Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-17T06:00:49.044220Z
Paper Citation Record · LEDGER
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
As of 4 August 2026, this Paper Citation Record lists 100 of 195 outbound references and 59 inbound Pith citation observations for arXiv:2411.12021.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T11:34:09.245584Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T18:27:31.628688Z
Reference resolution
100 of 195 outbound references displayed
- verified exact89
- verified fuzzy11
- unresolved0
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- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 06fe5c3a-28d0-422e-9632-71ca605ad543 · outbound
This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.281618Z
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 739d7087-9215-4162-b44c-b0dc945202b7 · outbound
This paper cites Huchra, M.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Huchra, M
Reference 2
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.056890Z
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 c0926b26-37f1-4fd8-b537-a6e30fdf585a · outbound
This paper cites Davis, G.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Davis, G
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.060236Z
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 659220e5-643a-4b35-a81b-bb5fa3dfbdd8 · outbound
This paper cites Efstathiou, W.J.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Efstathiou, W.J
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.063437Z
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 99b761e7-4a6b-4518-b90b-4b372f9b1b19 · outbound
This paper cites The 2dF Galaxy Redshift Survey: Spectra and redshifts.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The 2dF Galaxy Redshift Survey: Spectra and redshifts
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.288066Z
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 68fb28bd-9650-4ca3-949d-e515b582c0f2 · outbound
This paper cites The 2.5 m Telescope of the Sloan Digital Sky Survey.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The 2.5 m Telescope of the Sloan Digital Sky Survey
Reference 6
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.293657Z
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 079a9cb5-cb0e-4c78-9d65-8bb5e20c8788 · outbound
This paper cites The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.299053Z
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 836ed1a3-0ef4-4ec9-90ac-1be56743587e · outbound
This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
Reference 8
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.304111Z
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 851877c7-4531-496c-aac0-c82cf30caa1a · outbound
This paper cites The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
Reference 9
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.310324Z
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 c9b8a040-ccc1-4cbd-a1f9-023e19ea43e9 · outbound
This paper cites A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
Reference 10
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.316018Z
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 07c26054-7e93-428c-af71-aa21997df34e · outbound
This paper cites A test of the nature of cosmic acceleration using galaxy redshift distortions.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A test of the nature of cosmic acceleration using galaxy redshift distortions
Reference 11
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.321499Z
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 1c2748fa-d648-4ad0-b973-ba02c5711584 · outbound
This paper cites The DESI Experiment, a whitepaper for Snowmass 2013.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The DESI Experiment, a whitepaper for Snowmass 2013
Reference 12
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.326897Z
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 1b3de6ca-002d-4adf-bf85-3541412eb310 · outbound
This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The DESI Experiment Part I: Science,Targeting, and Survey Design
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.332466Z
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 5b0c30df-b81b-42a5-933d-6ad090555b2c · outbound
This paper cites The DESI Experiment Part II: Instrument Design.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The DESI Experiment Part II: Instrument Design
Reference 14
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.337456Z
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 1957c6df-cd6e-4dca-bc5a-37c0e96ce909 · outbound
This paper cites Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
Reference 15
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T07:10:47.812900Z
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 2f74992c-5d49-467f-9c86-4710612ce00a · outbound
This paper cites The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI).
