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Paper Citation Record · LEDGER

Risk-based framework to determine climate-informed design storms for road drainage infrastructure

As of 20 August 2026, this Paper Citation Record lists 80 of 80 outbound references and 0 inbound Pith citation observations for arXiv:2508.10183.

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pith.paper-citation-record.v1
2508.10183 v1

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Outbound references

Observation e19bcb19-5736-419b-98b8-606f0276c101 · outbound

This paper cites Small-Scale Challenges to the $\Lambda$CDM Paradigm.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Small-Scale Challenges to the $\Lambda$CDM Paradigm

Reference 1

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Observation a37ef4c3-404b-4de0-a030-32bfc679d56a · outbound

This paper cites Cold dark matter: controversies on small scales.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Cold dark matter: controversies on small scales

Reference 2

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Observation dc80c553-ed2a-4101-861b-055d7582fd68 · outbound

This paper cites Fluid Dark Matter.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Fluid Dark Matter

Reference 3

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Observation 33909a28-bd47-462d-8f7d-8736044581f7 · outbound

This paper cites Repulsive Dark Matter.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Repulsive Dark Matter

Reference 4

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 5

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 6

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure String Axiverse

Reference 7

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Observation 10cb9087-3aed-43cd-80d2-8b5fba0a546e · outbound

This paper cites Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter

Reference 8

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Observation 5fbeed95-0feb-4320-9175-d0a85cea975e · outbound

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 9

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Observation 35b8848d-a443-48fc-bc67-e50f6fff1ea7 · outbound

This paper cites Ultralight scalars as cosmological dark matter.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Ultralight scalars as cosmological dark matter

Reference 10

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Observation 7c593f44-cccc-40a1-b9e1-8dcd01c0a13a · outbound

This paper cites Cosmic Structure as the Quantum Interference of a Coherent Dark Wave.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Cosmic Structure as the Quantum Interference of a Coherent Dark Wave

Reference 11

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Observation 709950e7-9b7f-4a6f-a0f1-3f0fea59b0e7 · outbound

This paper cites Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations

Reference 12

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Observation 2e028191-0059-4058-9ce3-c6b9c301d6fd · outbound

This paper cites Wave Dark Matter.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Wave Dark Matter

Reference 13

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Observation 84990f65-209d-4c57-ac2e-41324bace7e5 · outbound

This paper cites Accurate method for ultralight axion CMB and matter power spectra.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Accurate method for ultralight axion CMB and matter power spectra

Reference 14

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Observation e24c5a48-8323-4b85-b3dd-31ac4d8b7f24 · outbound

This paper cites Hydrodynamics of ultralight complex scalar field dark matter and its impact on the growth of structure.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Hydrodynamics of ultralight complex scalar field dark matter and its impact on the growth of structure

Reference 15

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 16

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Observation 7f163fdb-d207-4e27-ba95-1831efd2734c · outbound

This paper cites Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results

Reference 17

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Observation 2f981c13-1eee-43a5-8cba-7a4e46f05147 · outbound

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Angular Momentum and Vortex Formation in Bose-Einstein-Condensed Cold Dark Matter Haloes

Reference 18

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Observation 0abe1fed-399e-46fd-97d0-034a15c28da2 · outbound

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Contrasting Galaxy Formation from Quantum Wave Dark Matter, $\psi$DM, with $\Lambda$CDM, using Planck and Hubble Data

Reference 19

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Observation f0669c29-b8f3-48ec-bea9-346761c0b9ef · outbound

This paper cites Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics

Reference 20

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure The halo mass function and filaments in full cosmological simulations with fuzzy dark matter

Reference 21

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Observation d46cf6ae-2257-4fee-9016-6108710bce8e · outbound

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Implications of a Pre-reionization 21 cm Absorption Signal for Fuzzy Dark Matter

Reference 22

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates

Reference 23

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe

Reference 24

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure How accurately can 21 cm tomography constrain cosmology?

