I am currently leading an effort to perform a uniform processing of all archival Hubble Space Telescope imaging and slitless spectroscopy observations relevant for studying distant galaxies (e.g., reasonably high galactic latitudes, avoiding large foreground galaxies, including WFC3/IR).

Full data release forthcoming.

Preliminary imaging mosaics of the CANDELS survey fields including are available below, which include all available ACS/WFC, WFC3/UVIS, and WFC3/IR observations and are precisely aligned to the GAIA DR2 frame.

CANDELS - AEGIS, GOODS-N, GOODS-S, and UDS fields

COSMOS - ACS + WFC3 mosaics of the entire square-degree COSMOS field.

With a generous allocation of Spitzer DDT time in 2019, we are acquiring IRAC imaging of hundreds of extragalactic HST archival fields that are amenable to detecting galaxies at z>8 (Spitzer-DDT-14253, Co-PI Mauro Stefanon @ Leiden).