The Complete Spitzer Survey of Stellar Structure in Galaxies (CS4G)

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Table 1

Survey and instrument properties.

Survey	Galaxies	Scale	FWHM	Depth
IRAC	44	0ʹ.ʹ600	2ʹ.ʹ1	26.8
IRAC ^(a)	11	0ʹ.ʹ750	2ʹ.ʹ1	26.8
DES	102	0ʹ.ʹ263	0ʹ.ʹ9	28.4
LS	169	0ʹ.ʹ263 ^(b)	1ʹ.ʹ0	27.9
SDSS	77	0ʹ.ʹ396	1ʹ.ʹ1	26.4
LT	15	0ʹ.ʹ150	1ʹ.ʹ4	28.3
NTT	3	0ʹ.ʹ241	1ʹ.ʹ2	27.6
HST	1	0ʹ.ʹ050	0ʹ.ʹ1	27.5

Notes. The depth column represents the surface brightness limit [3σ, 10ʺ × 10ʺ] in units of mag arcsec⁻². ^(a)For this set of galaxies, the IRAC images are from S⁴ G fields. ^(b)For 41 galaxies, the mosaics have a pixel scale of 0ʹ.ʹ269.

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