Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals | Paper Citation Record

Observation 1b67af47-089d-4785-a9ac-ebd43af252cb · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.403369Z

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Observation 6d362a13-3b1f-4ed8-908f-d4bff6e64087 · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.456371Z

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Observation 29b3e57f-d19a-4224-b284-eba8779b73e3 · outbound

This paper cites 8 presents the response of 2Fto variations in indi- vidual parameters while keeping other parameters fixed at their true values.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals 8 presents the response of 2Fto variations in indi- vidual parameters while keeping other parameters fixed at their true values

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.609420Z

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Observation 80a7590f-959c-491c-9059-33b0d7aa0431 · outbound

This paper cites degeneracy tracks.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals degeneracy tracks

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.736988Z

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Observation 37c97df6-7116-4dd0-9e98-1ee38ef84e4c · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.799200Z

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Observation 934180c9-a885-4f23-aab3-a1861d67289a · outbound

This paper cites In theF- statistic framework, the orbital phase Φ 0,n of each indi- vidual harmonic can be analytically recovered, but re- mains subject to a constant shift dependent onγ 0.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals In theF- statistic framework, the orbital phase Φ 0,n of each indi- vidual harmonic can be analytically recovered, but re- mains subject to a constant shift dependent onγ 0

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:28.927775Z

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Observation 3bc7e507-b048-447a-a343-f8343ba301c9 · outbound

This paper cites X-MRIs: Extremely Large Mass-Ratio Inspirals.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals X-MRIs: Extremely Large Mass-Ratio Inspirals

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.004230Z

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Observation 56a12c9b-499f-40d9-9299-9fe008f7a061 · outbound

This paper cites Gravitational waves from bodies orbiting the Galactic Center black hole and their detectability by LISA.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Gravitational waves from bodies orbiting the Galactic Center black hole and their detectability by LISA

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.090007Z

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Observation e6356ad8-2d84-43f2-b755-7187a8d2ce4e · outbound

This paper cites SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.175530Z

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Observation 6b8e0ce8-7907-4aa0-8f0d-96268dfea721 · outbound

This paper cites SgrA* spin and mass estimates through the detection of multiple extremely large mass-ratio inspirals.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals SgrA* spin and mass estimates through the detection of multiple extremely large mass-ratio inspirals

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.245973Z

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Observation 3353115f-a14c-4321-9818-da93763b99c6 · outbound

This paper cites Amaro-Seoane, arXiv preprint arXiv:2510.20898 (2025), arXiv:2510.20898 [astro-ph.HE].

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Amaro-Seoane, arXiv preprint arXiv:2510.20898 (2025), arXiv:2510.20898 [astro-ph.HE]

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.370446Z

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Observation 31e0b563-6365-41eb-ab8d-6eb75ef4d982 · outbound

This paper cites A forest of gravitational waves in our Galactic Centre.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals A forest of gravitational waves in our Galactic Centre

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.409575Z

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Observation 4c3cd7f2-b010-4b2e-bcd7-f4c4c74674e6 · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.476182Z

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Observation 29bb19a6-9b3e-4483-8519-25edb4bda850 · outbound

This paper cites Amaro-Seoane, inHandbook of Gravitational Wave Astronomy, edited by C.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Amaro-Seoane, inHandbook of Gravitational Wave Astronomy, edited by C

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.550325Z

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Observation 853a9553-049e-4e4b-9fca-a651848f4875 · outbound

This paper cites Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.608120Z

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Observation 8c26c225-898a-42e8-ae7d-4a7ba00e8b8d · outbound

This paper cites Eckart, R.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Eckart, R

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.767395Z

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Observation 604716cd-4bf3-4a35-b2f6-e2ac578b9ea9 · outbound

This paper cites The Galactic Center Massive Black Hole and Nuclear Star Cluster.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The Galactic Center Massive Black Hole and Nuclear Star Cluster

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.808841Z

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Observation 01511129-2b8e-41ad-82ff-08dcaab7dcf5 · outbound

This paper cites Stellar Dynamics in the Galactic centre: Proper Motions and Anisotropy.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Stellar Dynamics in the Galactic centre: Proper Motions and Anisotropy

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.874032Z

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Observation 774341cf-19c3-41f2-92a3-bf8cbd250d5b · outbound

