Speaker
Dr
Cristina Sbarra
(INFN-PD & Bologna University)
Description
We present the results of the analysis of Markarian 180 (1ES 1133+704), a BL Lac object embedded in a giant elliptical galaxy, obtained for a period of 45 days, during which multiwavelenght observations were on going. The Mrk 180 is associated to a quasar- like object whose distance can be determined unambiguously, thanks to the well done measurement of absorption line that gives the redshift (z=0.046; Ulrich 1978).
The source Mrk 180 was observed for 45 days, during which it was possible to discovery a change of emissivity, at the energies 100 MeV – 300 GeV. Results of the analysis are shown.
Primary author
Dr
Cristina Sbarra
(INFN-PD & Bologna University)
Co-authors
Dr
Denis Bastieri
(INFN-PD & Padova University)
Dr
Luigi Tibaldo
(INFN-PD & Padova University)
Dr
Riccardo Rando
(INFN-PD & Padova University)
Dr
Sara Buson
(INFN-PD & Padova University)
