Table 2

Wave bands used to derive the UV continuum slope for individual galaxies.

Redshift Mean Filters Rest-frame
range redshift wavelengths (Å)
(1) (2) (3) (4)

2.90 ≦ zsp ≦ 4.44 3.6 F775W, F850LP, F105W 1700−2300
4.44 <zsp ≦ 5.58 4.9 F105W, F125W, F140Wa 1800−2100 (1800−2400)b
5.58 <zsp ≦ 6.66 6.0 F125W, F140Wa, F160W 1800−2200

Notes. (1) Spectroscopic redshift ranges of the three redshift bins. (2) Mean redshift of each redshift bin. (3) HST filters used to estimate UV continuum slopes. (4) Typical rest-frame wavelengths probed by UV continuum slopes.


F140W is used if it is available.


Value in the parenthesis is the wavelength range in the case that F140W is available.

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