Paper Citation Record · LEDGER

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals

As of 23 August 2026, this Paper Citation Record lists 44 of 44 outbound references and 0 inbound Pith citation observations for arXiv:2411.14191.

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

pith.paper-citation-record.v1
2411.14191 v3

Coverage vector

measured 44 of 44 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Outbound references

Observation e434d68b-e035-46bc-82b2-532fa30169a0 · outbound

This paper cites an unresolved cited work.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-08-12T15:30:39.737071Z

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Observation 6822032e-7f0f-496a-9e3c-467431cd1c28 · outbound

This paper cites an unresolved cited work.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-12T15:30:39.722604Z

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Observation 192f5e99-c8d1-414e-bdcb-a6c63c64a20a · outbound

This paper cites The static arm lengths given are those assumed in [7].

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals The static arm lengths given are those assumed in [7]

Reference 3

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Observation ba7e9e96-bdbf-4a25-a482-5289b99fa516 · outbound

This paper cites Non- geometric tilt-to-length coupling in space interferometry: mechanisms and analytical descriptions.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Non- geometric tilt-to-length coupling in space interferometry: mechanisms and analytical descriptions

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.637857Z

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Observation 4c53ecee-2b99-4294-901e-828e76f8e6a9 · outbound

This paper cites LISA: unveiling a hidden universe.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA: unveiling a hidden universe

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.680133Z

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Observation 321f9b15-3471-41bc-bc66-c384aaa72d25 · outbound

This paper cites LISA definition study report.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA definition study report

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.666658Z

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Observation 4e4627f3-9d20-4e5c-93d0-c5cd1197eef2 · outbound

This paper cites Geometric tilt- to-length coupling in precision interferometry: mecha- nisms and analytical descriptions.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Geometric tilt- to-length coupling in precision interferometry: mecha- nisms and analytical descriptions

Reference 7

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Observation 9d46584e-f5f8-401e-8684-42704cc45580 · outbound

This paper cites Paczkowski et al.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Paczkowski et al

Reference 8

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Observation 13edb416-d40d-42cc-aa08-e8d8b9815501 · outbound

This paper cites Preliminary results on the suppression of sensing cross-talk in LISA Pathfinder.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Preliminary results on the suppression of sensing cross-talk in LISA Pathfinder

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.623475Z

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Observation 428461e5-79a0-40ae-9eb9-6ca803558515 · outbound

This paper cites Armano, H.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Armano, H

Reference 10

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Observation feb1739d-7f17-4f5a-b3d3-79b9df93e990 · outbound

This paper cites Paczkowski, R.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Paczkowski, R

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.594625Z

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Observation 579b8f9f-c9bd-4882-8580-08efd28df38d · outbound

This paper cites Houba, S.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Houba, S

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.521949Z

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Observation 2a009544-4149-4f40-a913-c7daa1f79601 · outbound

This paper cites George, J.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals George, J

Reference 13

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Observation b77b4c59-fba3-4c52-ae2e-a18e2ef0297d · outbound

This paper cites Hartig, J.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Hartig, J

Reference 14

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Observation 66a013c8-50ee-41ab-9eaa-040c11d0e0b5 · outbound

This paper cites Houba, S.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Houba, S

Reference 15

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Observation b7af4ebc-1bfe-4f2a-b557-837d27dd871c · outbound

This paper cites Time-delay interferometry.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Time-delay interferometry

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.466298Z

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Observation 0fed2f7e-a2f1-4b5a-97f3-6b125bd8cad9 · outbound

This paper cites Wegener, S.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Wegener, S

Reference 17

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Observation cc99983b-4ecd-4723-90e0-f4f73b4c7670 · outbound

This paper cites Auto- matic alignment of optical interferometers.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Auto- matic alignment of optical interferometers

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.494302Z

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Observation 0544fc24-14fe-48b0-99b5-41b7d6346474 · outbound

This paper cites Methods for simulat- ing the readout of lengths and angles in laser interfer- ometers with Gaussian beams.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Methods for simulat- ing the readout of lengths and angles in laser interfer- ometers with Gaussian beams

Reference 19

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Observation ca9b22c4-f249-4a00-9cc9-7db094e990a6 · outbound

This paper cites Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Uncovering gravitational-wave backgrounds from noises of unknown shape with LISA

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.408660Z

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Observation 5b69b376-c68a-4b10-a453-31d1b2c0c544 · outbound

This paper cites Second- generation time-delay interferometry.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Second- generation time-delay interferometry

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.451905Z

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Observation a54b0b1f-efd2-45ef-9feb-721d881c1a66 · outbound

This paper cites Wanner, S.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Wanner, S

Reference 22

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Observation 201bf3a9-f571-403f-b201-dad88e5b00eb · outbound

This paper cites LISA optimal sensitivity.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA optimal sensitivity

