Pith. sign in

Paper Citation Record · LEDGER

The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 38 inbound Pith citation observations for arXiv:1602.04531.

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

pith.paper-citation-record.v1
1602.04531 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 38 of 38 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 38 of 38 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:36:24.883746Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T20:06:29.399869Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation aaa5b336-cff6-459c-a4ae-ff2c358892fe · inbound

From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back) cites this paper.

From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back) The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-14T14:17:26.448998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:17:26.448998Z digest=sha256:91b2c004e02a95fc45f5e601d451f0b4c50ebc532c07258774e590a6df0bca14

Observation cf31e6fa-56b2-4305-b392-8b9fdd67b171 · inbound

Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO cites this paper.

Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-14T13:03:14.524592Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:03:14.524592Z digest=sha256:15a57609d1b30307fc520114c603cfb781790fadfe60f8ab34c059c6cb0a9c26

Observation 963c1c60-7467-406e-84db-625183f24f6e · inbound

Lower bound on the primordial black hole merger rate cites this paper.

Lower bound on the primordial black hole merger rate The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-14T11:08:41.296437Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T11:08:41.296437Z digest=sha256:c232ff6978f53cea400926d338b68dd57c71ebbdd37767715c42743fd7365b46

Observation 93cd79f5-2812-4255-a5c6-a1dcd88ca387 · inbound

The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range cites this paper.

The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T10:21:18.934439Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:21:18.934439Z digest=sha256:31254306cc9a151d954ec5c8844f3e318522a3433aad8904e647f0cee7579758

Observation edc908cc-a5b2-45e5-83bc-dc3a86482906 · inbound

Primordial Black Holes as Dark Matter: Recent Developments cites this paper.

Primordial Black Holes as Dark Matter: Recent Developments The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-05-16T12:15:13.312958Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-16T12:15:12.881226Z digest=sha256:1e1e705ac8ba0ab61ae1e964ae0041daacef475476349cc216b4bdf476c0e094

Observation 3d49679d-7604-4e61-aa30-b30c51ea0f43 · inbound

Astrophysics with the Laser Interferometer Space Antenna cites this paper.

Astrophysics with the Laser Interferometer Space Antenna The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 6

Resolution
verified exact
local_arxiv, observed 2026-05-25T08:23:22.995108Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:5436941f0d69f9c697738eb2a9fd91cacde23f63ac74648778020c93ddee18e9

Observation dc9efb9e-fc2a-4416-93c1-5e16246a2f1d · inbound

Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA cites this paper.

Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 18

Resolution
verified exact
local_arxiv, observed 2026-05-24T01:35:55.733362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-24T01:34:53.946159Z digest=sha256:5551d210e703f4ce0b29ffee98af551cadc8e51717fc1eedeb4cad40807df5b4

Observation 0d6dd101-1762-4640-a546-b3a07daef628 · inbound

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM cites this paper.

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-11T13:49:12.567060Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:49:12.567060Z digest=sha256:7449478a53ceaecbc0ca925c52b5015d47efed1c338a3aa4b5c617af53a87a71

Observation ebeee171-9701-4943-b5ad-cc93a2942db1 · inbound

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM cites this paper.

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-11T13:46:54.532072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:46:54.532072Z digest=sha256:2bf21f7b259e9673c55b1d132aa41b5975e6740087fe7636b5d5358dd9e34a7d

Observation 3890b5b8-3525-4649-8a3c-37ae832913b5 · inbound

Topological dark energy from black-hole formations and mergers through the gravity-thermodynamics approach cites this paper.

Topological dark energy from black-hole formations and mergers through the gravity-thermodynamics approach The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-10T23:12:12.836660Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:12:12.836660Z digest=sha256:a8b60ca8c5cb328d956c6f6eac7c507ba5c97ac547f0583bf13b2a0cb3febe63

Observation e8085093-12fd-4318-b730-8ce5edbbe8d1 · inbound

Observational implications of Wald-Gauss-Bonnet topological dark energy cites this paper.

Observational implications of Wald-Gauss-Bonnet topological dark energy The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T14:00:11.028801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:00:11.028801Z digest=sha256:ff40c9685ebd2eac2ee00485f18def14833efbcd5704ff5512c93a838436becb

Observation 171e507a-40d3-4eee-b19d-61c4fb6c34fb · inbound

Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors cites this paper.

Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-08T11:43:23.758814Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:43:23.758814Z digest=sha256:7d588a07615a94c2e548b66c73f2ca22df9f3ac5b977af8eeed7f58c30573f34

Observation b4707442-fd3b-4953-a98d-d23cd6698507 · inbound

Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations cites this paper.

Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-15T21:36:24.883746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T21:36:24.883746Z digest=sha256:aa2badc3021bd70ed53f7d44f06f60397afb3bd60013547db3a92edc28163e64

Observation 467c58ec-eebf-4b97-917d-8d3c2864b93a · inbound

Inferring the pair-instability mass gap from gravitational wave data cites this paper.

Inferring the pair-instability mass gap from gravitational wave data The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-07T05:02:00.945607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:02:00.945607Z digest=sha256:90dea8072c097adec7b0b7cf63f77742b222548bb582b011eb268fae704dc656

Observation d697034b-c387-47d2-bf27-a5850418e702 · inbound

Disentangling spinning and nonspinning binary black hole populations with spin sorting cites this paper.

Disentangling spinning and nonspinning binary black hole populations with spin sorting The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-05-19T02:22:56.311244Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-19T02:22:28.762392Z digest=sha256:28c47cd9bf83bb16a8fce27c353c4e9bfcb34b26017f9efde35e0e111091abe7

Observation b071ad51-83b3-44c3-91f4-081d0516d4b4 · inbound

An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources cites this paper.

An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-05-18T17:06:39.261724Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-18T17:06:36.862923Z digest=sha256:1d96359ebcb1ceb51a10f416cedc99f0080412361309fbad613fc8386d95c192

Observation 473947eb-b70d-436a-857c-b1bacd312d98 · inbound

Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors cites this paper.

Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-04T07:36:39.968979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T07:36:39.968979Z digest=sha256:cc78219b146b38f37d652a33a94417834d1d2386488b2bbca35f4f96a6e13b2e

Observation 89f2a6f6-f2ec-4fac-9799-b2f0248c5657 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:23.865950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:23.865950Z digest=sha256:2f726002b732cf34e59d03fbb22ff3cb5b979deb59b4657730a8a5aa8e6c56c6

Observation bbe5c436-5857-40dc-8268-5dce8223aab1 · inbound

Population Properties of Binary Black Holes with Eccentricity cites this paper.

Population Properties of Binary Black Holes with Eccentricity The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 27

Resolution
verified exact
local_arxiv, observed 2026-05-16T02:30:31.441795Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-16T02:28:53.190725Z digest=sha256:ae165eedc1d13730ea9df58e572d18663bf59797edc49e1ab660f11b1deaf41d

Observation a331a250-4ada-46e2-a47e-a95167b24186 · inbound

The impact of the formation channel on gravitational-wave-galaxy cross-correlations cites this paper.

The impact of the formation channel on gravitational-wave-galaxy cross-correlations The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-02T23:08:01.663341Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T23:08:01.663341Z digest=sha256:9e0f755dcda3c0fe8e7b5d44130193feea42f68383ef9c2008e237ccf43d2440

Observation 0f05e0b4-450a-4cb5-a731-985799da3b61 · inbound

The Black Hole Mass Gap as a New Probe of Millicharged Particles cites this paper.

The Black Hole Mass Gap as a New Probe of Millicharged Particles The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 91

Resolution
verified exact
arxiv_id, observed 2026-05-13T21:03:19.773982Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-13T21:01:01.821843Z digest=sha256:351753fa4a542d5b128f5a9d4dab5d8d433b0acff4fc0ff417679ea1b49e05c7

Observation d8a83e54-ecad-486b-b537-562109cb309b · inbound

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes cites this paper.

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 9

Resolution
verified exact
arxiv_id, observed 2026-05-12T10:21:28.428325Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-07T06:35:15.070035Z digest=sha256:fe97d55450e5a13d549d765f3969e1fa14769334e6bbd69789ee60ae5d131899

Observation edfcbd34-02e9-4da8-8323-c9264265033c · inbound

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes cites this paper.

Constraining Dipole Radiation with Multiband Gravitational Waves from Eccentric Binary Black Holes The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-02T15:13:21.607736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T15:13:21.607736Z digest=sha256:bdf2c5ff02cb27bafa90775a51df09083fee006e9e75e4327d802ff736c0798a

Observation 1c7d17c6-93bf-44da-8933-16f383e2f3fe · inbound

Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum cites this paper.

Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 15

Resolution
verified exact
arxiv_id, observed 2026-05-11T20:51:12.927308Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-08T07:48:04.948543Z digest=sha256:6360b781fdb46078458c50af344c55b927e72ee7cccc2877b58c89a09dd1e800

Observation 5d52f1d3-f2f9-4a94-ba0e-af1856dba0a3 · inbound

Assessing the imprint of eccentricity in GW signatures using two independent waveform models cites this paper.

