I knew the Fermi Gamma-ray Space Telescope would be good for something. Not only did it discover the first pulsar that blinks only in gamma-rays instead of the usual radio waves, it has discovered a total of 16 of them so far, and not doubt it will discover many more. And the gamma-ray telescope has not been in orbit for even a year yet!
Einstein@Home is a distributed computing project that has been helping LIGO sift through data from its laser-interferometry based gravitational wave detector. Now it is also sifting through data from the Arecibo radio telescope to search for radio pulsars orbiting around very heavy objects such as another neutron star or even a black hole. It will not only provide more indirect observations for gravitational waves like what was provided by the first binary pulsars discovered, but it will also reveal potential candidates where gravitational waves could be measured directly with gravitational wave observatories.
Pulsars are rapidly spinning neutron stars which emit beams of light, which can include radio waves, visible light, and even X-rays, from the magnetic poles powered by the neutron star's powerful rotation. We see pulsars as they seemingly "blink" on and off with extreme regularity as the beam rotates and points to our direction once every rotation. In fact, the regularity had astronomers thinking they may have discovered signals from an extraterritorial intelligence when pulsars were first discovered. Most pulsars discovered before now "blinked" in radio waves.
Via the Bad Astronomer, we hear news that the Fermi Gamma-ray Space Telescope has discovered a new kind of pulsar, one which only "blinks" in gamma-rays. One speculation is that it's not really a different kind of pulsar, but rather that the gamma-ray beam is more broader than the radio wave beam so that we only see it "blinking" in gamma-rays. This strikes me as odd since I would have thought it would be the other way around. Whatever the case may be, it's mind-blowing to consider the amounts of energy the pulsar must be emitting.