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THE 2014 ALMA LONG BASELINE CAMPAIGN: OBSERVATIONS OF ASTEROID 3 JUNO AT 60 KILOMETER RESOLUTION

  • Authors: T. R. Hunter, R. Kneissl, A. Moullet, C. L. Brogan, E. B. Fomalont, C. Vlahakis, Y. Asaki, D. Barkats, W. R. F. Dent, R. E. Hills, A. Hirota, J. A. Hodge, C. M. V. Impellizzeri, E. Liuzzo, R. Lucas, N. Marcelino, S. Matsushita, K. Nakanishi, L. M. Pérez, N. Phillips, A. M. S. Richards, I. Toledo, R. Aladro, D. Broguiere, J. R. Cortes, P. C. Cortes, D. Espada, F. Galarza, D. Garcia-Appadoo, L. Guzman-Ramirez, A. S. Hales, E. M. Humphreys, T. Jung, S. Kameno, R. A. Laing, S. Leon, G. Marconi, A. Mignano, B. Nikolic, L.-A. Nyman, M. Radiszcz, A. Remijan, J. A. Rodón, T. Sawada, S. Takahashi, R. P. J. Tilanus, B. Vila Vilaro, L. C. Watson, T. Wiklind, I. De Gregorio-Monsalvo, J. Di Francesco, J. Mangum, H. Francke, J. Gallardo, J. Garcia, S. Gonzalez, T. Hill, T. Kaminski, Y. Kurono, C. Lopez, F. Morales, K. Plarre, S. Randall, T. van kempen, L. Videla, E. Villard, P. Andreani, J. E. Hibbard, and K. Tatematsu

2015 The Astrophysical Journal Letters 808 L2.

  • Provider: AAS Journals

Caption: Figure 3.

Residual images of Planck brightness temperature (﹩{T}_{B}﹩) in equatorial offset coordinates created by removing a model image of uniform brightness from the images in Figure 2. The open circle indicates the location of the subsolar point. The color scale range is ±30 K with respect to the median values of ﹩{T}_{B}﹩ in column 8 of Table 2. The south pole drawn is the same as in Figure 1, and the sense of rotation is clockwise. The different position angle here is due to the combination of the coordinate system, the foreshortening effect of the heavily inclined pole, and the significant heliocentric latitude.

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