Weighted Webs: Morphology-Informed Marked Fields | Paper Citation Record

Observation 40796934-ebdc-4620-a11b-e22ffc61f63e · outbound

This paper cites Zeldovich,Gravitational instability: An Approximate theory for large density perturbations,Astron.

Weighted Webs: Morphology-Informed Marked Fields Zeldovich,Gravitational instability: An Approximate theory for large density perturbations,Astron

Reference 1

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Observation 4817886e-bc0f-4362-8fc8-a2a11af618e8 · outbound

This paper cites Gunn and J.R.

Weighted Webs: Morphology-Informed Marked Fields Gunn and J.R

Reference 2

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Observation 51540f4a-a416-4c9f-b08d-cfe18a9444d8 · outbound

This paper cites How Filaments are Woven into the Cosmic Web.

Weighted Webs: Morphology-Informed Marked Fields How Filaments are Woven into the Cosmic Web

Reference 3

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Observation 0de25594-d5a7-47d4-a0f2-771e021f766f · outbound

This paper cites The large-scale structure of the Universe.

Weighted Webs: Morphology-Informed Marked Fields The large-scale structure of the Universe

Reference 4

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Observation e3c704c0-208e-43e7-9e14-45af12d4fb42 · outbound

This paper cites van de Weygaert and W.

Weighted Webs: Morphology-Informed Marked Fields van de Weygaert and W

Reference 5

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Observation 5e814b1f-90d3-4a0a-9854-6f95be3a732e · outbound

This paper cites Evolution of the cosmic web.

Weighted Webs: Morphology-Informed Marked Fields Evolution of the cosmic web

Reference 7

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Observation 4b016e34-574d-466d-ba22-cc41b52a685c · outbound

This paper cites Tracing the cosmic web.

Weighted Webs: Morphology-Informed Marked Fields Tracing the cosmic web

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.082389Z

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Observation 9cbe798b-4f8d-4d3e-bc8e-2750114b2930 · outbound

This paper cites Non-Linear Evolution of the Bispectrum of Cosmological Perturbations.

Weighted Webs: Morphology-Informed Marked Fields Non-Linear Evolution of the Bispectrum of Cosmological Perturbations

Reference 9

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Observation 7ee14c88-42b6-4336-83bb-3066ea8e48dd · outbound

This paper cites Large-Scale Structure of the Universe and Cosmological Perturbation Theory.

Weighted Webs: Morphology-Informed Marked Fields Large-Scale Structure of the Universe and Cosmological Perturbation Theory

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.245037Z

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Observation 550d70a2-e8f9-44af-8453-b77df3335f53 · outbound

This paper cites Robust Morphological Measures for Large-Scale Structure in the Universe.

Weighted Webs: Morphology-Informed Marked Fields Robust Morphological Measures for Large-Scale Structure in the Universe

Reference 11

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Observation 7eec4912-16f3-4849-9c7a-e4542c54e035 · outbound

This paper cites Beyond genus statistics: a unifying approach to the morphology of cosmic structure.

Weighted Webs: Morphology-Informed Marked Fields Beyond genus statistics: a unifying approach to the morphology of cosmic structure

Reference 12

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Observation 97a44a93-e0d9-4741-8be9-a349260a3e68 · outbound

This paper cites Persistent homology of the cosmic web. I: Hierarchical topology in $\Lambda$CDM cosmologies.

Weighted Webs: Morphology-Informed Marked Fields Persistent homology of the cosmic web. I: Hierarchical topology in $\Lambda$CDM cosmologies

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.454661Z

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Observation a1f70ff9-9bb7-44bc-b070-ebf8bce9247f · outbound

This paper cites The Topology of the Cosmic Web in Terms of Persistent Betti Numbers.

Weighted Webs: Morphology-Informed Marked Fields The Topology of the Cosmic Web in Terms of Persistent Betti Numbers

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.458524Z

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Observation 8d4912b5-1ad6-40f2-84f8-8488533d9d37 · outbound

This paper cites Cheng, Y.-S.

Weighted Webs: Morphology-Informed Marked Fields Cheng, Y.-S

Reference 15

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Observation 6c12d8b0-bc97-496d-95e5-57b565cb409c · outbound

This paper cites Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform.

