Optimized sampling for view interpolation in light fields using local dictionaries

Author(s):  
David C. Schedl ◽  
Clemens Birklbauer ◽  
Oliver Bimber
2017 ◽  
Vol 26 (2) ◽  
pp. 603-618
Author(s):  
Chao-Tsung Huang ◽  
Yu-Wen Wang ◽  
Li-Ren Huang ◽  
Jui Chin ◽  
Liang-Gee Chen

2018 ◽  
Vol 168 ◽  
pp. 93-103 ◽  
Author(s):  
David C. Schedl ◽  
Clemens Birklbauer ◽  
Oliver Bimber

2004 ◽  
Vol 04 (04) ◽  
pp. 585-604 ◽  
Author(s):  
YASUYUKI MATSUSHITA ◽  
STEPHEN LIN ◽  
HEUNG-YEUNG SHUM ◽  
XIN TONG ◽  
SING BING KANG

Densely-sampled image representations such as the light field or Lumigraph have been effective in enabling photorealistic image synthesis. Unfortunately, lighting interpolation with such representations has not been shown to be possible without the use of accurate 3D geometry and surface reflectance properties. In this paper, we propose an approach to image-based lighting interpolation that is based on estimates of geometry and shading from relatively few images. We decompose light fields captured at different lighting conditions into intrinsic images (reflectance and illumination images), and estimate view-dependent scene geometries using multi-view stereo. We call the resulting representation an Intrinsic Lumigraph. In the same way that the Lumigraph uses geometry to permit more accurate view interpolation, the Intrinsic Lumigraph uses both geometry and intrinsic images to allow high-quality interpolation at different views and lighting conditions. The joint use of geometry and intrinsic images is effective in computing shadow masks for shadow prediction at new lighting conditions. We illustrate our approach with images of real scenes.


2016 ◽  
Vol 2016 (19) ◽  
pp. 1-6 ◽  
Author(s):  
Bart Goossens ◽  
Simon Donné ◽  
Jan Aelterman ◽  
Jonas De Vylder ◽  
Dirk Van Haerenborgh ◽  
...  

2017 ◽  
Vol 36 (4) ◽  
pp. 1
Author(s):  
Clemens Birklbauer ◽  
David C. Schedl ◽  
Oliver Bimber

2021 ◽  
Vol 2021 (1) ◽  
Author(s):  
JiJi Fan ◽  
Zhong-Zhi Xianyu

Abstract Light fields with spatially varying backgrounds can modulate cosmic preheating, and imprint the nonlinear effects of preheating dynamics at tiny scales on large scale fluctuations. This provides us a unique probe into the preheating era which we dub the “cosmic microscope”. We identify a distinctive effect of preheating on scalar perturbations that turns the Gaussian primordial fluctuations of a light scalar field into square waves, like a diode. The effect manifests itself as local non-Gaussianity. We present a model, “modulated partial preheating”, where this nonlinear effect is consistent with current observations and can be reached by near future cosmic probes.


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