Table 1.
CEERS survey bands (plus F090W observations) and technical details.
| Camera | Filter | λpivot(μm) | FWHM | PSF enclosed | Point-source Limiting |
|---|---|---|---|---|---|
| Flux (d = 0.2″) | AB magnitude (5σ) | ||||
| JWST/NIRCam SW | F090W | 0.9022 | 0.056″ | 0.70 | 29.06 |
| JWST/NIRCam SW | F115W | 1.1543 | 0.066″ | 0.80 | 29.16 |
| JWST/NIRCam SW | F150W | 1.6592 | 0.070″ | 0.80 | 29.12 |
| JWST/NIRCam SW | F200W | 1.9886 | 0.077″ | 0.76 | 29.32 |
| JWST/NIRCam LW | F277W | 2.7617 | 0.123″ | 0.64 | 29.53 |
| JWST/NIRCam LW | F356W | 3.5684 | 0.142″ | 0.58 | 29.40 |
| JWST/NIRCam LW | F410M | 4.0822 | 0.155″ | 0.56 | 28.70 |
| JWST/NIRCam LW | F444W | 4.4043 | 0.161″ | 0.52 | 29.03 |
| HST/ACS | F435W | 0.4329 | 0.112″ | 0.66 | 28.72 |
| HST/ACS | F606W | 0.5922 | 0.118″ | 0.70 | 28.77 |
| HST/ACS | F814W | 0.8046 | 0.124″ | 0.63 | 28.49 |
| HST/WFC3 | F105W | 1.0550 | 0.235″ | 0.35 | 27.55 |
| HST/WFC3 | F125W | 1.2486 | 0.244″ | 0.33 | 27.67 |
| HST/WFC3 | F140W | 1.3923 | 0.247″ | 0.32 | 26.99 |
| HST/WFC3 | F160W | 1.5370 | 0.254″ | 0.30 | 27.68 |
Notes. The first and second columns list the available instruments and band name, while the third column λpivot shows the pivotal wavelengths expressed in micrometers. The fourth column displays each filter’s FWHM in units of arcseconds, whereas the fifth column contains the PSF enclosed flux in a 0.2″diameter (d) aperture. Finally, we report in the last columns the 5σ depths associated with the CEERS catalog described in Sect. 3, calculated as medians of the 5σ depths in each CEERS pointing for each band (see Table 1 of Finkelstein et al. 2024 for a comprehensive overview). These values were estimated for a point source by utilizing the measured noise function in the field. This was done using an aperture with a 0.2″diameter, with a correction applied to account for the total flux based on the enclosed flux within the PSF of each band.
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