Figure 4 from Radio Variability of a Fermi Large Area Telescope Bright Source 0FGL J1847.8+3223

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Radio Variability of a Fermi Large Area Telescope Bright Source 0FGL J1847.8+3223

Authors: S. Kida, K. Niinuma, K. Tekefuji, T. Tanaka, T. Aoki, K. Asuma, S. Nakagawa, H. Uehara, H. Akamatsu, A. Imai, H. Miyata, J. Ikouga, A. Otsubo, K. Odai, R. Kodama, Y. Takanashi, N. Nakamizo, Y. Yamada, R. Hiruma, N. Furukawa, N. Matsumura, and T. Daishido

KIDA et al. 2010 The Astrophysical Journal Letters 714 L36.

Provider: AAS Journals

Caption: Figure 4.

Top: the gamma-ray light curve of B2 1846+32A measured above 100 MeV with the EGRET and the Fermi LAT. Bottom: the radio light curve of B2 1846+32A taken with Greenbank, VLA, and WASEDA NASU at 1.4 GHz between 1983 and 2005. The radio light curve is in a rising state before the Fermi observations.

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