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)
Reference 16
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.348840Z
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 e73ca3f5-a04d-40ca-a4cd-81ca39ccb49f · outbound
This paper cites The Optical Corrector for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Optical Corrector for the Dark Energy Spectroscopic Instrument
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.354546Z
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 cb748a2c-7c35-4607-b00a-7079a45c453f · outbound
This paper cites The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.361201Z
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 d5b1976e-5765-45a8-a669-d91354e65768 · outbound
This paper cites Survey Operations for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Survey Operations for the Dark Energy Spectroscopic Instrument
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.367339Z
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 19f3aab8-1320-4c3e-a277-7e529e57b0ed · outbound
This paper cites Overview of the DESI Milky Way Survey.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Overview of the DESI Milky Way Survey
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.373469Z
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 e4ec84fa-a463-4ea0-bb39-134b4a7e78be · outbound
This paper cites Peebles and J.T.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Peebles and J.T
Reference 21
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.116928Z
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 a7cd99cb-13be-4852-88de-1f2a87f4f706 · outbound
This paper cites Sunyaev and Y.B.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Sunyaev and Y.B
Reference 22
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.066865Z
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 e9add908-811f-49ba-9b6c-e27ac8d357cf · outbound
This paper cites Bond and G.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Bond and G
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.070034Z
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 79185e6a-89d2-4823-90a0-44528e1c8b86 · outbound
This paper cites A Sound Horizon-Free Measurement of $H_0$ in DESI 2024.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A Sound Horizon-Free Measurement of $H_0$ in DESI 2024
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.379385Z
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 7c9e9ca8-56f5-4b4f-a8d6-d019fbf41015 · outbound
This paper cites Alcock and B.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Alcock and B
Reference 25
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.076260Z
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 83c97103-4818-4655-8750-62667efc335a · outbound
This paper cites Kaiser,Clustering in real space and in redshift space, MNRAS227(1987) 1.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Kaiser,Clustering in real space and in redshift space, MNRAS227(1987) 1
Reference 26
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.079308Z
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 755fba1a-a39b-4197-90bd-df0297825fab · outbound
This paper cites Linear Redshift Distortions: A Review.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Linear Redshift Distortions: A Review
Reference 27
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.385334Z
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 8112f1d1-5a2d-4e4e-9d49-ee582a02e517 · outbound
This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.391352Z
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 ae69f134-9dba-46d3-b5a0-269383a23ed5 · outbound
This paper cites Novell-Masot, H.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Novell-Masot, H
Reference 29
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.088764Z
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 409408a4-7d6c-4e7c-98e0-e48e3b0efff3 · outbound
This paper cites Large-Scale Galaxy Bias.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Large-Scale Galaxy Bias
Reference 30
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.397022Z
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 1c6e2048-7035-4ea8-8e53-2dc78d82fba2 · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.402148Z
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 1b86f16e-7fb6-4b8c-9abd-79923e0fb1ae · outbound
This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.408433Z
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 ce40b3f3-a983-4e9c-975e-a39fbbbbf43d · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.414730Z
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 3f300511-70e1-4a38-b920-2c43d27b5ddd · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.421189Z
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 647dd313-00ab-41f8-85b0-4d38ffd05e58 · outbound
This paper cites RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
Reference 35
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.427867Z
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 98d2543d-b539-4d2f-970c-6d4ef9705db6 · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
Reference 36
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.434343Z
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 5a5933eb-6ca3-45e0-aa7a-3b1a1c5222c4 · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
Reference 37
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.440934Z
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 3c6e44d9-3ea4-4a9d-99d6-d6f690541f40 · outbound
This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.447937Z
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 ca491298-94c8-4779-8518-2d9c4012a0d7 · outbound
This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
Reference 39
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.454696Z
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 3e134ef1-726d-469b-8bbf-e400c475ab70 · outbound
This paper cites Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.460871Z
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 8f6c2333-769c-4b78-8a1d-d32f13cc60d9 · outbound
This paper cites Cosmological Non-Linearities as an Effective Fluid.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Cosmological Non-Linearities as an Effective Fluid
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.466685Z
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 a4ec9a0f-0748-48a3-914f-cbca10b42468 · outbound
This paper cites The Effective Field Theory of Cosmological Large Scale Structures.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Effective Field Theory of Cosmological Large Scale Structures
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.472760Z
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 030af981-c2d9-4513-92ee-f708acfc56cc · outbound
This paper cites A Lagrangian effective field theory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A Lagrangian effective field theory
