Pith. sign in

Paper Citation Record · LEDGER

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

As of 10 August 2026, this Paper Citation Record lists 100 of 104 outbound references and 7 inbound Pith citation observations for arXiv:2507.00118.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2507.00118 v1

Coverage vector

measured 100 of 104 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:30:54.992988Z

measured 107 of 107 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:30:54.279301Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-17T04:19:00.846851Z

Reference resolution

100 of 104 outbound references displayed

  • verified exact2
  • verified fuzzy0
  • unresolved98
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 7627e816-bdc8-473c-86ef-70ff4f90f75a · outbound

This paper cites Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.279301Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.279301Z digest=sha256:fbd4023917766ddd738a36a281727010363b128838796f16adbe06ff95a1a6e8

Observation b948eff6-c865-42fa-97a6-36cac3a48b2b · outbound

This paper cites For instance, even at the level of the power spec- trum alone, there are eleven EFT nuisance parameters that must be marginalized over to constrain cosmological parameters.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors For instance, even at the level of the power spec- trum alone, there are eleven EFT nuisance parameters that must be marginalized over to constrain cosmological parameters

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.285266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.285266Z digest=sha256:8b8796558c0f3ecd02c575434b2ac554c958d25fc8d70e596ea2b665b579c64f

Observation 65f33602-5cde-4140-b847-19fa394a003a · outbound

This paper cites We will present the detail of each experiment here and explain the pa- rameters varied in this section.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors We will present the detail of each experiment here and explain the pa- rameters varied in this section

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.290088Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.290088Z digest=sha256:0fb8bbe183185539e534c6132d1043d6e5375a4c4b7f1b087a9a154c623d8329

Observation a7b177c1-a02c-4be8-a916-bd2e1570c49b · outbound

This paper cites Gaussian.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Gaussian

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.295851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.295851Z digest=sha256:5441b3ce89aa9beccdc09cffb7afc9d3070264ac664166a8d7f2b02a5a8f7aa5

Observation 1c695ac2-f751-4021-9798-8fcde43f4e3b · outbound

This paper cites an unresolved cited work.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Unresolved cited work

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.301672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.301672Z digest=sha256:e7f8d21d98552796015194994740710a689789c90364efc95d688efdf64015ec

Observation 859a32ee-f9e7-4e8d-8a01-585c5b411b1e · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.306260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.306260Z digest=sha256:907400a591feec3b69e1081d89d146a87b8a0049758aad1ceeb842fbcd524361

Observation 059a5092-64a5-47b4-b966-81424a55fa32 · outbound

This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.311700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.311700Z digest=sha256:837711538c29ea04d975c99f539df0c11a94639d6e131d0f1b9a5c190eb8c13b

Observation c6f8f6ad-b20f-4c34-9f71-bcbaa61ec642 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.316372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.316372Z digest=sha256:05e470c264a89316b6219393a9b396827417dab8cf02e91ac106f888988f57d5

Observation 77796c6b-a2a1-4ae0-a30b-0afd3987f2e0 · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.324449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.324449Z digest=sha256:7374ecffddfd7868f6309ad7e3acb1975ad2f247c05ff8c1379fec49316b65c2

Observation 7ce3cee7-64de-410a-a3f1-ab12539422f0 · outbound

This paper cites Euclid Definition Study Report.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Euclid Definition Study Report

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.331878Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.331878Z digest=sha256:75bac882dd3bc74707b30f9f897716de2ef40693555c7fcb90fe3e4b5ed07c3a

Observation 65d0bdf3-da30-4182-8e37-a162fa87b3e5 · outbound

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

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors LSST: from Science Drivers to Reference Design and Anticipated Data Products

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.337528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.337528Z digest=sha256:b61ab3698c4e2493e1b92ce7544caf4a0cbc0f3670cd7738a42046b60a6abdee

Observation 3be237c7-4291-478c-8f68-e8c26dc3b16c · outbound

This paper cites The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.344966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.344966Z digest=sha256:78aa796e3dbbee387589033511105377b536a4f09bb9a732ad29fd2cff7018cc

Observation 841d6954-b332-4b65-bcf8-bf40391528ed · outbound

This paper cites The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.350992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.350992Z digest=sha256:0cf90a618838e5700869a971974f8ed534ea53960cbca176a835cb26d6d210cf