Reference 25

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure 21-cm cosmology

Reference 26

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Rise of the First Stars: Supersonic Streaming, Radiative Feedback, and 21-cm Cosmology

Reference 27

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Fuzzy Dark Matter at Cosmic Dawn: New 21-cm Constraints

Reference 28

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Fuzzy Dark Matter and the 21cm Power Spectrum

Reference 29

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Exploring delaying and heating effects on the 21-cm signature of fuzzy dark matter

Reference 30

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Closing the window on fuzzy dark matter with the 21cm signal

Reference 31

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Hydrogen Epoch of Reionization Array (HERA)

Reference 32

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Redundant Array Configurations for 21 cm Cosmology

Reference 33

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure A Model For Halo Formation With Axion Mixed Dark Matter

Reference 34

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

Reference 35

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Greig and A

Reference 36

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Risk-based framework to determine climate-informed design storms for road drainage infrastructure Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal

Reference 37

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Observation 5d0ef123-d966-4bff-a363-7d3b33a71d52 · outbound

This paper cites The Impact of the First Galaxies on Cosmic Dawn and Reionization.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Impact of the First Galaxies on Cosmic Dawn and Reionization

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Observation 5c58bd7b-be1f-4214-b1fa-931bb3c8fe9e · outbound

This paper cites Reionization and the Cosmic Dawn with the Square Kilometre Array.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Reionization and the Cosmic Dawn with the Square Kilometre Array

Reference 39

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Observation e1d79464-6fa8-4491-9259-91365be86ff1 · outbound

This paper cites Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?

Reference 40

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Observation ea76a2a5-329b-4fe0-8261-8672825d0ef4 · outbound

This paper cites 21-cm Tomography of the Intergalactic Medium at High Redshift.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure 21-cm Tomography of the Intergalactic Medium at High Redshift

Reference 41

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Observation 640cdb66-e799-493b-99d3-f0b2f9a00e96 · outbound

This paper cites Redshift Space Distortion of the 21cm Background from the Epoch of Reionization I: Methodology Re-examined.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Redshift Space Distortion of the 21cm Background from the Epoch of Reionization I: Methodology Re-examined

Reference 42

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source=pdf_text observed=2026-08-05T20:39:31.939836Z digest=sha256:ba21ce70343c1d8be912bc54e8f2d9b7a38fbe0b10876de8c4191674707bf9ad

Observation 82a39485-971c-493e-a2c1-53dd36381c41 · outbound

This paper cites Linear Polarization of the 21 cm Line from the Epoch of Reionization.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Linear Polarization of the 21 cm Line from the Epoch of Reionization

Reference 43

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local_arxiv, observed 2026-08-05T20:39:37.442649Z

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Observation 7f09d8e5-6b6d-43f7-8b7e-9c364b9b8eca · outbound

This paper cites 21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure 21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal

Reference 44

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Observation f6af3dd6-16e9-403e-b897-096e6c09fe6e · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 45

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Observation de5de629-a236-4c05-9b3e-4f37d986c3ad · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 46

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source=pdf_text observed=2026-08-05T20:39:32.302423Z digest=sha256:67231d12bbcee1b89545589406227ccc8b9b22630276db2e3045c8b796a56be6

Observation eefdbc90-e95f-456c-95a6-7e448fc31e30 · outbound

This paper cites Large scale bias and the peak background split.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Large scale bias and the peak background split

Reference 47

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source=pdf_text observed=2026-08-05T20:39:32.422588Z digest=sha256:3722e0662daead3009158a390f5062c4c7628d25022937b064c13c02d481085e

Observation 4d4e7af9-b538-45f7-9c89-27476f2e1115 · outbound

This paper cites Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes

Reference 48

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Observation f0af8ee6-1976-4edf-b13a-93ac583b17ef · outbound

This paper cites Jenkins, C.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Jenkins, C

Reference 49

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source=pdf_text observed=2026-08-05T20:39:32.650999Z digest=sha256:88bb9ac6f00a013621cde941759843ce8dfc71981fbabf6a917c522f820dd373

Observation 42420443-54bd-453b-8add-b3b375134f47 · outbound

This paper cites An analytic model for the spatial clustering of dark matter haloes.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure An analytic model for the spatial clustering of dark matter haloes

Reference 50

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source=pdf_text observed=2026-08-05T20:39:32.760501Z digest=sha256:77510ca1f21df72a19cf583e226a2edfb9fe9b1c84bf9101cb239b8baefbe100

Observation 7211a8e0-5fb6-4e5a-b430-8c3793a4968a · outbound

This paper cites Halo Models of Large Scale Structure.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Halo Models of Large Scale Structure

Reference 51

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source=pdf_text observed=2026-08-05T20:39:32.831733Z digest=sha256:ed02cfade747c4109ae76c33fa5d0491db8a9984689dd70140e09ed2c2cb7b3b

