A5026523096- Astrophysics and Cosmic Phenomena
- Gamma-ray bursts and supernovae
- Astrophysical Phenomena and Observations
- Dark Matter and Cosmic Phenomena
- Particle Detector Development and Performance
- Neutrino Physics Research
- Galaxies: Formation, Evolution, Phenomena
- Pulsars and Gravitational Waves Research
- Radiation Detection and Scintillator Technologies
- Nuclear Physics and Applications
- Radio Astronomy Observations and Technology
- Electrowetting and Microfluidic Technologies
- High-Energy Particle Collisions Research
- Particle physics theoretical and experimental studies
- Integrated Circuits and Semiconductor Failure Analysis
- Astronomical Observations and Instrumentation
- Microfluidic and Capillary Electrophoresis Applications
- Biosensors and Analytical Detection
- Advanced Optical Sensing Technologies
- Atmospheric Ozone and Climate
- Radioactivity and Radon Measurements
- Advanced X-ray and CT Imaging
- Opportunistic and Delay-Tolerant Networks
- Microfluidic and Bio-sensing Technologies
- Advanced Biosensing Techniques and Applications
United Imaging Healthcare (China)
2024
Max Planck Institute for Nuclear Physics
2022-2024
Institut de Recherche sur les Lois Fondamentales de l'Univers
2023
CEA Paris-Saclay
2023
Université Paris-Saclay
2023
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
2023
ETH Zurich
2023
Laboratoire Leprince-Ringuet
2023
Istituto Nazionale di Fisica Nucleare, Sezione di Padova
2023
Université de Montpellier
2023
Context. The detection of quasi-periodic oscillations (QPOs) in the light curves active galactic nuclei (AGNs) can provide insights into physics super-massive black holes (SMBHs) powering these systems and could represent a signature existence SMBH binaries, setting fundamental constraints on evolution Universe. Aims. identification long-term QPOs, characterized by periods order several months to years, is particularly challenging only be achieved via all-sky monitoring instruments that...
In this work, results and data are reported on key aspects of sample processing protocols performed on-chip in a digital microfluidic lab-on-a-chip. We report the experiments processing, including preconcentration dilution, injection or dispensing, mixing. It is shown that high speed transport mixing analytes reagents can be using biological solutions without system contamination.
The central molecular zone (CMZ) is a unique environment in our Galaxy, with extreme conditions to test understanding of the gas, dust, and cosmic-ray (CR) physics. Our goal estimate total gas mass direction Galactic centre (GC), quantify various associated uncertainties, discuss implications for estimates CR energy densities dust opacities. 21 cm line carbon monoxide isotopes ( (J = 1 → 0) 0; J 2 1), 1)) emission maps were used derive column density. CMZ separated from disk contribution...
P38 kinase plays a vital role in the inflammation mediated by tumor necrosis factor-α and interleukin-1β pathways, thus inhibitors of p38 provide effective approach for treatment inflammatory diseases. Presently, combined study threedimensional quantitative structure-activity relationship, molecular docking dynamics (MD) was undertaken to explore structural insights 174 2-thioimidazole compounds influencing p38α inhibitory activities. Both ligand-based resultant comparative field analysis...
Abstract Identification of Cherenkov light generated by muons has been suggested as a promising way to dramatically improve the background rejection power Imaging Atmospheric Telescope (IACT) arrays at high energies. However, muon identification remains challenging task, for which efficient algorithms are still being developed. We present an approach in which, rather than identifying from muons, we simply consider presence other main shower image IACTs with large mirror area. show that case...
Abstract The Tarantula Nebula in the Large Magellanic Cloud is known for its high star formation activity. At center lies young massive cluster R136, providing a significant amount of energy that makes nebula shine so brightly at many wavelengths. Recently, clusters have been suggested to also efficiently produce very high-energy cosmic rays, potentially beyond PeV energies. Here, we report detection very-high-energy γ -ray emission from direction R136 with High Energy Stereoscopic System,...
The detection of quasi-periodic oscillations (QPOs) in the emission active galactic nuclei (AGNs) can provide insights into physics super-massive black-holes (SMBHs) powering these systems, and could represent a signature existence SMBH binaries. identification long term QPOs, characterized by periods on order several months to years, is particularly challenging only be achieved via all-sky monitoring instruments like Fermi-LAT satellite. We aim identify QPOs $\gamma$-ray light-curves...
Identification of Cherenkov light generated by muons has been suggested as a promising way to dramatically improve the background rejection power Imaging Atmospheric Telescopes (IACT) arrays at high energies. However, muon identification remains challenging task, for which efficient algorithms are still being developed. We present an algorithm in which, rather than identifying from muons, we simply consider presence other main shower image IACT with large mirror area. show that case H.E.S.S....
The Galactic Centre (GC) region is a highly interesting for very high energy gamma-ray studies due to its proximity and diverse sources. It also unique place Dark Matter (DM) searches, since we expect large amount of DM in this it nearby. Currently new detector under development observe the GC region, called Southern Wide field-of-view Gamma-ray Observatory (SWGO). This instrument will be first water Cherenkov located Hemisphere sensitive >100 GeV gamma rays. In our work, are going present...
Specific probes against targets play siginificant role in biosensing and bioanalysis.The landscape phage library f8/8 displaying random octapeptides on the pVIII coat protein of fd-tet, demonstrating many excellent features including multivalency, stability, high structural homogeneity.In this talk, we present our recent advance selecting specific clones binding with different such as free prostate-specific antigen (fPSA), cellulase, ubiquitous pathogens from library.Then developed a series...
Identification of Cherenkov light generated by muons has been suggested as a promising way to dramatically improve the background rejection power Imaging Atmospheric Telescope (IACT) arrays at high energies. However, muon identification remains challenging task, for which efficient algorithms are still being developed. We present an approach in which, rather than identifying from muons, we simply consider presence other main shower image IACTs with large mirror area. show that case H.E.S.S....