Light curves and Spectra

Here, we present pre-reduced data of our monitoring program. The data reduction is constantly in progress and new results are posted progressively. The plots below are for illustration purposes only. Note: Fermi-GST/LAT publicly accessible light curves can be found, here.

The data shown here (in any of the available formats) are strictly  and solely for visualization of the corresponding source’s activity. They are by NO MEANS meant to be used in publications or other public usage without the written permission of the F-GAMMA team.  If you are interested in any data sharing, do not hesitate to contact: E. Angelakis.

More sources are here.

Source Sample

Our present sample comprises a list of about 60 potential Fermi gamma-ray sources. They often are 'famous', quite strong and flat-spectrum (EGRET) blazars which will also be the target of future, intensive broad-band campaigns planned by the Fermi/LAT AGN team including also other facilities (e.g. Swift, RXTE, Suzaku, Chandra, XMM, Integral, Spitzer). Furthermore, many of these sources are also regularly observed by VLBI, i.e. are part of (i) the MOJAVE VLBI monitoring program (M. L. Lister & D. C. Homan, 2005), (ii) the Boston 43 GHz VLBA monitoring program (e.g. S. G. Jorstad & A. P. Marscher 2005) and/or (iii) a new GMVA 3 mm-VLBI program.