Observation 7c10a6a2-fbcf-4d4b-a302-82daf0eba191 · outbound

This paper cites In the Beginning: The First Sources of Light and the Reionization of the Universe.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure In the Beginning: The First Sources of Light and the Reionization of the Universe

Reference 52

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source=pdf_text observed=2026-08-05T20:39:32.912970Z digest=sha256:600116b045c1277a2d5daad1dae5419ffc4fe164eacf358c4a5b6e2e323bd7a7

Observation e40b6852-755d-43c9-b820-5b3bcbcf24bb · outbound

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

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Planck 2018 results. VI. Cosmological parameters

Reference 53

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source=pdf_text observed=2026-08-05T20:39:33.005427Z digest=sha256:466d0ccb4472d3dfea528fb08b313b665c534df80ce59bc673d3be730a5b3dc2

Observation 1e54870e-ae11-487c-a78f-eb04de6f017a · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 54

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source=pdf_text observed=2026-08-05T20:39:33.124366Z digest=sha256:8e1c2d514d3d7c82cf662cbc7a9e96b6300734387e442f95c46c0b136e9c72e8

Observation a5c50935-ac84-4228-b9e4-222a56f807be · outbound

This paper cites Model-independent evidence in favor of an end to reionization by z~6.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Model-independent evidence in favor of an end to reionization by z~6

Reference 55

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source=pdf_text observed=2026-08-05T20:39:33.282778Z digest=sha256:bba5305bef6babea7aa5d9847abd620cbaf4a30bb1c1af8ad251829bc8acae86

Observation fc8daf8d-4db6-427f-8d24-c7c51eb50328 · outbound

This paper cites (Nearly) Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at $z\sim 5-7$ Using Dark Pixel Fractions in Ly$\alpha$ and Ly$\beta$ Forests.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure (Nearly) Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at $z\sim 5-7$ Using Dark Pixel Fractions in Ly$\alpha$ and Ly$\beta$ Forests

Reference 56

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source=pdf_text observed=2026-08-05T20:39:33.380079Z digest=sha256:a4e684817e60b414f984e71d0543e9bc4d5b886f355f397cdfeb1b791325f108

Observation 2af3ebd8-c0ff-40f9-9478-3f3daea67d54 · outbound

This paper cites Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models

Reference 57

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source=pdf_text observed=2026-08-05T20:39:33.537334Z digest=sha256:63677a5877c8ff27b3f88c608344ae27cad7d3467ac4a590990575119bce1603

Observation 505b38b3-a5e0-4e3b-92a4-9c793f2e53e2 · outbound

This paper cites The Evolution of the Lyman-Alpha Luminosity Function During Reionization.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Evolution of the Lyman-Alpha Luminosity Function During Reionization

Reference 58

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Observation 3bde848c-3d0c-43f1-98a5-ebcb54a18ce3 · outbound

This paper cites The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly$\alpha$ Emission from Galaxies.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly$\alpha$ Emission from Galaxies

Reference 59

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Observation 552b4044-0edc-4aef-b236-b16a6403a2b5 · outbound

This paper cites Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5

Reference 60

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source=pdf_text observed=2026-08-05T20:39:33.920915Z digest=sha256:001a9644b8eef6ca43d62eb24ef84c8f21724df2df7e45a5b88f2b1d2a335a6f

Observation de874d63-7cc7-4a84-af5a-63f7745d20df · outbound

This paper cites Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey

Reference 61

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source=pdf_text observed=2026-08-05T20:39:33.991685Z digest=sha256:45bd0308db3fdf3465533c8e4540c27f735a8eb0723499966e40b309b1c5cedf

Observation 60a58be0-d721-4b50-addb-ababe79bff29 · outbound

This paper cites IGM damping wing constraints on reionisation from covariance reconstruction of two $z\gtrsim7$ QSOs.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure IGM damping wing constraints on reionisation from covariance reconstruction of two $z\gtrsim7$ QSOs

Reference 62

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Observation 1f68c4ef-eb02-4e39-a50a-b6b01cc2cbd0 · outbound

This paper cites IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample

Reference 63

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source=pdf_text observed=2026-08-05T20:39:34.135099Z digest=sha256:93245a4d81452930967ef6aa37a3583390f2a48ab6958a8f94c9e799df465861

