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1. The Nd150 ( He3 , t ) and Sm150 ( t , He3 ) reactions with applications to ββ decay of Nd150

   https://doi.org/10.1103/PhysRevC.83.064318  

   Guess, C. J. ; Adachi, T. ; Akimune, H. ; Algora, A. ; Austin, Sam M. ; Bazin, D. ; Brown, B. A. ; Caesar, C. ; Deaven, J. M. ; Ejiri, H. ; et al ( June 2011 , Physical Review C)
2. Crystal and molecular structure of 4-fluoro-1 H -pyrazole at 150 K

   https://doi.org/10.1107/S2056989023003055  

   Ahmed, Basil M. ; Zeller, Matthias ; Mezei, Gellert ( May 2023 , Acta Crystallographica Section E Crystallographic Communications)

   Only two 4-halo-1H-pyrazole crystal structures are known to date (chloro and bromo, the structure of 4-iodo-1H-pyrazole has not been reported yet). The triclinic structure of 4-fluoro-1H-pyrazole, C₃H₃FN₂(P\overline{1}), reported here is not isomorphous with those of the chloro and bromo analogues (which are isomorphous, orthorhombicPnma). To avoid sublimation during the measurement, diffraction data were collected at 150 K. Two crystallographically unique 4-fluoro-1H-pyrazole moieties linked by an N—H...N hydrogen bond are found in the asymmetric unit. Unlike the trimeric supramolecular motifs found in the structures of the chloro and bromo analogues, 4-fluoro-1H-pyrazole forms one-dimensional chains by intermolecular hydrogen bonding in the crystal.

    

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3. Loss rates for high- n, 49≲n≲150, 5sns ( S13 ) Rydberg atoms excited in an Sr84 Bose-Einstein condensate

   https://doi.org/10.1103/physreva.102.063317  

   Kanungo, S. K. ; Whalen, J. D. ; Lu, Y. ; Killian, T. C. ; Dunning, F. B. ; Yoshida, S. ; Burgdörfer, J. ( December 2020 , Physical Review A)

   null (Ed.)
4. Quantum Interference between Light Sources Separated by 150 Million Kilometers

   https://doi.org/10.1103/PhysRevLett.123.080401  

   Deng, Yu-Hao ; Wang, Hui ; Ding, Xing ; Duan, Z.-C. ; Qin, Jian ; Chen, M.-C. ; He, Yu ; He, Yu-Ming ; Li, Jin-Peng ; Li, Yu-Huai ; et al ( August 2019 , Physical Review Letters)
5. Cosmology Large Angular Scale Surveyor (CLASS): pointing stability and beam measurements at 90, 150, and 220 GHz

   https://doi.org/10.1117/12.2630649  

   Datta, Rahul ; Brewer, Michael K. ; Denes Couto, Jullianna D. ; Eimer, Joseph R. ; Li, Yunyang ; Xu, Zhilei ; Appel, John W. ; Bustos, Ricardo ; Chuss, David ; Cleary, Joseph ; et al ( August 2022 , Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI)

   Zmuidzinas, Jonas ; Gao, Jian-Rong (Ed.)

   The Cosmology Large Angular Scale Surveyor (CLASS) telescope array surveys 75% of the sky from the Atacama desert in Chile at frequency bands centered near 40, 90, 150, and 220 GHz. CLASS measures the largest-angular scale (θ ≳ 1 ° ) CMB polarization with the aim of constraining the tensor-to-scalar ratio, r, measuring the optical depth to reionization, τ , to near the cosmic variance limit, and more. The CLASS Q-band (40 GHz), W-band (90 GHz), and dichroic high frequency (150/220 GHz) telescopes have been observing since June 2016, May 2018, and September 2019, respectively. On-sky optical characterization of the 40 GHz instrument has been published. Here, we present preliminary on-sky measurements of the beams at 90, 150, and 220 GHz, and pointing stability of the 90 and 150/220 GHz telescopes. The average 90, 150, and 220 GHz beams measured from dedicated observations of Jupiter have full width at half maximum (FWHM) of 0.615±0.019° , 0.378±0.005° , and 0.266 ± 0.008° , respectively. Telescope pointing variations are within a few % of the beam FWHM. 

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