Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories | Paper Citation Record

Observation 912092c4-ecbf-4be7-8e54-87b0633bb821 · outbound

This paper cites Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.888716Z

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Observation 7f1b1ed7-bfeb-4ef6-adbf-c9e31a10b66f · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.893568Z

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Observation 2eed9374-8752-4174-bdf5-850180f8e502 · outbound

This paper cites Advanced LIGO.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Advanced LIGO

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.897228Z

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Observation 6ec75d1d-3951-42fd-8993-98b420dc23b9 · outbound

This paper cites Advanced Virgo: a 2nd generation interferometric gravitational wave detector.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Advanced Virgo: a 2nd generation interferometric gravitational wave detector

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.901302Z

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Observation b9cccb5b-3611-4859-b425-a956db894c2f · outbound

This paper cites Acernese and P.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Acernese and P

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.905136Z

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Observation e3b08e35-a857-4979-b6ba-122a19c92ebe · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.908798Z

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Observation 73accff5-89f6-4d07-980a-8efcf2e731ea · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.912753Z

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Observation 0d953973-1192-4245-9aff-9b863e3edce9 · outbound

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

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.920345Z

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Observation a0a44dec-cbc7-4c4f-9a8a-fd91681a4efe · outbound

This paper cites GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.924371Z

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Observation d2bd42a6-b861-48d1-ad52-5e1e6ec3d974 · outbound

This paper cites Science Case for the Einstein Telescope.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Science Case for the Einstein Telescope

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.932202Z

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Observation e5780663-df7f-4d98-a527-f21983be74a9 · outbound

This paper cites The Science of the Einstein Telescope.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The Science of the Einstein Telescope

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.936163Z

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Observation 83976adb-b8d0-497e-a6e2-92dd92f4241c · outbound

This paper cites Punturo et al.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Punturo et al

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.940024Z

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Observation 68049916-e1eb-45d9-b13c-1f89e995bb20 · outbound

This paper cites A Horizon Study for Cosmic Explorer: Science, Observatories, and Community.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories A Horizon Study for Cosmic Explorer: Science, Observatories, and Community

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.943753Z

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Observation e9ff7777-88f7-4101-b55f-4dbbed259501 · outbound

This paper cites Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.947573Z

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Observation 8355b923-159f-477b-b454-c3dcfc73bb46 · outbound

This paper cites Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.951544Z

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Observation e73a9271-672d-4678-9603-9d74d35e3538 · outbound

This paper cites Probing multiple populations of compact binaries with third-generation gravitational-wave detectors.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Probing multiple populations of compact binaries with third-generation gravitational-wave detectors

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.955422Z

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Observation b2cf8c11-b674-4eac-a4e5-c80bcadeaa4d · outbound

This paper cites Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\texttt{GWFAST}$.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\texttt{GWFAST}$

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.959159Z

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Observation b70a820c-b2f1-4c96-a25f-c6026244f327 · outbound

This paper cites Constraining Population III stellar demographics with next-generation gravitational-wave observatories.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Constraining Population III stellar demographics with next-generation gravitational-wave observatories

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.962966Z

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Observation 34518c2d-b375-41d9-bf11-a3beafa422e9 · outbound

This paper cites Fishbach, D.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Fishbach, D

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.966969Z

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Observation 51c3b170-e104-42d1-953b-a164a2090355 · outbound

This paper cites LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.970458Z

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Observation e156f897-1013-4170-a567-e6e23df3186b · outbound

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

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-4.0: Population Properties of Merging Compact Binaries

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.974395Z

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Observation 231599a8-5f24-45fd-8805-218cf7ce8bb5 · outbound

This paper cites Natarajan et al.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Natarajan et al

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.977978Z

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This paper cites Quasars and the Intergalactic Medium at Cosmic Dawn.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Quasars and the Intergalactic Medium at Cosmic Dawn

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.981602Z

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Observation 6ed13593-c0ec-44bb-a759-62156c901608 · outbound

This paper cites The Formation and Evolution of Massive Black Holes.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The Formation and Evolution of Massive Black Holes

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.985410Z

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Observation adb27700-4132-4529-9f0b-567c094b66a4 · outbound

This paper cites Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Massive black hole binaries in LISA: constraining cosmological parameters at high redshifts

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.989253Z

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Observation 82a47aef-a210-48d0-8586-50538dbe3ba3 · outbound

