Close-in giant exoplanets with temperatures greater than 2,000 K (“ultra-hot Jupiters”) have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble and Spitzer Space Telescopes1–3. However, previous studies have yielded inconsistent results because the small sizes of the spectral features and the limited information content

Doping of perovskite semiconductor1 and passivation of its grain boundaries2 remain challenging but essential for advancing high-efficiency perovskite solar cells. Particularly, that’s crucial to build the perovskite/indium tin oxide (ITO) Schottky contact based inverted devices without pre-depositing a layer of hole-transport material3-5. Here we report a dimethylacridine-based molecular doping process

The extremely rapid assembly of the earliest galaxies during the first billion years of cosmic history is a major challenge for our understanding of galaxy formation physics (1; 2; 3; 4; 5). The advent of JWST has exacerbated this issue by confirming the existence of galaxies in significant numbers as early as the first few hundred million years (6; 7; 8). Perhaps even more surprisingly, in some galaxies

Plasma membrane rupture (PMR) in dying cells undergoing pyroptosis or apoptosis requires the cell-surface protein NINJ11. PMR releases proinflammatory cytoplasmic molecules, collectively called damage-associated molecular patterns (DAMPs), that activate immune cells. Therefore, inhibiting NINJ1 and PMR may limit the inflammation that is associated with excessive cell death. Here we describe an anti-NINJ1

Voltage-gated ion channels (VGICs) comprise multiple structural units whose assembly is required for function1,2. There is scant structural understanding of how VGIC subunits assemble and whether chaperone proteins are required. High-voltage activated calcium channels (CaVs)3,4 are paradigmatic multi-subunit VGICs whose function and trafficking is powerfully shaped by interactions between pore-forming