A HST/WFC3 Multi-cycle Treasury Program, led by Sandy Faber, has been awarded to the AEGIS collaboration. We will now be able to add a chunk of high-resolution, supremely sensitive J and H band imaging and ACS parallels to the fantastic existing sets of data in our favorite regions of sky, including the EGS. In Groth, this will amount to a contiguous region of 3x15 WFC3 tiles or about 200 sq arcmins.

More info can be found at the HST Multi-cycle Treasury Program web page