Table 1.
Specs of the broadband surveys used in the analysis.
λobs | zLyα |
![]() |
Jνobs | ![]() |
|
---|---|---|---|---|---|
[Å] | [″/px] | [Jy/sr] | [Jy2/sr2] | ||
ULTRASAT | [2300, 2900] | [0.9, 1.4] | 5.45 | 264 | 422 |
GALEX | [1350, 1750] | [0.1, 0.4] | 5 (50) | 237 | 1959 |
[1750, 2800] | [0.4, 1.3] | 79 |
Notes. ULTRASAT specs are from Shvartzvald et al. (2024); GALEX specs are from Martin et al. (2005). The redshift range zLyα is computed for the Lyα line λLyα = 1216 Å; other parts of the UV spectrum are shifted to different ranges. We indicate both the pixel scale Lpix and (in parenthesis) the effective scale of the pixels used in Sect. 4. The monopole Jνobs and the variance are estimated using Eqs. (10) and (2), respectively.
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