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Survey Description

The Fourstar Galaxy Evolution Survey (ZFOURGE) was conducted using the FourStar imager (Persson et al. 2013) on the 6.5m Magellan Baade telescope at Las Campanas Observatory. The use of medium-band filters in the near-IR (van Dokkum et al. 2009) allows for accurate sampling at wavelengths that bracket the Balmer break of galaxies leading to more well-constrained photometric redshifts at 1 < z < 4 than with broadband filters alone. In conjunction with existing optical through mid-IR photometry, this dataset provides a comprehensive sampling of the 0.3 – 8 micron spectral energy distribution of galaxies.

ZFOURGE is composed of three 11′ x 11′ pointings with coverage in the CDFS (Giacconi et al. 2002), COSMOS (Capak et al. (2007) and UDS (Lawrence et al. 2007). The 5sigma depth in a circular aperture of D=0.6” in the Ks band is 26.2-26.5 in the CDFS, COSMOS and UDS fields respectively at a typical seeing of ~0.4″. For more information regarding ZFOURGE consult Straatman et al. (2016).


5 sigma AB magnitude depths (CDFS, COSMOS, UDS; D=0.6” apertures)

J1 25.6 26.0 25.6
J2 25.5 26.0 25.9
J3 25.5 25.7 25.6
Hs 24.9 25.1 25.1
Hl 25.0 24.9 25.2
Ks 26.2-26.5 25.5 25.7

Ks depths correspond to a co-addition of the Fourstar imaging with public Ks-band imaging.


[Field] [Coordinates] [Total Survey Area] [Number of Objects] [Kband FWHM]
CDFS [03 32 27, -27 45 52] [128 sq. arcmin] [30911] [0.46”]
COSMOS [10 00 31, +02 17 03] [135 sq. arcmin] [20786] [0.47”]
UDS [02 17 15, -05 11 53] [189 sq. arcmin] [22093] [0.44”]
Survey of a figure 4
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