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.478717Z
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 0793c4bd-5ac6-47d5-a6f7-ac4ea98f5595 · outbound
This paper cites Redshift Space Distortions in the Effective Field Theory of Large Scale Structures.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
Reference 44
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.484407Z
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 6d213974-e6ec-4840-b756-85156164eca0 · outbound
This paper cites Bias in the Effective Field Theory of Large Scale Structures.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Bias in the Effective Field Theory of Large Scale Structures
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.489647Z
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 4fb0d9a8-2ada-4c7b-bb55-dff657b2fd08 · outbound
This paper cites Biased Tracers and Time Evolution.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Biased Tracers and Time Evolution
Reference 46
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.494736Z
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 b23a8518-bcff-48ee-80be-70d2f6a5f7ef · outbound
This paper cites Biased Tracers in Redshift Space in the EFT of Large-Scale Structure.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Biased Tracers in Redshift Space in the EFT of Large-Scale Structure
Reference 47
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.499229Z
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 f71107a5-b293-4db7-834b-24e15172a249 · outbound
This paper cites Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory
Reference 48
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.504190Z
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 3548bc77-4e00-4d9c-8d80-5ea4393f39bc · outbound
This paper cites Perturbative description of bias tracers using consistency relations of LSS.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Perturbative description of bias tracers using consistency relations of LSS
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.509249Z
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 aea514c7-a210-4519-80d3-5c08ef5c4ba4 · outbound
This paper cites Redshift-Space Distortions in Lagrangian Perturbation Theory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Redshift-Space Distortions in Lagrangian Perturbation Theory
Reference 50
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.514471Z
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 8ca40d03-8dd8-4b18-975b-516c7a24eb28 · outbound
This paper cites Limits on $w$CDM from the EFTofLSS with the PyBird code.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Limits on $w$CDM from the EFTofLSS with the PyBird code
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.519173Z
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 f64b6345-6206-4b97-a74f-8bb3f6ce5d71 · outbound
This paper cites On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.524632Z
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 1275f6c4-cf05-43f3-b331-b7be869dc734 · outbound
This paper cites Nonlinear Evolution of Baryon Acoustic Oscillations.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Nonlinear Evolution of Baryon Acoustic Oscillations
Reference 53
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.529963Z
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 deec167f-941c-41b1-be0f-e405a84f273c · outbound
This paper cites How does non-linear dynamics affect the baryon acoustic oscillation?.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars How does non-linear dynamics affect the baryon acoustic oscillation?
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.535189Z
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 23d1550f-9721-47fc-aaee-bea43cd3cb53 · outbound
This paper cites Equivalence Principle and the Baryon Acoustic Peak.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Equivalence Principle and the Baryon Acoustic Peak
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.539906Z
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 6e80f9d5-ade2-4c3e-9546-506163591fa6 · outbound
This paper cites The IR-resummed Effective Field Theory of Large Scale Structures.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The IR-resummed Effective Field Theory of Large Scale Structures
Reference 56
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.544829Z
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 ddee5859-f7c5-4554-82a9-dbf92e09c515 · outbound
This paper cites Perturbation theory, effective field theory, and oscillations in the power spectrum.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Perturbation theory, effective field theory, and oscillations in the power spectrum
Reference 57
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.549457Z
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 cca02226-8f1b-42d0-9c8d-6923282208d9 · outbound
This paper cites Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.554778Z
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 2c04d298-d4aa-4473-b6b0-152a392a0637 · outbound
This paper cites Infrared Resummation for Biased Tracers in Redshift Space.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Infrared Resummation for Biased Tracers in Redshift Space
Reference 59
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.559521Z
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 c5e8847a-3e48-47e7-ba8a-035bfeb518e5 · outbound
This paper cites Cosmological Parameters from the BOSS Galaxy Power Spectrum.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Cosmological Parameters from the BOSS Galaxy Power Spectrum
Reference 60
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.564731Z
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 ba33f96c-afee-453f-a2fb-cb08122304c9 · outbound
This paper cites The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
Reference 61
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.569731Z
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 6c8b22af-2185-4142-86da-442b967c5f03 · outbound
This paper cites Modeling features in the redshift-space halo power spectrum with perturbation theory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Modeling features in the redshift-space halo power spectrum with perturbation theory
Reference 62
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.574646Z
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 0df14dbe-45e4-4c46-9bfa-677e55d88d3a · outbound
This paper cites Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.579700Z
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 556ce96c-4e86-4daa-86f5-484f744432e1 · outbound
This paper cites Consistency of effective field theory analyses of the BOSS power spectrum.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Consistency of effective field theory analyses of the BOSS power spectrum
Reference 64
