When the supermassive black holes at the center of galaxies accrete material, they can eject powerful jets of charged particles at speeds approaching that of light. These particles in turn emit radiation across the electromagnetic spectrum, from radio to gamma-rays. When the jets happen to be aligned toward the Earth, these objects are called blazars, and in a flare they can emit as much radiation as a million billion suns.
NASA’s Fermi Gamma Ray Astronomy satellite, launched in 2008, has detected many bright gamma-ray sources, but determining what they are and if any are blazars is difficult because Fermi’s resolution on the sky is only about the size of a quarter full moon, and that large area of sky typically contains many sources that could be emitting in the gamma-rays. Moreover, blazars are notoriously variable at high energies and their irregular flickering can make them difficult to pinpoint exactly. Extensive observations of possible candidates with optical or other facilities can be successful but are very time consuming.
A team of astronomers including CfA astronomers Raffaele D’Abrusco and Howard Smith found that the infrared colors of blazars are generally unique because the emission, rather than from hot dust as is typical, is instead coming from processes associated with the blazar jets. They used color data from the Wide-field Infrared Survey Explorer (WISE) in conjunction with catalogs of radio source to identify the most promising gamma-ray candidate objects in the Fermi survey and for the past several years have followed them up, with a success rate confirming blazars of about 90 percent.
The same team of astronomers has now extended their original 2014 work using all the most recent data collected by Fermi and a new algorithm for analyzing the WISE data, and have produced two new catalogs of WISE blazar candidates with a total of 15,120 candidate sources. The new work will enable many more detailed followup analyses of gamma-ray blazars, as well as other kinds of blazars. The gamma-ray sky is known to reflect, in its dramatic appearance, many other kinds of extreme physical processes, for example possible dark matter annihilation activity in some scenarios, and the new catalogs will enable a much more complete investigation of the dominant contributor to the gamma-ray universe: blazars.
Provided by: Harvard-Smithsonian Center for Astrophysics
More information: Raffaele D’Abrusco et al. Two new catalogs of blazar candidates in the WISE infrared sky. astro-ph.HE (2019). arxiv.org/abs/1903.11124
Image: An artist’s conception of the Fermi Gamma-Ray Astronomy spacecraft in orbit. Astronomers using infrared observations to help identify Fermi blazar sources amongst the many candidates in a Fermi field-of-view have published two new catalogs of gamma-ray blazars.