Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T06:32:08.971654Z
Paper Citation Record · LEDGER
Optimal and exact wide-angle power spectrum estimation
As of 18 August 2026, this Paper Citation Record lists 96 of 96 outbound references and 0 inbound Pith citation observations for arXiv:2607.05513.
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Reference resolution
96 of 96 outbound references displayed
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External citation measurements
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Outbound references
Observation e33d5a38-6be8-4a51-84b8-9a99c92f258c · outbound
This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.
Optimal and exact wide-angle power spectrum estimation The DESI Experiment Part I: Science,Targeting, and Survey Design
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation f3714f22-ed7d-43de-bbbb-f9b7915c74c9 · outbound
This paper cites Mellier, Abdurro’uf, J.A.
Optimal and exact wide-angle power spectrum estimation Mellier, Abdurro’uf, J.A
Reference 2
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation bdf0cac8-1c9a-4651-925f-2d482739fcf9 · outbound
This paper cites Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report.
Optimal and exact wide-angle power spectrum estimation Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation d486c74d-e000-4a20-bcf9-ad9d5c191724 · outbound
This paper cites The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document.
Optimal and exact wide-angle power spectrum estimation The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 020462cd-1391-468d-be3c-8d718f5d5845 · outbound
This paper cites Bock, A.M.
Optimal and exact wide-angle power spectrum estimation Bock, A.M
Reference 5
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation d9e08bd2-69c7-4751-81f4-430f3f3d5bb2 · outbound
This paper cites The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects.
Optimal and exact wide-angle power spectrum estimation The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation e035b327-ac74-421a-9ddb-868f06fe1fde · outbound
This paper cites Geometric Biases in Power-Spectrum Measurements.
Optimal and exact wide-angle power spectrum estimation Geometric Biases in Power-Spectrum Measurements
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d54946b0-265e-4a23-8b90-b7e670d65bdc · outbound
This paper cites Wide Angle Effects in Future Galaxy Surveys.
Optimal and exact wide-angle power spectrum estimation Wide Angle Effects in Future Galaxy Surveys
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation e1e1a2dd-b5f1-4251-91a5-ec776300e0ec · outbound
This paper cites Redshift-space distortions with wide angular separations.
Optimal and exact wide-angle power spectrum estimation Redshift-space distortions with wide angular separations
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 875ae883-82d8-4f75-8381-dbaeb33319c2 · outbound
This paper cites Interpreting measurements of the anisotropic galaxy power spectrum.
Optimal and exact wide-angle power spectrum estimation Interpreting measurements of the anisotropic galaxy power spectrum
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation c93fd814-a6ab-4455-bbd0-d116ca66e162 · outbound
This paper cites Wide-Angle Effects in the Power Spectrum Multipoles in Next-Generation Redshift Surveys.
Optimal and exact wide-angle power spectrum estimation Wide-Angle Effects in the Power Spectrum Multipoles in Next-Generation Redshift Surveys
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ed7732d-5a09-4269-b34f-85c9bae900e4 · outbound
This paper cites Kaiser,Clustering in real space and in redshift space,Mon.
Optimal and exact wide-angle power spectrum estimation Kaiser,Clustering in real space and in redshift space,Mon
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50910f01-1a9c-4c22-add8-56e0a7a8995f · outbound
This paper cites Lilje and G.
Optimal and exact wide-angle power spectrum estimation Lilje and G
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a1df5507-db6f-45ec-8d4f-ef1f1c430faa · outbound
This paper cites Hamilton,Measuring Omega and the Real Correlation Function from the Redshift Correlation Function,Astrophys.
Optimal and exact wide-angle power spectrum estimation Hamilton,Measuring Omega and the Real Correlation Function from the Redshift Correlation Function,Astrophys
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 8eb83973-b896-455b-b175-2dd3daffc78b · outbound
This paper cites McGill,The redshift projection.
Optimal and exact wide-angle power spectrum estimation McGill,The redshift projection
Reference 15
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b989de77-53d1-42f4-9ccf-c12da3d85606 · outbound
This paper cites A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey.
Optimal and exact wide-angle power spectrum estimation A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 92082f15-a211-45cf-8d59-48bb033affe8 · outbound
This paper cites Measuring line-of-sight dependent Fourier-space clustering using FFTs.
