ALT A four-panel line graph showing spectral flux versus wavelength in micrometers. The y-axis on all panels is labeled "Flux F_lambda 10^(-17) W/m^2/micron" and the x-axis is "Wavelength micron". Each of the four panels focuses on a different wavelength range (approximately 0.95-1.1, 1.2-1.35, 1.5-1.65, and 2.0-2.2 microns). The graphs contain multiple colored spectral lines (black, red, cyan, and light gray) displaying various peaks and troughs. Text labels with chemical formulas are placed above specific spectral features across the panels, pointing out the absorption or emission bands of H2O, NH3, H2, and CH4, often appearing in combinations (e.g., NH3+H2, H2O+NH3) at their characteristic wavelengths.

ALT A large, face-on spiral galaxy, IC 5332, dominates the left side of the image against the deep blackness of space. The galaxy features a glowing, compact yellow-white central core with delicate, feathery spiral arms winding gracefully outward. These symmetric arms are intricately laced with dark dust lanes and dotted with vibrant pink and purple clusters of active star formation. The surrounding background is densely populated by a "blizzard" of countless smaller, distant galaxies of various shapes, sizes, and brightnesses, alongside a few prominent, brilliant foreground stars.

ALT A deep space composite image from Gemini North and ALMA showing a gravitational lens against a pitch-black background. At the center is a bright, glowing reddish-orange foreground galaxy. Wrapping tightly around the top of this central galaxy is a thin, curved yellow-gold arc of light, which is the distorted, lensed image of a more distant star-forming galaxy nicknamed 'Shadow Blaster.' Directly to the lower right of the main red galaxy sits a small, distinct, bright blue cosmic object. A few other faint, blurry orange and reddish background galaxies are loosely scattered in the upper-left and lower-left areas of the frame.