Paper Citation Record · LEDGER

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

As of 4 August 2026, this Paper Citation Record lists 100 of 151 outbound references and 25 inbound Pith citation observations for arXiv:2511.20757.

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

pith.paper-citation-record.v1
2511.20757 v2

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Outbound references

Observation bb2d54ab-8a19-4947-9332-bfdc97580e84 · outbound

This paper cites Chudaykin, M.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Chudaykin, M

Reference 1

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Observation b9beea03-0b66-48b3-a9dc-cd58db771ea7 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 2

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Observation b52cb65c-78b8-4635-9880-109195777272 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 3

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Observation 00401dad-f505-426f-86f0-79d2b35e340c · outbound

This paper cites Gu, et al., Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements, Nature Astron.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Gu, et al., Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements, Nature Astron

Reference 4

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Observation d005f7f1-e10b-4c63-9d1b-4423bfc2f020 · outbound

This paper cites DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics

Reference 5

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Observation 59ef16e0-09a3-45f9-8597-dc84f6ca266f · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Reference 6

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Observation 8482ee3f-2ea9-49a2-ba8e-dff132033a9b · outbound

This paper cites DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 7

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Observation d6e545a4-bb64-4709-8a01-4ef19fd20b56 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 8

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Observation bf6423a5-7bb3-43ed-b921-65a14c694ec9 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Pantheon+ Analysis: Cosmological Constraints

Reference 9

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Observation 570371b4-9225-49b6-8e1d-c1ea5b681df5 · outbound

This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 10

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Observation e31fdae8-5cf5-41e1-b060-b31df00895d6 · outbound

This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 11

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This paper cites The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration

Reference 12

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Observation 5cc40486-9ce3-41d4-ab74-db721179c583 · outbound

This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 13

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Observation 388d0b30-5940-4b5d-b352-036b8ab1f54c · outbound

This paper cites Baryon Acoustic Oscillations from a Different Angle.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Baryon Acoustic Oscillations from a Different Angle

Reference 14

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Observation 26a96e16-7a77-44fe-aafd-39e263113941 · outbound

This paper cites Interpreting DESI's evidence for evolving dark energy.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Interpreting DESI's evidence for evolving dark energy

Reference 15

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Observation 16662a56-9da0-4946-b8b4-db5f54254bcc · outbound

This paper cites Cortˆ es and A.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cortˆ es and A

Reference 16

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Observation 31a25709-3fa3-41b8-b3a6-473f4999a61f · outbound

This paper cites The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results

Reference 17

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Observation c5b0086f-6e9c-4ac8-8d41-1f4cb4ff975f · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering

Reference 18

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

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

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

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Observation 27f4851f-09aa-4860-a997-deba44c9b5bb · outbound

This paper cites Silva and R.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Silva and R

Reference 20

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Observation 887a24af-4fea-4d7f-8c57-a9017340bcd2 · outbound

This paper cites Consistency tests between SDSS and DESI BAO measurements.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Consistency tests between SDSS and DESI BAO measurements

Reference 21

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Observation 2fd47ff0-7698-4094-9d5a-21cf6d4931b9 · outbound

This paper cites Modified gravity interpretation of the evolving dark energy in light of DESI data.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Modified gravity interpretation of the evolving dark energy in light of DESI data

Reference 22

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Observation fe77b47d-c7b0-4fcd-a130-9425f15bf41a · outbound

This paper cites Chaudhary, S.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Chaudhary, S

Reference 23

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Observation 96c9f987-e3cd-46c1-9561-bd29c04c1243 · outbound

This paper cites Calibrating Dark Energy.

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

Reference 24

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Observation 958a4f8d-47d3-4d60-993b-4326439aeb89 · outbound

This paper cites Underdetermination of dark energy.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Underdetermination of dark energy

Reference 25

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Observation f4d4c930-5933-4600-bed8-832295d1a5a0 · outbound

This paper cites To CPL, or not to CPL? What we have not learned about the dark energy equation of state.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses To CPL, or not to CPL? What we have not learned about the dark energy equation of state

Reference 26

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Observation d960720e-ca59-49b6-b511-2e203f5a6581 · outbound

This paper cites The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae

Reference 27

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Observation e360e746-73e0-4ffb-8864-29b6bf627fa0 · outbound

This paper cites Robustness of dark energy phenomenology across different parameterizations.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Robustness of dark energy phenomenology across different parameterizations

