442b-b99b-e8c7adf65eba · outbound

This paper cites and LeBlanc , F.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations and LeBlanc , F

Reference 72

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arxiv_id, observed 2026-07-07T23:34:19.243702Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation bbab2c9e-0cbe-470d-a5d7-af586616c564 · outbound

This paper cites The Radiative Efficiency of Accretion Flows in Individual AGN.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Radiative Efficiency of Accretion Flows in Individual AGN

Reference 73

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local_arxiv, observed 2026-07-07T23:34:19.377521Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation c310baa4-ea48-45f2-b4da-dcf63b35f64f · outbound

This paper cites 2001 , eprint=.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations 2001 , eprint=

Reference 74

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 3a0a7d67-ea8a-469b-867a-764a248f4bd4 · outbound

This paper cites 2025 , eprint=.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations 2025 , eprint=

Reference 75

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Source-reported events for the cited work

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Observation 1c962f51-6ad7-4c35-ac1a-4f9ec0c6646d · outbound

This paper cites , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations , keywords =

Reference 76

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verified exact
doi, observed 2026-07-07T23:34:19.213486Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:f41e2d4fc3f1f486d8a5a5df3a3fb6f917b9250e3aa95de0b7ef21ab6767e7c3

Observation 227960c0-58dd-4f07-bc67-097648250506 · outbound

This paper cites Impact of the observation frequency coverage on the significance of a gravitational wave background detection in PTA data.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Impact of the observation frequency coverage on the significance of a gravitational wave background detection in PTA data

Reference 77

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local_arxiv, observed 2026-07-07T23:34:19.444582Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 2d641e23-b216-4870-9ec2-8458b65497a1 · outbound

This paper cites A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties

Reference 78

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local_arxiv, observed 2026-07-07T23:34:19.470003Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:548f0b9e99de3568ea2016c374a62bd733c27ac4ca03e3da17f197a26535f6f0

Observation 1437c447-3368-4b1c-a806-dda48524983b · outbound

This paper cites Testing strengths, limitations and biases of current Pulsar Timing Arrays detection analyses on realistic data.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Testing strengths, limitations and biases of current Pulsar Timing Arrays detection analyses on realistic data

Reference 79

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.472690Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation b7b829b5-abfc-48e5-9ec8-ffcc7a6588f5 · outbound

This paper cites Planck confronts large scale structure: methods to quantify discordance.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Planck confronts large scale structure: methods to quantify discordance

Reference 80

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.290029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 5aac17db-d70e-476a-a9b3-1e416cbdb80e · outbound

This paper cites The Astrophysical Journal , keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The Astrophysical Journal , keywords =

Reference 81

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Source-reported events for the cited work

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source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:ecb9248639ea200f0665a7307f680263dd12f4969a6b8c47b4216ffc73be0535

Observation 9c039ace-a55b-4074-bcb4-0f8cc330142a · outbound

This paper cites Tension between the power spectrum of density perturbations measured on large and small scales.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Tension between the power spectrum of density perturbations measured on large and small scales

Reference 82

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.164851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation a93c6274-79ca-43df-a6ed-f365efdb23f7 · outbound

This paper cites Massive black hole binary inspiral and spin evolution in a cosmological framework.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Massive black hole binary inspiral and spin evolution in a cosmological framework

Reference 83

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.437043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8401983a85135f621a9340e8e5f8bcbb01bf53cb25ebe3837113732fa330684d

Observation 645dbb3c-00b4-4153-b2ab-7cd728b1c335 · outbound

This paper cites Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band

Reference 84

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.399845Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 5b38a93f-db4d-4478-b324-fc2cd737f4fb · outbound

This paper cites and Veronesi, B.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations and Veronesi, B

Reference 85

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.311742Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation acd6abf9-2b67-43cf-9712-9a55015e9ba0 · outbound

This paper cites L., Kocevski, D.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations L., Kocevski, D

Reference 86

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arxiv_id, observed 2026-07-07T23:34:19.626014Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 24f0780c-3c33-4d90-90ab-2f14fb6a2010 · outbound

This paper cites Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays

Reference 87

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verified exact
local_arxiv, observed 2026-07-07T23:34:19.351808Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8e2a009512c8b9ab1296b69ef7f1ef4152ccc1fd69c7f45724071a2a12f3634b

