Figure 8 from Extremely Red Submillimeter Galaxies: New z ≳ 4–6 Candidates Discovered Using ALMA and Jansky VLA

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Extremely Red Submillimeter Galaxies: New z ≳ 4–6 Candidates Discovered Using ALMA and Jansky VLA

Authors: Soh Ikarashi, R. J. Ivison, Karina I. Caputi, Kouichiro Nakanishi, Claudia D. P. Lagos, M. L. N. Ashby, Itziar Aretxaga, James S. Dunlop, Bunyo Hatsukade, David H. Hughes, Daisuke Iono, Takuma Izumi, Ryohei Kawabe, Kotaro Kohno, Kentaro Motohara, Kouji Ohta, Yoichi Tamura, Hideki Umehata, Grant W. Wilson, Kiyoto Yabe, and Min S. Yun

2017 The Astrophysical Journal 835 286.

Provider: AAS Journals

Caption: Figure 8.

ALMA uv-distance vs. amplitude plots of ASXDF1100.053.1 and 231.1. Black solid points are the observed data. Binning sizes in uv distance are 100 kλ out to 500 kλ and 500 kλ between 500 and 1500 kλ. The black line is a uv-amp model of the best-fit Gaussian component. The blue line and shaded area are possible solutions for the corrected source size, with errors based on Monte Carlo simulations.

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