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Source: paper_references, paper_reference_links, observed 2026-08-14T10:40:21.635042Z
Paper Citation Record · LEDGER
As of 15 August 2026, this Paper Citation Record lists 100 of 123 outbound references and 0 inbound Pith citation observations for arXiv:1908.10757.
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100 of 123 outbound references displayed
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Tetrad formalism for exact cosmological observables Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
Reference 1
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Observation 97846079-c09c-4d25-b9b7-5f6432a394dc · outbound
Tetrad formalism for exact cosmological observables Planck 2018 results. VI. Cosmological parameters
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Observation 807fb556-3126-4d1d-a248-0665d35bc605 · outbound
Tetrad formalism for exact cosmological observables Planck 2018 results. I. Overview and the cosmological legacy of Planck
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Observation 3323645e-0812-4304-b6bd-7b41423032aa · outbound
Tetrad formalism for exact cosmological observables Cosmological Constraints from the SDSS Luminous Red Galaxies
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Observation 2f2cb74a-2dc4-4fcc-9bde-49062faaf7ce · outbound
Tetrad formalism for exact cosmological observables The DESI Experiment, a whitepaper for Snowmass 2013
Reference 5
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Observation 47b0415b-e53e-4f3a-8646-f7387ebd9ca3 · outbound
Tetrad formalism for exact cosmological observables Unresolved cited work
Reference 6
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Observation ae2c2d99-4d72-4c68-84dd-c3c25e56c3dd · outbound
Tetrad formalism for exact cosmological observables Wide-Field InfraRed Survey Telescope (WFIRST) Final Report
Reference 7
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Observation 0dab73ff-fb6d-4ec5-ba8a-4f9e76e429b4 · outbound
Tetrad formalism for exact cosmological observables Unresolved cited work
Reference 8
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Observation 1aa4992e-ed84-45ee-88c6-515769cc8565 · outbound
Tetrad formalism for exact cosmological observables Euclid Definition Study Report
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Observation 651534fd-6c26-4156-b5e5-b1c941b17b8a · outbound
Tetrad formalism for exact cosmological observables Lensed CMB power spectra from all-sky correlation functions
Reference 10
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Observation 4f898182-dad5-45b7-9ee3-9b8b8d50eadf · outbound
Tetrad formalism for exact cosmological observables Weak Gravitational Lensing of the CMB
Reference 11
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Observation 58af62bc-6f69-49d3-b4c9-d27bf1bcc157 · outbound
Tetrad formalism for exact cosmological observables Weak lensing of the CMB
Reference 12
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Observation 64ca51da-3359-41d9-9313-a703037ce55f · outbound
Tetrad formalism for exact cosmological observables The shape of the CMB lensing bispectrum
Reference 13
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Observation fde2242c-de93-403c-813f-5289b11a418f · outbound
Tetrad formalism for exact cosmological observables Impact of polarisation on the intrinsic CMB bispectrum
Reference 14
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Observation 0ca06d27-7b0f-4d5b-9f09-ae321bb3ae4e · outbound
Tetrad formalism for exact cosmological observables Do we care about the distance to the CMB? Clarifying the impact of second-order lensing
Reference 15
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Observation eb2517c0-a39f-4699-bf5b-0a20ec057514 · outbound
Tetrad formalism for exact cosmological observables CMB-lensing beyond the Born approximation
Reference 16
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Observation 03d6f5fd-dff5-4f1e-9d17-949041dfd34b · outbound
Tetrad formalism for exact cosmological observables Impact of next-to-leading order contributions to CMB lensing
Reference 17
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Observation 0fadca1d-aec5-4dfb-82b9-cf78fc90539c · outbound
Tetrad formalism for exact cosmological observables CMB-lensing beyond the leading order: temperature and polarization anisotropies
Reference 18
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Observation 7a8da872-b88a-4a31-a341-46eb7c097baa · outbound
Tetrad formalism for exact cosmological observables Impact of post-Born lensing on the CMB
Reference 19
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Tetrad formalism for exact cosmological observables Emission-angle and polarization-rotation effects in the lensed CMB
Reference 20
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Observation 22833f75-0330-4575-a61d-554fbc44326a · outbound
Tetrad formalism for exact cosmological observables Rotation of the CMB polarisation by foreground lensing
Reference 21
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Tetrad formalism for exact cosmological observables Galaxy number counts to second order and their bispectrum
Reference 22
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Observation 7fa1576b-afa7-4946-a6fb-f03200f87fe6 · outbound
Tetrad formalism for exact cosmological observables Observed galaxy number counts on the lightcone up to second order: I. Main result
Reference 23
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Observation 20774c93-6287-45b6-adae-de71fe53e335 · outbound
Tetrad formalism for exact cosmological observables Observed galaxy number counts on the lightcone up to second order: II. Derivation
Reference 24
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Tetrad formalism for exact cosmological observables The bispectrum of relativistic galaxy number counts
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Tetrad formalism for exact cosmological observables Higher order relativistic galaxy number counts: dominating terms
Reference 26
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Observation 5e973a19-2c77-4ce3-8173-276fc439d5d1 · outbound
Tetrad formalism for exact cosmological observables Non-Gaussianities due to Relativistic Corrections to the Observed Galaxy Bispectrum
Reference 27
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Tetrad formalism for exact cosmological observables A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
Reference 28
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Observation ef602657-0c47-4d3b-a5af-13fc30f8cfec · outbound
Tetrad formalism for exact cosmological observables Imprints of local lightcone projection effects on the galaxy bispectrum. II
