Young, star-forming galaxies can be characterized by their strong Lyman-α emission. An overdensity of such a population in one region of the sky is believed to mark a forming proto-cluster. An enhancement of submillimetre galaxies near the core of this proto-cluster, and a large-scale correlation between the submillimetre galaxies and the low-mass Lyman-a emitters suggests synchronous formation of the two different types of star-forming galaxies.
- Yoichi Tamura
- Kotaro Kohno
- Ryohei Kawabe