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Paper Citation Record · LEDGER

Modelling noise in gravitational-wave observatories with transdimensional models

As of 16 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 0 inbound Pith citation observations for arXiv:2501.03285.

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pith.paper-citation-record.v1
2501.03285 v2

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58 of 58 outbound references displayed

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Outbound references

Observation d6c0819f-a530-4284-828e-15cfd75c98a4 · outbound

This paper cites The prior on NPL follows a discrete uniform distribution DU [0, 5].

Modelling noise in gravitational-wave observatories with transdimensional models The prior on NPL follows a discrete uniform distribution DU [0, 5]

Reference 1

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This paper cites The prior on Nline follows a discrete uniform distribution DU [0, 20].

Modelling noise in gravitational-wave observatories with transdimensional models The prior on Nline follows a discrete uniform distribution DU [0, 20]

Reference 2

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This paper cites Each shaplelet is characterized by three parameters: β, fsh, and Ash.

Modelling noise in gravitational-wave observatories with transdimensional models Each shaplelet is characterized by three parameters: β, fsh, and Ash

Reference 3

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Observation 64a77008-028f-45fe-bd4c-ad0d9114c5e6 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 4

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Observation b5208f7c-7090-4ca9-a733-8ad6afa5dad0 · outbound

This paper cites Table of Priors.

Modelling noise in gravitational-wave observatories with transdimensional models Table of Priors

Reference 5

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 6

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This paper cites That is, we fit only the narrow- band features (σline and σNBS) within the frequency bins that were notched out in step 2.

Modelling noise in gravitational-wave observatories with transdimensional models That is, we fit only the narrow- band features (σline and σNBS) within the frequency bins that were notched out in step 2

Reference 7

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Observation 8bdccc83-09a0-4ccc-bd57-639132e92991 · outbound

This paper cites This process is possible because the frequency bins notched out in step 2 and reintroduced in step 4 can be treated as independent datasets.

Modelling noise in gravitational-wave observatories with transdimensional models This process is possible because the frequency bins notched out in step 2 and reintroduced in step 4 can be treated as independent datasets

Reference 8

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This paper cites proposal distribution.

Modelling noise in gravitational-wave observatories with transdimensional models proposal distribution

Reference 9

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This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 10

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 11

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Observation d413135d-bbc5-462f-a474-71d2fac8bae8 · outbound

This paper cites The maximum am- plitude is given by Amax sh (f ) = 3.85 × σ(f )BB med.

Modelling noise in gravitational-wave observatories with transdimensional models The maximum am- plitude is given by Amax sh (f ) = 3.85 × σ(f )BB med

Reference 12

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This paper cites The second level focuses exclusively on high-quality data, which reduces computation time while retaining the most critical data points.

Modelling noise in gravitational-wave observatories with transdimensional models The second level focuses exclusively on high-quality data, which reduces computation time while retaining the most critical data points

Reference 13

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Observation 88c89976-beb4-42e9-acc6-cc8fe16a8604 · outbound

This paper cites It relies on the availability of the lines location prior described in Appendix B 1.

Modelling noise in gravitational-wave observatories with transdimensional models It relies on the availability of the lines location prior described in Appendix B 1

Reference 14

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Observation 9bb840d2-0891-4a9c-943c-54a5ef79c0d5 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 15

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Observation 01bd90b7-55fc-4b41-aabd-bc9f5cdc3cff · outbound

This paper cites Acernese et al., Advanced Virgo: a second-generation interferometric gravitational wave detector, Classical and Quantum Gravity 32, 024001 (2014).

Modelling noise in gravitational-wave observatories with transdimensional models Acernese et al., Advanced Virgo: a second-generation interferometric gravitational wave detector, Classical and Quantum Gravity 32, 024001 (2014)

Reference 16

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 17

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This paper cites Talbot, E.

Modelling noise in gravitational-wave observatories with transdimensional models Talbot, E

Reference 18

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

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This paper cites Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo.

Modelling noise in gravitational-wave observatories with transdimensional models Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

Reference 21

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This paper cites Open data from the third observing run of LIGO, Virgo, KAGRA and GEO.