Reference 29
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Tetrad formalism for exact cosmological observables Imprints of local lightcone projection effects on the galaxy bispectrum. III Relativistic corrections from nonlinear dynamical evolution on large-scales
Reference 30
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Tetrad formalism for exact cosmological observables Imprints of local lightcone projection effects on the galaxy bispectrum IV: Second-order vector and tensor contributions
Reference 31
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Observation 61e93586-dcb9-45fd-9628-03f5afbe65c5 · outbound
Tetrad formalism for exact cosmological observables The observed galaxy bispectrum from single-field inflation in the squeezed limit
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Observation c178d6c0-d4ba-49dd-b449-cc46dc8e1042 · outbound
Tetrad formalism for exact cosmological observables The Full-Sky Angular Bispectrum in Redshift Space
Reference 33
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Observation d6e474d2-49f9-48fe-9537-1ae582e3adcf · outbound
Tetrad formalism for exact cosmological observables The dipole of the galaxy bispectrum
Reference 34
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Observation fedfe58d-27c1-46c1-9768-2c4b18628d06 · outbound
Tetrad formalism for exact cosmological observables Non-linear contributions to angular power spectra
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Tetrad formalism for exact cosmological observables Galaxy number counts at second order: an independent approach
Reference 36
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Observation 625d5e53-9aa9-4a90-bef6-3ae318849372 · outbound
Tetrad formalism for exact cosmological observables Full-sky lensing shear at second order
Reference 37
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Observation 09136d17-c9e9-4c28-9298-7033908e34bd · outbound
Tetrad formalism for exact cosmological observables Cosmic shear bispectrum from second-order perturbations in General Relativity
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Observation 9eeba69a-d6b9-4984-b732-6fd3d1fd29eb · outbound
Tetrad formalism for exact cosmological observables Nonlinear relativistic corrections to cosmological distances, redshift and gravitational lensing magnification. I - Key results
Reference 39
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Observation 46a1fdcd-ae7c-44e6-8957-a56704036c95 · outbound
Tetrad formalism for exact cosmological observables Nonlinear relativistic corrections to cosmological distances, redshift and gravitational lensing magnification. II - Derivation
Reference 40
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Tetrad formalism for exact cosmological observables Non-linear relativistic contributions to the cosmological weak-lensing convergence
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Tetrad formalism for exact cosmological observables The luminosity distance-redshift relation up to second order in the Poisson gauge with anisotropic stress
Reference 42
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Tetrad formalism for exact cosmological observables Cosmological ensemble and directional averages of observables
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Tetrad formalism for exact cosmological observables Full-sky weak lensing: a nonlinear post-Friedmann treatment
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Tetrad formalism for exact cosmological observables Peculiar velocity effects in high-resolution microwave background experiments
Reference 47
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Tetrad formalism for exact cosmological observables Gravitational Lensing from a Spacetime Perspective
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Tetrad formalism for exact cosmological observables Relativistic Effect in Galaxy Clustering
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Tetrad formalism for exact cosmological observables Beyond the Linear-Order Relativistic Effect in Galaxy Clustering: Second-Order Gauge-Invariant Formalism
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Tetrad formalism for exact cosmological observables Formulating Weak Lensing from the Boltzmann Equation and Application to Lens-lens Couplings
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Tetrad formalism for exact cosmological observables Gauge-Transformation Properties of Cosmological Observables and its Application to the Light-Cone Average
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Tetrad formalism for exact cosmological observables Gauge-Invariant Formalism of Cosmological Weak Lensing
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Tetrad formalism for exact cosmological observables General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
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Tetrad formalism for exact cosmological observables Nugier, Lightcone Averaging and Precision Cosmology , Ph.D
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Tetrad formalism for exact cosmological observables Bernstein, Kinetic Theory In The Expanding Universe , Cambridge Monographs on Mathematical Physics
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Observation 41f9d900-1201-4c51-8176-0ce423878ccc · outbound
Tetrad formalism for exact cosmological observables Cosmic Microwave Background Polarization
Reference 94
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Observation 62dd877e-5861-4bf9-813e-44212ec6f9ae · outbound
Tetrad formalism for exact cosmological observables Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
Reference 95
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Observation 7618a267-bc13-4ed4-81bf-a15766692a82 · outbound
Tetrad formalism for exact cosmological observables Dodelson, Modern Cosmology
Reference 96
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Tetrad formalism for exact cosmological observables Durrer, The Cosmic Microwave Background
Reference 97
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Tetrad formalism for exact cosmological observables Weinberg, Cosmology
Reference 98
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Observation 9a1d3f2b-937a-4c9f-904b-5a34ea5013fb · outbound
Tetrad formalism for exact cosmological observables Gauge Invariant Cosmological Perturbation Theory
Reference 99
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Observation 6b1a84cf-4a9c-4299-b9a8-aa92fe30ee1a · outbound
Tetrad formalism for exact cosmological observables Cosmological Magnetic Fields: Their Generation, Evolution and Observation
Reference 100
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