This paper cites The Growth of Black Holes from Population III Remnants in the Renaissance Simulations.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The Growth of Black Holes from Population III Remnants in the Renaissance Simulations

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:30.363107Z

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No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 4f34d9d7-c98c-4bd5-a2fe-86a570517ba6 · outbound

This paper cites Massive Black Holes as Population III Remnants.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Massive Black Holes as Population III Remnants

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:28.996279Z

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Observation 189441c5-b0ef-4542-904c-d2374d5e1a5d · outbound

This paper cites Very high redshift quasars and the rapid emergence of super-massive black holes.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Very high redshift quasars and the rapid emergence of super-massive black holes

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Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:30.334380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 14946fa2-0e5e-48a2-805c-f7f66ef7c810 · outbound

This paper cites Pair-Instability Supernovae, Gravity Waves, and Gamma-Ray Transients.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Pair-Instability Supernovae, Gravity Waves, and Gamma-Ray Transients

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.003153Z

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Observation dc5168f3-23e7-44f0-93e3-562379398ced · outbound

This paper cites Magnetic fields catalyze massive black hole formation and growth.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Magnetic fields catalyze massive black hole formation and growth

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.007213Z

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Observation 0c795ed1-4ead-419c-9ffd-78f795ef1efc · outbound

This paper cites Overview of the JWST Advanced Deep Extragalactic Survey (JADES).

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.011199Z

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Observation 3eb32ae7-6987-41da-a8db-86bc6cb935ce · outbound

This paper cites JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.015001Z

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This paper cites Chira et al.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Chira et al

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Source-reported events for the cited work

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Observation d803f004-4170-4023-a0b3-bc3e88ba2654 · outbound

This paper cites Detection of stellar light from quasar host galaxies at redshifts above 6.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Detection of stellar light from quasar host galaxies at redshifts above 6

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.022925Z

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Observation db249dce-9432-41d3-93d8-f3363ed36a55 · outbound

This paper cites The accretion of a solar mass per day by a 17-billion solar mass black hole.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The accretion of a solar mass per day by a 17-billion solar mass black hole

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Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:30.188393Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 754121a5-8f05-4d63-8d98-021d13f128d0 · outbound

This paper cites Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.030577Z

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Observation 164a5ac3-b665-485b-98d4-caea937a9c79 · outbound

This paper cites The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.034471Z

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Observation 58ca96df-9a3b-4b25-9f89-30d4e1d2a7a6 · outbound

This paper cites Gravitational Waves from the Remnants of the First Stars.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Gravitational Waves from the Remnants of the First Stars

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.038344Z

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Observation ee833d84-04f2-4b8d-a310-e064e1318fd4 · outbound

This paper cites On the likelihood of detecting gravitational waves from Population III compact object binaries.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories On the likelihood of detecting gravitational waves from Population III compact object binaries

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.042091Z

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Observation 8a764953-de1f-4a34-a92d-c625b2ef1f9b · outbound

This paper cites Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Population III Binary Black Holes: Effects of Convective Overshooting on Formation of GW190521

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.045994Z

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Observation 5a499573-b473-4986-b734-53c66b70ed19 · outbound

This paper cites Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Merger rate density of binary black holes through isolated Population I, II, III and extremely metal-poor binary star evolution

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.050117Z

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Observation d52799a1-7bf0-4cbb-8a04-fe14ac3edea9 · outbound

This paper cites Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Constraining high-redshift stellar-mass primordial black holes with next-generation ground-based gravitational-wave detectors

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.053915Z

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Observation 648b0f49-6c11-42e4-b1f7-d84a60781771 · outbound

This paper cites Gravitational waves from Population III binary black holes formed by dynamical capture.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Gravitational waves from Population III binary black holes formed by dynamical capture

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.057883Z

Source-reported events for the cited work

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Observation 043fc9c9-7f51-458c-9934-4bb86d57ab1a · outbound

This paper cites Massive binary black holes from Population II and III stars.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Massive binary black holes from Population II and III stars

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Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:30.077517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 873a7a58-ba3d-428b-8116-457e28f76393 · outbound

This paper cites Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.065630Z

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Observation ac8d3e77-ffed-4dff-8d2d-a332274a6c62 · outbound

