HST F160W Imaging of Very Massive Galaxies at $1.5<z<3.0$: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates

We present a targeted follow-up Hubble Space Telescope WFC3 F160W imaging study of very massive galaxies $(\log(M_{\rm{star}}/M_{\odot})> 11.2)$ selected from a combination of ground-based near-infrared galaxy surveys (UltraVISTA, NMBS-II, UKIDSS UDS) at $1.5

Keywords:

• Extrapolation
• imaging study
• Universe
• Astrophysics
• theoretical models
• Number density
• Population
• Physics
• Galaxy
• Stellar mass

• Correction
• Source
• Cite
• Save
• Machine Reading By IdeaReader