More Like this

1. 35 challenges in materials science being tackled by PIs under 35(ish) in 2021

   https://doi.org/10.1016/j.matt.2021.11.003  

   Aguado, Brian; Bray, Laura J.; Caneva, Sabina; Correa-Baena, Juan-Pablo; Di Martino, Giuliana; Fang, Chengcheng; Fang, Yin; Gehring, Pascal; Grosso, Gabriele; Gu, Xiaodan; et al (December 2021, Matter)
2. Putative Pore Structures of Amyloid β 25–35 in Lipid Bilayers

   https://doi.org/10.1021/acs.biochem.3c00323  

   Dutta, Ankita; Sepehri, Aliasghar; Lazaridis, Themis (September 2023, Biochemistry)
3. The cost of ectoparasitism in Cliff Swallows declines over 35 years

   https://doi.org/10.1002/ecm.1446  

   Brown, Charles R.; Hannebaum, Stacey L.; O’Brien, Valerie A.; Page, Catherine E.; Rannala, Bruce; Roche, Erin A.; Wagnon, Gigi S.; Knutie, Sarah A.; Moore, Amy T.; Brown, Mary B. (May 2021, Ecological Monographs)
4. The Arecibo Pisces-Perseus Supercluster Survey: Declination Strip 35

   McMichael, Chelsey; Ribaudo, Joseph; Koopmann, Rebecca A.; Haynes, Martha P.; APPSS Team, Undergraduate ALFALFA (January 2018, American Astronomical Society, AAS Meeting)

   The Arecibo Pisces-Perseus Supercluster Survey (APPSS) will provide strong observational constraints on the mass-infall rate onto the main filament of the Pisces-Perseus Supercluster. The survey data consist of HI emission-line spectra of cluster galaxy candidates, obtained primarily at the Arecibo Observatory (with ALFA as part of the ALFALFA Survey and with the L-Band Wide receiver as part of APPSS observations). Here we present the details of the data reduction process and spectral-analysis techniques used to determine if a galaxy candidate is at a velocity consistent with the Supercluster, as well as the detected HI-flux and rotational velocity of the galaxy, which will be used to estimate the corresponding HI-mass. We discuss the results of a preliminary analysis on a subset of the APPSS sample, corresponding to 98 galaxies located within ~1.5° of DEC = +35.0°, with 65 possible detections. We also highlight several interesting emission-line features and galaxies discovered during the reduction and analysis process and layout the future of the APPSS project. This work has been supported by NSF grants AST-1211005 and AST-1637339. 

   more » « less
5. Tachykinin Neuropeptides and Amyloid β (25–35) Assembly: Friend or Foe?

   https://doi.org/10.1021/jacs.2c03845  

   Liu, Xikun; Ganguly, Pritam; Jin, Yingying; Jhatro, Michael J.; Shea, Joan-Emma; Buratto, Steven K.; Bowers, Michael T. (August 2022, Journal of the American Chemical Society)