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.
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- PKS 2149-758: Dutka et al.
2012
- Several: Abdo et al.
2010
- Centaurus A: Abdo et al., 2010
- PKS 2052-47: Chang et al.
2009
- PKS 1454-354: Abdo et al.
2009
The Master Thesis of Felicia Krauss contains several blazar SEDs of TANAMI sources.
Other AGN SED studies that use TANAMI data are, e.g.:
