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Paper Citation Record · LEDGER

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries

As of 21 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 0 inbound Pith citation observations for arXiv:2508.20418.

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

pith.paper-citation-record.v1
2508.20418 v2

Coverage vector

measured 51 of 51 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Reference resolution

51 of 51 outbound references displayed

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External citation measurements

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Outbound references

Observation 489a1b98-86c4-4a6e-a5ed-6914a4f2c86a · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 1

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Observation 7a4e28f6-f78f-4fbb-abf6-d4d3c26158ed · outbound

This paper cites Tortoise coordi- nates (r∗,pr∗) are used to enhance numerical stability, particularly near the EOB horizon analogue.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Tortoise coordi- nates (r∗,pr∗) are used to enhance numerical stability, particularly near the EOB horizon analogue

Reference 2

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Observation 99ed2938-99c8-4b41-a2f4-08025a118270 · outbound

This paper cites These modes are constructed symbolically within NRPy and gen- erated into optimized C code.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries These modes are constructed symbolically within NRPy and gen- erated into optimized C code

Reference 3

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Observation 646cbe72-5eea-4cc5-8660-55fbdd4ac98e · outbound

This paper cites The target values for the right-hand side of Eqs.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries The target values for the right-hand side of Eqs

Reference 4

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Observation 691a8b54-090e-4587-9c19-ced3ef627575 · outbound

This paper cites The functional form of the NQC corrections (Eq.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries The functional form of the NQC corrections (Eq

Reference 5

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Observation bda05d6b-f958-4290-b31a-1642639fd164 · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 6

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Observation 0473ecbb-b6e0-493e-925e-1aa544050bb2 · outbound

This paper cites Figure 1 shows that altering the interpolation bound- ary conditions induces slightly larger mismatches than round-off perturbations.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Figure 1 shows that altering the interpolation bound- ary conditions induces slightly larger mismatches than round-off perturbations

Reference 7

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Observation c19298fe-f1c5-4037-b912-7d22ef3900fc · outbound

This paper cites Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors

Reference 8

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Observation 5b0bde6b-71ae-4f9a-9edf-ffb8b8ac0fce · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 9

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Observation 8dd4e22c-9933-4589-8b3e-ce392f689674 · outbound

This paper cites This work was performed in part at the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-2210452.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries This work was performed in part at the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-2210452

Reference 10

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Observation bbf016e7-3807-404b-a1fa-4b9052db0155 · outbound

This paper cites Gravitational Wave Tests of General Relativity with Ground-Based Detectors and Pulsar Timing Arrays.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Gravitational Wave Tests of General Relativity with Ground-Based Detectors and Pulsar Timing Arrays

Reference 11

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Observation 0e57dd00-22c9-4c4d-8e07-0d42ccf63065 · outbound

This paper cites A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey

Reference 12

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Observation 69f1a153-9fdb-48a3-8fcb-97fd53916255 · outbound

This paper cites Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Reference 13

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Reference 14

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Observation a4a695e0-25ae-4493-a0ad-4bd2edc7d4bd · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 19

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Observation a72511a8-b492-47dd-a688-dda03a5cd561 · outbound

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

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries

Reference 20

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Observation cec4eca1-2220-4c70-92dd-93eeb949800a · outbound

This paper cites Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes

Reference 23

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This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 28

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Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 29

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Reference 30

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Observation 6d18c950-6a85-4a95-b6cd-57ccbe4c7a82 · outbound

This paper cites pySEOBNR: a software package for the next generation of effective-one-body multipolar waveform models.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries pySEOBNR: a software package for the next generation of effective-one-body multipolar waveform models

Reference 31

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Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 32

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Observation 7652cd08-ebb5-423f-874b-bc9975182dff · outbound

This paper cites Analytic systematics in next-generation of effective-one-body gravitational waveform models for future observations.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Analytic systematics in next-generation of effective-one-body gravitational waveform models for future observations

