De-baryonifying halos via optimal transport | Paper Citation Record

Observation d2eee693-576d-4fb0-954b-68c4d1d6b291 · outbound

This paper cites Since all elements of xd are physically expected to be non-zero positive,xd takes values on the standard simplex.2 It is beneficial to map the 256 dimensional simplex to R255.

De-baryonifying halos via optimal transport Since all elements of xd are physically expected to be non-zero positive,xd takes values on the standard simplex.2 It is beneficial to map the 256 dimensional simplex to R255

Reference 1

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Observation 77b4a7df-bc69-40e2-97da-56750306cec4 · outbound

This paper cites We will use the Illustris TNG-300 simulation [45–50] as a test set.

De-baryonifying halos via optimal transport We will use the Illustris TNG-300 simulation [45–50] as a test set

Reference 2

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Observation 2fa86a70-15a2-4960-ba79-61fffdf70a8d · outbound

This paper cites overlap bias.

De-baryonifying halos via optimal transport overlap bias

Reference 3

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Observation f202a788-f38f-4114-8424-9679783b90ca · outbound

This paper cites A non-linear solution to the $S_8$ tension?.

De-baryonifying halos via optimal transport A non-linear solution to the $S_8$ tension?

Reference 4

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Observation f899f926-d646-49c0-ada7-2042e0a3c7e9 · outbound

This paper cites Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies.

De-baryonifying halos via optimal transport Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.501646Z

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Observation 79842a9a-5c22-4d47-9340-594181797103 · outbound

This paper cites The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the $S_8$ tension.

De-baryonifying halos via optimal transport The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the $S_8$ tension

Reference 6

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Observation 22921237-328d-46d6-aeb1-1eefde3ded12 · outbound

This paper cites Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback.

De-baryonifying halos via optimal transport Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback

Reference 7

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Observation 659e695c-a616-4d7a-95a7-d4cb62000ecf · outbound

This paper cites Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics.

De-baryonifying halos via optimal transport Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics

Reference 8

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Observation 9a2453b0-89c6-42f8-b9fe-132770b94c8c · outbound

This paper cites Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present.

De-baryonifying halos via optimal transport Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.520258Z

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Observation 41cd45d4-ecc1-4bd0-afa9-834a43139300 · outbound

This paper cites Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters.

De-baryonifying halos via optimal transport Implications of feedback solutions to the $S_8$ tension for the baryon fractions of galaxy groups and clusters

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.524774Z

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Observation f722bf22-e950-4803-9efc-0f2fa43a28a4 · outbound

This paper cites The impact of baryonic physics and massive neutrinos on weak lensing peak statistics.

De-baryonifying halos via optimal transport The impact of baryonic physics and massive neutrinos on weak lensing peak statistics

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:49.659216Z

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Observation f95ed67a-df3b-4a08-9cf6-65fbeb40b3e1 · outbound

This paper cites Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum.

De-baryonifying halos via optimal transport Constraining neutrino mass with tomographic weak lensing one-point probability distribution function and power spectrum

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.532626Z

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Observation 100b95cf-8d8e-48fa-92ff-ae3c2d65f374 · outbound

This paper cites The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps.

De-baryonifying halos via optimal transport The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.551974Z

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Observation fb1724e7-e8b6-443d-b676-047ca42029ad · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

De-baryonifying halos via optimal transport KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.640252Z

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Observation 5f9700bc-f759-4c88-a619-b3f61e4d1004 · outbound

This paper cites Amon et al., Phys.

De-baryonifying halos via optimal transport Amon et al., Phys

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.713343Z

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Observation f9bf738f-c796-439d-a242-83bdad1318ef · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra.

De-baryonifying halos via optimal transport Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.770008Z

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Observation d29fe478-0034-47d9-b3e1-2558868c4959 · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions.

De-baryonifying halos via optimal transport Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.774294Z

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Observation 25f8cf58-f3b6-41ef-9b77-9b8cd44e735e · outbound

This paper cites An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models.

De-baryonifying halos via optimal transport An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.779449Z

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Observation 2c3f3736-9ae5-41f8-a2ad-e56a83f7c0cc · outbound

This paper cites Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces.

