TCS-CAIN: a deep multi-colour NIR survey of the Galactic plane [PDF]
A. Cabrera‐Lavers +4 more
openalex +1 more source
Robust C–V Ratio Technique for Profiling Defects in Proton‐Irradiated 4H‐SiC
A noise‐robust C–V ratio technique is introduced to profile radiation‐induced defects in proton‐irradiated 4H‐SiC Schottky diodes. By using analytical capacitance ratios instead of numerical differentiation, the method directly extracts trap‐density and effective trap‐energy profiles at room temperature.
Kibeom Kim +4 more
wiley +1 more source
Pattern functions of the Astrometric Gravitational Wave Antenna. [PDF]
Santucci F, Crosta M, Lattanzi MG.
europepmc +1 more source
Magnetic fields in the Southern Galactic Plane Survey [PDF]
M. Haverkorn +5 more
openalex +1 more source
Heterogeneous Integration of Flipped Oxide Heterostructure Membranes for Nanoelectronics
A flipped electronically reconfigurable STO/LAO freestanding membrane is demonstrated and integrated with various host platforms via controlled transfer. Using ultra‐low‐voltage electron‐beam lithography, conductive nanostructures are created at the buried STO/LAO interface. This novel approach enables heterogeneous integration of flipped complex oxide
Ruiqi Sun +9 more
wiley +1 more source
The connection between the fastest astrophysical jets and the spin axis of their black hole. [PDF]
Fender RP, Motta SE.
europepmc +1 more source
A Radio Survey of the Galactic Plane at a Frequency of 408 Mc/s. II. The Continuum Emission from the Galactic Disk [PDF]
M. I. Large +2 more
openalex +1 more source
Device Performance of Emerging Photovoltaic Materials (Version 6)
Efficiency of single junction perovskite (circles), organic (hexagons), dye sensitized (pentagons), kesterite (diamonds), Sb2Se3 (right triangle), and AgBiS2 (left triangles) solar cells at emerging‐pv.org over the last decade. ABSTRACT This 6th annual Emerging PV Report surveys peer‐reviewed advances since August 2024 across perovskite, organic ...
Osbel Almora +29 more
wiley +1 more source
Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula. [PDF]
LHAASO Collaborationxurenfeng@ihep.ac.cnk-wang@smail.nju.edu.cnchensz@ihep.ac.cnryliu@nju.edu.cnxisq@ihep.ac.cnhushicong@ihep.ac.cn.
europepmc +1 more source