Modelling noise in gravitational-wave observatories with transdimensional models Open data from the third observing run of LIGO, Virgo, KAGRA and GEO

Reference 22

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Modelling noise in gravitational-wave observatories with transdimensional models Transdimensional inference for gravitational-wave astronomy with Bilby

Reference 23

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This paper cites Ashton et al., Bilby: A User-friendly Bayesian In- ference Library for Gravitational-wave Astronomy, The Astrophysical Journal Supplement Series 241, 27 (2019).

Modelling noise in gravitational-wave observatories with transdimensional models Ashton et al., Bilby: A User-friendly Bayesian In- ference Library for Gravitational-wave Astronomy, The Astrophysical Journal Supplement Series 241, 27 (2019)

Reference 24

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Modelling noise in gravitational-wave observatories with transdimensional models Bayesian inference for compact binary coalescences with BILBY: Validation and application to the first LIGO--Virgo gravitational-wave transient catalogue

Reference 25

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Modelling noise in gravitational-wave observatories with transdimensional models Allen, W

Reference 26

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

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Modelling noise in gravitational-wave observatories with transdimensional models Gupta and N

Reference 28

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Modelling noise in gravitational-wave observatories with transdimensional models Thrane and C

Reference 29

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Modelling noise in gravitational-wave observatories with transdimensional models Cahillane and G

Reference 30

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This paper cites Refregier, Shapelets — I.

Modelling noise in gravitational-wave observatories with transdimensional models Refregier, Shapelets — I

Reference 31

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 32

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This paper cites Abbott et al.

Modelling noise in gravitational-wave observatories with transdimensional models Abbott et al

Reference 33

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Modelling noise in gravitational-wave observatories with transdimensional models ”Abbott, T

Reference 34

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Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 35

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Observation cab9f670-1e6a-496a-be42-d8a52afce3fa · outbound

This paper cites Abbott et al.

Modelling noise in gravitational-wave observatories with transdimensional models Abbott et al

Reference 36

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Observation 77d4394c-d3fb-427e-9129-70fb85540376 · outbound

This paper cites Bradbury, R.

Modelling noise in gravitational-wave observatories with transdimensional models Bradbury, R

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-10T22:11:27.114109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 216617a6-9a22-4e55-870d-b2a5c024f47c · outbound

This paper cites Pratten et al., Computationally efficient models for the dominant and subdominant harmonic modes of pre- cessing binary black holes, Phys.

Modelling noise in gravitational-wave observatories with transdimensional models Pratten et al., Computationally efficient models for the dominant and subdominant harmonic modes of pre- cessing binary black holes, Phys

Reference 38

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 62102cd5-8478-4a65-92c3-894e66304d92 · outbound

This paper cites Payne, C.

Modelling noise in gravitational-wave observatories with transdimensional models Payne, C

Reference 39

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 202b923f-762c-434d-8246-bac9f467c121 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 40

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.548909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 0406a545-bc28-4a06-b1ad-d546ad7e0cb7 · outbound

This paper cites Abbott et al.

Modelling noise in gravitational-wave observatories with transdimensional models Abbott et al

Reference 41

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation dbef8896-c1fe-48b8-ab95-cb7b81fe5ef4 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 42

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.523700Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation f3e7d3ab-9698-46bd-bb05-f2ff808835b9 · outbound

This paper cites Abbott et al., Population properties of compact ob- jects from the second LIGO-Virgo Gravitational-Wave Transient Catalog, Astrophys.

Modelling noise in gravitational-wave observatories with transdimensional models Abbott et al., Population properties of compact ob- jects from the second LIGO-Virgo Gravitational-Wave Transient Catalog, Astrophys

Reference 43

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation f780f61d-7e0c-4236-8a91-82d40207f2bf · outbound

This paper cites Abbott et al.

Modelling noise in gravitational-wave observatories with transdimensional models Abbott et al

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.497689Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 95cd5df9-5368-4a71-aa9c-e310bac25b88 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 45

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.484120Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 73e44762-2216-48d4-ad64-37081175ce36 · outbound

This paper cites Possible Causes of False General Relativity Violations in Gravitational Wave Observations.

