This plot displays the layouts of JWST MIRI observations completed by March 2024 for five HST extragalactic deep field surveys. These observations have integrated data from multiple programs, covering a total area of approximately 0.21 square degrees and encompassing at least 2 to 6 MIRI broad bands (with only the F770W band shown in the plot).

Below is a detailed breakdown of the MIRI imaging observations sources for each field:

l  COSMOS 

MIRI imaging observations for the COSMOS field were obtained from the following programs:

Program 1727 (PIs: Jeyhan Kartaltepe and Caitlin Casey)

Program 1837 (PI: James Dunlop)

l  EGS 

For the EGS field, MIRI imaging observations were sourced from:

Program 1345 (PI: Steven Finkelstein)

l  GOODS-N 

For the GOODS-N field, MIRI imaging observations were sourced from:

Program 1181 (PI: Daniel Eisenstein)

Program 1264 (PI Luis Colina Robledo).

l  GOODS-S 

For the GOODS-S field, MIRI imaging observations were sourced from:

Program 1180 (PI: Daniel Eisenstein)

Program 1207 (PI George Rieke)

Program 1283 (PI: Göran Östlin)

Program 2516 (PIs: Jacqueline Hodge and Elisabete da Cunha)

l  UDS 

Lastly, for the UDS field, MIRI imaging observations were sourced from:

Program 1837 (PI: James Dunlop)