Reference 33

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Observation 7cc0e952-e449-41d9-bf1d-ce3f7769ce5d · outbound

This paper cites Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy

Reference 34

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Reference 35

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Observation d27b22ce-343c-4896-a6c9-a5877484bee6 · outbound

This paper cites qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries qnm: A Python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients

Reference 36

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Observation 7192f4f2-36cc-4731-8969-b6762a39fb3d · outbound

This paper cites Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models SEOBNRv5

Reference 37

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Reference 38

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unresolved
no resolver link, observed 2026-08-15T16:50:52.752677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.752677Z digest=sha256:8d842b6e55887a655b27b79e8568bca2bb9b43bc4dfca1a67db8d523e9129856

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-08-15T16:50:53.135615Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.757322Z digest=sha256:d39fa38308302e536bfa3f42500f24381a296d857f3f2d1eaa9301a5bd7393b8

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.761812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.761812Z digest=sha256:3231469d50875ed1eab4397b2780fbed9de74236ed0a28f96935f024a6eddfe6

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.765974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.765974Z digest=sha256:222d391117b4bbe08a251208be63af5bc876f3d6b292d5ea0f3c31799503da48

Observation 2d6bcc30-0134-4b4a-bdc8-410c8b8a22ed · outbound

This paper cites Meurer et al., SymPy: symbolic computing in Python, PeerJ Comput.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Meurer et al., SymPy: symbolic computing in Python, PeerJ Comput

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-08-15T16:50:53.552802Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.770475Z digest=sha256:ebd92c5e40d7c1f15c5e5e4f27e980057566e3ba4e0692fd8633f3c3361711f9

Observation ca5cb31c-1b60-449d-a2ea-a81b8939e28f · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.774742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.774742Z digest=sha256:562a0243ba393b400a902ccde34abe53522f7fe3ad8d9c9dacdf3da24c15cbaf

Observation 05bd6b3b-9ab9-490f-8d82-592c63448fd1 · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.778941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.778941Z digest=sha256:b6dcb6e3f515ce3b120531d7dc616185578c0a81c17e94ffa41c6732c5c7111f

Reference 45

Resolution
verified fuzzy
raw_fallback, observed 2026-08-15T16:50:53.529870Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.783182Z digest=sha256:31981f21a88bf1fdca4c55d9d9a7cb77553f86fd09eb142dd0aa5996ee5701f1

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-08-15T16:50:53.515753Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.787353Z digest=sha256:bf4013dbf04b24a391973fe08e1849dc11053a9f643382579b2ed475dd35a1e3

Observation 059b27d0-49ab-4faf-961e-52306ae8c8e9 · outbound

This paper cites an unresolved cited work.

Spinning Effective-to-Backwards One Body ($\texttt{SEBOB}$): combining Effective One-Body inspirals and Backwards One-Body merger-ringdowns for aligned spin black hole binaries Unresolved cited work

Reference 47

Resolution
unresolved
raw_fallback, observed 2026-08-15T16:50:53.501531Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.791630Z digest=sha256:bc0513f2c41f2f8af8b8be354560fb55aa57685891f77e46dd40cb71a094b0ee

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-08-15T16:50:52.900959Z

Source-reported events for the cited work

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

source=pdf_text observed=2026-08-15T16:50:52.796163Z digest=sha256:44683e4272bd190408b185e2d8f0d13fb5f8039b3f71a8673785ce1033d8e84d

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.800908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.800908Z digest=sha256:f7493063e44a1316f96154cd0d0fd0d7821c020bb082e3b38acee965acfcdba8

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.805438Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.805438Z digest=sha256:2fd6543dcee8d345bf2f9fb0b802192cecea72bc5f027602034abb5accdc8d83

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-15T16:50:52.810043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T16:50:52.810043Z digest=sha256:d224553b09b78763f6c60aa27a76e363633bffbaa69783e7ccfc364e5b915b98

Pith citing papers

No inbound Pith citation observations are available.