Observation ccd98637-fad4-41ee-b570-15966766157d · outbound

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

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors First results from the IllustrisTNG simulations: matter and galaxy clustering

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.355930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.355930Z digest=sha256:a386ead6565e8acb325d65eba8d84a10eac75c7fd02b785275e040989a417af6

Observation 2e029b6c-689e-416c-9996-ac310b37ccf8 · outbound

This paper cites The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.363314Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.363314Z digest=sha256:d26da5ae5e289f38d3ca4191d521b3b671284de911f17d459ff273043a5cad47

Observation 7244e37d-b665-4e7c-ab34-3e1ecb783b6b · outbound

This paper cites The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.370356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.370356Z digest=sha256:2badee09538655318c288315a7a118fa9913347708e11c6571a244318e156f7c

Observation d028dafd-7fcc-4f30-98ad-9682fb9ca8f4 · outbound

This paper cites The Dark Side of the Halo Occupation Distribution.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Dark Side of the Halo Occupation Distribution

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.375843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.375843Z digest=sha256:9fce30fc0d0374c0394f37b35194fcb27324d8c5fd8e6c2b3b756c58e26ab689

Observation 08972ae1-87a5-44a3-848f-9b1434612cda · outbound

This paper cites Zheng, A.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Zheng, A

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.381658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.381658Z digest=sha256:a844eee0f7f2cf21610832f52e45df8d20ad22e5a0586bd8281b56fde049e225

Observation 96ebd98d-b822-4865-b1bf-3f040d0dec8b · outbound

This paper cites Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.387381Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.387381Z digest=sha256:de9acc08351144afdfb70d75518e955e971ee832030876a96450f550d2395ad9

Observation b26f42e3-b5d7-420a-8ac5-05be2197b9d5 · outbound

This paper cites The Connection between Galaxies and their Dark Matter Halos.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Connection between Galaxies and their Dark Matter Halos

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.393471Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.393471Z digest=sha256:a9ac68797c41e2ea6cde1ebfdbb6c3fa58ff1a4c09e848a3d447c7a5299855e9

Observation 60fdbb4f-6d48-4c48-b7c4-bf093963d716 · outbound

This paper cites A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.402080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.402080Z digest=sha256:03e6ae0cee70f312115e3f180b84e9dd1ae88064ba2da7e89debcc1b9c4860c1

Observation 9726fccf-5757-44c4-993b-30b6979dbeb4 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.408199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.408199Z digest=sha256:2e77806a1b5862f9b4055d8241a5a7736f136d4c6a770929d8ca699dfb9e7ba5

Observation 512607ed-c6e5-461f-9070-761d05fe4856 · outbound

This paper cites Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.413066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.413066Z digest=sha256:db19d5f27626962c2a5efde1610bf7d905039d6141c9ac1c0b31943e12a80f1e

Observation 28513114-1913-4f40-9ecc-7beaf7fef39e · outbound

This paper cites SUNBIRD: A simulation-based model for full-shape density-split clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors SUNBIRD: A simulation-based model for full-shape density-split clustering

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.418513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.418513Z digest=sha256:ab41007fe1d48b618836bba324ec76a8eaea3c7bcf2a3270969f72579d25556e

Observation 993400d3-19b4-4c30-b03d-518b7541fd2b · outbound

This paper cites Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.423644Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.423644Z digest=sha256:1ab3bc08bb2e029d5f4c416d5d6a2977e806cea2be4ee1559bacf1181e46a5b6

Observation 82692922-1dc1-4e42-a7a1-cbe7eab81a28 · outbound

This paper cites ${\rm S{\scriptsize IM}BIG}$: The First Cosmological Constraints from the Non-Linear Galaxy Bispectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors ${\rm S{\scriptsize IM}BIG}$: The First Cosmological Constraints from the Non-Linear Galaxy Bispectrum

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.432891Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.432891Z digest=sha256:49cdce5a2534feb576beabe831628e7b4f0c5afb622cdad5d0cae5cf6c703e60

Observation 2e7d8c29-a067-43a8-aa82-21c253cdd66c · outbound

This paper cites ${\rm S{\scriptsize IM}BIG}$: Cosmological Constraints from the Redshift-Space Galaxy Skew Spectra.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors ${\rm S{\scriptsize IM}BIG}$: Cosmological Constraints from the Redshift-Space Galaxy Skew Spectra

