Pith. sign in

Paper Citation Record · LEDGER

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum

As of 18 August 2026, this Paper Citation Record lists 36 of 36 outbound references and 0 inbound Pith citation observations for arXiv:2505.14258.

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

pith.paper-citation-record.v1
2505.14258 v1

Coverage vector

measured 36 of 36 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:44:30.874573Z

measured 36 of 36 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

36 of 36 outbound references displayed

  • verified exact2
  • verified fuzzy5
  • unresolved29
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation d962ea26-fb6f-498c-8c84-61d0a9801ec0 · outbound

This paper cites A History of Dark Matter.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum A History of Dark Matter

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:26.734832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:26.734832Z digest=sha256:b1c06b2800906a62d7bfc8493a30deff995d861aa5eb9a0c33c2b8f5b49f36a9

Observation 05247df1-eaab-4794-9d04-6e2dcb0ec730 · outbound

This paper cites Dark matter and the early Universe: a review.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Dark matter and the early Universe: a review

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:26.864953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:26.864953Z digest=sha256:f1914575ac510eb93ba8ab523e0ff59e7041c51bd215f72f52ae259f16453f29

Observation 8ca5eb3b-ca65-4226-9b0b-7233cd7d1b70 · outbound

This paper cites Halo Formation in Warm Dark Matter Models.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Halo Formation in Warm Dark Matter Models

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:26.966326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:26.966326Z digest=sha256:8518860b16ea48baca33db744143813126bed471835f3b5d6c3d2422b5554bb1

Observation f1c7a6e2-e3f8-4e1b-b6da-48d753ce8d7d · outbound

This paper cites The Statistics of Density Peaks and the Column Density Distribution of the Lyman-Alpha Forest.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The Statistics of Density Peaks and the Column Density Distribution of the Lyman-Alpha Forest

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.102774Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.102774Z digest=sha256:d3df70c423be506ee6fc6205fed2ed290d86f14f7b0f978685e413fe00c63106

Observation b03f1baa-9859-4236-9ab6-58c15e61b1d9 · outbound

This paper cites Matter Power Spectrum from the Lyman-Alpha Forest: Myth or Reality?.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Matter Power Spectrum from the Lyman-Alpha Forest: Myth or Reality?

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.249838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.249838Z digest=sha256:fc669181023d613fd5c3b43c878859c74190b9a33fd06a4497c3fb70bd84e5c3

Observation d07ca234-077c-44a9-9dcd-5087a90a72a4 · outbound

This paper cites Lyman-alpha constraints on warm and on warm-plus-cold dark matter models.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Lyman-alpha constraints on warm and on warm-plus-cold dark matter models

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.421101Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.421101Z digest=sha256:90edcf24fd78f6d3aba4c17fe8c7f7d334d7038cc8d478ff94bdbb0b3f2c2d78

Observation 80c9bbb4-a6e9-493b-9f20-e8c704a94c8e · outbound

This paper cites How to constrain warm dark matter with the Lyman $\alpha$ forest.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum How to constrain warm dark matter with the Lyman $\alpha$ forest

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.555370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.555370Z digest=sha256:037dc18b32478c7356daf166c14d70242febcf0ac405fee0415e64b754410a7d

Observation 6b797607-37c7-4d60-bfe9-4889c0d84147 · outbound

This paper cites Equation of State of the Photoionized Intergalactic Medium.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Equation of State of the Photoionized Intergalactic Medium

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.694822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.694822Z digest=sha256:f6d9071c80ca8e7eb18e46ca4334caf2a89f554bc07d87ef2453b5d647423f9d

Observation a40fd258-f58b-4086-8dad-8873a1bd1e6f · outbound

This paper cites Probing the Universe with the Lyman-alpha Forest: I. Hydrodynamics of the Low Density IGM.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Probing the Universe with the Lyman-alpha Forest: I. Hydrodynamics of the Low Density IGM

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:27.844961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:27.844961Z digest=sha256:54e603e63d80f8a7031af292e9629a3e3715d0718609a363cef6dc8d48515576

Observation 4d62896c-e62a-4185-a4de-f2c9b496cef3 · outbound

This paper cites The broadening of Lyman-alpha forest absorption lines.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The broadening of Lyman-alpha forest absorption lines

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.001876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.001876Z digest=sha256:a088f00a570c8c4579d1811ddac47c48d31c786a1bc01a64670bf4f0dff73e1d