De-baryonifying halos via optimal transport Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.783421Z

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Observation f2e024c1-f25c-45ce-8c02-5de7dfb7dc72 · outbound

This paper cites Modeling baryonic physics in future weak lensing surveys.

De-baryonifying halos via optimal transport Modeling baryonic physics in future weak lensing surveys

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.787758Z

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Observation d7edc3d9-1eab-4811-a110-eeddfe4c516a · outbound

This paper cites HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback.

De-baryonifying halos via optimal transport HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.792005Z

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Observation 9b32e2a3-ec7b-430d-8959-37b33a9aa34d · outbound

This paper cites Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe.

De-baryonifying halos via optimal transport Dark Energy Survey Year 1 Results: Constraining Baryonic Physics in the Universe

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.796584Z

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Observation 39048d38-ee2e-491f-86c7-4ab8de3c9fd1 · outbound

This paper cites Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra.

De-baryonifying halos via optimal transport Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.800437Z

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Observation 2f6642cd-ba05-4d38-9012-2c5681c7a051 · outbound

This paper cites The contribution of massive haloes to the matter power spectrum in the presence of AGN feedback.

De-baryonifying halos via optimal transport The contribution of massive haloes to the matter power spectrum in the presence of AGN feedback

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.805160Z

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Observation 8942be0a-542c-4adf-8649-303ff8090b85 · outbound

This paper cites Field-level inference of cosmic shear with intrinsic alignments and baryons.

De-baryonifying halos via optimal transport Field-level inference of cosmic shear with intrinsic alignments and baryons

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.810332Z

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Observation bc98e8c6-eacf-4b5c-87bb-b44af50e08fe · outbound

This paper cites Dai and U.

De-baryonifying halos via optimal transport Dai and U

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.867390Z

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Observation 0e292885-8649-4800-a764-f477a31c911e · outbound

This paper cites A new method to quantify the effects of baryons on the matter power spectrum.

De-baryonifying halos via optimal transport A new method to quantify the effects of baryons on the matter power spectrum

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.820058Z

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Observation d66e6fe2-5aca-41ab-a0b2-1bdbf8214c98 · outbound

This paper cites Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix.

De-baryonifying halos via optimal transport Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.824490Z

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Observation 186a27b6-b1c9-496e-81cf-8c80b9f50108 · outbound

This paper cites Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics.

De-baryonifying halos via optimal transport Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.893992Z

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Observation dc1d4de1-5c3a-4acd-9420-7f4ce7c4e99a · outbound

This paper cites Baryonification extended to thermal Sunyaev Zeldovich.

De-baryonifying halos via optimal transport Baryonification extended to thermal Sunyaev Zeldovich

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.953229Z

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Observation fb3b7517-0e1b-404a-8b50-f0164e5c76ad · outbound

This paper cites Map-level baryonification: Efficient modelling of higher-order correlations in the weak lensing and thermal Sunyaev-Zeldovich fields.

De-baryonifying halos via optimal transport Map-level baryonification: Efficient modelling of higher-order correlations in the weak lensing and thermal Sunyaev-Zeldovich fields

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:47.991719Z

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Observation 6983345a-effd-45db-8f0e-5fa45e9afca0 · outbound

This paper cites Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons.

De-baryonifying halos via optimal transport Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.059012Z

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Observation a2ad3bad-e961-4591-a496-9b5cd18317fb · outbound

This paper cites Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations.

De-baryonifying halos via optimal transport Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:49.242910Z

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Observation 739501f1-170a-4a3e-aa87-ff4d06c4c577 · outbound

This paper cites A gradient based method for modeling baryons and matter in halos of fast simulations.

De-baryonifying halos via optimal transport A gradient based method for modeling baryons and matter in halos of fast simulations

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.140814Z

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Observation 4a606f64-c164-4c16-a18f-7b90e8a42bdb · outbound

This paper cites A field-level emulator for modeling baryonic effects across hydrodynamic simulations.

De-baryonifying halos via optimal transport A field-level emulator for modeling baryonic effects across hydrodynamic simulations

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.145804Z

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Observation 61abfbb9-9c73-409f-89b3-a4ee039a55e5 · outbound

This paper cites Euclid Definition Study Report.

De-baryonifying halos via optimal transport Euclid Definition Study Report

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.150306Z

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Observation 8a1c7484-85ac-43df-be98-e5101f4cc8ea · outbound

This paper cites Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS).

