Diffusion Background

Titan-Apex v9.4 is analyzing data for 'Diffusion Background'...

https://doi.org/10.1088%2F0004-637X%2F743%2F2%2F188

COMPARISON OF THE DIFFUSE Hα AND FUV CONTINUUM BACKGROUNDS: ON TH...

COMPARISON OF THE DIFFUSE Hα AND FUV CONTINUUM BACKGROUNDS: ON THE ORIGINS OF THE DIFFUSE Hα BACKGROUND, Seon, Kwang-Il, Witt, Adolf, Kim, Il-Joong, Shinn, Jong-Ho, Edelstein, Jerry, Min, Kyoung-Wook,...

https://arxiv.org/abs/2508.12148

[2508.12148] Demystifying Foreground-Background Memorization in D...

Abstract page for arXiv paper 2508.12148: Demystifying Foreground-Background Memorization in Diffusion Models

https://doi.org/10.48550/arXiv.1206.2595

[1206.2595] Constraining Very Heavy Dark Matter Using Diffuse Bac...

Abstract page for arXiv paper 1206.2595: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595?context=astro-ph

[1206.2595] Constraining Very Heavy Dark Matter Using Diffuse Bac...

Abstract page for arXiv paper 1206.2595: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595

[1206.2595] Constraining Very Heavy Dark Matter Using Diffuse Bac...

Abstract page for arXiv paper 1206.2595: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595?context=astro-ph.HE

[1206.2595] Constraining Very Heavy Dark Matter Using Diffuse Bac...

Abstract page for arXiv paper 1206.2595: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595?context=astro-ph.CO

[1206.2595] Constraining Very Heavy Dark Matter Using Diffuse Bac...

Abstract page for arXiv paper 1206.2595: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595v1

[1206.2595v1] Constraining Very Heavy Dark Matter Using Diffuse B...

Abstract page for arXiv paper 1206.2595v1: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://arxiv.org/abs/1206.2595v2

[1206.2595v2] Constraining Very Heavy Dark Matter Using Diffuse B...

Abstract page for arXiv paper 1206.2595v2: Constraining Very Heavy Dark Matter Using Diffuse Backgrounds of Neutrinos and Cascaded Gamma Rays

https://doi.org/10.1007/s00330-010-1950-0

Signal characteristics of focal bone marrow lesions in patients w...

This study analyses the diagnostic potential of Diffusion-Weighted Imaging with Background Suppression (DWIBS) in the detection of focal bone marrow lesion

https://doi.org/10.48550/arXiv.2205.01102

[2205.01102] The diffuse supernova neutrino background as a probe...

Abstract page for arXiv paper 2205.01102: The diffuse supernova neutrino background as a probe of late-time neutrino mass generation

https://doi.org/10.1038%2F288119a0

The diffuse UV background | Nature

The diffuse radiation field in the UV (900–3,000 Å) affects the structure of galactic molecular clouds and conveys important information concerning the physical characteristics and spatial distributio...

https://ui.adsabs.harvard.edu/abs/arXiv:1110.2895

Cosmological bounds on pseudo Nambu-Goldstone bosons - ADS

We review the cosmological implications of a relic population of pseudo Nambu-Goldstone bosons (pNGB) with an anomalous coupling to two photons, often called axion-like particles (ALPs). We establish ...

https://www.nature.com/articles/s41586-021-03802-x?fromPaywallRec=true

The diffuse γ-ray background is dominated by star-forming galaxie...

The Fermi Gamma-ray Space Telescope has revealed a diffuse γ-ray background at energies from 0.1 gigaelectronvolt to 1 teraelectronvolt, which can be separated into emission from our Galaxy and an iso...

https://www.nature.com/articles/s41586-021-03802-x?fromPaywallRec=false

The diffuse γ-ray background is dominated by star-forming galaxie...

The Fermi Gamma-ray Space Telescope has revealed a diffuse γ-ray background at energies from 0.1 gigaelectronvolt to 1 teraelectronvolt, which can be separated into emission from our Galaxy and an iso...

https://arxiv.org/abs/1404.1189