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.583867Z
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 9a282fbb-5efd-4eef-aecf-d3607e88a00b · outbound
This paper cites Noriega and A.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Noriega and A
Reference 65
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.098286Z
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 27940d73-c4d6-4e60-8935-e3d8baffad3f · outbound
This paper cites A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.588867Z
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 809b9706-ef32-40bb-beb9-68aa8f22c991 · outbound
This paper cites Blind Observers of the Sky.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Blind Observers of the Sky
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.593242Z
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 7ab3d282-cbbe-45f1-a864-e62e098c8f59 · outbound
This paper cites Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.597730Z
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 b7f2c4af-b477-4683-9c66-a78dac5201eb · outbound
This paper cites Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.602156Z
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 c6f31c60-68c2-4496-8489-0c510a58a9ea · outbound
This paper cites A comparison of template vs. direct model fitting for redshift-space distortions in BOSS.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
Reference 70
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.606744Z
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 c15c0a74-08e9-475a-b9ab-f48db6d7a6f2 · outbound
This paper cites An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond
Reference 71
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.610880Z
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 562ffc69-3215-457d-a799-5ca9c43fda94 · outbound
This paper cites Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond
Reference 72
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.615290Z
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 d4fdb45f-364a-4e8c-b1cf-29cb2ae7af91 · outbound
This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:34:55.175109Z
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 a2b719ff-d28d-4295-a4ee-f10998f68ebf · outbound
This paper cites DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T07:30:58.099479Z
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 eb86e349-1878-4ead-912b-6362d3501758 · outbound
This paper cites Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples
Reference 75
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.628649Z
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 e62f749f-a401-46b7-be6c-85b19e0bbbca · outbound
This paper cites Data Release 1 of the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Data Release 1 of the Dark Energy Spectroscopic Instrument
Reference 76
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.633404Z
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 28b761ca-4cf1-4209-bd9a-07c4b6d143d3 · outbound
This paper cites Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument
Reference 77
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.638132Z
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 221bdef1-4b63-4f4e-926c-fd8d9f84f380 · outbound
This paper cites The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Target-selection Pipeline for the Dark Energy Spectroscopic Instrument
Reference 78
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.642914Z
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 cc79f8ab-e374-4574-8074-196d3b1de5fb · outbound
This paper cites DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
Reference 79
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.647153Z
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 183d6b85-b3eb-4cc8-8374-69b0d833720e · outbound
This paper cites Target Selection and Validation of DESI Luminous Red Galaxies.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Target Selection and Validation of DESI Luminous Red Galaxies
Reference 80
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.652005Z
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 e21f54fa-677f-4c82-afcd-c0ab84d18f4b · outbound
This paper cites Target Selection and Validation of DESI Emission Line Galaxies.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Target Selection and Validation of DESI Emission Line Galaxies
Reference 81
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.656766Z
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 ef2e5dc8-7b64-4a94-b036-37d9c1cc7798 · outbound
This paper cites Target Selection and Validation of DESI Quasars.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Target Selection and Validation of DESI Quasars
Reference 82
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.661400Z
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 07cdd1b6-252e-4f3d-a9b8-7b18de7a83cd · outbound
This paper cites DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
Reference 83
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.665884Z
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 5e1faea6-1c8b-4818-b3a9-6898e2bdaf2d · outbound
This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
Reference 84
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.670739Z
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 dd47840d-e383-48b6-85b2-4cbd7715999f · outbound
This paper cites Zhao et al.,Impact and mitigation of imaging systematics for DESI 2024 full shape analysis,in preparation(2024).
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Zhao et al.,Impact and mitigation of imaging systematics for DESI 2024 full shape analysis,in preparation(2024)
Reference 85
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-17T06:00:50.095282Z
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 8fa9bbdb-fbbf-4c7d-8878-b5bb59963b68 · outbound
This paper cites Overview of the DESI Legacy Imaging Surveys.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Overview of the DESI Legacy Imaging Surveys
Reference 86
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.675066Z
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 d7af1fe8-6936-4d33-9302-f250ab0fe9cc · outbound
This paper cites Mitigating Imaging Systematics for DESI 2024 Emission Line Galaxies and Beyond.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Mitigating Imaging Systematics for DESI 2024 Emission Line Galaxies and Beyond
Reference 87
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.679920Z
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 7a3c737e-f225-4b9d-b7fd-3df3e7821a62 · outbound
This paper cites Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024
Reference 88
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.684790Z
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 75f91ed1-da60-466d-bc87-6196c3ff02c1 · outbound
