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Synchrotron beamlines are highly versatile tools for a wide range of scientific measurements using X-rays, offering invaluable insights into the structural, electronic, and magnetic properties of materials. These facilities excel due to their ability to provide continuously tunable photon energies with high resolution, a broad energy range spanning from infrared photons to hard X-rays, exceptional coherence, and extremely high brilliance.
The Physics of the Accelerating Universe (PAU) camera is an optical narrow band and broad band imaging instrument mounted at the prime focus of the William Herschel Telescope. We describe the image calibration procedure of the PAU Survey data. We rely on an external photometric catalogue to calibrate our narrow band data using stars that have been observed by both datasets.
We present the first clustering measurement of Strong Blended Lyman α (SBLA) absorption systems by measuring their cross-correlation with the Lyman α forest. SBLAs are a new population of absorbers detected within the Lyman α forest. We find a bias of 2.329 ± 0.057, consistent with that of Damped Lyman α absorbers (DLAs). For DLAs, we recover a bias of 2.331 ± 0.057 larger than previously reported.
Reversible carbon–boron bond formation at platinum centers through σ-BH complexes† Pablo Ríos, a Rocío Martín-de la Calle,a Pietro Vidossich,b Francisco José Fernández-de-Córdova,a Agustí Lledós*c and Salvador Conejero *a Abstract A reversible carbon–boron bond formation has been observed in the reaction of the coordinatively unsaturated, cyclometalated, Pt(II) complex [Pt(ItBuiPr′)(ItBuiPr)][BArF], 1, with tricoordinated boranes HBR2.
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