Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 45 inbound Pith citation observations for arXiv:2001.10914.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T10:22:31.033906Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T19:40:06.502559Z
Reference resolution
0 of 0 outbound references displayed
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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 21804ad9-7361-413a-92b9-3afdb7e415bb · inbound
Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes cites this paper.
Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 22
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T21:55:09.284758Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation ea9a8f73-e03e-4bf2-9b91-853bc0ebeed0 · inbound
GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.
GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 58
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T07:45:53.133211Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 5ac20a59-0a30-49f4-8b1c-c1f2c7095174 · inbound
Tests of General Relativity with GWTC-3 cites this paper.
Tests of General Relativity with GWTC-3 IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 112
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T02:40:31.243343Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 364c05fb-48b7-44e1-be3d-c69e860598b7 · inbound
Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object cites this paper.
Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 83
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T23:58:38.729328Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 8dd58132-3a3f-4884-b0cf-a12c27a98da6 · inbound
Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna cites this paper.
Probing intermediate-mass black hole binaries with the Lunar Gravitational-wave Antenna IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T10:22:31.033906Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9bf9a441-7fba-4d40-8353-8f0f608d27ef · inbound
Black hole spectroscopy: from theory to experiment cites this paper.
Black hole spectroscopy: from theory to experiment IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 296
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T01:31:23.943326Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 45e67659-4048-45c3-a634-aae70c31edb7 · inbound
AthenaK simulations of the binary black hole merger GW150914 cites this paper.
AthenaK simulations of the binary black hole merger GW150914 IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:57:54.271762Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d56588e8-2b10-4132-ac2f-bea3b10375e3 · inbound
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia cites this paper.
Detectability and Parameter Estimation for Einstein Telescope Configurations with GWJulia IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:29:59.339031Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ca0d61a9-5a7e-4b67-b79c-32b02c1182b9 · inbound
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA cites this paper.
Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 114
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:08:46.190679Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 23935cb4-1f6d-4307-b9c1-c55463da0e5e · inbound
PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown cites this paper.
PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:31:47.310851Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b750ba8-5b32-4ea9-9d10-00f6c9e3de15 · inbound
Primordial black holes versus their impersonators at gravitational wave observatories cites this paper.
Primordial black holes versus their impersonators at gravitational wave observatories IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-05-21T22:15:42.099117Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 032e37ad-d09b-43de-8a43-f727d99cfeeb · inbound
Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog cites this paper.
Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 76
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T10:11:14.462834Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation cf7c9820-874a-429b-a50c-c384fee31022 · inbound
Impact of facility timing and coordination for next-generation gravitational-wave detectors cites this paper.
Impact of facility timing and coordination for next-generation gravitational-wave detectors IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T07:12:26.733921Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 388105b3-2b71-4bcd-b5ba-ba4525aa2cc6 · inbound
Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary cites this paper.
Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 165
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-18T05:55:57.167572Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b023e808-d174-4688-b2a6-78fc85e846b3 · inbound
Scalar fields around black hole binaries in LIGO-Virgo-KAGRA cites this paper.
Scalar fields around black hole binaries in LIGO-Virgo-KAGRA IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 97
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T05:50:56.812185Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 012f97e7-cb5e-4d73-b7f0-9ec6741f7692 · inbound
Learning Post-Newtonian Corrections from Numerical Relativity cites this paper.
Learning Post-Newtonian Corrections from Numerical Relativity IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 43
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T22:35:25.219188Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b36a1b88-bd25-4331-a331-48fb906d5b40 · inbound
Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? cites this paper.
Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing? IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 112
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T18:57:08.822161Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47afbe33-e542-47e5-924c-3acfc1ae068b · inbound
Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations cites this paper.
Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T12:21:07.793950Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3df0cfd-eecb-4abd-96fa-fdd43efceb23 · inbound
Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition cites this paper.
Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 58
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T16:38:06.350871Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 2b21a1e2-c004-4ee9-b1a4-7a6dd149d601 · inbound
Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries cites this paper.
Systematic biases in parameter estimation on LISA binaries. II. The effect of excluding higher harmonics for spin-aligned, high-mass binaries IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T03:09:41.148860Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6aa4f667-36de-4de0-896a-418d3b6d06b0 · inbound
Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz cites this paper.
Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T20:21:15.047824Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4f0dc427-ddf8-4a73-88ea-d9b104ae1e73 · inbound
Distinguishability of magnetic massive black holes from environmental mimics with inspiral gravitational waves cites this paper.
Distinguishability of magnetic massive black holes from environmental mimics with inspiral gravitational waves IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-05-15T15:40:08.720055Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 345eb620-da78-4770-8a89-f1a3581c5d0c · inbound
Advancing the Effective-One-Body Framework in the Test-Mass Limit cites this paper.