Optimal and exact wide-angle power spectrum estimation Measuring line-of-sight dependent Fourier-space clustering using FFTs
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation 7406632d-3a08-4ce6-81a6-dd1e320a4070 · outbound
This paper cites Fast Estimators for Redshift-Space Clustering.
Optimal and exact wide-angle power spectrum estimation Fast Estimators for Redshift-Space Clustering
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a64514d5-4aec-437a-93da-57dfa9c00ec7 · outbound
This paper cites Rapid modelling of the redshift-space power spectrum multipoles for a masked density field.
Optimal and exact wide-angle power spectrum estimation Rapid modelling of the redshift-space power spectrum multipoles for a masked density field
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation cce7b224-55d9-4a67-bf74-4c86729ada69 · outbound
This paper cites An optimal FFT-based anisotropic power spectrum estimator.
Optimal and exact wide-angle power spectrum estimation An optimal FFT-based anisotropic power spectrum estimator
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation e85a932e-7107-4dc2-97be-a148cad5116b · outbound
This paper cites Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics.
Optimal and exact wide-angle power spectrum estimation Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5b2893b9-6c71-4239-87ad-f2d42b04f84c · outbound
This paper cites Spherical Redshift Distortions.
Optimal and exact wide-angle power spectrum estimation Spherical Redshift Distortions
Reference 22
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation 4e0f7579-e00f-4faa-b9df-4d41f06145da · outbound
This paper cites Zaroubi and Y.
Optimal and exact wide-angle power spectrum estimation Zaroubi and Y
Reference 23
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 58c303ef-746e-42b6-a00a-93eb56364656 · outbound
This paper cites Redshift Space Distortions of the Correlation Function in Wide Angle Galaxy Surveys.
Optimal and exact wide-angle power spectrum estimation Redshift Space Distortions of the Correlation Function in Wide Angle Galaxy Surveys
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a4186db9-dd89-49e6-9837-b17958532c72 · outbound
This paper cites Linear Redshift Distortions: A Review.
Optimal and exact wide-angle power spectrum estimation Linear Redshift Distortions: A Review
Reference 25
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation db834e09-528c-4d34-9f42-64805e96af29 · outbound
This paper cites Bharadwaj,Radial redshift space distortions,The Astrophysical Journal516(1999) 507.
Optimal and exact wide-angle power spectrum estimation Bharadwaj,Radial redshift space distortions,The Astrophysical Journal516(1999) 507
Reference 26
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 527574ca-dbac-4f06-99e5-0bbea78d6d69 · outbound
This paper cites A Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift Survey.
Optimal and exact wide-angle power spectrum estimation A Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift Survey
Reference 27
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation a43c056a-8036-4f14-a25d-e05849c0a0bc · outbound
This paper cites A Spherical Harmonic Analysis of Redshift Space.
Optimal and exact wide-angle power spectrum estimation A Spherical Harmonic Analysis of Redshift Space
Reference 28
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 93878812-1c08-4a7a-8984-1ff13f783af0 · outbound
This paper cites SuperFaB: a fabulous code for Spherical Fourier-Bessel decomposition.
Optimal and exact wide-angle power spectrum estimation SuperFaB: a fabulous code for Spherical Fourier-Bessel decomposition
Reference 29
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 812c52fd-82ef-4268-bb1a-f768caa724ec · outbound
This paper cites Harmonic analysis of isotropic fields on the sphere with arbitrary masks.
Optimal and exact wide-angle power spectrum estimation Harmonic analysis of isotropic fields on the sphere with arbitrary masks
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f5fc84aa-8630-41cc-819c-299d3d0cde77 · outbound
This paper cites Validation of Spherical Fourier-Bessel power spectrum analysis with lognormal simulations and eBOSS DR16 LRG EZmocks.
Optimal and exact wide-angle power spectrum estimation Validation of Spherical Fourier-Bessel power spectrum analysis with lognormal simulations and eBOSS DR16 LRG EZmocks
Reference 31
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Unavailable: canonical work link unavailable.
Observation e2c5e463-c6a8-490f-85e1-fc41b2a45637 · outbound
This paper cites The Galaxy Bispectrum in the Spherical Fourier-Bessel Basis.