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.437956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.437956Z digest=sha256:ecf4220e912a26e6a0e901a3f07a848bdd34c7b54ca6f757527db2a4fe166668

Observation cda9db17-3dc0-4abb-8086-7f5205640115 · outbound

This paper cites Cosmological Non-Linearities as an Effective Fluid.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Non-Linearities as an Effective Fluid

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.445267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.445267Z digest=sha256:130078e844b4f04715068a85ef5e06fa80192fd355f7a00a13ef486376ed14a7

Observation e173aefe-af18-4c3a-adb4-6a806d5f32cf · outbound

This paper cites The Effective Field Theory of Cosmological Large Scale Structures.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Effective Field Theory of Cosmological Large Scale Structures

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.449829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.449829Z digest=sha256:9e6c1320fc29cd5f75cfd7ee1dfec2bf8a0ee536cb2a41e2c8ab87936f816462

Observation c6fdbfd8-23ba-41ab-92b1-a10cf69491a4 · outbound

This paper cites Effective Field Theory for Large Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Effective Field Theory for Large Scale Structure

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.455647Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.455647Z digest=sha256:cd99eabff32d3187c89ba8a1b8f0e1942907fea8583cd6fc3f8ac326cc17661d

Observation ad56386c-41b2-48ed-b734-ed23b5cf9830 · outbound

This paper cites Large-Scale Galaxy Bias.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Large-Scale Galaxy Bias

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.463076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.463076Z digest=sha256:d3e3908ee7f121b8636e9d2eb38b66229605c63cb21d61a52d119501491a07af

Observation adf1a551-a00b-4ddf-8c7d-85562050b64a · outbound

This paper cites Cosmological Parameters from the BOSS Galaxy Power Spectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Parameters from the BOSS Galaxy Power Spectrum

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.468523Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.468523Z digest=sha256:9a34f0adc0de081922f735e93c39d1803d24b457a6b63a170938164ba29d8a0c

Observation 0fe581c5-b8e8-4418-92f3-b1695c0451e1 · outbound

This paper cites The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.477397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.477397Z digest=sha256:d096388fe91d244504008a02e67b5897f027758f45f2f198dceed3391a117444

Observation 362c9707-1c22-4e7a-815d-3e5ce77abc14 · outbound

This paper cites A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.485586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.485586Z digest=sha256:fb97b2a9dc4538720b70f33cfd31c5167f5dd0d4efe441d5408f934a552a70df

Observation 6e46ea83-d6e9-44cd-898e-0c2dffffa2fb · outbound

This paper cites The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.494259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.494259Z digest=sha256:6326b7428b46c0b30f0d75e273ef65014f68d008a21b2a2c9a004647970c9b93

Observation b68a82a7-386e-446a-a1e3-9bdd59b3d449 · outbound

This paper cites Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.499689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.499689Z digest=sha256:463b6cbdd3f3af79778c4d8be983012bcb43e491b6db8e227e529c6d42045b4b

Observation 182c724b-6cb6-4312-9164-103bae84968d · outbound

This paper cites Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.506129Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.506129Z digest=sha256:1ee8273c81df4a7de7bfbc6b1ccf5c68818434a3c84f39210d68cb15e4253f90

Observation b4923a69-91ba-418f-a76f-4265391df4ba · outbound

This paper cites Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.513122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.513122Z digest=sha256:e9734f2c5fae582602087b98e1f38620adcc559e7fc15dfbdd5b84501818d66b

Observation 7e63e80b-c6b4-4250-8c8b-6d7561b66e1d · outbound

This paper cites Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.521158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.521158Z digest=sha256:f87066d0dfc9415134ee668d0ea0b77568446fc91cad40bb3e41f1c5a587f3e6

Observation 43e5637a-9167-4d1f-970d-37c0e4b33df5 · outbound

This paper cites BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.527370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.527370Z digest=sha256:f9f93e6ee620093222c1120bb587425b214f3fd1b7c8b92e5e352e78d2463886

Observation 2c5c067b-d1c0-4b97-bc48-49935e6864ca · outbound

This paper cites The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.532095Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.532095Z digest=sha256:02eb31f072fcbe3dce32413c95c69b50716b0d37293731fa9c3873d83d4952e5