Observation 9f74ec06-aa25-4250-896f-d31696086762 · outbound

This paper cites Damping wings in the Lyman-{\alpha} forest: a model-independent measurement of the neutral fraction at 5.4<z<6.1.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Damping wings in the Lyman-{\alpha} forest: a model-independent measurement of the neutral fraction at 5.4<z<6.1

Reference 64

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Observation 2883ac63-86bd-4fa0-a782-aaf1c67d9954 · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 65

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Observation 085c768f-cdd2-41ee-8df7-e1a8f3b5ce88 · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 66

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Observation d7642b41-7878-41b6-b040-2402b04b7a7b · outbound

This paper cites Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array

Reference 67

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Observation fb79e8f7-9e0c-4b42-90e5-f22101cb3dc9 · outbound

This paper cites Signatures of X-rays in the early Universe.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Signatures of X-rays in the early Universe

Reference 68

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Observation ed5e9bee-c2be-4515-8788-0abb054f48e0 · outbound

This paper cites an unresolved cited work.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Unresolved cited work

Reference 69

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 90a631ac-5717-469b-9cc6-f9db0dc726be · outbound

This paper cites What is the SKA-Low Sensitivity for Your Favourite Radio Source ?.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure What is the SKA-Low Sensitivity for Your Favourite Radio Source ?

Reference 70

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local_arxiv, observed 2026-08-05T20:39:36.455641Z

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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-08-05T20:39:34.744073Z digest=sha256:067a58bcc0762efc898732e50f1ce1ffea1e7f62b43aed689d471c15095be032

Observation 749f8c91-9334-4821-8188-8c39be452790 · outbound

This paper cites Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts

Reference 71

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source=pdf_text observed=2026-08-05T20:39:34.824277Z digest=sha256:b04b2f495c4600f61d7e5626242b76f1f689565194b9e06a6d8180d982408379

Observation 02837381-0969-4d65-bba4-c33f25bbaee6 · outbound

This paper cites The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts

Reference 72

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source=pdf_text observed=2026-08-05T20:39:34.900632Z digest=sha256:9809f06478fd3920597975e5a2e00b0feb6b7d66674ba76c2ef88d9c98381382

Observation 5335d02c-1073-4c82-b2cc-10989932517e · outbound

This paper cites What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization

Reference 73

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source=pdf_text observed=2026-08-05T20:39:34.996022Z digest=sha256:ac3f1ebbd9e2f14e328768795837506dfb1ec1dcc799849ed5f34e2b80199bcb

Observation 988366d1-1806-4766-a778-dddff87aa754 · outbound

This paper cites Constraining High Redshift X-ray Sources with Next Generation 21 cm Power Spectrum Measurements.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Constraining High Redshift X-ray Sources with Next Generation 21 cm Power Spectrum Measurements

Reference 74

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local_arxiv, observed 2026-08-05T20:39:36.183908Z

Source-reported events for the cited work

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Observation 29d330ce-a53e-4453-867d-b431e9ff3955 · outbound

This paper cites Data Analysis for Precision 21 cm Cosmology.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Data Analysis for Precision 21 cm Cosmology

Reference 75

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Observation 3bcf3f90-cf17-4860-a560-0d1cf8d0ec05 · outbound

This paper cites A Sensitivity and Array-Configuration Study for Measuring the Power Spectrum of 21cm Emission from Reionization.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure A Sensitivity and Array-Configuration Study for Measuring the Power Spectrum of 21cm Emission from Reionization

Reference 76

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Observation 6739a25c-3ee0-495a-8f5b-832288647a20 · outbound

This paper cites New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7

Reference 77

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Observation 8a708d70-d159-4e06-beb0-48535f914ef1 · outbound

This paper cites Four Fundamental Foreground Power Spectrum Shapes for 21 cm Cosmology Observations.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Four Fundamental Foreground Power Spectrum Shapes for 21 cm Cosmology Observations

Reference 78

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Observation 5856a083-ed01-4a57-8cb8-62d2d7169bf1 · outbound

This paper cites Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Constraining the unexplored period between reionization and the dark ages with observations of the global 21 cm signal

Reference 79

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Observation 43ea961a-0a61-42a8-bf27-7d8fd73719d6 · outbound

This paper cites Constraining cosmology and ionization history with combined 21 cm power spectrum and global signal measurements.

Risk-based framework to determine climate-informed design storms for road drainage infrastructure Constraining cosmology and ionization history with combined 21 cm power spectrum and global signal measurements

Reference 80

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local_arxiv, observed 2026-08-05T20:39:35.896287Z

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