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1. Thermophysical properties of additively manufactured (AM) GRCop-42 and GRCop-84

   https://doi.org/10.1016/j.mtcomm.2023.106665  

   Chen, Yehong; Zeng, Congyuan; Ding, Huan; Emanet, Selami; Gradl, Paul R.; Ellis, David L.; Guo, Shengmin (August 2023, Materials Today Communications)
2. Stress localization investigation of additively manufactured GRCop-42 thin-wall structure

   https://doi.org/10.1016/j.tws.2024.112022  

   Sahoo, Subhadip; Keleshteri, Mohammad M; Mayeur, Jason R; Hazeli, Kavan (August 2024, Thin-Walled Structures)
3. The ⁴¹ Ar(n,y) ⁴² Ar reaction

   https://doi.org/10.1051/epjconf/202328401037  

   Sahoo, R. N.; Paul, M.; Köster, U.; Scott, R.; Tessler, M.; Zylstra, A.; Avila, M. L.; Dickerson, C.; Jayatissa, H.; Kohen, M.S.; et al (January 2023, EPJ Web of Conferences)

   Mattoon, C.M.; Vogt, R.; Escher, J.; Thompson, I. (Ed.)

   The cross-section of the thermal neutron capture⁴¹Ar(n,γ)⁴²Ar(t_1/2=32.9 y) reaction was measured by irradiating a⁴⁰Ar sample at the high-flux reactor of Institut Laue-Langevin (ILL) Grenoble, France. The signature of the two-neutron capture has been observed by measuring the growth curve and identifying the 1524.6 keV γ-lines of the shorter-lived⁴²K(12.4 h) β⁻daughter of⁴²Ar. Our preliminary value of the⁴¹Ar(n,γ)⁴²Ar thermal cross section is 240(80) mb at 25.3 meV. For the first time, direct counting of⁴²Ar was performed using the ultra-high sensitivity technique of noble gas accelerator mass spectrometry (NOGAMS) at Argonne National Laboratory, USA. 

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4. N -Amino peptide scanning reveals inhibitors of Aβ ₄₂ aggregation

   https://doi.org/10.1039/D0RA02009E  

   Tillett, Khalilia C.; Del Valle, Juan R. (April 2020, RSC Advances)

   The aggregation of amyloids into toxic oligomers is believed to be a key pathogenic event in the onset of Alzheimer's disease. Peptidomimetic modulators capable of destabilizing the propagation of an extended network of β-sheet fibrils represent a potential intervention strategy. Modifications to amyloid-beta (Aβ) peptides derived from the core domain have afforded inhibitors capable of both antagonizing aggregation and reducing amyloid toxicity. Previous work from our laboratory has shown that peptide backbone amination stabilizes β-sheet-like conformations and precludes β-strand aggregation. Here, we report the synthesis of N -aminated hexapeptides capable of inhibiting the fibrillization of full-length Aβ 42 . A key feature of our design is N -amino substituents at alternating backbone amides within the aggregation-prone Aβ 16–21 sequence. This strategy allows for maintenance of an intact hydrogen-bonding backbone edge as well as side chain moieties important for favorable hydrophobic interactions. An N -amino scan of Aβ 16–21 resulted in the identification of peptidomimetics that block Aβ 42 fibrilization in several biophysical assays. 

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5. XQR-30: Black hole masses and accretion rates of 42 z   ≳  6 quasars

   https://doi.org/10.1051/0004-6361/202346317  

   Mazzucchelli, C.; Bischetti, M.; D’Odorico, V.; Feruglio, C.; Schindler, J.-T.; Onoue, M.; Bañados, E.; Becker, G. D.; Bian, F.; Carniani, S.; et al (August 2023, Astronomy & Astrophysics)

   We present bolometric luminosities, black hole masses, and Eddington ratios for 42 luminous quasars at z  ≳ 6 using high signal-to-noise ratio VLT/X-shooter spectra, acquired as part of the enlarged ESO Large Programme XQR-30 . In particular, we derived the bolometric luminosities from the rest-frame 3000 Å luminosities using a bolometric correction from the literature, as well as the black hole masses by modeling the spectral regions around the C  IV 1549 Å and the Mg  II 2798 Å emission lines, with scaling relations calibrated in the Local Universe. We find that the black hole masses derived from both emission lines are in the same range and the scatter of the measurements agrees with expectations from the scaling relations. The Mg  II -derived masses are between ∼(0.8−12) ×10 9   M ⊙ and the derived Eddington ratios are within ∼0.13−1.73, with a mean (median) of 0.84(0.72). By comparing the total sample of quasars at z  > 5.8, from this work and from the literature, to a bolometric luminosity distribution-matched sample at z  ∼ 1.5, we find that quasars at high redshift host slightly less massive black holes, which accrete slightly more rapidly than those at lower z , with a difference in the mean Eddington ratios of the two samples of ∼0.27. These findings are in agreement with the results of recent works in the literature. 

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