Observation 74198b84-c3a5-435c-be5e-fa10d082c97a · outbound

This paper cites Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Simulation-Based Priors without Simulations: an Analytic Perspective on EFT Parameters of Galaxies

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.537353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.537353Z digest=sha256:0302a7053dcd62d8afc80f7c4753d6e6b0cdc71cb285448186df31735f33ddbc

Observation 94be9440-a4bb-4d81-9d0b-9de6642ff03d · outbound

This paper cites High-redshift Millennium and Astrid galaxies in effective field theory at the field level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors High-redshift Millennium and Astrid galaxies in effective field theory at the field level

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.542883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.542883Z digest=sha256:a163c197f942e749cf8e996a6dedc416fdde59d20f4704f83013b0b755a8234d

Observation 896f3ed7-7609-45dc-a18e-d285c75a3e6f · outbound

This paper cites An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.548679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.548679Z digest=sha256:d90a3bfa200e259ecc8ddf1bd2b17c3ca7b4372c42b6883737e9426812441495

Observation 39d009c2-ccc9-4728-8e81-cf9683eea983 · outbound

This paper cites Modeling HI at the field level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling HI at the field level

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.555606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.555606Z digest=sha256:e93d8560e8d049f5f135700174422612950dc2510d307259650b6d0a26f6272a

Observation c551da39-4a9f-4bf7-9ce2-f9ebe6e32f90 · outbound

This paper cites Hybrid SBI or How I Learned to Stop Worrying and Learn the Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Hybrid SBI or How I Learned to Stop Worrying and Learn the Likelihood

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.561851Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.561851Z digest=sha256:209dda2da403befc0e56941088049007f3b60219364f5bae27a114737ddfcc6a

Observation 7f33f24b-94f7-46f1-bc80-b5f37e5c6751 · outbound

This paper cites Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Mapping the galaxy-halo connection to the galaxy bias: implication to the HOD-informed prior

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.567911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.567911Z digest=sha256:76972b148a783999af6cd7a72a67de981afcd4b1651a310df78b092dbc3a19c9

Observation e75f5742-3386-42f7-b8e1-8b40c8f6d9b7 · outbound

This paper cites HOD-informed prior for EFT-based full-shape analyses of LSS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors HOD-informed prior for EFT-based full-shape analyses of LSS

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.574685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.574685Z digest=sha256:6aebf1b141c9eb3f5491055da762b9c1d297b9a0dab574010b8822e52c1b12ae

Observation 7f0724c3-f259-4c4c-9b22-79120d8e7404 · outbound

This paper cites Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.580118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.580118Z digest=sha256:c422879e54bddb7a74af357dbbe98c524d15de9c42969d9e0337eb359e4091f1

Observation 3875fad6-16e4-4553-928a-bfe10ddb3f19 · outbound

This paper cites Modeling Galaxy Surveys with Hybrid SBI.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Galaxy Surveys with Hybrid SBI

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.585910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.585910Z digest=sha256:7f1dabd4d9ba4eac8978d3a0b18f5c5f9c8d7bc5b39c72d48b6e4471e1df967c

Observation 24c3fe6e-9c34-4c03-8e33-53a5387d221b · outbound

This paper cites Modeling Biased Tracers at the Field Level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Biased Tracers at the Field Level

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.591396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.591396Z digest=sha256:a1e2a4264b4f6739d26efbff247bfe12cad32c2380a52cbabed40850931b6a11

Observation 33b44dfa-d6e4-4610-a6af-c6e8c12f7398 · outbound

This paper cites Modeling Galaxies in Redshift Space at the Field Level.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Modeling Galaxies in Redshift Space at the Field Level

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.597407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.597407Z digest=sha256:fe8d495a07e88a19a0f2da32c90e2fb77abcaf68081bd62f2c14c9356fe90296

Observation c9bb7fb0-d01e-44c3-aff0-38401457e8be · outbound

This paper cites Improving cosmological analyses of HI clustering by reducing stochastic noise.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.602992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.602992Z digest=sha256:e485e9276cb1b2969b21ac35224d098b60a929820b733569b3d0f823ac368508

Observation 268b9c65-657d-4f74-85d9-e5056529770f · outbound

This paper cites Near optimal bispectrum estimators for large-scale structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Near optimal bispectrum estimators for large-scale structure

