Astrophys. J. 699, 649–666 (2009)

How does one find dwarves in a crowd of giants? Evgenya Shkolnik at the Carnegie Institution of Washington in Washington DC and her colleagues searched X-ray data gathered by the now-defunct German satellite ROSAT for nearby M-class dwarf stars less than 300 million years old.

Previous surveys placed greater emphasis on higher mass, higher luminosity Sun-like stars. The team identified 185 likely candidates before ruling out older interlopers by spectroscopy. The 144 remaining, some as small as 10% of the mass of the Sun, have a better chance than easier-to-spot, higher-mass stars of revealing the early formation of rocky Earth-like planets.

If any of the dwarves do host planets, their proximity to Earth (most are within 25 parsecs) will make them relatively easy to study in detail.