De-baryonifying halos via optimal transport Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)

Reference 37

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Observation 0c94a897-9728-48ad-b439-88222c1b8504 · outbound

This paper cites Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report.

De-baryonifying halos via optimal transport Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

Reference 38

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Observation faa934cc-f87c-444e-beb2-54ffc357c623 · outbound

This paper cites LSST: from Science Drivers to Reference Design and Anticipated Data Products.

De-baryonifying halos via optimal transport LSST: from Science Drivers to Reference Design and Anticipated Data Products

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.163109Z

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Observation ac9f5e40-5deb-46ed-9077-01a0d51ccd98 · outbound

This paper cites Optimal Transport Reconstruction of Baryon Acoustic Oscillations.

De-baryonifying halos via optimal transport Optimal Transport Reconstruction of Baryon Acoustic Oscillations

Reference 40

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Observation 787bb089-f705-4f42-b2c4-646cc19e89a3 · outbound

This paper cites Optimal Transport Reconstruction of Biased Tracers in Redshift Space.

De-baryonifying halos via optimal transport Optimal Transport Reconstruction of Biased Tracers in Redshift Space

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.172761Z

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Observation dc7c6428-ea96-4298-90d4-80d17deb238b · outbound

This paper cites Displacement Field Analysis via Optimal Transport: Multi-Tracer Approach to Cosmological Reconstruction.

De-baryonifying halos via optimal transport Displacement Field Analysis via Optimal Transport: Multi-Tracer Approach to Cosmological Reconstruction

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.204659Z

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Observation ab7a55f8-ac00-4cf4-a7f5-172ea6bae7b2 · outbound

This paper cites The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback.

De-baryonifying halos via optimal transport The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.271036Z

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Observation f0e621f1-05af-4432-97a9-2634e8e74530 · outbound

This paper cites Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data.

De-baryonifying halos via optimal transport Inferring the impact of feedback on the matter distribution using the Sunyaev Zel'dovich effect: Insights from CAMELS simulations and ACT+DES data

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.330596Z

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Observation 1f1025c7-ae28-4f90-96be-631560dfab63 · outbound

This paper cites Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations.

De-baryonifying halos via optimal transport Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.334606Z

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Observation 9a9594ad-0124-4df2-bd11-fbba9f324288 · outbound

This paper cites The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores.

De-baryonifying halos via optimal transport The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.339134Z

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Observation ed93a76a-d8ec-4362-a988-b9c781af3385 · outbound

This paper cites Aitchison, Journal of the Royal Statisti- cal Society: Series B (Methodological) 44, 139 (1982), https://academic.oup.com/jrsssb/article- pdf/44/2/139/49097906/jrsssb_44_2_139.pdf.

De-baryonifying halos via optimal transport Aitchison, Journal of the Royal Statisti- cal Society: Series B (Methodological) 44, 139 (1982), https://academic.oup.com/jrsssb/article- pdf/44/2/139/49097906/jrsssb_44_2_139.pdf

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.856050Z

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Observation 8a3ab49d-3cb0-484e-810d-6fa0681e7a8e · outbound

This paper cites First results from the IllustrisTNG simulations: the galaxy color bimodality.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: the galaxy color bimodality

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.346913Z

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Observation 77a32fb9-ca26-41db-ac2f-86759cd5db31 · outbound

This paper cites First results from the IllustrisTNG simulations: radio haloes and magnetic fields.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.351089Z

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Observation 616dc0bd-aded-4e94-8f9c-959594db1475 · outbound

This paper cites First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.355006Z

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Observation 50c30b9c-9b34-4f7b-abf8-f9a7a11c8b5b · outbound

This paper cites First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.358804Z

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Observation 3a91abf0-1adb-4edc-90d6-1aa1e9edae12 · outbound

This paper cites First results from the IllustrisTNG simulations: matter and galaxy clustering.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: matter and galaxy clustering

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.361871Z

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Observation d1133012-7083-4ae7-ade4-10ac01137283 · outbound

This paper cites The IllustrisTNG Simulations: Public Data Release.