Optimal and exact wide-angle power spectrum estimation The Galaxy Bispectrum in the Spherical Fourier-Bessel Basis
Reference 32
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f021e49e-835b-4b21-837b-e80e6d30c317 · outbound
This paper cites Fast Theoretical Predictions for Spherical Fourier Analysis of Large-Scale Structures.
Optimal and exact wide-angle power spectrum estimation Fast Theoretical Predictions for Spherical Fourier Analysis of Large-Scale Structures
Reference 33
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation de7fca30-dc59-4747-85ae-a145699fb5f6 · outbound
This paper cites Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis.
Optimal and exact wide-angle power spectrum estimation Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis
Reference 34
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation baba1bc7-b427-480e-ad61-c3d1b0778184 · outbound
This paper cites Wen, H.S.G.
Optimal and exact wide-angle power spectrum estimation Wen, H.S.G
Reference 35
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dbcab2d7-6c60-4c97-a6ca-8bbec8889182 · outbound
This paper cites Demonstrating the Use of the Spherical Fourier Bessel Basis for Large Scale Clustering Systematics Discovery and Mitigation with eBOSS.
Optimal and exact wide-angle power spectrum estimation Demonstrating the Use of the Spherical Fourier Bessel Basis for Large Scale Clustering Systematics Discovery and Mitigation with eBOSS
Reference 36
- Resolution
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Unavailable: canonical work link unavailable.
Observation 297fba1c-8ede-4d97-96b6-9c6c08afa9ef · outbound
This paper cites Beyond the plane-parallel approximation for redshift surveys.
Optimal and exact wide-angle power spectrum estimation Beyond the plane-parallel approximation for redshift surveys
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 94296274-6d9f-4858-a9df-893429dcc630 · outbound
This paper cites Wide Angle Redshift Distortions Revisited.
Optimal and exact wide-angle power spectrum estimation Wide Angle Redshift Distortions Revisited
Reference 38
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation 518abe1c-387e-478f-ab09-78150e949740 · outbound
This paper cites Non-Perturbative Effects of Geometry in Wide-Angle Redshift Distortions.
Optimal and exact wide-angle power spectrum estimation Non-Perturbative Effects of Geometry in Wide-Angle Redshift Distortions
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a93baa8a-1bb3-4476-a643-038f27675fe0 · outbound
This paper cites Shaw and A.
Optimal and exact wide-angle power spectrum estimation Shaw and A
Reference 40
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation 71d31d98-9261-4d94-b6a6-03bd1aff9867 · outbound
This paper cites Simulating Redshift-Space Distortions for Galaxy Pairs with Wide Angular Separation.
Optimal and exact wide-angle power spectrum estimation Simulating Redshift-Space Distortions for Galaxy Pairs with Wide Angular Separation
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 754a3c0a-7237-4f82-ae0f-d3b5a31a2332 · outbound
This paper cites Alcock and B.
Optimal and exact wide-angle power spectrum estimation Alcock and B
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b1e2e1a-fdc5-4386-a587-8ef219b096fb · outbound
This paper cites The Correlation Function in Redshift Space: General Formula with Wide-angle Effects and Cosmological Distortions.
Optimal and exact wide-angle power spectrum estimation The Correlation Function in Redshift Space: General Formula with Wide-angle Effects and Cosmological Distortions
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9e1495d2-703f-4ff9-ba59-9679cf536b7c · outbound
This paper cites Alcock-Paczynski effects on wide-angle galaxy statistics.
Optimal and exact wide-angle power spectrum estimation Alcock-Paczynski effects on wide-angle galaxy statistics
Reference 44
- Resolution
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dfeb030a-50db-4242-82f6-cca589f69d9e · outbound
This paper cites New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects.
Optimal and exact wide-angle power spectrum estimation New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a4ab37d2-091e-4ce5-8dda-2dd032de0b9a · outbound
This paper cites The linear power spectrum of observed source number counts.
Optimal and exact wide-angle power spectrum estimation The linear power spectrum of observed source number counts
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed778709-26f2-4e6c-a9f3-d71a038f8594 · outbound
This paper cites What galaxy surveys really measure.