Weighted Webs: Morphology-Informed Marked Fields Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.466653Z

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Observation f0ad4359-bb47-4080-a3b5-e9e0aa3526f1 · outbound

This paper cites Cosmic voids: a novel probe to shed light on our Universe.

Weighted Webs: Morphology-Informed Marked Fields Cosmic voids: a novel probe to shed light on our Universe

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.471216Z

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Observation 57b8d98c-5bed-4a39-913b-327e7252be4b · outbound

This paper cites Davies, M.

Weighted Webs: Morphology-Informed Marked Fields Davies, M

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.475674Z

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Observation 6cfafbad-d51b-4ad5-a720-a4aa1099cbef · outbound

This paper cites Weak lensing peak statistics in the era of large scale cosmological surveys.

Weighted Webs: Morphology-Informed Marked Fields Weak lensing peak statistics in the era of large scale cosmological surveys

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.479042Z

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Observation a01d1f11-adff-44cf-baf8-3cdeba7cadee · outbound

This paper cites Stoyan,On Correlations of Marked Point Processes,Mathematische Nachrichten116(1984) 197.

Weighted Webs: Morphology-Informed Marked Fields Stoyan,On Correlations of Marked Point Processes,Mathematische Nachrichten116(1984) 197

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.482840Z

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Observation 7015b368-77b4-4f2e-b9c1-9a3dfc0faae5 · outbound

This paper cites Luminosity- and morphology-dependent clustering of galaxies.

Weighted Webs: Morphology-Informed Marked Fields Luminosity- and morphology-dependent clustering of galaxies

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.486547Z

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Observation b3ecc275-120b-4e4b-be95-209386ab3f30 · outbound

This paper cites The Luminosity-Weighted or `Marked' Correlation Function.

Weighted Webs: Morphology-Informed Marked Fields The Luminosity-Weighted or `Marked' Correlation Function

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.490545Z

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Observation 883afd76-372f-4178-af88-3243b5eb771d · outbound

This paper cites Galaxy Zoo: Disentangling the Environmental Dependence of Morphology and Colour.

Weighted Webs: Morphology-Informed Marked Fields Galaxy Zoo: Disentangling the Environmental Dependence of Morphology and Colour

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.494750Z

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Observation b4697094-7a67-4a9b-8447-0abccd9f3482 · outbound

This paper cites an unresolved cited work.

Weighted Webs: Morphology-Informed Marked Fields Unresolved cited work

Reference 24

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Observation 1f897356-77a4-4893-bdf1-a2873b6688f4 · outbound

This paper cites Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function.

Weighted Webs: Morphology-Informed Marked Fields Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.501874Z

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Observation 74501529-9957-403c-ad66-5ae738308781 · outbound

This paper cites A marked correlation function for constraining modified gravity models.

Weighted Webs: Morphology-Informed Marked Fields A marked correlation function for constraining modified gravity models

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.505537Z

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Observation 149b1fd2-4694-4c6f-87bc-b02b3d56e3d9 · outbound

This paper cites Testing modified gravity using a marked correlation function.

Weighted Webs: Morphology-Informed Marked Fields Testing modified gravity using a marked correlation function

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.509269Z

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Observation e6c9a106-c702-4ff1-890b-6c5706d927fd · outbound

This paper cites Towards an optimal marked correlation function analysis for the detection of modified gravity.

Weighted Webs: Morphology-Informed Marked Fields Towards an optimal marked correlation function analysis for the detection of modified gravity

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.513476Z

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Observation 28b70585-969f-4b98-b1bb-71d6046c8948 · outbound

This paper cites Beyond delta: Tailoring marked statistics to reveal modified gravity.

Weighted Webs: Morphology-Informed Marked Fields Beyond delta: Tailoring marked statistics to reveal modified gravity

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.517347Z

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Observation e0eeaaf6-a671-4460-80ff-10405dbd55d9 · outbound

This paper cites Multipole analysis of redshift-space distortions around cosmic voids.

