The FourStar Galaxy Evolution Survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z~3.5

Abstract

The FourStar galaxy evolution survey (ZFOURGE) is a 45 night legacy program with the FourStar near-infrared camera on Magellan and one of the most sensitive surveys to date. ZFOURGE covers a total of $400{\mathrm{arcmin}}^2$ in cosmic fields CDFS, COSMOS and UDS, overlapping CANDELS. We present photometric catalogs comprising $>70,000$ galaxies, selected from ultradeep $K_s$-band detection images ($25.5-26.5$ AB mag, $5\sigma$, total), and $>80\%$ complete to $K_s<25.3-25.9$ AB. We use 5 near-IR medium-bandwidth filters ($J_1,J_2,J_3,H_s,H_l$) as well as broad-band $K_s$ at $1.05-2.16\mu m$ to $25-26$ AB at a seeing of $\sim 0.5$". Each field has ancillary imaging in $26-40$ filters at $0.3-8\mu m$. We derive photometric redshifts and stellar population properties. Comparing with spectroscopic redshifts indicates a photometric redshift uncertainty ${\sigma }_z=0.010,0.009$, and 0.011 in CDFS, COSMOS, and UDS. As spectroscopic samples are often biased towards bright and blue sources, we also inspect the photometric redshift differences between close pairs of galaxies, finding ${\sigma }_{z,pairs}=0.01-0.02$ at $1<z<2.5$. We quantify how ${\sigma }_{z,pairs}$ depends on redshift, magnitude, SED type, and the inclusion of FourStar medium bands. ${\sigma }_{z,pairs}$ is smallest for bright, blue star-forming samples, while red star-forming galaxies have the worst ${\sigma }_{z,pairs}$. Including FourStar medium bands reduces ${\sigma }_{z,pairs}$ by 50\% at $1.5<z<2.5$. We calculate SFRs based on ultraviolet and ultradeep far-IR $Spitzer$/MIPS and Herschel/PACS data. We derive rest-frame $U-V$ and $V-J$ colors, and illustrate how these correlate with specific SFR and dust emission to $z=3.5$. We confirm the existence of quiescent galaxies at $z\sim 3$, demonstrating their SFRs are suppressed by $>\times 15$.

arXiv comment39 pages, 35 figures, accepted for publication in ApJ, full data release available at http://zfourge.tamu.edu/

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• A PAH deficit in the starburst core of a distant spiral galaxy
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
• Compact [OIII] emission-line regions ("Green Seeds") in $\mathrm{H}\alpha$ emitters at Cosmic Noon from JWST Observations
• The Physical Properties of Star-Forming Galaxies with Strong [O III] Lines at z=3.25
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Ciii]$\lambda 1909$ emission as an alternative to Ly$\alpha$ in the reionization era: the dependence of Ciii] and Ly$\alpha$ at $3<z<4$ from the VANDELS survey
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• Extensive Lensing Survey of Optical and Near-Infrared Dark Objects (El Sonido): HST H-Faint Galaxies behind 101 Lensing Clusters
• The extension of the Fundamental Metallicity Relation beyond the BPT star-forming sequence: evidence for both gas accretion and starvation
• Introducing the FLAMINGOS-2 Split-K Medium Band Filters: The Impact on Photometric Selection of High-z Galaxies in the FENIKS-pilot survey
• Low star-formation activity and low gas content of quiescent galaxies at $z=$ 3.5-4.0 constrained with ALMA