Optimal and exact wide-angle power spectrum estimation What galaxy surveys really measure
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a342a50c-5a90-4cb5-96f9-817466b1568e · outbound
This paper cites Modeling relativistic contributions to the halo power spectrum dipole.
Optimal and exact wide-angle power spectrum estimation Modeling relativistic contributions to the halo power spectrum dipole
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2719bd00-69fa-4ae1-bad8-f90b9c9535af · outbound
This paper cites Beyond the plane-parallel and Newtonian approach: Wide-angle redshift distortions and convergence in general relativity.
Optimal and exact wide-angle power spectrum estimation Beyond the plane-parallel and Newtonian approach: Wide-angle redshift distortions and convergence in general relativity
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9743befd-e2ec-4ddf-9b94-16aefd3adb03 · outbound
This paper cites Large-scale 3D galaxy correlation function and non-Gaussianity.
Optimal and exact wide-angle power spectrum estimation Large-scale 3D galaxy correlation function and non-Gaussianity
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 974fb3c9-5234-47ce-852b-1a916e715bbc · outbound
This paper cites The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects.
Optimal and exact wide-angle power spectrum estimation The full-sky relativistic correlation function and power spectrum of galaxy number counts: I. Theoretical aspects
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e621dc86-de8d-4a20-b4e2-6408d449b5ab · outbound
This paper cites The observed galaxy power spectrum in General Relativity.
Optimal and exact wide-angle power spectrum estimation The observed galaxy power spectrum in General Relativity
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9a5410bd-a661-474e-a909-2fd1997c5bce · outbound
This paper cites Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum.
Optimal and exact wide-angle power spectrum estimation Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 27734b16-c54b-437f-ae09-7484947c031e · outbound
This paper cites The Zeldovich approximation and wide-angle redshift-space distortions.
Optimal and exact wide-angle power spectrum estimation The Zeldovich approximation and wide-angle redshift-space distortions
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1dc43c7f-c125-4ec5-a2b9-dcbb8eea8b92 · outbound
This paper cites Wide-angle effects in the galaxy bispectrum.
Optimal and exact wide-angle power spectrum estimation Wide-angle effects in the galaxy bispectrum
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e177c3a4-28d6-45bb-bfd3-1c6342398fca · outbound
This paper cites Wide angle effects for peculiar velocities.
Optimal and exact wide-angle power spectrum estimation Wide angle effects for peculiar velocities
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Unavailable: canonical work link unavailable.
Observation baf7a607-ae71-4a6c-85e2-4c8348a82df6 · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0.
Optimal and exact wide-angle power spectrum estimation The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bddcd69b-a666-4b95-86d4-cc424a48263e · outbound
This paper cites Efficient estimators for power spectrum and bispectrum multipole measurements.
Optimal and exact wide-angle power spectrum estimation Efficient estimators for power spectrum and bispectrum multipole measurements
Reference 58
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- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 7e738fd2-3dd2-4543-b8f8-2dba306581bb · outbound
This paper cites Power Spectrum Analysis of Three-Dimensional Redshift Surveys.
Optimal and exact wide-angle power spectrum estimation Power Spectrum Analysis of Three-Dimensional Redshift Surveys
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 19a6d8ae-f0d5-4f10-96b8-e79e01b1ce8a · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space.
Optimal and exact wide-angle power spectrum estimation The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation d097d0a2-f3ce-4543-9dfd-76c7079406ba · outbound
This paper cites MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets.
Optimal and exact wide-angle power spectrum estimation MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 39f1d2e5-2bfe-4a91-aa29-4f4b8a5be625 · outbound
This paper cites General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?.
Optimal and exact wide-angle power spectrum estimation General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 95bcadec-6bbd-4c57-8d61-d6e056a5b5c7 · outbound
This paper cites Galaxy Two-Point Correlation Function in General Relativity.
Optimal and exact wide-angle power spectrum estimation Galaxy Two-Point Correlation Function in General Relativity
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation ee02f2f4-0a02-4e6a-b30e-c18364eca4f3 · outbound
This paper cites Galaxy Power Spectrum in General Relativity.
Optimal and exact wide-angle power spectrum estimation Galaxy Power Spectrum in General Relativity
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 92a1dd32-4f1a-4d60-af5a-36a4027ef934 · outbound
This paper cites Large Scale Limit of the Observed Galaxy Power Spectrum.
