Image Details

Choose export citation format:

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 7.

ALMA images of ASXDF1100.053.1 and 231.1. First column: Cleaned ALMA 1100 μm continuum images taken in ALMA Cycles 1 and 2. Synthesized beams of the combined data are 0.″46 × 0.″35 (PA, 69°) and 0.″57 × 0.″48 (PA, 82°) for ASXDF1100.053.1 and 231.1, respectively. Contours are shown at 5, 10, 15, 20, and 25σ. The flux density unit is mJy beam−1. The rms noise level is shown at the bottom in each panel. Second column: Clean component maps of the combined ALMA images are shown in the middle panel. The clean component maps were obtained by cleaning down to 1σ. Third column: Synthesized beams for the combined ALMA images. Fourth column: Residual maps after subtracting the clean components convolved with the synthesized beams. The pixel scale is 0.″05 in all images.

Other Images in This Article

Show More

Copyright and Terms & Conditions