This paper cites Kroupa, C.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Kroupa, C

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:29.939582Z

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Observation ef8ee6eb-39b8-4d69-89b4-0d6d04ba8bce · outbound

This paper cites The distribution of stars around the Milky Way's black hole III: Comparison with simulations.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The distribution of stars around the Milky Way's black hole III: Comparison with simulations

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.001439Z

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Observation 7ce28a8a-eb99-4086-a1ed-b855d549b7d4 · outbound

This paper cites The nuclear cluster of the Milky Way: Our primary testbed for the interaction of a dense star cluster with a massive black hole.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The nuclear cluster of the Milky Way: Our primary testbed for the interaction of a dense star cluster with a massive black hole

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.073554Z

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Observation 76c14849-68e4-403b-b004-06175dd14dbb · outbound

This paper cites An Extremely Top-Heavy IMF in the Galactic Center Stellar Disks.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals An Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.144208Z

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Observation ed57403e-1493-4c3d-a960-2456b06700e6 · outbound

This paper cites On strong mass segregation around a massive black hole: Implications for lower-frequency gravitational-wave astrophysics.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals On strong mass segregation around a massive black hole: Implications for lower-frequency gravitational-wave astrophysics

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.220511Z

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Observation e7a3f817-32d0-4f19-9e24-d62e8ea31518 · outbound

This paper cites Laser Interferometer Space Antenna.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Laser Interferometer Space Antenna

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.337147Z

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Observation 7c2b3176-32e2-4ea4-8f15-419bc556828b · outbound

This paper cites LISA Definition Study Report.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals LISA Definition Study Report

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.414621Z

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Observation 1042a554-c105-466f-9c20-2dea3979a57f · outbound

This paper cites TianQin: a space-borne gravitational wave detector.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals TianQin: a space-borne gravitational wave detector

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.486848Z

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Observation 1ae491f4-24ec-4969-b454-5eb57c5d5a85 · outbound

This paper cites Meiet al.(TianQin), PTEP2021, 05A107 (2021), arXiv:2008.10332 [gr-qc].

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Meiet al.(TianQin), PTEP2021, 05A107 (2021), arXiv:2008.10332 [gr-qc]

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.550055Z

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Observation 22b0edb5-82bb-4574-9d9e-64539fb9eab2 · outbound

This paper cites Concepts and status of Chinese space gravitational wave detection projects.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Concepts and status of Chinese space gravitational wave detection projects

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.628629Z

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Observation c75b801c-68a2-4d70-9887-3338bfd73d58 · outbound

This paper cites Science with the TianQin observatory: Preliminary results on massive black hole binaries.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Science with the TianQin observatory: Preliminary results on massive black hole binaries

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.691908Z

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Observation 8ca1c83e-8ec9-4abe-832b-accf7c2268e2 · outbound

This paper cites Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.773660Z

Source-reported events for the cited work

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Observation 440cc3e2-da2b-4cc1-8282-68c45be3280b · outbound

This paper cites Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.856523Z

Source-reported events for the cited work

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Observation 8f849641-6fc6-496d-a6f8-0f49cc3f5bf6 · outbound

This paper cites Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:30.969933Z

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Observation 1cfdd910-d237-4b71-a9ef-0bbf4e8e2f00 · outbound

This paper cites Science with the TianQin Observatory: Preliminary Results on Stochastic Gravitational-Wave Background.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Science with the TianQin Observatory: Preliminary Results on Stochastic Gravitational-Wave Background

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.035991Z

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This paper cites Identification of Gravitational-waves from Extreme Mass Ratio Inspirals.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Identification of Gravitational-waves from Extreme Mass Ratio Inspirals

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.105761Z

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.175860Z

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This paper cites Near Real-Time Gravitational Wave Data Analysis of the Massive Black Hole Binary with TianQin.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Near Real-Time Gravitational Wave Data Analysis of the Massive Black Hole Binary with TianQin

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.274822Z

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This paper cites Searching for gravitational waves from stellar-mass binary black holes early inspiral.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Searching for gravitational waves from stellar-mass binary black holes early inspiral

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.498109Z

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Observation 0c38e7e1-8b3d-4af5-b106-87ba7a295723 · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Astrophysics with the Laser Interferometer Space Antenna