Assessing the imprint of eccentricity in GW signatures using two independent waveform models The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-05-14T19:22:51.083360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-14T19:19:56.792712Z digest=sha256:3bf8dab2921397d2f039df50d6c56ac1500931c530dc0a326b32cabe4d411f2f

Observation 0922c808-045d-4b11-ba21-26ef4c88bc9d · inbound

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM cites this paper.

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-06-29T10:43:18.939722Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-29T10:39:57.468339Z digest=sha256:78a14b13f3ca99ce9282b12711168bff5dd8c919dde4bdcc9e214e1698c1679b

Observation c619e44b-aaf4-48ce-8a2e-774737a5a7a5 · inbound

Mapping the star formation peak with LIGO A# and Next-Generation detectors cites this paper.

Mapping the star formation peak with LIGO A# and Next-Generation detectors The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 223

Resolution
metadata mismatch
local_arxiv, observed 2026-06-28T05:11:39.626766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ea343dcd4f4a60deacf909e4685240d6bd2ce6a623ba4761a43e5807a9bbf24e

Observation 4dc94591-fc19-4891-b6bd-0b8a8833c7be · inbound

The first decade of gravitational-wave measurements of black hole spins cites this paper.

The first decade of gravitational-wave measurements of black hole spins The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-06-28T00:21:27.818541Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:d7836a7fcb1f11648f863552c92b5027ec6e23ab5b0d4e747751744c392828e6

Observation 52a32684-561e-44a2-8478-1cc572067340 · inbound

The first decade of gravitational-wave measurements of black hole spins cites this paper.

The first decade of gravitational-wave measurements of black hole spins The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-02T12:20:50.847664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T12:20:50.847664Z digest=sha256:58b964e39fcaefcf81a16f8b8098c3a5a29b92be7a50dd2c29f51c9bafba012b

Observation 0274ccbb-e167-461b-a918-f177fa1c340a · inbound

The Chirp-Mass Ladder: A New Rung Emerges cites this paper.

The Chirp-Mass Ladder: A New Rung Emerges The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 262

Resolution
verified exact
local_arxiv, observed 2026-06-26T23:10:13.957502Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:182c7b0bbc37c52c32d7aa892d507b869276ee8ca080dc0039d967cc628a6a2a

Observation 4f3c55d5-8122-42de-9ece-9f4bbb4cd003 · inbound

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-06-26T09:59:18.401207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c4e3e3de50b2a2037ad278f4b8c35f5ffe1cae91536370bfca61ac6299457a1f

Observation 8337807c-db27-40de-b5a5-8723c2433eef · inbound

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO cites this paper.

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 191

Resolution
metadata mismatch
local_arxiv, observed 2026-06-27T01:30:20.726262Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d9817fa3b56cdd47e6353ce72804a9548d7231819014105d573ad24d286e515a

Observation e2aad704-ec13-4fb2-ad2f-7a8b424f5e26 · inbound

Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.

Constraints on Line-of-Sight Acceleration from O1-O4 The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-07-04T19:40:06.410588Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-06-25T21:10:34.484784Z digest=sha256:af3ff7fa42fc11b335a357586fff892f2870732f8847f08db55d2dc13c4a63b3

Observation 29fe376a-acdb-4c16-aa99-90ab6e576cc7 · inbound

Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.

Constraints on Line-of-Sight Acceleration from O1-O4 The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-02T10:17:28.859085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T10:17:28.859085Z digest=sha256:94829626644b10c8c028be35c47d3e67415dfe59309fb964b8cdb73a461e3397

Observation 89ccd278-6e4d-47ef-8e03-f103c6d0d0ce · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 26

Resolution
verified exact
local_arxiv, observed 2026-07-08T17:55:20.586047Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-07-08T17:53:06.845093Z digest=sha256:cab9a3b32a46e575406b1e87126f75e6051e02ac0a01e163f1fbe1eabee4ffa3

Observation 3acae516-541a-4969-b8e1-711a9d2b99c0 · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 51

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:06:29.401235Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8a499284836426e9764f44a83bd9a8bfb8d929e21698af4c6294d1aa7b879dc3

Observation 7a2e1c10-29ba-4dcf-939b-2880b011a7fb · inbound

Assessing the waveform systematics from parameter estimation to population inference with eccentricity cites this paper.

Assessing the waveform systematics from parameter estimation to population inference with eccentricity The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-01T23:22:35.061930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T23:22:35.061930Z digest=sha256:d714dc35229104a2017b1803962940d664d69b21a8ff4ddbd69a1df313ae7eb8

Observation 086c7be7-2c70-4525-8edf-191843427e56 · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-01T02:46:23.040863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T02:46:23.040863Z digest=sha256:29c42df363a5997d90b45c12eb57780f7960ae87115585a82c2f3efb461e4bea