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THE FUV TO NEAR-IR MORPHOLOGIES OF LUMINOUS INFRARED GALAXIES IN THE GOALS SAMPLE

2014 The Astronomical Journal 148 111.

  • Provider: AAS Journals

Caption: Figure 7.

The four panels on the left show the G-M20 values for the FUV rest-frame redshifted images. For each redshift bin, we connect the G-M20 values from an objectʼs lower redshift (gray) to its higher redshift (open circles) as defined in the legend. The two panels on the right show the average G and M20 values with simulated redshift (black circles). The vertical lines span the minimum and maximum values for that redshift bin. The dashed and solid lines illustrate the trend for G to decrease and flatten with increasing redshift, while M20 remains relatively stable.

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