TANAMI - Archive - Radio to Gamma-Ray SEDs
TANAMI data in the radio band at 8.4GHz and 22.3GHz are being used
to compile multiwavelength SEDs of blazars and other extragalactic
jets. Our team is conducting optical/UV/X-ray observations of TANAMI
sources with the Swift
satellite. Most TANAMI sources are also bright Gamma-Ray sources and
monitored by Fermi.
Below are four examples of blazar SEDs compiled by the Fermi/LAT team (Abdo
et al. 2010, ApJ 716, 30) that make use of TANAMI data.