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.609055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.609055Z digest=sha256:a69879b08951201c9bee9fe753ff7dd58f65ca0d6123890c28c7a9f67e041223

Observation 24fbea34-bc86-405f-a819-f387abd02e52 · outbound

This paper cites Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.615708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.615708Z digest=sha256:63507b3a469912081d521a644f20624f5f901eb9e07402b9c45175ba566f4ea9

Observation 60d97db2-4312-4cb7-bd71-9cee67f2db23 · outbound

This paper cites Cubic Halo Bias in Eulerian and Lagrangian Space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cubic Halo Bias in Eulerian and Lagrangian Space

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.621796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.621796Z digest=sha256:8e26e3ba6ff1ab18be73145686ca0498577221349e8191e18e133f4f1ba2209c

Observation 4dd19cb1-89c5-4a66-a8ec-bc15004b4f04 · outbound

This paper cites A rigorous EFT-based forward model for large-scale structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors A rigorous EFT-based forward model for large-scale structure

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.629657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.629657Z digest=sha256:540e7e648df7d7d3f314705c1939e4d2bde63370972f924801795aafe8f88852

Observation 9bbe2620-422f-4e3e-b8c4-3c14ecbb01a3 · outbound

This paper cites Cosmology Inference from Biased Tracers using the EFT-based Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Inference from Biased Tracers using the EFT-based Likelihood

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.637193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.637193Z digest=sha256:a8cde05ceb9a91ecc5c94d47d140de1ce8e62871c77e92ab24c2bd5031d65b20

Observation f8508abd-69d8-4873-814f-a3efc9a84c0a · outbound

This paper cites The EFT Likelihood for Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The EFT Likelihood for Large-Scale Structure

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.648337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.648337Z digest=sha256:ef2e8ff776d18de74451abfbc095b104b26248866abb6e3f052ac537b51a6d75

Observation 3fc4b614-45fa-4ed0-b210-5b2a58ed17a4 · outbound

This paper cites Simulations and symmetries.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Simulations and symmetries

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.660937Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.660937Z digest=sha256:df1f71a6876cddb884d69ac44c8af5583408cd003a309be76834b58ba916d846

Observation ee59ae21-c76f-4542-a9f4-8b72315fccce · outbound

This paper cites Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Sigma-Eight at the Percent Level: The EFT Likelihood in Real Space

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.667686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.667686Z digest=sha256:cad2664901070a419c8502d82821843b49566ae7bc6d725ab429c20dd68635b5

Observation 97896322-91fb-4021-aabe-08260ee25bb3 · outbound

This paper cites Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.674478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.674478Z digest=sha256:cdab467a5cc8a4e693ca1259529ac3b9a017d7ae147ce172959fda33511dc521

Observation 1b0303b6-899e-4907-b62e-e77ce9613cd5 · outbound

This paper cites Assembly bias in quadratic bias parameters of dark matter halos from forward modeling.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Assembly bias in quadratic bias parameters of dark matter halos from forward modeling

Reference 63

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:30:56.904024Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-08-06T21:30:54.683333Z digest=sha256:8e10d18800e23b6d461d189c72c15d70d7e9353d56aeadb2f930be5840adb0e3

Observation ebb1a074-51bf-4296-99a9-0fe0f4c4d64c · outbound

This paper cites Cosmology inference at the field level from biased tracers in redshift-space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology inference at the field level from biased tracers in redshift-space

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.690215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.690215Z digest=sha256:5d0cee9c7f2fa37a226d0361aa3966f534ef8f9285036cf020b0475649838214

Observation c7e36254-7807-48ed-b316-6b70830a3760 · outbound

This paper cites How much information can be extracted from galaxy clustering at the field level?.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors How much information can be extracted from galaxy clustering at the field level?

