Identification of a Novel Subset of Human Airway Epithelial Basal Stem Cells.

The basal cell maintains the airway's respiratory epithelium as the putative resident stem cell. Basal cells are known to self-renew and differentiate into airway ciliated and secretory cells. However, it is not clear if every basal cell functions as a stem cell.

Impacts of Heterogeneous Chemistry on Vertical Profiles of Martian Ozone.

We show a positive vertical correlation between ozone and water ice using a vertical cross-correlation analysis with observations from the ExoMars Trace Gas Orbiter's Nadir and Occultation for Mars Discovery instrument. This is particularly apparent during  = 0°-180°, Mars Year 35 at high southern latitudes, when the water vapor abundance is low. Ozone and water vapor are anti-correlated on Mars; Clancy et al.

Micelle-Based Nanocarriers for Targeted Delivery of Cargo to Pancreas.

Innovations in the field of amphiphilic block copolymers have led to the development of a series of attractive polymer-based drug and gene delivery micellar formulations. The amphiphilic block copolymers' low critical micelle concentration (CMC) results in highly stable nanoscale micelles possessing favorable in vivo safety profiles and biocompatibility, making them an excellent carrier choice for the systemic administration of various poorly soluble drugs. These micelles can also be used as an actively targeted drug delivery system.

Targeted delivery of harmine to xenografted human pancreatic islets promotes robust cell proliferation.

Type 1 diabetes (T1D) occurs as a consequence of the autoimmune destruction of insulin-producing pancreatic beta (β) cells and commonly presents with insulin deficiency and unregulated glycemic control. Despite improvements in the medical management of T1D, life-threatening complications are still common. Beta-cell replication to replace lost cells may be achieved by using small-molecule mitogenic drugs, like harmine.

Vertical Aerosol Distribution and Mesospheric Clouds From ExoMars UVIS.

The vertical opacity structure of the martian atmosphere is important for understanding the distribution of ice (water and carbon dioxide) and dust. We present a new data set of extinction opacity profiles from the NOMAD/UVIS spectrometer aboard the ExoMars Trace Gas Orbiter, covering one and a half Mars Years (MY) including the MY 34 Global Dust Storm and several regional dust storms. We discuss specific mesospheric cloud features and compare with existing literature and a Mars Global Climate Model (MGCM) run with data assimilation.