![f6 f6](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/f6.png)
![Screen-Shot-2018-05-31-at-6.39.14-PM Stellar mass in wave lengths](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/Screen-Shot-2018-05-31-at-6.39.14-PM.png)
![Cowley2018_1 ZFOURGE catalogues to construct two independent samples based on the mass-progenitors of the present-day Milky Way (MW) and Andromeda galaxy (M31)](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/Cowley2018_1.png)
![qfrac_delta-eps-converted-to-1024x401 Quiescent fraction versus overdensity in three different redshift ranges for two mass-selected samples.](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/qfrac_delta-eps-converted-to-1024x401-1.jpg)
![Forrest2017_2 Projected spatial density in all three ZFOURGE fields of the galaxies in the redshift range 3.42⩽z⩽3.56 and brighter than Ks](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2017/03/Forrest2017_2.png)
![allen2017_1 Galaxy stellar mass−size distributions for star-forming galaxies for redshifts 1](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/allen2017_1.jpg)
![figure1 CDFS, COSMOS, and UDS wavelengths](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/figure1.png)
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]
![forrest_composites Figure 2 of composite SEDs (colored points) are constructed from de-redshifted and scaled photometry of many galaxies (gray points).](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/forrest_composites.png)
![cowley-agn Infrared (top), X-ray (bottom-left) and radio (bottom-right) AGN hosts identified in ZFOURGE.](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2016/01/cowley-agn.png)
![Rees_2015_4 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.](https://zfourge.tamu.edu/wp-content/uploads/sites/8/2020/06/Rees_2015_4.png)
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]
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]
1 2