This paper cites ELG Spectroscopic Systematics Analysis of the DESI Data Release 1.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
Reference 89
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.689164Z
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 d2411412-7a69-4a3a-92f9-423bad8d1c0a · outbound
This paper cites Impact and mitigation of spectroscopic systematics on DESI DR1 clustering measurements.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Impact and mitigation of spectroscopic systematics on DESI DR1 clustering measurements
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.694281Z
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 381f008b-05c5-4c27-86c2-f235ecbacb53 · outbound
This paper cites Power Spectrum Analysis of Three-Dimensional Redshift Surveys.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Power Spectrum Analysis of Three-Dimensional Redshift Surveys
Reference 91
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.698481Z
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 4bcd3d35-2402-4548-b6fa-e29819a28039 · outbound
This paper cites Catalog-level blinding on the bispectrum for DESI-like galaxy surveys.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
Reference 92
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.703726Z
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 9a5d8fd1-4549-45f1-8342-fe75340e1f4e · outbound
This paper cites Andrade, J.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Andrade, J
Reference 93
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.708499Z
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 0f40fee4-7258-41de-b114-c7d75c05e30f · outbound
This paper cites The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.713545Z
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 426b36a3-7f09-4844-87af-c4d8d8823a20 · outbound
This paper cites The effect of primordial non-Gaussianity on halo bias.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The effect of primordial non-Gaussianity on halo bias
Reference 95
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.719089Z
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 f78602fe-0685-4181-9f70-42d62cf2953a · outbound
This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
Reference 96
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.724697Z
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 4cc7c855-d147-4eb2-8c91-7c5f990861a8 · outbound
This paper cites Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide
Reference 97
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.730478Z
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 8cd3e6f8-3f86-42a0-ad79-7e41e34e87e5 · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Planck 2018 results. VI. Cosmological parameters
Reference 98
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T06:00:49.735308Z
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 243b5c8e-a39e-426b-8f6b-e11dd0ff7f06 · outbound
This paper cites Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis
Reference 99
- Resolution
- verified exact
- arxiv_id, observed 2026-06-10T02:11:39.618266Z
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 b7ee57d5-a1c8-4def-be2c-6964e3c181d7 · outbound
This paper cites A comparison between ShapeFit compression and Full-Modelling method with PyBird for DESI 2024 and beyond,.
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars A comparison between ShapeFit compression and Full-Modelling method with PyBird for DESI 2024 and beyond,
Reference 100
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:49.744915Z
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 cb3785c3-5364-48ab-b798-cd9fb1f2fb54 · inbound
DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements cites this paper.
DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 1
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 c8022791-5342-4078-bef2-a5a048a8638b · inbound
DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints cites this paper.
DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 46
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 c3046403-73cb-432d-8c21-5bd32d107934 · inbound
DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest cites this paper.
DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 58
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 2ad8f9d2-486e-48e2-bb87-d1cb983bad8d · inbound
Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.
Extended Dark Energy analysis using DESI DR2 BAO measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 43
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 bf1013fe-9a8d-4c02-a96e-dbd4ad392872 · inbound
Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape cites this paper.
Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 98
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 f98d4bc0-c3e8-4121-9218-1d10cda69cd2 · inbound
Combined tracer analysis for DESI 2024 BAO cites this paper.
Combined tracer analysis for DESI 2024 BAO DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T00:31:56.868165Z
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 7ea38dcf-0fb7-4098-997c-ee51ef749b02 · inbound
Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias cites this paper.
Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 10
- Resolution
- verified exact
- local_arxiv, observed 2026-05-18T15:56:34.421623Z
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 2ce2584c-7dd3-4bd4-afbc-6bc2a6693e90 · inbound
Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.
Crosschecking Cosmic Distances from DESI BAO and DES SNe DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-05-18T10:32:33.865468Z
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 8f09b10b-8830-4311-8630-6f60c91c3572 · inbound
Crosschecking Cosmic Distances from DESI BAO and DES SNe cites this paper.
Crosschecking Cosmic Distances from DESI BAO and DES SNe DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:34:09.245584Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7ba06022-2e7d-4a17-ae09-e20a15e97e28 · inbound
$H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1 cites this paper.
$H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-05-18T05:35:56.154527Z
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 de117bc6-5804-46cf-87f6-37af0ceb9750 · inbound
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements cites this paper.
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 50
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 d3f63796-403a-4b7a-8ebb-8721fa8ba4ac · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 153
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 71239dd3-a5d6-4a36-a8a0-18c92663e63d · inbound
Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology cites this paper.
Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 d9acc81b-1af7-452b-8569-1ac445900e45 · inbound
The Linear Point Standard Ruler with DESI DR1 and DR2 Data cites this paper.