De-baryonifying halos via optimal transport The IllustrisTNG Simulations: Public Data Release

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.366482Z

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Observation 8764c1aa-da22-4dd5-b108-48e92b882db3 · outbound

This paper cites Confirmation of the standard cosmological model from red massive galaxies $\sim600$ Myr after the Big Bang.

De-baryonifying halos via optimal transport Confirmation of the standard cosmological model from red massive galaxies $\sim600$ Myr after the Big Bang

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.370786Z

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Observation e7570fd3-426e-4c49-b296-3bf94669aef3 · outbound

This paper cites The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters.

De-baryonifying halos via optimal transport The Uchuu-UniverseMachine dataset: Galaxies in and around Clusters

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:48.910977Z

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Observation 3d1675b0-ecc8-4301-a38e-0a65fbda9988 · outbound

This paper cites The Uchuu-SDSS galaxy lightcones: a clustering, RSD and BAO study.

De-baryonifying halos via optimal transport The Uchuu-SDSS galaxy lightcones: a clustering, RSD and BAO study

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:48.891013Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 074daec0-3426-45bc-98b9-652d8b68bda3 · outbound

This paper cites Uchuu-$\nu^2$GC galaxies and AGN: Cosmic variance forecasts of high-redshift AGN for JWST, Euclid, and LSST.

De-baryonifying halos via optimal transport Uchuu-$\nu^2$GC galaxies and AGN: Cosmic variance forecasts of high-redshift AGN for JWST, Euclid, and LSST

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:48.810168Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8f635403-73ca-4ac1-839d-876568afe69b · outbound

This paper cites The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations.

De-baryonifying halos via optimal transport The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.535932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8ee537f-d09f-4676-b001-0a7a21ae9945 · outbound

This paper cites The Quijote simulations.

De-baryonifying halos via optimal transport The Quijote simulations

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.540932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dfcc8d2c-efd5-4bcc-a4b0-77120a837c77 · outbound

This paper cites Halo concentrations in the standard LCDM cosmology.

De-baryonifying halos via optimal transport Halo concentrations in the standard LCDM cosmology

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.545512Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8c7d440-762b-4939-b6ec-463975842432 · outbound

This paper cites Papamakarios, T.

De-baryonifying halos via optimal transport Papamakarios, T

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.549118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4bd8e85e-6e31-421e-a5da-ef84aab938be · outbound

This paper cites Huang, D.

De-baryonifying halos via optimal transport Huang, D

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.835887Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 1cafd9a7-b803-4ac2-a91f-94685cd6d2f3 · outbound

This paper cites Van der Maaten and G.

De-baryonifying halos via optimal transport Van der Maaten and G

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.824614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 38b7e009-3af0-4724-8235-17c7974953b5 · outbound

This paper cites Nalisnick, A.

De-baryonifying halos via optimal transport Nalisnick, A

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.808682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 107c7906-a232-4529-9972-f47871482734 · outbound

This paper cites Du and I.

De-baryonifying halos via optimal transport Du and I

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.796919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 6d907732-4ccf-4f68-88ea-a720cec54a28 · outbound

This paper cites Knopp and R.

De-baryonifying halos via optimal transport Knopp and R

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.783495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 7fc1a4e1-bc47-4412-853f-e0089ea17e56 · outbound

This paper cites Feydy, T.

De-baryonifying halos via optimal transport Feydy, T

Reference 67

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T11:18:49.770679Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 62a16c32-2756-4fcb-a2ec-eb4e3952c98c · outbound

This paper cites Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach.

De-baryonifying halos via optimal transport Weak Lensing by Large-Scale Structure: A Dark Matter Halo Approach

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-12T11:18:48.677476Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 32b3114e-ba1d-49b4-b77c-d18c511db1b9 · outbound

This paper cites an unresolved cited work.

De-baryonifying halos via optimal transport Unresolved cited work

Reference 69

Resolution: unresolved; raw_fallback, observed 2026-08-12T11:18:49.757178Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 135ecefe-bf2d-4264-b7f2-160f5bb47374 · outbound

This paper cites Stochastic Interpolants: A Unifying Framework for Flows and Diffusions.

De-baryonifying halos via optimal transport Stochastic Interpolants: A Unifying Framework for Flows and Diffusions

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.585536Z

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Unavailable: canonical work link unavailable.

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