We present photometry, photometric redshifts and extra galactic number counts for ultra deep 15 micron mapping of the gravitational lensing cluster Abell 2218 (A2218), which is the deepest image taken by any facility at this wavelength. This data resolves the cosmic infrared background (CIRB) ...
We present photometry, photometric redshifts and extra galactic number counts for ultra deep 15 micron mapping of the gravitational lensing cluster Abell 2218 (A2218), which is the deepest image taken by any facility at this wavelength. This data resolves the cosmic infrared background (CIRB) be...
A spectral image producer produces a spectral image of arbitrary wavelength bands from the two kinds of image signals, whereas a general image producer produces a general image from those image signals captured under the general illumination light. 展开 ...
The calculated optical lateral resolutionδLdepends on the numerical aperture of the optics (= objective + optical zoom,NA), on the wavelength of the lightλand on a factorK: δL=K.λNA(3) The value ofKis 0.61 for bright field microscopy (= “classical” light microscopes). For laser-...
When illuminated by a plane wave, continuously self-imaging gratings (CSIGs) produce a field whose intensity profile is a propagation- and wavelength-invariant biperiodic array of bright spots. In the case of an extended and incoherent source, we show that CSIGs produce multiple images of the ...
3) and instrumentation that uses a piezo linear stage and camera, providing an avenue for the analysis of targets that are smaller than the wavelength of light. Fig. 1: High-throughput workflow for label-free single-DCV targeting and MS analysis. a, Schematic of MALDI MS workflow for high-...
Sharma, P., Bisht, I. & Sur, A. Wavelength-based attributed deep neural network for underwater image restoration.ACM Trans. Multimed. Comput. Commun. Appl.19, 1–23.https://doi.org/10.1145/3511021(2023). ArticleGoogle Scholar Vaswani, A.et al.Attention is all you need. InAdvances in ...
AN X-RAY INVESTIGATION OF THREE SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD We have investigated three supernova remnants (SNRs) in the LMC using multi-wavelength data. These SNRs are generally fainter than the known sample (see Se... Matthew,D.,Klimek,... - 《Astrophysical Journal》 ...
The experimental setup consisted of a portable tunable laser system (PhocusCore, Optotek, California, USA) of wavelength (λ = 532 nm), repetition rate of 10 Hz coupled to an ablation fiber (NeverTouch, Angiodynamics, New York, USA) of diameter 1000 µm. A high frequency line...
The techniques are intended for 2D (line) surface-breaking cracks with the size of the incident wavelength or greater. The probing wave mode is the anti-plane shear wave (SH-wave). Two methods are employed for the ultrasonic imaging. One is a synthetic aperture focusing technique (SAFT) and...