Table 1
Characteristics of the Euclid bands simulated for the high-redshift survey.
|
S 45 | S 15 | ZP | NEA | |
| Band | (nm) | (AB/arcsec2) | (mAB for 1e−/ s) | (arcsec2) | |
|
|
|||||
| y | 1048 | 22.47 | 22.75 | 24.03 | 0.56 |
| J | 1263 | 22.44 | 22.72 | 24.08 | 0.61 |
| H | 1658 | 22.31 | 22.60 | 24.74 | 0.77 |
Notes. Columns include: central wavelength, sky brightness (in AB magnitudes/arcsec2) at two separations from the ecliptic poles (45° and 15°), zero-points (for AB magnitudes and fluxes in e−/ s), and Noise Equivalent Area (NEA) of the PSF (defined by Eq. (A.1)). This is the area over which one integrates the sky background fluctuations when performing PSF photometry for faint sources, accounting for pixelisation at 0.3′′/pixel. The reported NEA values were averaged over source position within the central pixel.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.