Optimal and exact wide-angle power spectrum estimation Large Scale Limit of the Observed Galaxy Power Spectrum
Reference 65
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation dfa81729-ce24-42b9-bd70-920698d3d536 · outbound
This paper cites DESI luminous red galaxy samples for cross-correlations.
Optimal and exact wide-angle power spectrum estimation DESI luminous red galaxy samples for cross-correlations
Reference 66
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation e652b73c-5a06-479f-932a-bafc97edbf92 · outbound
This paper cites Doppler bias: impact of peculiar velocities on color selection and the large scale structure of galaxy surveys.
Optimal and exact wide-angle power spectrum estimation Doppler bias: impact of peculiar velocities on color selection and the large scale structure of galaxy surveys
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 5c350e04-f287-43c8-a81f-c8adf49be7bb · outbound
This paper cites Reconstruction of the remote dipole and quadrupole fields from the kinetic Sunyaev Zel'dovich and polarized Sunyaev Zel'dovich effects.
Optimal and exact wide-angle power spectrum estimation Reconstruction of the remote dipole and quadrupole fields from the kinetic Sunyaev Zel'dovich and polarized Sunyaev Zel'dovich effects
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 509008df-26f7-41cc-a64b-6a350d5d7f83 · outbound
This paper cites KSZ tomography and the bispectrum.
Optimal and exact wide-angle power spectrum estimation KSZ tomography and the bispectrum
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 0d0cc86b-ba02-4c39-9f66-9b3415cfdf87 · outbound
This paper cites Constraining local non-Gaussianities with kSZ tomography.
Optimal and exact wide-angle power spectrum estimation Constraining local non-Gaussianities with kSZ tomography
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation a360fd9d-ba39-4166-ae9f-9829fe24210d · outbound
This paper cites Kinetic Sunyaev Zel'dovich velocity reconstruction from Planck and unWISE.
Optimal and exact wide-angle power spectrum estimation Kinetic Sunyaev Zel'dovich velocity reconstruction from Planck and unWISE
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 023dd98f-1366-4f40-8ed3-a212b82c671e · outbound
This paper cites The Atacama Cosmology Telescope: Large-scale velocity reconstruction with the kinematic Sunyaev--Zel'dovich effect and DESI LRGs.
Optimal and exact wide-angle power spectrum estimation The Atacama Cosmology Telescope: Large-scale velocity reconstruction with the kinematic Sunyaev--Zel'dovich effect and DESI LRGs
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 44e6cd04-c9a4-4c83-952b-ae3bf6307bfd · outbound
This paper cites McCarthy, B.
Optimal and exact wide-angle power spectrum estimation McCarthy, B
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 9c8af9f1-9d9b-4e52-8160-02bde52a899e · outbound
This paper cites Constraints on local primordial non-Gaussianity with 3d Velocity Reconstruction from the Kinetic Sunyaev-Zeldovich Effect.
Optimal and exact wide-angle power spectrum estimation Constraints on local primordial non-Gaussianity with 3d Velocity Reconstruction from the Kinetic Sunyaev-Zeldovich Effect
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation cd0b548f-c63e-45c4-873c-53da7cf549d0 · outbound
This paper cites Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS.
Optimal and exact wide-angle power spectrum estimation Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 4ae4ad06-aeab-4bc0-8d46-fe18ce8ab5cb · outbound
This paper cites KSZ Velocity Reconstruction with ACT and DESI-LS using a Tomographic QML Power Spectrum Estimator.
Optimal and exact wide-angle power spectrum estimation KSZ Velocity Reconstruction with ACT and DESI-LS using a Tomographic QML Power Spectrum Estimator
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 86297648-b3c8-436e-b0c8-15d98bb53a2b · outbound
This paper cites Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6.
Optimal and exact wide-angle power spectrum estimation Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6
Reference 77
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation a3f73498-ec71-4e05-a4e9-d3f930e64861 · outbound
This paper cites The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope.
Optimal and exact wide-angle power spectrum estimation The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 49a8b8a4-d421-425d-b8a8-f9bf48f2928a · outbound
This paper cites Analyzing the cosmic variance limit of remote dipole measurements of the cosmic microwave background using the large-scale kinetic Sunyaev Zel'dovich effect.