This paper cites On the single-event-based identification of primordial black hole mergers at cosmological distances.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories On the single-event-based identification of primordial black hole mergers at cosmological distances

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.069394Z

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Observation 29bdfa9c-06ca-4f23-a311-82762c32c659 · outbound

This paper cites Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.072853Z

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Observation 203e03fc-fc4d-463a-9fda-9939a0fe1736 · outbound

This paper cites Vitale, D.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Vitale, D

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.076285Z

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Observation a7eccbc2-ed27-4bb8-84f0-3700c7f49195 · outbound

This paper cites Mancarella, F.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Mancarella, F

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.079475Z

Source-reported events for the cited work

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Observation 6808a638-ee81-45b6-8c06-6fdc74ddc4c1 · outbound

This paper cites Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.082563Z

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Observation 4cf1e36f-4416-42d9-a99b-438e1dc73b57 · outbound

This paper cites Bressan, P.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Bressan, P

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.085957Z

Source-reported events for the cited work

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Observation 61e84745-c8aa-4ac9-b0e0-aa62a5368ecb · outbound

This paper cites Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.089165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 563462da-5eee-4659-bc80-3475eb0d7799 · outbound

This paper cites The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.093073Z

Source-reported events for the cited work

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Observation 93a04b26-9767-49f7-8280-51bc680ba4a5 · outbound

This paper cites Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.097032Z

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Observation 597416a5-1510-4ced-9c21-7d8c4aa6169f · outbound

This paper cites IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.100881Z

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Observation a0e5e643-8f53-4b59-93d8-e3500ed08569 · outbound

This paper cites The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole

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Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.104797Z

Source-reported events for the cited work

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Observation ed4ac97e-0050-4b19-ac7f-77cdc438aa09 · outbound

This paper cites Bayesian coherent analysis of in-spiral gravitational wave signals with a detector network.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Bayesian coherent analysis of in-spiral gravitational wave signals with a detector network

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.108605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a808acd5-a742-43a0-90f4-eec1fe0459d8 · outbound

This paper cites Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.112462Z

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Observation 104b6e07-7264-45e6-8f2d-968901648b95 · outbound

This paper cites Skilling, Nested sampling for general Bayesian compu- tation, Bayesian Analysis 1, 833 (2006).

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Skilling, Nested sampling for general Bayesian compu- tation, Bayesian Analysis 1, 833 (2006)

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.116349Z

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Observation b3a0cb66-1773-48fa-9a23-96297689f650 · outbound

This paper cites Measuring precession in asymmetric compact binaries.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Measuring precession in asymmetric compact binaries

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.119946Z

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Observation 3d8e01ec-75b1-4921-9d64-683a8cee2bb9 · outbound

This paper cites dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.123887Z

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Observation a5946fee-a2b8-4c4f-a409-cacf941b1634 · outbound

This paper cites Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.127691Z

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Observation 816d467a-30a4-4c0d-ad0a-37537fd81272 · outbound

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

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.131548Z

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Observation 10337e6d-e4bf-4922-a673-7e8de12da97e · outbound

This paper cites GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.138739Z

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Observation a7455b40-4382-49ca-94ab-581b80589e70 · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.142649Z

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Observation d7f2962e-29ab-4804-91fe-d114016bbd71 · outbound

This paper cites Planck 2015 results. XIII. Cosmological parameters.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Planck 2015 results. XIII. Cosmological parameters

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.146503Z

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Observation b9c1230d-a7ee-4014-a61f-d46747375aa4 · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.150007Z

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Observation bd7bf4a3-68f3-471d-845d-f587b84e63f9 · outbound

This paper cites Urrutia, J.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Urrutia, J

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.153996Z

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Observation ca4f6077-3961-4489-8394-ce31407ee9c4 · outbound

This paper cites Is black-hole ringdown a memory of its progenitor?.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Is black-hole ringdown a memory of its progenitor?

