This plot displays the layouts of JWST NIRCam 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 0.72 square degrees and encompassing at least 4 to 8 NIRCam broad bands (with only the F444W band shown in the plot).

 

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

 

l  COSMOS 

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

 

Program 1727 (PIs: Jeyhan Kartaltepe and Caitlin Casey)

Program 1810 (PI: Sirio Belli)

Program 1837 (PI: James Dunlop)

Program 1840 (PIs: Javier Alvarez-Marquez and Takuya Hashimoto)

Program 2321 (PI: Philip Best)

Program 2514 (PIs: Christina Williams and Pascal Oesch)

Program 3990 (PIs: Takahiro Morishita, Charlotte Mason, Tommaso Treu, and Michele Trenti)

Program 6585 (PI: David Coulter)

 

l  EGS 

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

 

Program 1345 (PI: Steven Finkelstein)

Program 2234 (PI: Eduardo Banados)

Program 2279 (PI: Rohan Naidu)

Program 2514 (PI: Christina Williams) 

Program 2750 (PI: Pablo Arrabal Haro)

Program 3990 (PI:Takahiro Morishita)

 

l  GOODS-N 

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

 

Program 1181 (PI: Daniel Eisenstein)

Program 1895 (PI: Pascal Oesch)

Program 2514 (PI: Christina Williams) 

Program 2674 (PI: Pablo Arrabal Haro)

Program 3577 (PIs: Eiichi Egami and Fengwu Sun)

 

l  GOODS-S 

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

 

Program 1176 (PI: Rogier Windhorst)

Program 1180 (PI: Daniel Eisenstein)

Program 1210 (PI: Nora Luetzgendorf)

Program 1283 (PI: Göran Östlin)

Program 1286 (PI: Nora Luetzgendorf)

Program 1895 (PI: Pascal Oesch)

Program 1963 (PIs: Christina Williams, Michael Maseda, and Sandro Tacchella)

Program 2079 (PIs: Steven Finkelstein, Casey Papovich, and Norbert Pirzkal)

Program 2198 (PIs: Laia Barrufet and Pascal Oesch)

Program 2514 (PI: Christina Williams) 

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

Program 3215 (PIs: Daniel Eisenstein and Roberto Maiolino)

Program 3990 (PI: Takahiro Morishita)

Program 6541 (PI: Eiichi Egami)

 

l  UDS 

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

 

Program 1837 (PI: James Dunlop)

Program 2514 (PI: Christina Williams) 

Program 3990 (PI: Takahiro Morishita)