Reference 28

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Observation a19b61f3-9fc4-47c3-8f98-eb3c142f290a · outbound

This paper cites Reconstructing the dark energy density in light of DESI BAO observations.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Reconstructing the dark energy density in light of DESI BAO observations

Reference 29

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Observation dfa907c4-a654-44f5-b4f1-7d76b483863d · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors

Reference 30

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Observation e37fa29c-e0ca-4218-89f7-19b8af00cf87 · outbound

This paper cites A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state

Reference 31

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Observation 845f240e-4e01-4225-a26e-6c27c224be01 · outbound

This paper cites W., Montefalcone , G., McDonough , E., & Freese , K.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses W., Montefalcone , G., McDonough , E., & Freese , K

Reference 32

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Observation bfde0209-9c1b-4eed-824d-cc999cd8b2ce · outbound

This paper cites Super-acceleration as Signature of Dark Sector Interaction.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Super-acceleration as Signature of Dark Sector Interaction

Reference 33

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Observation 73867ffe-e9f8-4d7f-a5f3-89bb67e16d0b · outbound

This paper cites Can we be tricked into thinking that w is less than -1?.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Can we be tricked into thinking that w is less than -1?

Reference 34

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Observation 26062ac5-6f8a-4bd5-8ef9-e9f2610a670e · outbound

This paper cites Axio-Chameleons: A Novel String-Friendly Multi-field Screening Mechanism.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Axio-Chameleons: A Novel String-Friendly Multi-field Screening Mechanism

Reference 35

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Observation 5d5b73d1-b4e3-422b-aaf9-b9c736db2273 · outbound

This paper cites Khoury, M.-X.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Khoury, M.-X

Reference 36

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Observation 8f779cad-d7e3-4725-bc2e-2bb41ad5cf85 · outbound

This paper cites New constraints on interacting dark energy from DESI DR2 BAO observations.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 37

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Observation f5463c5d-198f-4c3a-8401-23a27d03193f · outbound

This paper cites Scant evidence for thawing quintessence.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Scant evidence for thawing quintessence

Reference 38

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Observation dcfcac12-8c8f-42cf-afc0-0c735587b069 · outbound

This paper cites Matching current observational constraints with nonminimally coupled dark energy.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Matching current observational constraints with nonminimally coupled dark energy

Reference 39

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Observation 74c0a758-4946-4e2b-ac8e-35356835db71 · outbound

This paper cites From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI

Reference 40

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Observation f355e996-e681-4af0-bb44-844eb55f85a5 · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Assessing cosmological evidence for non-minimal coupling

Reference 41

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Observation a472f647-ea25-4a99-aa2b-befa13c0c2ae · outbound

This paper cites Monodromic Dark Energy and DESI.

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

Reference 42

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Observation 64fe59c7-f860-4686-91ff-65b84f9cd1a5 · outbound

This paper cites A Minimal Axio-dilaton Dark Sector.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses A Minimal Axio-dilaton Dark Sector

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.019441Z

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Observation 84fc4507-fe6e-40b4-8300-ca8988824f85 · outbound

This paper cites Dark Energy and the Symbiosis Between Micro-physics and Cosmology (Naturally).

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Dark Energy and the Symbiosis Between Micro-physics and Cosmology (Naturally)

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.089303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 61e672c7-1bd1-4308-acde-8480b61ae49e · outbound

This paper cites Evolving Dark Sector and the Dark Dimension Scenario.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Evolving Dark Sector and the Dark Dimension Scenario

Reference 45

Resolution: verified exact; arxiv_id, observed 2026-06-01T03:02:51.978329Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e6f94552-d64c-4bf4-b2bb-558b29b687f4 · outbound

This paper cites an unresolved cited work.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Unresolved cited work

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.940454Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation c18a3340-ab32-488a-9b62-2f8d54f52c0b · outbound

This paper cites It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.236422Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation c0ea0542-f541-49e8-9d64-8e7af104f96a · outbound

This paper cites Ishak et al., (2024).

