Simulating JWST deep extragalactic imaging surveys and physical parameter recovery

Open Access

Table 1.

Summary of the JWST imaging data in CEERS and the HUDF – limiting magnitudes.

Name	Area ^(a)	NIRCam									MIRI
	[arcmin²]	F090W	F115W	F150W	F200W	F277W	F335M	F356W	F410M	F444W	F560W	F770W
CEERS_1	96.8	–	28.7	28.9	29.1	29.2	–	29.2	–	28.7	–	–
CEERS_2	4.6	–	28.7	28.9	29.1	29.2	–	29.2	–	28.7	25.9	25.9
HUDF_1	4.7	29.9	30.3	30.3	30.3	30.6	29.9	30.5	29.9	30.1	–	–
HUDF_2	2.3	29.9	30.3	30.3	30.3	30.6	29.9	30.5	29.9	30.1	28.1	–

Notes. The magnitudes are 5σ point-source limits measured in 0.2″ and 0.6″ diameter apertures for NIRCam and MIRI, respectively.

^(a)

The configurations without MIRI include the area of the configurations with MIRI.

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