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.646402Z

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Observation 1027ec47-4288-444a-b740-33215ffba59e · outbound

This paper cites Gravitational Wave Astronomy With TianQin.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Gravitational Wave Astronomy With TianQin

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Observation 3ca27fe8-3a4f-4abd-9b4d-ecc230f8ec70 · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals New Black Hole Spin Values for Sagittarius A* Obtained with the Outflow Method

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:31.871081Z

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Observation 3bed63be-1a24-4574-998f-603c080a0ab5 · outbound

This paper cites Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.018148Z

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This paper cites Monitoring stellar orbits around the Massive Black Hole in the Galactic Center.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Monitoring stellar orbits around the Massive Black Hole in the Galactic Center

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.117576Z

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals An upper limit on the spin of SgrA$^*$ based on stellar orbits in its vicinity

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.244618Z

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Observation ed7ba43c-5ef4-4a74-bbb3-a2749f9fd2a8 · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.333369Z

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This paper cites First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multi-wavelength Observations, Data Processing, and Calibration.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multi-wavelength Observations, Data Processing, and Calibration

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.389665Z

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Observation 082d22d2-a912-40ff-bedf-a9efa00967b0 · outbound

This paper cites First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals First Sagittarius A* Event Horizon Telescope Results. V. Testing Astrophysical Models of the Galactic Center Black Hole

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.454033Z

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This paper cites First Sagittarius A* Event Horizon Telescope Results. III: Imaging of the Galactic Center Supermassive Black Hole.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals First Sagittarius A* Event Horizon Telescope Results. III: Imaging of the Galactic Center Supermassive Black Hole

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.514753Z

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This paper cites First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals First Sagittarius A* Event Horizon Telescope Results. IV. Variability, Morphology, and Black Hole Mass

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.598847Z

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Akiyamaet al.(Event Horizon Telescope), Astrophys

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This paper cites Sagittarius A* -- The Milky Way Supermassive Black Hole.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Sagittarius A* -- The Milky Way Supermassive Black Hole

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.697416Z

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Observation 5dcdc50d-0d36-4b28-83f9-1a722c35980f · outbound

This paper cites Maggiore,Gravitational Waves.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Maggiore,Gravitational Waves

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.784750Z

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:32.884987Z

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This paper cites LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.001584Z

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Observation a92aa657-1f02-4bb5-bab2-1c8260f25a6b · outbound

This paper cites Moreno-Garrido, E.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Moreno-Garrido, E

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.104746Z

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Observation 7c670414-1b65-4ea1-9715-c9c255fcc4ff · outbound

This paper cites A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.246546Z

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Observation f06dae71-c1dc-4b64-b6bb-6fa6018f89c7 · outbound

This paper cites Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.354746Z

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Observation dff7ca3f-bec1-4ec0-aa5d-1cf9e9110cce · outbound

This paper cites Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

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Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.464892Z

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Observation 997b83c9-2ac7-494b-8e7d-088195e3ab2f · outbound

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Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

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Resolution: malformed identifier; no resolver link, observed 2026-08-03T06:36:33.674748Z

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Unavailable: canonical work link unavailable.

Observation c0922e12-9a55-4864-b605-6ddddd12b766 · outbound

This paper cites Lin,Identifying Extreme-Mass-Ratio Inspirals at the Galactic Center, Bachelor’s thesis, Peking University, Beijing, China (2022).

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Lin,Identifying Extreme-Mass-Ratio Inspirals at the Galactic Center, Bachelor’s thesis, Peking University, Beijing, China (2022)

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.828759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e48cd926-6ede-4dff-ab61-fa143b36709a · outbound

This paper cites The LISA verification binaries.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The LISA verification binaries

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.886404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0461c74-3b8b-4bd7-9ab2-4a801faf2138 · outbound

This paper cites an unresolved cited work.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:33.986137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37c86a81-8e85-46e9-8103-a7fc2d61fe56 · outbound

This paper cites The LISA Response Function.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The LISA Response Function

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.074848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 46476e6e-f113-4783-b97d-97a2e7dca9f2 · outbound

This paper cites an unresolved cited work.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.183092Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 902fa3ad-7566-4f4d-93c6-9a2b7aee90e8 · outbound