Observation 0ce9b2e3-b3bb-45c6-8525-5b2aef1db15a · outbound

This paper cites New Constraints on Warm Dark Matter from the Lyman-$\alpha$ Forest Power Spectrum.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum New Constraints on Warm Dark Matter from the Lyman-$\alpha$ Forest Power Spectrum

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.097208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.097208Z digest=sha256:6df3610d8e1d1cd198f06e234c19393eb8e98dfb7b5db4a5399aac3cdd472bd2

Observation 3aba870e-7237-4557-9840-eb8b3c8ae28b · outbound

This paper cites The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.249542Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.249542Z digest=sha256:e4805a19ec1afa8d57f8531d3254dd241790539532e5dd9ba96e4fcb73c0210c

Observation 27015eb5-ce4a-4780-bb24-c780ed165d57 · outbound

This paper cites Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.458860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.458860Z digest=sha256:528dfcee254de68739f90b09a4101ef6dadd4152a309c47a49a6a487661c0734

Observation 3ec90198-7e11-4a63-a1c2-7fd4603c47d9 · outbound

This paper cites Binney and S.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Binney and S

Reference 14

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T15:44:37.039564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:28.555425Z digest=sha256:6b9f80c64682f89303fe2374cb0cd0b4ab979131a7476e85145aadd0d6c8aa27

Observation b63de3e9-1254-4f23-88e6-d48a93fa8c1b · outbound

This paper cites Linear Gas Dynamics in the Expanding Universe: Why the Jeans Scale does not Matter.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Linear Gas Dynamics in the Expanding Universe: Why the Jeans Scale does not Matter

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.655161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.655161Z digest=sha256:4e7efc45bf2c7ed5d51dc58f81b77222f02cd72ef75b4731ad287af1b5fe9906

Observation 236cf864-f810-4801-a3af-638fda64dcf1 · outbound

This paper cites Characterizing the Pressure Smoothing Scale of the Intergalactic Medium.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Characterizing the Pressure Smoothing Scale of the Intergalactic Medium

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.745239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.745239Z digest=sha256:b33675544456f86176c23713fdf2718a4a057eeba2f62397d5c8ea93196000e8

Observation 1d340920-39cc-4ea1-b7f3-59428215361a · outbound

This paper cites Lumsden, A.F.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Lumsden, A.F

Reference 17

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T15:44:36.825512Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:28.845082Z digest=sha256:4cbe37b66178748c6cc0a07a6a57fd0bc92325bbd0fe28c5c59edcd7ba4c190d

Observation f111e293-4cda-4020-b4d6-f201759514aa · outbound

This paper cites The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The Lyman-$\alpha$ forest as a diagnostic of the nature of the dark matter

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:28.956603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:28.956603Z digest=sha256:19f55aa8d026188a58ba2b6589864ffe1173c389a022833e0465eaa7d26e26ed

Observation 526d6e43-7b29-4f8f-96d8-76bd56e14c75 · outbound

This paper cites SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.037673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.037673Z digest=sha256:ebcb5f41ab3b9c2bcf3e09643812326e3c2c7f92462996958461163de29f4a29

Observation 748b0337-01d5-426f-aa59-e4f8ab8619f1 · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.125006Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.125006Z digest=sha256:6f1df63fa4c77b0908f9b7055590a681dcff14affe748a0e59d3af2fd1a79315

Observation 5b93e16b-9896-4cbf-9dd1-b50d0a1c7f81 · outbound

This paper cites Cosmological Simulations with TreeSPH.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Cosmological Simulations with TreeSPH

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.255479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.255479Z digest=sha256:50c9ba8fb834ea3cc0c0ea4600709cb4cf6e6aba1e8afc02f6b998fec576b6ae

Observation 038aa66b-45b6-4245-b055-a83480c2bc26 · outbound

This paper cites Cosmological SPH simulations: A hybrid multi-phase model for star formation.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Cosmological SPH simulations: A hybrid multi-phase model for star formation

Reference 22

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:44:33.119284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:29.364916Z digest=sha256:a884c90aabb015ba2871a8302915c394778f76b920d3b803721bd720d101cecb

Observation 95a025d2-fa43-4eac-a879-602ac1c90025 · outbound

This paper cites Haardt, P.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Haardt, P

Reference 23

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T15:44:36.535000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:29.464881Z digest=sha256:88075112dbfcf945b31f3e47482ab0b109e020121d9c569d85d3364797ff0a73