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.157754Z

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Observation 74169b9a-6278-4557-9537-f8bf8f784f94 · outbound

This paper cites Modeling Ringdown: Beyond the Fundamental Quasi-Normal Modes.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Modeling Ringdown: Beyond the Fundamental Quasi-Normal Modes

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.161643Z

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Observation e85040d6-0196-4417-9866-02f5396cc83c · outbound

This paper cites Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Comparison of post-Newtonian mode amplitudes with numerical relativity simulations of binary black holes

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.165377Z

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Observation 5e49782c-9b88-48d8-a959-f9cbb726da45 · outbound

This paper cites Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.168804Z

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Observation c988046d-8a45-428b-9fdb-a48b39f4fe00 · outbound

This paper cites Persistence of post-Newtonian amplitude structure in binary black hole mergers.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Persistence of post-Newtonian amplitude structure in binary black hole mergers

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:29.672919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation f98f0927-6df2-4485-9257-8e6afbc62d2c · outbound

This paper cites Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.175793Z

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Observation bbb4e921-6a1b-471e-aeaa-5b19f5274f66 · outbound

This paper cites Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Towards models of gravitational waveforms from generic binaries II: Modelling precession effects with a single effective precession parameter

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.179169Z

Source-reported events for the cited work

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Observation 570bff0b-2e88-4bda-9811-6e92cea1c3bf · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.183087Z

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Observation 38a8b6c1-3626-442a-b53c-9eb9dd3b5af3 · outbound

This paper cites Validating Bayesian Inference Algorithms with Simulation-Based Calibration.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Validating Bayesian Inference Algorithms with Simulation-Based Calibration

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.186648Z

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Observation bbccfe11-7e94-4ca4-99ed-e8db539af414 · outbound

This paper cites Evolution of massive population III stars with rotation and magnetic fields.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Evolution of massive population III stars with rotation and magnetic fields

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.190660Z

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Observation c222d778-d54f-4bbf-95ce-4f6e09c0d8c7 · outbound

This paper cites Rotation and Internal Structure of Population III Protostars.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Rotation and Internal Structure of Population III Protostars

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:29.619348Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 4ab6e633-528d-4471-9feb-1bc2e1648f4f · outbound

This paper cites Constraining the Statistics of Population III Binaries.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Constraining the Statistics of Population III Binaries

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.198370Z

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Observation 56b3a155-c0b6-4166-a5fe-963c765c801d · outbound

This paper cites Advancing Astrophysics with the SKA II.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Advancing Astrophysics with the SKA II

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.202222Z

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Observation d625cd27-5cab-4fa1-881a-617c45dbb926 · outbound

This paper cites Cosmology from Synergies Between SKAO Surveys and Gravitational Wave Observations.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Cosmology from Synergies Between SKAO Surveys and Gravitational Wave Observations

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Resolution: verified exact; local_arxiv, observed 2026-08-07T22:32:29.576837Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 955a4ab8-4f17-49dc-a238-3e744629c3c4 · outbound

This paper cites Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Spectroscopic confirmation of four metal-poor galaxies at z=10.3-13.2

Reference 86

Resolution: malformed identifier; no resolver link, observed 2026-08-07T22:32:29.210063Z

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Observation 034a23b8-1151-467b-bbc8-05033acdef86 · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.213968Z

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Observation d45955b8-f6f0-4cf2-a049-3bb7630bd5b9 · outbound

This paper cites LISA Definition Study Report.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories LISA Definition Study Report

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.217607Z

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Observation 1d5eea75-8f43-4c15-b24f-839ec841d4f8 · outbound

This paper cites Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.221505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14faf647-d2e3-476f-a776-c0044cc00843 · outbound

This paper cites Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.225216Z

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Observation 70b8dd29-3a39-418c-aa37-d482c94a16fe · outbound

This paper cites Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.229125Z

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Observation e1226c57-8203-4923-9306-a4711c7dd962 · outbound

This paper cites Effect of lensing magnification on the apparent distribution of black hole mergers.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Effect of lensing magnification on the apparent distribution of black hole mergers

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.232951Z

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Observation 55207b28-f1f5-4cad-bf37-2061edebf361 · outbound

This paper cites Effect of gravitational lensing on the distribution of gravitational waves from distant binary black hole mergers.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Effect of gravitational lensing on the distribution of gravitational waves from distant binary black hole mergers

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.236845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dae6329-0284-4cec-a839-d8bf9085e368 · outbound

This paper cites Astropy: A Community Python Package for Astronomy.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Astropy: A Community Python Package for Astronomy

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.240707Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e101a49-8cfa-42b5-aa2c-9e2c14f90ae1 · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.244745Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8c3bf95-1113-47ef-871a-5182c6db58c9 · outbound

This paper cites an unresolved cited work.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories Unresolved cited work

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-07T22:32:29.248275Z

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