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.695470Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.695470Z digest=sha256:23aa7cf70e48d3db36c28eada38a02e63cd7b51631cbb09a6d4508b99c4a5959

Observation dc0cc32c-601e-4caa-ac83-26a2141b1c88 · outbound

This paper cites Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.702515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.702515Z digest=sha256:a64cf295ee1515c0da3a6756f916929dc1764f54fc35e60df778fb9137234f2e

Observation fa74b654-37d8-4dce-9900-b53cf2b137fb · outbound

This paper cites Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.709787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.709787Z digest=sha256:002adc3686db35efafdd03069a2908948443c57c663e2e04d9dff355a298b503

Observation 5c13206e-b906-4b19-8100-7f81b66174d7 · outbound

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

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. VI. Cosmological parameters

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.714968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.714968Z digest=sha256:925e61b97818330ba8e46eb99f406db7a602d6049444196287dc72e71ab48e27

Observation 10738bcc-2e83-4a36-8f49-a8a94afecda7 · outbound

This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.721619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.721619Z digest=sha256:b74f7a749971155c32d3872119358a25033f3929d17693c05034cfe918c8a16e

Observation e97eae9b-02e2-47cc-969a-9532b57029a0 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Pantheon+ Analysis: Cosmological Constraints

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.731173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.731173Z digest=sha256:a9889e2d2bd679fd2e2fd0e2ddcff1deb5b779df9c445858d74c2c47fb5af1b4

Observation d7274eac-984c-423f-9ba1-db78ab7cd6c9 · outbound

This paper cites Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.738095Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.738095Z digest=sha256:0b55c54582d5ebe225eb3e1a48952645d9f7d451f3d6a52c31207c706179941a

Observation 471ea66b-8d38-4fdf-a939-27ea97bfef10 · outbound

This paper cites Optimizing large-scale structure data analysis with the theoretical error likelihood.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Optimizing large-scale structure data analysis with the theoretical error likelihood

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.750452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.750452Z digest=sha256:5191c910d6cc67e34ec9b97ebe27c8ad3ef3461f749bfe50670054347954b482

Observation 8a9bd3e4-f1f0-4674-81d4-7586b88a5637 · outbound

This paper cites Precision analysis of the redshift-space galaxy bispectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Precision analysis of the redshift-space galaxy bispectrum

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.755827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.755827Z digest=sha256:56b9219c2f6c7207148d0e816aecb80e99b037783a82889876289fc1da0b121e

Observation 4335c02e-2b44-4be0-b32f-2a9e0b4c9093 · outbound

This paper cites Bernardeau, S.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Bernardeau, S

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.762212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.762212Z digest=sha256:40c1d85c4e0c2b606038ba7c16a1f887af032ce262713e19bee359d2c66d8ad5

Observation 4a6035af-076d-4dd6-8c24-1d27a0bf4f8d · outbound

This paper cites Non-linear perturbation theory extension of the Boltzmann code CLASS.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Non-linear perturbation theory extension of the Boltzmann code CLASS

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.771030Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.771030Z digest=sha256:11dd3eb212c8a9dfd0176cab368bcbfc47bba30b484a1e932ecda6db1524ca1f

Observation 60615dd3-48a2-4e3c-9fd8-73ed8c313026 · outbound

This paper cites The two-loop power spectrum in redshift space.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The two-loop power spectrum in redshift space

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.776062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.776062Z digest=sha256:326bd720280a1173ae595425dd02a58f3e445a981efa89aa370b4e9ebd535d73

Observation 24ea5e24-4408-4f56-b870-b761f369dc1e · outbound

This paper cites Fingers of God.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fingers of God

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.782634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.782634Z digest=sha256:fabaabb7fd98234447ac0827f043d1caa0e70874f852f403fd53d21baeee691f

Observation d4e5bc7f-97e2-45f3-a19e-503163d0b5d6 · outbound

This paper cites Biased Tracers in Redshift Space in the EFT of Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Biased Tracers in Redshift Space in the EFT of Large-Scale Structure

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.792128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.792128Z digest=sha256:8ccdacdfd7b6be34314480796b5234c9d51d4d29336aa432c4e25c15425abd94

Observation 07eab98a-09c6-4136-9572-3ba60e69d0b3 · outbound

This paper cites The Baryon Oscillation Spectroscopic Survey of SDSS-III.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors The Baryon Oscillation Spectroscopic Survey of SDSS-III

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.798320Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.798320Z digest=sha256:66f3bcaa3490f511d14949f75bde156c8c1e3c71832b48ec6af9b228423bffcd

Observation 16c4482b-0daa-4204-b43e-394505bff32a · outbound

This paper cites Cosmological constraints without fingers of God.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological constraints without fingers of God

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.805234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.805234Z digest=sha256:ad606b4a3650f47be4ddf6a40ba9f5d191e40421248e7b63a31deb24b34d2091

