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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy

As of 13 August 2026, this Paper Citation Record lists 37 of 37 outbound references and 0 inbound Pith citation observations for arXiv:2607.25349.

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2607.25349 v1

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Observation c37c8789-0d90-419b-bc4a-7f855fa288dc · outbound

This paper cites Sources with 0.4 mHz ≤ fi < 6.0 mHz are assigned to the unique 10 µHz bin satisfying fk,left ≤ fi < f k,right.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Sources with 0.4 mHz ≤ fi < 6.0 mHz are assigned to the unique 10 µHz bin satisfying fk,left ≤ fi < f k,right

Reference 1

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

Reference 2

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This paper cites 1 + 2.0 × 10−3 Hz f 4# , (D9) Pacc(f ) = (3 .0 × 10−15 m s−2)2 Hz−1 ×.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy 1 + 2.0 × 10−3 Hz f 4# , (D9) Pacc(f ) = (3 .0 × 10−15 m s−2)2 Hz−1 ×

Reference 3

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This paper cites Laser Interferometer Space Antenna.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Laser Interferometer Space Antenna

Reference 4

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

Reference 5

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

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This paper cites Nelemans, L.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Nelemans, L

Reference 7

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

Reference 8

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Observation 7c2f20b9-10bc-456e-872a-4e8414b9ff09 · outbound

This paper cites The LISA Gravitational Wave Foreground: A Study of Double White Dwarfs.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy The LISA Gravitational Wave Foreground: A Study of Double White Dwarfs

Reference 9

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This paper cites Observationally driven Galactic double white dwarf population for LISA.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Observationally driven Galactic double white dwarf population for LISA

Reference 10

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Observation 721b6b6a-afc0-4773-99f9-7a211d263298 · outbound

This paper cites The Mock LISA Data Challenges: from Challenge 1B to Challenge 3.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy The Mock LISA Data Challenges: from Challenge 1B to Challenge 3

Reference 11

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

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy LISA data analysis: Source identification and subtraction

Reference 13

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This paper cites A Solution to the Galactic Foreground Problem for LISA.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy A Solution to the Galactic Foreground Problem for LISA

Reference 14

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy A detection pipeline for galactic binaries in LISA data

Reference 15

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This paper cites Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Resolving Galactic binaries in LISA data using particle swarm optimization and cross-validation

Reference 16

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Resolving Galactic binaries using a network of space-borne gravitational wave detectors

Reference 17

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Prototype Global Analysis of LISA Data with Multiple Source Types

Reference 18

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Global Analysis of LISA Data with Galactic Binaries and Massive Black Hole Binaries

Reference 19

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Modular global-fit pipeline for LISA data analysis

Reference 20

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy An efficient GPU-accelerated multi-source global fit pipeline for LISA data analysis

Reference 21

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Cosmological Backgrounds of Gravitational Waves

Reference 23

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This paper cites Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects

Reference 24

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Test for LISA foreground Gaussianity and stationarity: galactic white-dwarf binaries

Reference 25

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Discriminating between a Stochastic Gravitational Wave Background and Instrument Noise

Reference 26

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground

Reference 27

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Prototype Stochastic Gravitational Wave Background Recovery in the LISA Global Fit Residual

Reference 28

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Cutler and É

Reference 29

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects

Reference 30

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Le Jeune and S

Reference 31

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This paper cites an unresolved cited work.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

Reference 32

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy The construction and use of LISA sensitivity curves

Reference 33

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This paper cites Cutler, Angular resolution of the LISA gravitational wave detector, Phys.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Cutler, Angular resolution of the LISA gravitational wave detector, Phys

Reference 34

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Unresolved cited work

Reference 35

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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Stochastic backgrounds of gravitational waves

Reference 36

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This paper cites Planck 2018 results. VI. Cosmological parameters.

Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy Planck 2018 results. VI. Cosmological parameters

Reference 37

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Pith citing papers

No inbound Pith citation observations are available.