Table 1
UV-optical-IR data in COSMOS2025.
| Instrument/Telescope (Survey) | Band | Central a λ [Å] | Width b [Å] | Depth c | PSF FWHM [arcsec] | Aper/Total d ratio |
|---|---|---|---|---|---|---|
| NIRCam | F115W | 11 622 | 2646 | 27.2 | 0.08 | 0.65 |
| F150W | 15 106 | 3348 | 27.4 | 0.08 | 0.64 | |
| F277W | 28 001 | 6999 | 28.1 | 0.15 | 0.45 | |
| F444W | 44 366 | 11 109 | 28.0 | 0.19 | 0.27 | |
| MIRI | F770W | 77 108 | 20 735 | 25.2 | 0.32 | 0.61 |
| MegaCam/CFHT | u* | 3858 | 598 | 27.3 | 0.86 | 0.53 |
| ACS/HS T | F814W | 8333 | 2511 | 27.5 | 0.13 | 0.46 |
| HSC/Subaru | g | 4847 | 1383 | 27.6 | 0.94 | 0.53 |
| r | 6219 | 1547 | 27.2 | 0.87 | 0.52 | |
| HSC-SSP | i | 7699 | 1471 | 27.0 | 0.81 | 0.56 |
| PDR3 | z | 8894 | 766 | 26.6 | 0.78 | 0.59 |
| y | 9761 | 786 | 26.0 | 0.92 | 0.51 | |
| NB0816 | 8168 | 110 | 26.0 | 0.83 | 0.52 | |
| NB0921 | 8168 | 133 | 26.0 | 0.79 | 0.57 | |
| NB1010 | 10 100 | 94 | 24.2 | 0.92 | 0.50 | |
| Suprime-Cam/Subaru | IB427 | 4266 | 207 | 25.7 | 1.03 | 0.53 |
| IA484 | 4851 | 229 | 26.2 | 1.02 | 0.53 | |
| IB505 | 5064 | 231 | 25.9 | 1.02 | 0.53 | |
| IA527 | 5261 | 243 | 26.1 | 1.02 | 0.53 | |
| IB574 | 5766 | 273 | 25.3 | 1.04 | 0.51 | |
| IA624 | 6232 | 300 | 26.1 | 1.02 | 0.54 | |
| IA679 | 6780 | 336 | 25.3 | 1.02 | 0.53 | |
| IB709 | 7073 | 316 | 25.7 | 1.02 | 0.53 | |
| IA738 | 7361 | 324 | 25.8 | 1.02 | 0.53 | |
| IA767 | 7694 | 365 | 25.3 | 1.02 | 0.53 | |
| IB827 | 8243 | 343 | 25.3 | 1.03 | 0.53 | |
| NB711 | 7121 | 72 | 25.2 | 1.02 | 0.54 | |
| NB816 | 8150 | 120 | 25.3 | 1.03 | 0.53 | |
| VIRCAM/VISTA UltraVISTA DR6 | Y | 10 216 | 923 | 25.8 | 1.11 | 0.41 |
| J | 12 525 | 1718 | 25.8 | 0.98 | 0.51 | |
| H | 16 466 | 2905 | 25.5 | 0.92 | 0.52 | |
| Ks | 21 557 | 3074 | 25.3 | 0.90 | 0.51 | |
| NB118 e | 11 909 | 112 | 25.1 | 1.04 | 0.51 | |
| IRAC/Spitzer | ch1 e | 35 686 | 7443 | 26.4 | 2.13 | 0.19 |
| ch2 e | 45 067 | 10119 | 26.3 | 2.15 | 0.19 | |
| ch3 e | 57 788 | 14 082 | 23.2 | 2.55 | 0.05 | |
| ch4 e | 79 958 | 28 796 | 23.1 | 2.33 | 0.20 | |
Notes. a Median of the transmission curve. b Full width of the transmission curve at half maximum. c 5σ depth computed in empty apertures with diameters of 1.0″ for the ground-based instruments, 0.15″ for the space-based JWST/NIRCam and HST/ACS, and 0.5″ for JWST/MIRI images, averaged over the NIRCam area. No aperture correction is applied. d Aperture-to-total flux ratio for a point source, using the corresponding aperture size for each band. e Not used in SED fitting.
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