Observation 1718676c-ef3f-4d2f-91b0-611c4e8e3325 · outbound

This paper cites Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations

Reference 88

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.481078Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:18cea35b85f9b7001f6990d29605522edff9c44f81d0dd685da94f3d3a74f010

Observation be424546-796c-4c8d-b6d2-428ea0928b6b · outbound

This paper cites Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Undermassive Host Galaxies of Five z~6 Luminous Quasars Detected with JWST

Reference 89

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local_arxiv, observed 2026-07-07T23:34:19.255164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 05f709f4-a52f-41c8-9538-fcb1d71b32a8 · outbound

This paper cites EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim6$.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $z\gtrsim6$

Reference 90

Resolution
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local_arxiv, observed 2026-07-07T23:34:19.183842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation cae58154-a6dc-4d28-8e05-4b58476d6e1e · outbound

This paper cites D., et al.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations D., et al

Reference 91

Resolution
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doi, observed 2026-07-07T23:34:19.307585Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 07b9c0b3-1732-4489-8be0-e22285c9b4fd · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 92

Resolution
verified exact
doi, observed 2026-07-07T23:34:19.511770Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:2830c1078351cbe6d8ad752c673147b826ed26c7c13732f5e8c14a529091763a

Observation 15b2e260-a046-4c35-8fd9-d731016b939e · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 93

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 7f8ad07d-7eb4-4f05-acb8-f1f2c7b3d919 · outbound

This paper cites A small and vigorous black hole in the early Universe.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations A small and vigorous black hole in the early Universe

Reference 94

Resolution
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local_arxiv, observed 2026-07-07T23:34:19.396642Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation 94628373-b457-4f98-aea4-26a84be24fc0 · outbound

This paper cites T., Ogilvie G.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations T., Ogilvie G

Reference 95

Resolution
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arxiv_id, observed 2026-07-07T23:34:19.433849Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:1eee40e51cf5a5e40e5be71cd8a8f07047cc2266ce68ba14f1379dd5dc40b7cc

Observation 7a93042c-482d-40c3-a350-061e2bff2534 · outbound

This paper cites How Big Can a Black Hole Grow?.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations How Big Can a Black Hole Grow?

Reference 96

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local_arxiv, observed 2026-07-07T23:34:19.402299Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7d6e0cfd94c5539888cc025689d1762a52c330ba5b961ad060a4fd6aad30c2a2

Observation c83db13d-838e-4e19-bce5-648a90dca880 · outbound

This paper cites The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTI.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTI

Reference 97

Resolution
metadata mismatch
local_arxiv, observed 2026-07-07T23:34:19.137302Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:21a65c70bc8ef71037de2b99dfe0f662371f88bcd7e2348a43352c56ab87d2ba

Observation 4596f81c-f081-4f92-b966-bb490e24de9d · outbound

This paper cites keywords =.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations keywords =

Reference 98

Resolution
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doi, observed 2026-07-07T23:34:19.321961Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:8ff29fec710dd255d4d2078b87d3105042d8450b3db7682657dd9db4c1da934b

Observation 30c53dfe-6bd8-4570-93e2-aaefb2731a59 · outbound

This paper cites Evaluating the prevalence of spurious correlations in pulsar timing array datasets.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Evaluating the prevalence of spurious correlations in pulsar timing array datasets

Reference 99

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local_arxiv, observed 2026-07-07T23:34:19.354368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0b297d7219b92f80afb1cc9af80164502af4293845051b6d9273fb5a6ac47a71

Observation 6c028f5f-2a2b-4319-b925-85f1fa69b1f7 · outbound

This paper cites and Chen, Siyuan and Keane, Evan F.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations and Chen, Siyuan and Keane, Evan F

Reference 100

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doi, observed 2026-07-07T23:34:19.557173Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-07T23:29:47.022382Z digest=sha256:5d04a42bfd33abe0b7f15f0b6bbb9152038e513240744556fbd8b7f3f9f9ad40

Pith citing papers

Observation 652d7c7b-0e7b-406a-9a78-d5fb78bac3ca · inbound

How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations cites this paper.

How to raise a supermassive black hole: interpreting early JWST AGN with the AESOPICA simulations Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations

Reference 264

Resolution
metadata mismatch
local_arxiv, observed 2026-08-01T00:41:15.127047Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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