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Ishak et al., (2024)

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.765669Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation db863f6f-1854-4150-9031-9648692f8acf · outbound

This paper cites Quintom cosmology and modified gravity after DESI 2024.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Quintom cosmology and modified gravity after DESI 2024

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.978088Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation af7741f5-90de-409a-8045-cc143942ef0f · outbound

This paper cites Chudaykin, M.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Chudaykin, M

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.060357Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f77b81bc-9f37-419b-936d-cbc737b10385 · outbound

This paper cites Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data

Reference 51

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.711771Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 7a248aaf-6962-42c3-accb-1f72a8cc9ceb · outbound

This paper cites No $\nu$s is Good News.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses No $\nu$s is Good News

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.824548Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9a25c2f3-873f-4111-815d-e6598aea8f67 · outbound

This paper cites The Cosmological Preference for Negative Neutrino Mass.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Cosmological Preference for Negative Neutrino Mass

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.747944Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9037015e-9996-434f-91bd-296a68fe49da · outbound

This paper cites Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

Reference 54

Resolution: metadata mismatch; local_arxiv, observed 2026-05-17T04:19:01.136728Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 1a24b158-c7ad-4ef1-8f42-47867232138d · outbound

This paper cites Graham, D.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Graham, D

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.133608Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b83c34e3-857d-43ee-84d1-cc9b7a75f95f · outbound

This paper cites Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 56

Resolution: metadata mismatch; arxiv_id, observed 2026-05-17T04:19:00.904434Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 590b578d-7301-4d1c-9b52-23b683338a79 · outbound

This paper cites Sailer, G.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Sailer, G

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.751838Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b9d83e1d-08c7-400d-be7c-dac5f0853156 · outbound

This paper cites Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.819282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f64332d7-8229-492e-a584-acad7d51a00c · outbound

This paper cites What will it take to measure individual neutrino mass states using cosmology?.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses What will it take to measure individual neutrino mass states using cosmology?

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.890574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 8ee37519-bf29-459e-9255-0a66834ad451 · outbound

This paper cites Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-$\alpha$ and Planck full-survey data

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.815215Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d2552992-490f-406a-82ce-8fa7621b948a · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data

Reference 61

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.724137Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e05d3b95-fa8f-4dc7-9078-947235e971ed · outbound

This paper cites Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.249402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 87ee421d-3046-468a-8a2e-88f192ab8d8c · outbound

This paper cites Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.196975Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 06452032-436a-4fd5-ac27-65cb83ff4a77 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.715496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ee82d3c4-b042-45ed-8618-f86804fb77e0 · 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.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.771267Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation dd0b74a9-ce3d-4d03-af0b-ffcc1fd8735f · outbound

This paper cites Data Release 1 of the Dark Energy Spectroscopic Instrument.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Data Release 1 of the Dark Energy Spectroscopic Instrument

Reference 66

Resolution: metadata mismatch; local_arxiv, observed 2026-05-17T04:19:00.944541Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 509f5fc4-8f89-40d1-91ed-56e4420c5693 · outbound

This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.211038Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 5f701c76-221f-40f7-aae9-6e0222aac8ba · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological Parameters from the BOSS Galaxy Power Spectrum

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.203185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 3722a04e-47d4-41d7-91b0-51a7606d5aec · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.782876Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 5522482c-bcbc-4008-9914-116bfaabcc3b · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO

Reference 71

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.874539Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 980a4528-f71d-43e6-ab12-6dde5c0e53bf · outbound

This paper cites Perturbation theory, effective field theory, and oscillations in the power spectrum.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Perturbation theory, effective field theory, and oscillations in the power spectrum

Reference 72

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.160062Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9b950e65-ee6d-4dab-a9b5-f56125ba354a · outbound

This paper cites On the Renormalization of the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses On the Renormalization of the Effective Field Theory of Large Scale Structures

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.991404Z

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Observation 439209ab-236e-418d-a1cb-3bd179ce5569 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Effective Field Theory of Cosmological Large Scale Structures

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.882193Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f34a71d4-113a-4a38-af64-cab3a29bb4d2 · outbound

This paper cites On the Velocity in the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses On the Velocity in the Effective Field Theory of Large Scale Structures

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.788704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation f501866b-ff12-433a-85a2-37afef26495c · outbound

This paper cites The Lagrangian-space Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Lagrangian-space Effective Field Theory of Large Scale Structures

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.924223Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b32c6ed0-9380-4acc-9d6a-d38c9ac9ac35 · outbound

This paper cites A Lagrangian effective field theory.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses A Lagrangian effective field theory

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.239732Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation bfd58abf-10d8-4dc7-886e-fbc1e9d3a23b · outbound

This paper cites The IR-resummed Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The IR-resummed Effective Field Theory of Large Scale Structures