The Linear Point Standard Ruler with DESI DR1 and DR2 Data DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 121
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T06:27:27.324247Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4493ca4c-31c9-40ea-b0e1-832d7bd654f2 · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 76
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T08:41:56.194579Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1e25b27-04b4-47a0-9eed-47f4ef897a2d · inbound
Large-scale Modeling of the Observed Power Spectrum Multipoles cites this paper.
Large-scale Modeling of the Observed Power Spectrum Multipoles DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T06:23:21.605051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9edffbc-a739-46fb-9ce1-9f6603731bfa · inbound
Early results in the search for extreme coronal line emitters with the Dark Energy Spectroscopic Instrument cites this paper.
Early results in the search for extreme coronal line emitters with the Dark Energy Spectroscopic Instrument DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T07:12:43.127873Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e35991be-2d87-4535-8a95-edbf226900bd · inbound
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum cites this paper.
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 137
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 60c476b7-18da-47f0-bb04-d2548877a6fc · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T23:55:20.447600Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0684b340-0718-4c48-8938-afaa0f082b37 · inbound
The BAO scale -- how standard is the standard ruler? cites this paper.
The BAO scale -- how standard is the standard ruler? DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T19:10:18.671031Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9e228772-95de-4f9b-ba2d-33078e8fd7b4 · inbound
DESI DR2 Baryon Acoustic Oscillations from the Lyman Alpha Forest Multipoles cites this paper.
DESI DR2 Baryon Acoustic Oscillations from the Lyman Alpha Forest Multipoles DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T18:54:28.945922Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7e0ec1c9-ff14-4917-b126-b67a4b1e3094 · inbound
A unified harmonic framework for dark siren cosmology cites this paper.
A unified harmonic framework for dark siren cosmology DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 32c9af56-5579-4193-8738-ebbcf497d025 · inbound
Local primordial non-Gaussianity using cross-correlations of DESI tracers cites this paper.
Local primordial non-Gaussianity using cross-correlations of DESI tracers DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 210638d1-bf53-4dc1-a8fb-a60140f0e43f · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 121
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 3f066c15-d442-48b5-a6f4-6bdbda192f82 · inbound
Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope cites this paper.
Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 94
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 846d30c1-6aeb-4554-aed4-ec9101956027 · inbound
Fast radio burst dispersion is an unbiased tracer of matter on large scales cites this paper.
Fast radio burst dispersion is an unbiased tracer of matter on large scales DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 9edee74a-154d-4a15-a2c8-472c9fdb80aa · inbound
Testing Scale-Dependent Modified Gravity with DESI DR1 cites this paper.
Testing Scale-Dependent Modified Gravity with DESI DR1 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 10
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 2cdb4b81-eb9e-46a2-bf3c-039964d2138e · inbound
Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas cites this paper.
Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 192
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 a7446845-b1df-44fb-a4e4-bd2c158b04a1 · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T23:25:07.673459Z
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 95d2d405-1e62-447b-b03e-fcef258df8f9 · inbound
Late-time reconstruction of non-minimally coupled gravity with a smoothness prior cites this paper.
Late-time reconstruction of non-minimally coupled gravity with a smoothness prior DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 fbd87d3f-4112-4d96-901f-6013525d805a · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 8
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T06:00:50.118019Z
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 8860a362-6e0f-4422-8d68-d6c7cd34e681 · inbound
Recoupled Dark Radiation reconciling CMB and DESI BAO measurements cites this paper.
Recoupled Dark Radiation reconciling CMB and DESI BAO measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 79
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T09:03:09.955639Z
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 ada363ca-f3f6-48e6-afc7-15db3a739b44 · inbound
Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes cites this paper.
Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 73
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T14:34:45.458453Z
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 324598e6-a233-4700-b465-6302728ef095 · inbound
The sound of dynamical dark energy and modified gravity cites this paper.
The sound of dynamical dark energy and modified gravity DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 14
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T20:52:37.537752Z
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 339dd10f-b359-4f18-beb7-e0d6859a0dec · inbound
Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity cites this paper.
Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T06:47:43.757847Z
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 8532b1c4-0ecd-445b-ae68-31e0fe97c9ca · inbound
Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity cites this paper.
Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T11:57:29.451802Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 173634bc-39be-4fb4-b176-18a53fcc4819 · inbound
Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints cites this paper.
Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 5
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-27T11:10:52.003901Z
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 8db5fb5c-396a-4e18-8777-5d3b02d7cb90 · inbound
Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations cites this paper.