Observation aea6ea0a-5e8f-44c1-9603-e1d8b2fb390c · outbound

This paper cites Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.812184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.812184Z digest=sha256:ad3e38db6a98d1f1f6cad543c7ec54b8d04268426a093c49739b72453d70f34e

Observation 7d2b3e01-f1f3-426e-9a74-1aacf2d8e193 · outbound

This paper cites Chudaykin, M.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Chudaykin, M

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.821297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.821297Z digest=sha256:f167a973ff2129663ea67b5043a372d65cbd41d0f005774031f0e1c2bd626cdb

Observation feb42ea7-1112-41c4-9b90-4b6c4baf9870 · outbound

This paper cites Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Without Windows: Quadratic Estimators for the Galaxy Power Spectrum

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.828529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.828529Z digest=sha256:ab6b6bfdf092eb3d390a0d1b78e82a1df8de65f53db1618f9100b0fdddb7135b

Observation e9cbe3ab-4b42-4b37-bea1-3bc084944636 · outbound

This paper cites Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.838718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.838718Z digest=sha256:a597ea5bae4a7dd5a2c96929cdd518fc6031eecb8ff3bf78ae37fdb60ce0206f

Observation 1955ea4f-5e9b-41b3-bac6-e9d22992b121 · outbound

This paper cites DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.846038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.846038Z digest=sha256:9ea7675f4be7a1f82e18489aa62b6012e3816cef35612de23dfbb8cbee6d59ef

Observation 0f0ef580-eb69-4d93-a027-d070f2668a19 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. V. CMB power spectra and likelihoods

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.852722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.852722Z digest=sha256:40037bbf5333e172559e13bc7df605dafde5d866402a07841a11e6e16c127583

Observation a361211a-4f7e-4633-b3cd-beb865f8577f · outbound

This paper cites Planck 2018 results. I. Overview and the cosmological legacy of Planck.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Planck 2018 results. I. Overview and the cosmological legacy of Planck

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.862860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.862860Z digest=sha256:79d7eecb080368b100e5ca9cc81bdaaec549f7830986bdb646de9f118b3e5022

Observation 06a98ab0-a570-4f88-b815-401737bf7649 · outbound

This paper cites Report of the Dark Energy Task Force.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Report of the Dark Energy Task Force

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.876685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.876685Z digest=sha256:52d5890c4f845d48214087bce463955e43f8cb0a279232f0435b42f4f9c33cc8

Observation dceb52c2-cde5-4240-afc1-e657ca23729c · outbound

This paper cites Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.881986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.881986Z digest=sha256:f1f73639a69e17380ce2f5e513c65d150c665bb986c47eb7fd332f617fddbcbd

Observation af26d374-4a05-41cc-b922-e983d4d7cd4e · outbound

This paper cites Sailer, G.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Sailer, G

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.889632Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.889632Z digest=sha256:aae8cdb866a5e7e69cc59c9d96f4b21bccfb5ee96f0afdfab0016b8fcf6a3306

Observation 25d43ac1-3d9a-4c54-b1e1-9f92b853261e · outbound

This paper cites Cosmological Constraints on Light (but Massive) Relics.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Cosmological Constraints on Light (but Massive) Relics

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.897815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.897815Z digest=sha256:3f201f9746ad18e494c4b115ef8164e70d9f84a5f8f14cf67b8a3049743eb2f4

Observation 6776c901-a329-4d7f-ab84-35a47692929f · outbound

This paper cites Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Ultra-light axions and the $S_8$ tension: joint constraints from the cosmic microwave background and galaxy clustering

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.928895Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.928895Z digest=sha256:29548665d007dac32e2489ebcdcad372fb135a43892eec1077139de0ce63a32b

Observation 2936a765-fc6b-48a2-a874-9b2b431f128c · outbound

This paper cites $S_8$ Tension in the Context of Dark Matter-Baryon Scattering.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors $S_8$ Tension in the Context of Dark Matter-Baryon Scattering

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.937966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.937966Z digest=sha256:11df5fc770dc7b8019011c5f6f3ca881a1befb040262dd6cb5901f4f6c5b6202

Observation ae889dbe-7ed5-4ee6-9d98-eb51b08a0ad5 · outbound

This paper cites Self-Interacting Neutrinos in Light of Large-Scale Structure Data.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Self-Interacting Neutrinos in Light of Large-Scale Structure Data