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:00.982424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9da27c08-c6f0-4bba-8786-12762d39c807 · outbound

This paper cites Redshift Space Distortions in the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Redshift Space Distortions in the Effective Field Theory of Large Scale Structures

Reference 79

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.179387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation b01c05ac-74ef-4806-a4d6-e625d992d051 · outbound

This paper cites Bias in the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Bias in the Effective Field Theory of Large Scale Structures

Reference 80

Resolution: metadata mismatch; local_arxiv, observed 2026-05-17T04:19:01.182954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 6e299ae5-547e-4503-bd96-1c1128532ce0 · outbound

This paper cites On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.166644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 3affbdb4-4206-457c-8d52-f9270a4bf8ae · outbound

This paper cites The Effective Field Theory of Large-Scale Structure in the presence of Massive Neutrinos.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The Effective Field Theory of Large-Scale Structure in the presence of Massive Neutrinos

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.153725Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 97506592-1e09-4a97-80b3-62cc1a1111e0 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological Non-Linearities as an Effective Fluid

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.156757Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9ac74737-6d1d-4821-8a05-8f40deb0249d · outbound

This paper cites Renormalized Halo Bias.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Renormalized Halo Bias

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.186771Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 004d4e54-3e7e-440c-8375-4bb0495df981 · outbound

This paper cites Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity

Reference 85

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.008400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 3bec285c-8e07-4455-a55b-4d7ca2328d55 · outbound

This paper cites Redshift-Space Distortions in Lagrangian Perturbation Theory.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Redshift-Space Distortions in Lagrangian Perturbation Theory

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.126792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 94e718be-f6ff-4750-9ac4-dee136b42d7a · outbound

This paper cites Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.143888Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation ef7c2cbf-1443-46e6-a7c8-3580291f4cf7 · outbound

This paper cites Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation

Reference 88

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.147180Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation bdb185cb-b620-4b8f-b0ea-525601010287 · outbound

This paper cites Infrared Resummation for Biased Tracers in Redshift Space.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Infrared Resummation for Biased Tracers in Redshift Space

Reference 89

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.246558Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 56d5dde2-a209-4e0f-95cd-742fb4f79997 · outbound

This paper cites Clustering of dark matter tracers: renormalizing the bias parameters.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Clustering of dark matter tracers: renormalizing the bias parameters

Reference 90

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.075743Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 4c068e5c-86c9-4596-8892-2944acbe4095 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS

Reference 91

Resolution: verified exact; local_arxiv, observed 2026-05-17T04:19:01.094524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d5bb79e7-3e3d-416c-b84d-701dfe0c23bd · outbound

This paper cites Effective Field Theory for Large Scale Structure.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Effective Field Theory for Large Scale Structure

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.108477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 46895d4f-52a3-432a-8d09-ec07ca3f7170 · outbound

This paper cites Cosmological constraints from the full-shape galaxy power spectrum in SDSS-III BOSS using the BACCO hybrid Lagrangian bias emulator.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological constraints from the full-shape galaxy power spectrum in SDSS-III BOSS using the BACCO hybrid Lagrangian bias emulator

Reference 93

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.072390Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d3a4193d-fe0b-4476-820b-d25e14b76022 · outbound

This paper cites The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.050153Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 335e0153-36c0-4430-b6b1-a4b2a91a1ae0 · outbound

This paper cites Limits on primordial non-Gaussianities from BOSS galaxy-clustering data.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Limits on primordial non-Gaussianities from BOSS galaxy-clustering data

Reference 95

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.069285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 98dc5833-ec84-40ba-ab6b-0cc0887c0e98 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Full-shape analysis with simulation-based priors: constraints on single field inflation from BOSS

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.063225Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e75303d0-d3aa-4a02-b1af-e1febb3e707e · outbound

This paper cites Cosmological constraints without fingers of God.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological constraints without fingers of God

Reference 97

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.053553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 11c8732a-268c-459a-ad3f-0d2377e68f59 · outbound

This paper cites Cosmological constraints from the power spectrum of eBOSS emission line galaxies.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological constraints from the power spectrum of eBOSS emission line galaxies

Reference 98

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.218135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d3e1ed2f-9a83-4f44-9267-c3bf19a7c6a0 · outbound

This paper cites Cosmological constraints from the power spectrum of eBOSS quasars.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmological constraints from the power spectrum of eBOSS quasars

Reference 99

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.260059Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 0bc5aeea-e095-4b3a-96b0-a664bd3a16b9 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Precision analysis of the redshift-space galaxy bispectrum

Reference 100

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.056989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 637cc6b5-bb2f-4650-bc6f-57015bbfafd0 · outbound

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

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:01.066241Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Pith citing papers

Observation 4a64253d-446a-4051-8e20-4d8061c89309 · inbound

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity cites this paper.