This paper cites Tinto and S.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Tinto and S

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.235316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c94771e6-faf6-4538-9f51-b8ae5afbdea3 · outbound

This paper cites GWSpace: a multi-mission science data simulator for space-based gravitational wave detection.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals GWSpace: a multi-mission science data simulator for space-based gravitational wave detection

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.427144Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3097f9c9-2651-435d-a8b6-00ec517d7c1e · outbound

This paper cites Wang and C.-G.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Wang and C.-G

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.501351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 182c05d0-9dec-4dd0-9c28-e3b59cb98b59 · outbound

This paper cites Data analysis of gravitational-wave signals from spinning neutron stars. I. The signal and its detection.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Data analysis of gravitational-wave signals from spinning neutron stars. I. The signal and its detection

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.595174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0834f760-62c2-4fa5-8408-4a4645eb8843 · outbound

This paper cites LISA data analysis: Source identification and subtraction.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals LISA data analysis: Source identification and subtraction

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.726687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 736baaa4-6760-4cd5-8f99-962120c72cd8 · outbound

This paper cites The generalized F-statistic: multiple detectors and multiple GW pulsars.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals The generalized F-statistic: multiple detectors and multiple GW pulsars

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.807711Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2361b529-d716-4789-af80-4b2328246cb8 · outbound

This paper cites Prix, Gravitational waves from spinning neutron stars, inNeutron Stars and Pulsars, edited by W.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Prix, Gravitational waves from spinning neutron stars, inNeutron Stars and Pulsars, edited by W

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:34.880653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf105171-7bba-4bcc-b092-a6dcfc3ebe1f · outbound

This paper cites Targeted search for continuous gravitational waves: Bayesian versus maximum-likelihood statistics.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Targeted search for continuous gravitational waves: Bayesian versus maximum-likelihood statistics

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.038953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 437b9e37-f54b-4533-a0fd-863cbc9fe020 · outbound

This paper cites Improved short-segment detection statistic for continuous gravitational waves.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Improved short-segment detection statistic for continuous gravitational waves

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.197306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c8c6e151-a1fe-4991-aad4-8b689fefe9ff · outbound

This paper cites Hierarchical search method for gravitational waves from stellar-mass binary black holes in noisy space-based detector data.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Hierarchical search method for gravitational waves from stellar-mass binary black holes in noisy space-based detector data

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.246130Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2adbfc49-2816-401a-8f81-66fa969e1c03 · outbound

This paper cites Bandopadhyay and C.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Bandopadhyay and C

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.348585Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5681ba0-5331-4ed4-adcc-4ffd15b380fc · outbound

This paper cites Bratton and J.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Bratton and J

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.570968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96f46860-8d1f-4512-8ce3-58c79c97e50e · outbound

This paper cites Mohanty,Swarm Intelligence Methods for Statistical Regression(CRC Press).

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Mohanty,Swarm Intelligence Methods for Statistical Regression(CRC Press)

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.679839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85e7730e-d771-4254-8168-8df2a22dd1ad · outbound

This paper cites an unresolved cited work.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.789141Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 401c4818-f9f9-40dc-9010-d531976c076a · outbound

This paper cites Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:35.894104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ad81c94-f589-4406-8d40-b7ece42b6847 · outbound

This paper cites an unresolved cited work.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.057338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f97e7127-13a2-4d57-ae8f-4605861460f3 · outbound

This paper cites LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.163982Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d5ff124-06a9-4e87-888a-601feac06cab · outbound

This paper cites Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.270122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c632d0c5-f26e-45ea-9965-f71884dbee4b · outbound

This paper cites Kennedy and R.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Kennedy and R

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.343257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70f36e01-2461-4304-8ca5-18473637276c · outbound

This paper cites Engelbrecht,Fundamentals of Computational Swarm Intelligence(2005).

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Engelbrecht,Fundamentals of Computational Swarm Intelligence(2005)

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.405091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ecd9bbe-06be-44ed-b94e-865ccef37c46 · outbound

This paper cites Shi and R.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Shi and R

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.477203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2c888207-3ef5-4c43-8649-fe6d7e887956 · outbound

This paper cites Dark matter annihilation at the galactic center.

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals Dark matter annihilation at the galactic center

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-03T06:36:36.583436Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Outbound references

Pith citing papers