Weighted Webs: Morphology-Informed Marked Fields Multipole analysis of redshift-space distortions around cosmic voids

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.521505Z

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Observation 3f0c9873-e5c9-466c-8dfe-fac1344c951a · outbound

This paper cites Cosmological Information in the Marked Power Spectrum of the Galaxy Field.

Weighted Webs: Morphology-Informed Marked Fields Cosmological Information in the Marked Power Spectrum of the Galaxy Field

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.525234Z

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Observation 4b75a808-68f4-44f6-bd41-3a2962c1b454 · outbound

This paper cites {\sc SimBIG}: Cosmological Constraints using Simulation-Based Inference of Galaxy Clustering with Marked Power Spectra.

Weighted Webs: Morphology-Informed Marked Fields {\sc SimBIG}: Cosmological Constraints using Simulation-Based Inference of Galaxy Clustering with Marked Power Spectra

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.529097Z

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Observation f48a3e3c-777d-40e8-97de-b52a65b81f71 · outbound

This paper cites Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12.

Weighted Webs: Morphology-Informed Marked Fields Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.532900Z

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Observation 9d6bce9c-e589-44f6-8eeb-b87d4076904c · outbound

This paper cites A new test of gravity -- I: Introduction to the method.

Weighted Webs: Morphology-Informed Marked Fields A new test of gravity -- I: Introduction to the method

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.536616Z

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Observation 09550bdb-c6dd-468d-a374-0f952693b301 · outbound

This paper cites First Constraints from Marked Angular Power Spectra with Subaru Hyper Suprime-Cam Survey First-Year Data.

Weighted Webs: Morphology-Informed Marked Fields First Constraints from Marked Angular Power Spectra with Subaru Hyper Suprime-Cam Survey First-Year Data

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.540620Z

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Observation 34490e2b-341d-4886-87f3-069c1e41436a · outbound

This paper cites Hitting the mark: Optimising Marked Power Spectra for Cosmology.

Weighted Webs: Morphology-Informed Marked Fields Hitting the mark: Optimising Marked Power Spectra for Cosmology

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.544429Z

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Observation f4e2ca07-68e8-4d4d-8f22-642675e985da · outbound

This paper cites What does the Marked Power Spectrum Measure? Insights from Perturbation Theory.

Weighted Webs: Morphology-Informed Marked Fields What does the Marked Power Spectrum Measure? Insights from Perturbation Theory

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.548206Z

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Observation 3c1cd913-eaee-4613-93a3-b7bf0406a93e · outbound

This paper cites Modeling the Marked Spectrum of Matter and Biased Tracers in Real- and Redshift-Space.

Weighted Webs: Morphology-Informed Marked Fields Modeling the Marked Spectrum of Matter and Biased Tracers in Real- and Redshift-Space

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.552169Z

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Observation ace40173-4271-4361-8827-0419a8c27a5d · outbound

This paper cites The constraining power of the Marked Power Spectrum: an analytical study.

Weighted Webs: Morphology-Informed Marked Fields The constraining power of the Marked Power Spectrum: an analytical study

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.556268Z

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Observation b2731a5e-db84-4d75-9328-e3d667927538 · outbound

This paper cites An Analytically Tractable Marked Power Spectrum.

Weighted Webs: Morphology-Informed Marked Fields An Analytically Tractable Marked Power Spectrum

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.560140Z

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Observation 7ebdb682-6a1a-405b-aab9-6f703ec44177 · outbound

This paper cites Ebina, M.

Weighted Webs: Morphology-Informed Marked Fields Ebina, M

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.564793Z

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Observation 1abf8e59-9c3a-4771-ad0d-a33ff225c9ed · outbound

This paper cites Marinucci, M.

Weighted Webs: Morphology-Informed Marked Fields Marinucci, M

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.568416Z

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Observation 5c69e37f-f5fe-42f5-b02f-57c7c2fe8c5f · outbound

This paper cites Halo abundances within the cosmic web.

Weighted Webs: Morphology-Informed Marked Fields Halo abundances within the cosmic web

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.572464Z

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Observation d8b0541a-b8b1-4c24-80de-e65a1d1acf18 · outbound

This paper cites Cosmic web dependence of galaxy clustering and quenching in SDSS.