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.943883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.943883Z digest=sha256:dcbecbaad53de5bcdd3493e540550ea5267992954d9a8b835b7090efdf634678

Observation aa32c113-7843-4f99-a6af-2dca5d223134 · outbound

This paper cites Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.952619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.952619Z digest=sha256:565586295b557dbd11924d9b244ecfc55ac9635aa854b0c40db897c7dca3b87e

Observation 6ee0b670-4b72-4528-9c04-e3036eef26df · outbound

This paper cites Constraining Early Dark Energy with Large-Scale Structure.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Early Dark Energy with Large-Scale Structure

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.963624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.963624Z digest=sha256:fc78264ce0601e6063cccf2bb9c92c15a79b64fdf22cf1846dc5386f390afedf

Observation c5a782d2-dd8c-4258-ab35-7e6311778b24 · outbound

This paper cites Observational constraints on early dark energy.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Observational constraints on early dark energy

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.972872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.972872Z digest=sha256:d2c91116140bb87d7cf81bd4d7cab1ed2db7a370ca6d821b9bf520cdf2c31934

Observation 324792a2-152c-4057-895a-97f1ad8f17a5 · outbound

This paper cites Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Learning Theory Informed Priors for Bayesian Inference: A Case Study with Early Dark Energy

Reference 98

Resolution
verified exact
local_arxiv, observed 2026-08-06T21:30:55.435171Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-08-06T21:30:54.978829Z digest=sha256:0234b57738fecf0896c249fa9c05591e8db72099c9b3b1b41059292751e25648

Observation d1435927-83d1-465f-84b0-039d03b1b317 · outbound

This paper cites Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.985193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.985193Z digest=sha256:90ac71e34987d31512a1d2eddf0d3251a74cf0cacd6f2f2971525162fc599562

Observation 34a3ceae-d536-4fed-a7b0-6d2733582732 · outbound

This paper cites Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.992988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.992988Z digest=sha256:7b729f1f3e155ed71c6129551bc3f9f86f099e28f5896a0fa9cc3e94a977b58b

Pith citing papers

Observation 7627e816-bdc8-473c-86ef-70ff4f90f75a · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-06T21:30:54.279301Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:30:54.279301Z digest=sha256:fbd4023917766ddd738a36a281727010363b128838796f16adbe06ff95a1a6e8

Observation 92a54218-4e62-4b03-abfc-0497aee76a41 · inbound

Low-redshift constraints on structure growth from CMB lensing tomography cites this paper.

Low-redshift constraints on structure growth from CMB lensing tomography Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-04T10:38:03.277184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:38:03.277184Z digest=sha256:2ba3d716102c0fcc7af3f4960a2f199c5a4a6741f978d96fdad254922b790204

Observation 6fe91a3a-8e3a-4a4c-9803-22430536034f · inbound

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-17T04:19:00.848615Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-17T04:15:18.730245Z digest=sha256:aeb70c30e544cd67ccd0ad217d6e7ab74345f34e6bf6ab1665937c8ee8ec39e5

Observation c73080c8-c333-41d7-94bd-bea54d664cfa · inbound

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 208

Resolution
unresolved
no resolver link, observed 2026-08-03T08:42:10.727237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T08:42:10.727237Z digest=sha256:5c7e3092ee9eec89a08a1e8a9df6da3376c7f444c7a3f5ad77057e153ad8a9e5

Observation 33633291-b3c8-4815-8f7b-1db39fa99e55 · inbound

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors cites this paper.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-02T22:01:22.296024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T22:01:22.296024Z digest=sha256:bd1e06fe4fc808f771011b932ea8e0d40e78429adfcdb7f1461d6552eb830266

Observation 3915240b-d39b-4c0c-97f4-5097f27d6bd2 · inbound

Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-02T02:52:34.323473Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T02:52:34.323473Z digest=sha256:115d98802dceeb544c2cf5f75a6e418210f740265709687de5eaeb8c0937dce8

Observation 6c098446-e334-4594-8221-dd37cccb6e3e · inbound

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) cites this paper.

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors

Reference 109

Resolution
unresolved
no resolver link, observed 2026-07-31T11:32:43.680106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T11:32:43.680106Z digest=sha256:dc22431454e4daa602af6d484b806d44c75fb74fd5bcccb028909a1ed50fcce2