Observation dc155154-9324-4aa2-a518-7fda42b2d26c · outbound

This paper cites Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.574747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.574747Z digest=sha256:83d99258f82b1fd7e6d76ebde3f78d74fdf0bc423eb789fdf5de20860d3746f5

Observation 216eea13-dbdb-47e1-9e8b-b5fdbf3e127d · outbound

This paper cites Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.673482Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.673482Z digest=sha256:178f8aea51450c8c8f1256dd06a6444a33d321d3a01358fca3f6b02dda400626

Observation 78d2d150-1bcc-4c40-845f-7ebc1d84dc0c · outbound

This paper cites Higher-order initial conditions for mixed baryon-CDM simulations.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Higher-order initial conditions for mixed baryon-CDM simulations

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.776808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.776808Z digest=sha256:1d3aa136db8e355397a12ebebd84604c00924f2294ff62f9781f3184a4c7628a

Observation 5a2ffc0b-3e7e-47cc-9141-c75ededd25c4 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:29.897389Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:29.897389Z digest=sha256:6e31b172ccf1b9aa9b9663aa50704cc081e2014d9fa526de76aee67a5894d800

Observation c261c774-1ba0-4971-8cd3-0084e6fda464 · outbound

This paper cites Resolving the high redshift Lyman-alpha forest in smoothed particle hydrodynamics simulations.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Resolving the high redshift Lyman-alpha forest in smoothed particle hydrodynamics simulations

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.025680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.025680Z digest=sha256:8053424cdc564ad5c98d343b58b89924e4b8a67bbc89ec3508c9b12c36d8d61c

Observation bb4cf556-3fab-42af-a2c8-06fa2263f225 · outbound

This paper cites The Lyman-$\alpha$ forest in optically-thin hydrodynamical simulations.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The Lyman-$\alpha$ forest in optically-thin hydrodynamical simulations

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.135299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.135299Z digest=sha256:02fe59222aa73d0cfc24196d4da5964f8bd548f324b5b2360f64371f4b33a033

Observation c73f984a-565c-4d5a-84c5-a64ebcc6fb9e · outbound

This paper cites The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:44:31.754766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:30.255092Z digest=sha256:56d043aab1b260558c00bcc93fbb180fe74be8e14c4c059edd131ee9a076d6c2

Observation 6ea87f17-6607-48bb-aa1a-c363801b5b77 · outbound

This paper cites The cosmological simulation code GADGET-2.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum The cosmological simulation code GADGET-2

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.364996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.364996Z digest=sha256:4d70280a3150f5adb9466852144a08a170479ac69b52725ba9630b57ea5b01f1

Observation 1b810455-a49b-4e49-aec7-a5d2d3b468b1 · outbound

This paper cites specwizard a python package for computing mock quasar absorption spectra.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum specwizard a python package for computing mock quasar absorption spectra

Reference 32

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T15:44:36.184929Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:30.433257Z digest=sha256:66207bfff06f3dc94ff2f68047b3c7e89f7e7667cb07c35789620d70fd415d1a

Observation d8394156-baca-4b39-8c8c-429bc791b851 · outbound

This paper cites Borrow and A.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Borrow and A

Reference 33

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T15:44:35.877074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T15:44:30.577911Z digest=sha256:69a00abb7e88e09c4be46336b7c5a00abeaff20e777159d42291c895036fc420

Observation 0af9abb6-99a0-4897-9a7c-254eb16497a7 · outbound

This paper cites Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- II. KODIAQ, SQUAD & XQ-100.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- II. KODIAQ, SQUAD & XQ-100

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.675147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.675147Z digest=sha256:40748a5501931f9544a298c5ff43b1ff09a242f29061fa42b9884124260d0ef8

Observation cb36aa1a-3405-47f5-adc9-8e6968ffcbf5 · outbound

This paper cites Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman-$\alpha$ flux power spectrum

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.790185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.790185Z digest=sha256:65ae88146fce2f7e639026f2abe654b5abc005419b344460c20058baa5638a68

Observation 99fda53d-ff84-49fa-b3df-edf7800fb5d3 · outbound

This paper cites Convergence of small scale Ly$\alpha$ structure at high-$z$ under different reionization scenarios.

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum Convergence of small scale Ly$\alpha$ structure at high-$z$ under different reionization scenarios

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-07T15:44:30.874573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:44:30.874573Z digest=sha256:d8ef3ecf09aa7a06497a5c15d717eb3ef3a433c203e70447d5b7f3168fb98770

Pith citing papers

No inbound Pith citation observations are available.