Weighted Webs: Morphology-Informed Marked Fields Cosmic web dependence of galaxy clustering and quenching in SDSS

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.576600Z

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Observation 43226fa3-4ccd-4b12-a331-fedcde36e8ea · outbound

This paper cites A Dynamical Classification of the Cosmic Web.

Weighted Webs: Morphology-Informed Marked Fields A Dynamical Classification of the Cosmic Web

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.580461Z

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Observation f4d6811c-b408-449b-b3da-cd3e502ff98a · outbound

This paper cites A theoretical view of the T-web statistical description of the cosmic web.

Weighted Webs: Morphology-Informed Marked Fields A theoretical view of the T-web statistical description of the cosmic web

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.584179Z

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Observation 454acb34-3326-45c7-9c1f-5d32147ed42e · outbound

This paper cites Armijo and L.

Weighted Webs: Morphology-Informed Marked Fields Armijo and L

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.588164Z

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Observation 751b1e3c-708e-4735-8bd5-c43aa4a922c5 · outbound

This paper cites Doroshkevich,Spatial structure of perturbations and origin of galactic rotation in fluctuation theory,Astrophysics6(1970) 320.

Weighted Webs: Morphology-Informed Marked Fields Doroshkevich,Spatial structure of perturbations and origin of galactic rotation in fluctuation theory,Astrophysics6(1970) 320

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.591824Z

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Observation 5a0037bb-5474-4312-87bc-367ada1e5eb8 · outbound

This paper cites Constraining Peaks in Gaussian Primordial Density Fields: an Application of the Hoffman-Ribak Method.

Weighted Webs: Morphology-Informed Marked Fields Constraining Peaks in Gaussian Primordial Density Fields: an Application of the Hoffman-Ribak Method

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.595716Z

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Observation 3bfa43c2-1ea5-481f-977d-dc8fb3d9e63f · outbound

This paper cites Bardeen, J.R.

Weighted Webs: Morphology-Informed Marked Fields Bardeen, J.R

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.599603Z

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Observation 8019fd7b-f9b3-4d33-929c-1a27d361cb67 · outbound

This paper cites Environmental dependence in the ellipsoidal collapse model.

Weighted Webs: Morphology-Informed Marked Fields Environmental dependence in the ellipsoidal collapse model

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.603182Z

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Observation ae4f2a07-42bc-4468-a1e1-602f22d9ef25 · outbound

This paper cites Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS.

Weighted Webs: Morphology-Informed Marked Fields Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.607194Z

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Observation 926c47b2-b934-4526-850c-144affb9c605 · outbound

This paper cites Large-Scale Galaxy Bias.

Weighted Webs: Morphology-Informed Marked Fields Large-Scale Galaxy Bias

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.611211Z

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Observation b4793463-e394-45fb-9b8f-1910d9acbe88 · outbound

This paper cites Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids.

Weighted Webs: Morphology-Informed Marked Fields Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.615185Z

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Observation 6481e75c-329c-437b-a2cd-e5338dda6b34 · outbound

This paper cites The Quijote simulations.

Weighted Webs: Morphology-Informed Marked Fields The Quijote simulations

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.619032Z

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Observation 92990021-55a9-4e90-8f88-ca8debe0b460 · outbound

This paper cites Pylians: Python libraries for the analysis of numerical simulations.

Weighted Webs: Morphology-Informed Marked Fields Pylians: Python libraries for the analysis of numerical simulations

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.622836Z

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Observation 032fc1c6-6e41-42e1-bfe9-df62074d2d7a · outbound

This paper cites Quantification of high dimensional non-Gaussianities and its implication to Fisher analysis in cosmology.

Weighted Webs: Morphology-Informed Marked Fields Quantification of high dimensional non-Gaussianities and its implication to Fisher analysis in cosmology

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.626631Z

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Observation 8d5b9de6-add7-482e-912f-9347b334f7b2 · outbound

This paper cites Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix.

Weighted Webs: Morphology-Informed Marked Fields Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T00:53:53.630489Z

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Observation be46c065-e333-4c7d-a851-5268340669ac · outbound

This paper cites Deep learning insights into cosmological structure formation.

Weighted Webs: Morphology-Informed Marked Fields Deep learning insights into cosmological structure formation

Reference 59

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