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-05-16T18:01:08.941066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 8d5ca3bc-cb7a-4653-9ce2-a74c155a2ae1 · 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 Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-03T08:41:49.515835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38ae72ce-97d9-45d5-8fee-70c7b07d2a16 · inbound

An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics cites this paper.

An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T23:55:18.157672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5f0e17d-5912-41f6-942d-f76a9a0cfbab · inbound

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

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T22:01:21.105198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d431921-176c-4b19-b98b-6298f2d0e3fa · inbound

Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.

Measuring neutrino mass in light of ACT DR6 and DESI DR2 Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 105

Resolution: verified exact; local_arxiv, observed 2026-05-15T13:15:50.450159Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 48ef6489-9cd1-42f4-a2f1-f4430d992dc7 · inbound

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses cites this paper.

FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-05-11T06:25:59.326039Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 45695392-e8b8-4e87-b370-192bcf061f6f · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-05-12T00:21:26.530612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d81ca8c2-842c-4d2c-8ba7-c0595acc0b39 · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-05-11T22:01:13.913891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 5ce68840-cc7b-4a05-abd4-8404d5fd21af · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-05-11T17:56:05.749335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 50fa79db-82eb-4960-9029-42476f7bbd88 · inbound

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges cites this paper.

Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-06-30T23:25:07.670453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 2d5d73a5-4c84-465a-9302-5f69a9c0b68c · inbound

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis cites this paper.

Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-05-14T17:42:32.656104Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 4db769b0-6c46-466f-b0ab-7695802889f2 · inbound

Probing late-time deviations from $\Lambda$CDM with a quadratic dark energy expansion cites this paper.

Probing late-time deviations from $\Lambda$CDM with a quadratic dark energy expansion Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-05-21T02:44:25.288824Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 06329db8-6004-438f-aab5-c71250c64c25 · inbound

Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum cites this paper.

Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 8

Resolution: metadata mismatch; local_arxiv, observed 2026-05-21T03:13:56.152913Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 0ca601e2-c23e-4a10-a9ff-6504234a59c0 · inbound

Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering cites this paper.

Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 39

Resolution: verified exact; local_arxiv, observed 2026-06-29T10:43:18.424796Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation a02293f8-38bf-4af6-9a29-76bb3da8ae71 · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 124

Resolution: verified exact; local_arxiv, observed 2026-07-02T10:46:53.134752Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation c9ae62f9-a749-4e06-8974-0b99d946fc17 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-07-02T14:57:03.991999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 41b26803-5558-4f6d-8573-df22bb7b9391 · inbound

Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit? cites this paper.

Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit? Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-07-04T07:09:38.644388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 047f1b0d-618d-4752-b7fb-eb1e35f39a25 · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-02T10:41:32.026345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 79e04f10-d65a-4cc3-88c9-628f7f6930ae · inbound

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics cites this paper.

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-07-01T12:25:44.401083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 08e0a3de-76d5-4260-9a40-777cba5845af · inbound

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-07-01T01:15:13.326950Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 0592e622-a502-472c-a9f6-5c1d44e41bff · inbound

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T09:29:12.739338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f99bb77e-54da-42d3-ae3e-026f7dc33732 · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 156

Resolution: verified exact; local_arxiv, observed 2026-07-02T06:16:43.346673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation a19fd6de-8477-438e-b341-5efb0e771320 · inbound

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering cites this paper.

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-02T00:29:39.671866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cdee1380-9ff7-4639-b0e3-d4b2d1194584 · inbound

Measuring Cosmic Neutrino Masses Independently of Dark Energy cites this paper.

Measuring Cosmic Neutrino Masses Independently of Dark Energy Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 63

Resolution: unresolved; no resolver link, observed 2026-07-31T06:22:31.598679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9243c3e8-8ed4-4842-b8fa-687155214ffd · inbound

Inflation, Open Universes, and Dark Energy cites this paper.

Inflation, Open Universes, and Dark Energy Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses

Reference 59

Resolution: unresolved; no resolver link, observed 2026-07-31T07:10:45.719377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.