Advancing the Effective-One-Body Framework in the Test-Mass Limit IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-07-15T14:26:35.666160Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9476ee6a-4e2c-4d08-8261-91c9564ccf15 · inbound
Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests cites this paper.
Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 119
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T00:11:25.155489Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7fa45466-e7a1-455e-815a-cfb50397bf67 · inbound
Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors cites this paper.
Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 130
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T10:31:02.732072Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation df7c4aa0-5361-40fb-bd46-b95b5cb2c3bf · inbound
Novel ringdown tests of general relativity with black hole greybody factors cites this paper.
Novel ringdown tests of general relativity with black hole greybody factors IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 118
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T11:06:04.577360Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 4bd4ec06-3a2d-4819-8dc1-b6939335e4c2 · inbound
Mitigating Systematic Errors in Parameter Estimation of Binary Black Hole Mergers in O1-O3 LIGO-Virgo Data cites this paper.
Mitigating Systematic Errors in Parameter Estimation of Binary Black Hole Mergers in O1-O3 LIGO-Virgo Data IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 52
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T15:11:07.041949Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 8319e90f-835d-44f6-88b6-22e219a6c931 · inbound
Mitigating Systematic Errors in Parameter Estimation of Binary Black Hole Mergers in O1-O3 LIGO-Virgo Data cites this paper.
Mitigating Systematic Errors in Parameter Estimation of Binary Black Hole Mergers in O1-O3 LIGO-Virgo Data IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 52
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-19T17:03:09.299786Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 423b4be0-dd6a-434f-9978-334637df22fd · inbound
Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework cites this paper.
Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T06:10:37.579664Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation e826e546-4b73-4fa5-958f-258c41cb132f · inbound
Inpainting over the cracks: challenges of applying pre-merger searches for massive black hole binaries to realistic LISA datasets cites this paper.
Inpainting over the cracks: challenges of applying pre-merger searches for massive black hole binaries to realistic LISA datasets IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 23
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-14T17:42:31.380064Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 623a05c0-09d1-4e10-a45b-a28a86794475 · inbound
Shaping black hole resonances I. Black hole ringdown as a spectral filtering process cites this paper.
Shaping black hole resonances I. Black hole ringdown as a spectral filtering process IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 57
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T13:14:41.127391Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 58e0adc9-dab3-42a4-ac7d-dfb06231f645 · inbound
Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences cites this paper.
Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 125
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-02T00:36:25.013362Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 6ea0520b-fd8b-41e6-8dfc-cd37e1bae07a · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 65
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-02T09:26:51.270127Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 22597ad9-4c1c-4a30-8b48-cd6ff7f503e8 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:33.639121Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ada24c6-8aa9-4e6f-a27d-a685157df965 · inbound
Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity cites this paper.
Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 55
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T23:57:28.499773Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 77bcb446-e71f-4a76-b5cc-f51b0d98eaf6 · inbound
Improving low-latency multi-messenger follow-up of neutron star-black hole mergers with mode-by-mode filtering cites this paper.
Improving low-latency multi-messenger follow-up of neutron star-black hole mergers with mode-by-mode filtering IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 76
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-03T18:08:46.519151Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation d8e88de2-1655-4296-95fd-cf1d18e40e69 · inbound
Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters cites this paper.
Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 62
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-04T01:39:25.254568Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation a2605b91-9ae5-41ca-87ee-3f88ed9678c8 · inbound
Finite-Core Signatures in LISA-Band Wave-Optics Lensing by Low-Mass Dark Matter Halos cites this paper.
Finite-Core Signatures in LISA-Band Wave-Optics Lensing by Low-Mass Dark Matter Halos IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 45
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-04T04:59:36.962104Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 6ed8c5b0-a279-41dc-b61e-758e89a76bc7 · inbound
Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.
Constraints on Line-of-Sight Acceleration from O1-O4 IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 62
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T19:40:06.503909Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 0f480349-1c68-4cf3-9aec-816f065b7170 · inbound
Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.
Constraints on Line-of-Sight Acceleration from O1-O4 IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T10:17:31.324695Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4c704949-0759-45dd-8e94-34dd04affce9 · inbound
Fast, accurate, and differentiable: a neural-network surrogate for NRSur7dq4 precessing binary black hole waveforms cites this paper.
Fast, accurate, and differentiable: a neural-network surrogate for NRSur7dq4 precessing binary black hole waveforms IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T04:58:16.645035Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4d67ff15-43ba-4182-bbed-a0d367fc2e7c · inbound
Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.
Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 163
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:39:00.628785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9d95383-7815-4d1f-9567-520116d73472 · inbound
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T21:28:07.549539Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ef0f5527-9155-4865-802b-7aa47a2e1035 · inbound
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.
High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:15:14.228953Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 597416a5-1510-4ced-9c21-7d8c4aa6169f · inbound
Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.
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
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T22:32:29.100881Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.