Reference 23

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Observation d88f6988-05cd-4875-8cd8-e46cd557754a · outbound

This paper cites PyTDI (1.3.1).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals PyTDI (1.3.1)

Reference 24

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Observation 9317a575-1bb5-4135-8555-6ce761b99b67 · outbound

This paper cites Technical Report No.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Technical Report No

Reference 25

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Observation 94329af4-a73d-4076-a9a7-10806a30139f · outbound

This paper cites LISANode (1.4).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISANode (1.4)

Reference 26

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Observation 2420a6c9-1e95-47ee-af39-ddd37ca31da4 · outbound

This paper cites Optical Simulations.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Optical Simulations

Reference 27

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Observation 8fede01f-84ff-412e-8ec9-b7c50c5e5769 · outbound

This paper cites Unified model for the LISA measurements and instrument simulations.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Unified model for the LISA measurements and instrument simulations

Reference 28

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Observation a5272ea5-0912-490e-8c86-d1c718cff3d0 · outbound

This paper cites LISA Orbits (2.3).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA Orbits (2.3)

Reference 29

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Observation 0430544b-2764-4b86-b435-5aeab71f5f87 · outbound

This paper cites LISA Con- stants (1.3).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA Con- stants (1.3)

Reference 30

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Observation 5a9b8442-ba77-4459-993b-7c4f831360b4 · outbound

This paper cites Trajectory design for the ESA LISA mission.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Trajectory design for the ESA LISA mission

Reference 31

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Observation 315bb976-3d09-443a-8d42-c9f3cdd0437b · outbound

This paper cites LISA GW Response (1.1).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA GW Response (1.1)

Reference 32

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Observation 428470b0-d079-4c0f-a2fe-3c3d1092f0f3 · outbound

This paper cites LISA Data Challenge San- gria (LDC2a) (Version v2) [Data set].

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA Data Challenge San- gria (LDC2a) (Version v2) [Data set]

Reference 33

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Observation b5feccb4-a0bd-495d-af47-3c5af2840fd2 · outbound

This paper cites LISA Data Chal- lenge software (1.2.0).

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA Data Chal- lenge software (1.2.0)

Reference 34

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Observation 793f2e6e-adb7-4068-9944-2376aa62bf62 · outbound

This paper cites Cosmology with the laser interferometer space antenna.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Cosmology with the laser interferometer space antenna

Reference 35

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Observation 2bf084f6-e01f-4c79-8c4d-10195c40ee9e · outbound

This paper cites LISA galactic binaries with astrometry from Gaia DR3.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA galactic binaries with astrometry from Gaia DR3

Reference 36

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Observation 8eed8137-8df4-4600-822a-236562cf20de · outbound

This paper cites Abbott, T.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Abbott, T

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.304388Z

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Observation c0ce0ddd-a511-42e7-b6e9-8a172ca70404 · outbound

This paper cites Impact of the noise knowledge uncertainty for the science exploitation of cos- mological and astrophysical stochastic gravitational wave background with LISA.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Impact of the noise knowledge uncertainty for the science exploitation of cos- mological and astrophysical stochastic gravitational wave background with LISA

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.290097Z

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Observation 7e22b901-fc90-4470-b31f-89777ab5ad8e · outbound

This paper cites Stochastic gravitational wave background reconstruction for a nonequilateral and unequal-noise LISA constella- tion.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Stochastic gravitational wave background reconstruction for a nonequilateral and unequal-noise LISA constella- tion

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.275267Z

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Observation 68c41eef-72f2-4a65-bcdf-8acbabde30b6 · outbound

This paper cites Stochastic gravitational wave background from stellar origin binary black holes in LISA.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Stochastic gravitational wave background from stellar origin binary black holes in LISA

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.243881Z

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Observation b7a46d20-8512-4242-a91c-85828e6502bf · outbound

This paper cites LISA Data Challenge: Sangria.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA Data Challenge: Sangria

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.228093Z

Source-reported events for the cited work

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Observation 95c8ab43-c9e5-4dca-9597-add59f6b6972 · outbound

This paper cites New LISA dynamics feedback control scheme: Common-mode isolation of test mass control and probes of test-mass acceleration.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals New LISA dynamics feedback control scheme: Common-mode isolation of test mass control and probes of test-mass acceleration

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.213239Z

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Observation 733a9f46-b560-4b83-9b6e-c9aaa6401071 · outbound

This paper cites LISA dynamics and control: Closed-loop simulation and numerical demonstration of time delay interferometry.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals LISA dynamics and control: Closed-loop simulation and numerical demonstration of time delay interferometry

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T15:30:39.198089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 836088e3-2c6d-4abc-a2ad-862cd09d1579 · outbound

This paper cites an unresolved cited work.

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals Unresolved cited work

Reference 2023

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

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