Okay, let's look at a typical net article. This one is from April 18th 2014:
A better than 50/50 chance Kepler-186f has technological life.
The article goes into a lot of detail about how the signals are detected and analyzed. However, let's look at the planet itself.
It orbits the star, Kepler 186, which is a type M1 red dwarf.
The only stars that are expected to have life are F, G, and K. Our sun is type G which is in the middle of this range. Stars half the mass of our sun would require the planets to be in so close that they would get tide-locked. And, stars more than 1.5x the mass of our sun burn too hot and fast. BTW, when I suggested that the habitable zone extended from Earth to Mars, that is for a type G. It would be in a little closer with type K and out a bit farther with type F.
So, based on the star alone we can assume there is zero chance that Kepler 186f has life. But, let's look at the planet itself.
Kepler 186f is about 1.15 Earth radii or about 30-60% more mass. So, with a sun like ours it would need to be a little farther out in its orbit.
Kepler 186 only has 4% as much solar radiation as our sun. So, you would need an orbit of about 0.2 AU. Kepler 186f is at 0.38 AU which would make it too far away if it were Earth sized. However, the extra mass makes it about right. However, with an orbit at about where Mercury is, this planet would be tide locked. This may not make sense to everyone. Basically, the star is about half the sun's mass so gravity is about half. However, since gravity is the inverse square of the distance, you get 1/0.38^2 = 7. Divide by two and you get 3.5X the gravitational attraction that the Earth gets. This would tide lock the planet.