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