Modelling noise in gravitational-wave observatories with transdimensional models Possible Causes of False General Relativity Violations in Gravitational Wave Observations

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T22:11:27.154419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:11:27.154419Z digest=sha256:bb1aa1384cd1a3da680de5ae7400fa337306a30ed4171f2176018fb8813ccd52

Observation a2dd59af-dec6-42a5-b58e-eee10bc0a679 · outbound

This paper cites Payne, S.

Modelling noise in gravitational-wave observatories with transdimensional models Payne, S

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.470833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 9d6ddbdd-0b4b-4644-a68a-896936b6a436 · outbound

This paper cites Biscoveanu, C.-J.

Modelling noise in gravitational-wave observatories with transdimensional models Biscoveanu, C.-J

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T22:11:27.162853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:11:27.162853Z digest=sha256:89f4338f39b1744318671d783e9921d5cf8aec6c54689259886a3bd5ba2cbd26

Observation fed21515-61d0-4a6d-b733-aa8d10cb92b4 · outbound

This paper cites Gravitational-wave astronomy with an uncertain noise power spectral density.

Modelling noise in gravitational-wave observatories with transdimensional models Gravitational-wave astronomy with an uncertain noise power spectral density

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T22:11:27.166837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:11:27.166837Z digest=sha256:8659d554347ab86fb81960b47dfebfed19cb5af857287cebe1cd51feca9b517b

Observation fd394e2e-b92a-47f6-abb6-c94e8c9a8ec9 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 50

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.458640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 7f08bb03-b624-46a3-a9f8-c24773e7c156 · outbound

This paper cites Chatziioannou, N.

Modelling noise in gravitational-wave observatories with transdimensional models Chatziioannou, N

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.446918Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation e3405140-d2e9-4950-9278-562d5fdfb1f6 · outbound

This paper cites Plunkett, S.

Modelling noise in gravitational-wave observatories with transdimensional models Plunkett, S

Reference 52

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.434613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation c2f5f7d6-f77d-43a7-9de3-1f3a5c8838ac · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 53

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.422131Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation e64da45e-10b4-433e-8578-085e2b48e48e · outbound

This paper cites Chatziioannou, C.-J.

Modelling noise in gravitational-wave observatories with transdimensional models Chatziioannou, C.-J

Reference 54

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.408973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 2f805e6a-6d83-4a67-96d6-a42a86ec5c4a · outbound

This paper cites Davis, T.

Modelling noise in gravitational-wave observatories with transdimensional models Davis, T

Reference 55

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.392445Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-10T22:11:27.191997Z digest=sha256:7d3fb3ce09f9a9312e3f9cdb5e9d261e4944c019b62dc797855865f81670f50a

Observation 41e850b3-3eaa-4ba1-bca8-4c0f3cb405e0 · outbound

This paper cites Hourihane, K.

Modelling noise in gravitational-wave observatories with transdimensional models Hourihane, K

Reference 56

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:11:27.379789Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation d5aaecdb-3d74-470d-b089-6878a67e4681 · outbound

This paper cites Does spacetime have memories? Searching for gravitational-wave memory in the third LIGO-Virgo-KAGRA gravitational-wave transient catalogue.

Modelling noise in gravitational-wave observatories with transdimensional models Does spacetime have memories? Searching for gravitational-wave memory in the third LIGO-Virgo-KAGRA gravitational-wave transient catalogue

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-10T22:11:27.200960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:11:27.200960Z digest=sha256:fe6fba35b9fade5c6314b33fcb5fbd3ac2d50166d8b8676109aaec9bbf6e5742

Observation 2c59589c-f2ea-49b4-8abe-3148a8a128b9 · outbound

This paper cites an unresolved cited work.

Modelling noise in gravitational-wave observatories with transdimensional models Unresolved cited work

Reference 58

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:11:27.366291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Pith citing papers

No inbound Pith citation observations are available.