Impact of inhomogeneous curvature on growth rate measurements from magnitude fluctuations DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 92
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-26T23:00:12.102717Z
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 805e7b59-3ca1-402e-96a0-6db0fc357ff1 · inbound
DESI Data Release 2 ELGs: Property-dependent subsamples, imaging systematics, and clustering cites this paper.
DESI Data Release 2 ELGs: Property-dependent subsamples, imaging systematics, and clustering DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 29
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T01:29:22.726076Z
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 d3af106a-b271-4086-9d85-f16fc44c6b26 · inbound
Cosmological constraints from the DESI DR1 Bispectrum Full-Shape and DR2 BAO cites this paper.
Cosmological constraints from the DESI DR1 Bispectrum Full-Shape and DR2 BAO DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T12:09:49.566657Z
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 d2d546b0-c416-4f11-8398-e8c844f5a8b0 · inbound
The 3D clustering of Lyman Alpha Emitters measured with DESI cites this paper.
The 3D clustering of Lyman Alpha Emitters measured with DESI DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 101
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T18:10:01.424630Z
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 d0e90d34-f7ec-4b20-8e25-ea9e0ee22ef3 · inbound
First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.
First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 49
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T15:29:56.434207Z
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 07338822-749a-41e0-b2d6-074cb6f6cc51 · inbound
Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy cites this paper.
Spherical Collapse and Halo Formation in a Cosmology with Decaying Dark Matter and a Semi-Cosmographic Dark Energy DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 41
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T14:19:54.186320Z
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 357f890b-dc3f-43be-aec8-acd243bdd609 · 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 DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 17
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T12:25:44.275908Z
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 443e7054-7970-4cb2-9926-24228a4e7c7a · inbound
Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.
Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T06:27:41.607043Z
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 79ed6503-d26e-4719-95cb-209efd81c0fd · inbound
Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.
Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T08:00:27.085537Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f9d2878f-5920-402c-a7dc-e30ecdfe112d · inbound
Cosmology with HI Intensity Mapping cites this paper.
Cosmology with HI Intensity Mapping DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 98
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:43:52.393274Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 22e3002a-aae7-43f5-ba96-c8358ec33ad4 · inbound
The Status of Single Scalar Field Dark Energy cites this paper.
The Status of Single Scalar Field Dark Energy DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 158
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T18:27:31.630001Z
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 e312ed2f-b9a9-45aa-908e-dce4eaa2d589 · inbound
Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data cites this paper.
Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 81
- Resolution
- malformed identifier
- no resolver link, observed 2026-07-13T04:28:42.548746Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e7a6e212-1507-4cf7-9ce1-63ab7c821550 · inbound
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 278
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T14:25:37.540627Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2b354597-9ee0-4446-b867-ddfecfde68ec · inbound
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.
Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 284
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:33:06.704177Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a323a03e-aeb2-4548-9e93-5ee27d78cad9 · inbound
Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number cites this paper.
Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:53:20.799396Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cf260b0f-4162-4f96-874d-0841e5ce6337 · inbound
Stacked Reverberation Mapping of High Redshift Quasars in DESI. I. Feasibility Analysis cites this paper.
Stacked Reverberation Mapping of High Redshift Quasars in DESI. I. Feasibility Analysis DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T06:28:10.084484Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7db86d9f-07d9-43fe-8afa-4d7f7f515668 · inbound
General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints cites this paper.
General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 133
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T01:25:44.382093Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ade3bd84-64b3-4c29-aca1-36d91b661db8 · inbound
DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.
DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:53:03.628684Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation aca808e6-7908-4c76-981e-a0bb1877872a · inbound
DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.
DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T01:45:55.683928Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41c504dc-9fb3-4a1c-b6f7-5ccf3ff0e9b2 · inbound
Validation of the DESI DR2 Ly$\alpha$ forest full-shape analysis cites this paper.
Validation of the DESI DR2 Ly$\alpha$ forest full-shape analysis DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:50:03.305180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 91dbfbab-8f70-4eb1-b3a4-3d98d73a6269 · inbound
Lyman-$\alpha$ forest holography: 3D predictions from 1D measurements cites this paper.
Lyman-$\alpha$ forest holography: 3D predictions from 1D measurements DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 112
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:50:53.486275Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 17cb57af-bc20-489f-b978-63250a194b0a · inbound
Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction cites this paper.
Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T01:55:11.166398Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.