Publications

Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1 < z < 4

Forrest et al. 2018, The Astrophysical Journal
[Summary] [ADS] [arxiv]

Stellar mass in wave lengths

The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function

Papovich et al. 2018, The Astrophysical Journal
[Summary] [ADS] [arxiv]

ZFOURGE catalogues to construct two independent samples based on the mass-progenitors of the present-day Milky Way (MW) and Andromeda galaxy (M31)

Decoupled black hole accretion and quenching: the relationship between BHAR, SFR and quenching in Milky Way- and Andromeda-mass progenitors since z = 2.5

Cowley et al. 2018, Monthly Notices of the Royal Astronomical Society
[Summary] [ADS] [arxiv]

Quiescent fraction versus overdensity in three different redshift ranges for two mass-selected samples.

Effect of Local Environment and Stellar Mass on Galaxy Quenching and Morphology at 0.5 < z < 2.0

Kawinwanichakij et al. 2017, The Astrophysical Journal
[Summary] [ADS] [arxiv]

Projected spatial density in all three ZFOURGE fields of the galaxies in the redshift range 3.42⩽z⩽3.56 and brighter than Ks

Discovery of Extreme [OIII]+Hβ Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South

Forrest et al. 2017, Astrophysical Journal Letters
[Summary] [ADS] [arxiv]

Galaxy stellar mass−size distributions for star-forming galaxies for redshifts 1

The Size Evolution of Star-forming Galaxies since z~7 Using ZFOURGE

Allen et al. 2017, Astrophysical Journal Letters
[Summary] [ADS] [arxiv]

CDFS, COSMOS, and UDS wavelengths

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

Straatman et al. 2016, Astrophysical Journal Supplements
[Summary] [arxiv] [Media] [Animation] [TAMU News Release]

Figure 2 of composite SEDs (colored points) are constructed from de-redshifted and scaled photometry of many galaxies (gray points).

UV to IR Luminosities and Dust Attenuation Determined from ~4000 K-Selected Galaxies at 1 < z < 3 in the ZFOURGE Survey

Forrest et al. 2016, Astrophysical Journal Letters
[Summary] [ADS] [astro-ph]

Infrared (top), X-ray (bottom-left) and radio (bottom-right) AGN hosts identified in ZFOURGE.

ZFOURGE catalogue of AGN candidates: an enhancement of 160μm-derived star-formation rates in active galaxies to z = 3.2

Cowley et al. 2015, Astrophysical Journal
[Summary] [ADS] [astro-ph]

Low redshifts radio-AGN hosts are typically found in quiescent galaxies but above a redshift of 1.5 they become predominantly found in star-forming galaxies with high dusts contents.

Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25

Rees et al. 2016, Monthly Notices of the Royal Astronomical Society
[Summary] [ADS] [Arxiv]

95% Stellar mass-completeness limit vs. redshift computed for quiescent galaxies in three datasets.

Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5

Kawinwanichakij et. al. 2015, Astrophysical Journal
[Summary] [ADS] [astro-ph]

tomczak-2015-Fig7-leftonly

The SFR-M* Relation and Empirical Star-Formation Histories from ZFOURGE at 0.5 < z < 4

Tomczak et al. 2016, Astrophysical Journal
[Summary] [ADS] [astro-ph] [media] [table 1]

The quiescent galaxies have high stellar mass densities.

The sizes of massive quiescent and star forming galaxies at z~4 with ZFOURGE and CANDELS

Straatman et al. 2015, Astrophysical Journal Letters
[Summary] [ADS] [Arxiv]

Mass-size relation for our sample of quiescent (left) and star-forming (right) field and cluster galaxies at z = 2.1.

The Differential Size Growth of Field and Cluster Galaxies at z = 2.1 Using the ZFOURGE Survey

Allen et al. 2015, The Astrophysical Journal
[Summary] [ADS] [astro-ph]

False-color imaging shows the approximate rest-frame U, B, V-band (blue, green, red, respectively) using CANDELS imaging.

ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z = 3 to 0.5

Papovich et al. 2015, Astrophysical Journal
[Summary] [ADS] [astro-ph] [TAMU Press Release] [STScI Press Release]

The difference in satellite content is made clearer by inspecting the cumulative number of satellites.

The distribution of satellites around massive galaxies at 1< z < 3 in ZFOURGE/CANDELS: dependence on star formation activity

Kawinwanichakij et al. 2014, The Astrophysical Journal
[Summary] [astro-ph] [ADS]

Observed stacked SEDs for the mass-limited z = 3 - 4 ZFOURGE galaxies.

Exploring the z=3-4 massive galaxy population with ZFOURGE: the prevalence of dusty and quiescent galaxies

Spitler et al. 2014, Astrophysical Journal Letters
[Summary] [astro-ph] [ADS] [Summary Image]

Representative examples of the spectral energy distributions of the quiescent galaxies.

A substantial population of massive quiescent galaxies at z~4 from ZFOURGE

Straatman et al., 2014, Astrophysical Journal Letters
[Summary] [MQ/AAO] [astro-ph] [ADS] [media] [Dutch Press Release]

zfourge smfs publications

Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies

Tomczak et al. 2014, Astrophysical Journal
[Summary] [astro-ph] [ADS] [media]

UV luminosity function of galaxies at z~7.

Discovery of Lyman Break Galaxies at z~7 from the ZFOURGE Survey

Tilvi et al. 2013, Astrophysical Journal
[Summary] [astro-ph] [ADS]

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