Optimal and exact wide-angle power spectrum estimation Analyzing the cosmic variance limit of remote dipole measurements of the cosmic microwave background using the large-scale kinetic Sunyaev Zel'dovich effect
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 3b11fb63-720e-4b9a-8bcc-2281e00a9fbc · outbound
This paper cites Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges.
Optimal and exact wide-angle power spectrum estimation Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation f797d3a3-7ba6-484d-82d2-cde95a602071 · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
Optimal and exact wide-angle power spectrum estimation Planck 2018 results. VI. Cosmological parameters
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 0b8fc41e-33e0-418e-a574-78bb063a3fed · outbound
This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.
Optimal and exact wide-angle power spectrum estimation The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation f80a6d3f-b016-4ed5-b013-575493835f30 · outbound
This paper cites Tegmark,How to measure cmb power spectra without losing information,Phys.
Optimal and exact wide-angle power spectrum estimation Tegmark,How to measure cmb power spectra without losing information,Phys
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 25376978-58a1-4bff-bdeb-a083ed8f2450 · outbound
This paper cites Hybrid Estimation of CMB Polarization Power Spectra.
Optimal and exact wide-angle power spectrum estimation Hybrid Estimation of CMB Polarization Power Spectra
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation fbe0f4bb-b26a-4517-9ad2-14608f713e39 · outbound
This paper cites Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight.
Optimal and exact wide-angle power spectrum estimation Beyond Yamamoto: Anisotropic Power Spectra and Correlation Functions with Pairwise Lines-of-Sight
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 3d16b98b-3075-41b7-a341-a7f09df51252 · outbound
This paper cites Gravitational redshift and other redshift-space distortions of the imaginary part of the power spectrum.
Optimal and exact wide-angle power spectrum estimation Gravitational redshift and other redshift-space distortions of the imaginary part of the power spectrum
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9bd5395-21ed-4ee1-9b5a-954f50c17daa · outbound
This paper cites FFTLog: Fast Fourier or Hankel transform.
Optimal and exact wide-angle power spectrum estimation FFTLog: Fast Fourier or Hankel transform
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 1c75dc7c-8781-4455-b071-175b4ba0f132 · outbound
This paper cites Asymmetric galaxy correlation functions.
Optimal and exact wide-angle power spectrum estimation Asymmetric galaxy correlation functions
Reference 88
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e389c847-bfa5-466b-9e99-a04360c7f6da · outbound
This paper cites Wide-angle effects in multi-tracer power spectra with Doppler corrections.
Optimal and exact wide-angle power spectrum estimation Wide-angle effects in multi-tracer power spectra with Doppler corrections
Reference 89
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Observation 40413b07-5fde-475a-b2cb-83f4257dc68f · outbound
This paper cites Myths and Truths Concerning Estimation of Power Spectra.
Optimal and exact wide-angle power spectrum estimation Myths and Truths Concerning Estimation of Power Spectra
Reference 90
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
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Observation 9d426333-7f91-40ac-a8a8-afb56a415535 · outbound
This paper cites If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics.
Optimal and exact wide-angle power spectrum estimation If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9fef124a-ba5d-457e-8be9-4df1df2c5714 · outbound
This paper cites Integral constraints in spectroscopic surveys.
Optimal and exact wide-angle power spectrum estimation Integral constraints in spectroscopic surveys
Reference 92
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 36b921df-e90a-4289-992b-938a1ccd1352 · outbound
This paper cites Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators.
Optimal and exact wide-angle power spectrum estimation Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators
Reference 93
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4955d030-c98b-4a8d-bc53-1b1966e27885 · outbound
This paper cites Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis.
Optimal and exact wide-angle power spectrum estimation Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 37d8e321-acaa-46a4-a1fd-9444ea4885bc · outbound
This paper cites Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation.
Optimal and exact wide-angle power spectrum estimation Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation
Reference 95
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- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4c993790-88c3-4ca4-bbc6-7357aab59fbf · outbound
This paper cites triangle condition.
Optimal and exact wide-angle power spectrum estimation triangle condition
Reference 96
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:32:08.971654Z
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Pith citing papers
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