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Phibss: Molecular Gas, Extinction, Star Formation, and Kinematics in the z = 1.5 Star-forming Galaxy EGS13011166

  • Authors: R. Genzel, L. J. Tacconi, J. Kurk, S. Wuyts, F. Combes, J. Freundlich, A. Bolatto, M. C. Cooper, R. Neri, R. Nordon, F. Bournaud, A. Burkert, J. Comerford, P. Cox, M. Davis, N. M. Förster Schreiber, S. García-Burillo, J. Gracia-Carpio, D. Lutz, T. Naab, S. Newman, A. Saintonge, K. Shapiro Griffin, A. Shapley, A. Sternberg, and B. Weiner

Genzel et al. 2013 The Astrophysical Journal 773 68.

  • Provider: AAS Journals

Caption: Figure 2.

Comparison of images. Top row: integrated CO flux map in color (ABC-configurations, 0 farcs7 × 0 farcs8 FWHM) and (left) WFC3 HST H-band map as white contours, ~0 farcs3 FWHM; (center) inferred stellar mass distribution from SED fitting white contours, 0 farcs75 FWHM; and (right) extinction-corrected star formation rate distribution inferred from SED fitting (white contours, 0 farcs75 resolution). Bottom row: (left) CO-integrated flux map in white contours (AB-configuration, 0 farcs56 × 0 farcs68 FWHM) and HST WFC3 H-band map (red, 0 farcs3 FWHM) and ACS V-band map (green, 0 farcs3 FWHM), (center) CO-integrated flux map in white contours, (AB-configuration, 0 farcs56 × 0 farcs68 FWHM) and HST A V-map (red, 0 farcs35 FWHM) and (right) ACS V-band map (blue, 0 farcs35 FWHM). (Right) HST ACS V-band (green), and A V-map in white contours and stellar mass map (red), both inferred from SED modeling. All HST maps are smoothed to 0 farcs35 FWHM. The pixel scale is 0 farcs06.

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