Figure 6 from NO EVIDENCE OF INTRINSIC OPTICAL/NEAR-INFRARED LINEAR POLARIZATION FOR V404 CYGNI DURING ITS BRIGHT OUTBURST IN 2015: BROADBAND MODELING AND CONSTRAINT ON JET PARAMETERS

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NO EVIDENCE OF INTRINSIC OPTICAL/NEAR-INFRARED LINEAR POLARIZATION FOR V404 CYGNI DURING ITS BRIGHT OUTBURST IN 2015: BROADBAND MODELING AND CONSTRAINT ON JET PARAMETERS

Authors: Y. T. Tanaka, R. Itoh, M. Uemura, Y. Inoue, C. C. Cheung, M. Watanabe, K. S. Kawabata, Y. Fukazawa, Y. Yatsu, T. Yoshii, Y. Tachibana, T. Fujiwara, Y. Saito, N. Kawai, M. Kimura, K. Isogai, T. Kato, H. Akitaya, M. Kawabata, T. Nakaoka, K. Shiki, K. Takaki, M. Yoshida, M. Imai, S. Gouda, Y. Gouda, H. Akimoto, S. Honda, K. Hosoya, A. Ikebe, K. Morihana, T. Ohshima, Y. Takagi, J. Takahashi, K. Watanabe, D. Kuroda, T. Morokuma, K. Murata, T. Nagayama, D. Nogami, Y. Oasa, and K. Sekiguchi

2016 The Astrophysical Journal 823 35.

Provider: AAS Journals

Caption: Figure 6.

Left: broadband spectrum of V404 Cyg in ﹩\nu -\nu {F}_{\nu }﹩ representation. The Kanata/HONIR and Swift/XRT fluxes were quasi-simultaneously observed on MJD 57193, while RATAN-600 and INTEGRAL data were not simultaneous. One-zone synchrotron and SSC emissions are also drawn by solid red and blue lines, respectively. The black dashed line indicates the optically thick synchrotron emission from an outer jet, with a spectral shape of ﹩{F}_{\nu }\propto {\nu }^{0}﹩. Right: same as the left panel, but for the quasi-simultaneous Kanata/HONIR and Swift/XRT fluxes observed on MJD 57194.

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