The spectroscopic component of the High Latitude Wide Area Survey measures redshifts of tens of millions of galaxies via grism spectroscopy using the WFI over at least a 1700 deg2 region that overlaps the region.
Credit Data provided by Z. Zhai and Y. Wang (Caltech/IPAC); Data Visualization/J. DePasquale and D. Player (STScI)
A candidate for a galaxy at z≈9.6, magnified by a factor of ~15 by the foreground cluster MACSJ1149+2223 (z ≈ 0.54). The object was found in an HST survey using the WFC3IR camera (Zheng et al. 2012). This young object is seen when the universe is only about 500 million years old.
This figure illustrates the power of Roman’s wide field for studying galaxy clusters. In 2000 square degrees, the High Latitude Wide Area Survey will observe some 200 Abell clusters and a much larger number of more distant galaxy clusters. (Note: Purple circle represents estimated halo size of Rubin’s galaxy)
[Credit] Hubble callout of Rubin’s Galaxy/ NASA, ESA, and B. Holwerda (University of Louisville); Background Image/DSS; Image Composition/J. DePasquale (STScI)
A composite figure shows the region of Andromeda covered by the Roman Space Telescope simulation. It would be able to image the main body of Andromeda in just a few pointings, surveying the galaxy nearly 1500 times faster than Hubble. Credit: GSFC/SVS