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.

(a)

F140W is used if it is available.

(b)

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

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