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Table 1

Sample selection.

Filter Wavelength M⊙ Bright limita Mean color Faint limitb MX limitc N(z)d N(color)e N(χ2+color)f
(X) (μm) (AB mag) (AB mag) (X − r) (AB mag) (AB mag)
FUV 0.152 16.02 19.0 5.26 23.0 − 11.5, − 19.5 7678 4931 3985
NUV 0.231 10.18 19.0 4.17 22.0 − 13.4, − 20.0 7948 5355 4260
u 0.356 6.38 19.0 2.22 20.0 − 13.4, − 20.5 10 581 9008 7362
g 0.472 5.15 18.0 0.77 18.5 − 14.4, − 22.0 11 328 10 091 8317
r 0.618 4.71 18.0 0.00 17.8 − 14.4, − 23.0 11 330 11 043 9228
i 0.750 4.56 17.2 –0.34 17.5 − 14.9, − 23.0 11 316 10 981 9179
z 0.896 4.54 17.0 –0.61 17.2 − 15.4, − 23.5 11 115 10 465 8737
Y 1.032 4.52 16.5 –0.78 17.0 − 15.9, − 24.0 10 591 9739 8089
J 1.251 4.57 16.5 –0.92 16.9 − 15.9, − 24.0 10 569 9601 7985
H 1.638 4.71 16.0 –1.05 16.9 − 16.4, − 24.0 10 751 9950 8289
K 2.208 5.19 16.0 –1.01 16.9 − 16.4, − 24.0 10 717 9655 8055
W1 3.379 5.94 16.5 –0.38 17.5 − 15.9, − 23.5 11 230 10 209 8572
W2 4.629 6.61 17.0 0.06 17.8 − 15.4, − 23.0 11 230 9675 8098
W3 12.33 8.40 15.0 0.53 18.0 − 17.4, − 24.5 11 230 8014 6706
W4 22.00 9.10 15.0 3.92 22.0 − 17.4, − 24.5 11 230 10 472 8728

Notes.

(a)

Apparent magnitude limit where the color bias is negligible.

(b)

Adopted apparent magnitude limit used for calculating luminosity and stellar mass functions of galaxies.

(c)

Absolute magnitude range where the luminosity function is reliable.

(d)

Number of galaxies that have detections in respective bands.

(e)

Number of galaxies in different bands after color cuts explained in Sect. 3.2.

(f)

Number of galaxies in different bands after color and χ2 cuts (see Sect. 4 for details).

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