Figure 5 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 5.

Left: quasi-simultaneous (within 1 hr) ﹩\nu -{F}_{\nu }﹩ plotted measurements of V404 Cyg observed by Kanata/HONIR and Swift/XRT on MJD 57193. The simultaneous K_s- and R-band fluxes measured during the orphan K_s-band flare are shown with magenta stars. Right: same as the left panel, but for the Kanata/HONIR and Swift/XRT data taken on MJD 57194. Also shown in both panels are preliminary nonsimultaneous 2.4–21.7 GHz RATAN-600 fluxes from Trushkin et al. (2015a). For illustrative purposes only, dashed lines indicating various spectral indices (﹩\alpha =0﹩ and −1.0 in both, plus additional ﹩\alpha =0.2﹩ in left panel; ﹩{F}_{\nu }\propto {\nu }^{\alpha }﹩) are shown.

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