Far-infrared measurements of galaxies in the early Universe would reveal their detailed properties, but have been lacking for the more typical galaxies where most stars form; here an archetypal, early Universe star-forming galaxy is detected at far-infrared wavelengths, allowing its dust mass, total star-formation rate and dust-to-gas ratio to be calculated.
- Darach Watson
- Lise Christensen
- Michał Jerzy Michałowski