The Cosmic Evolution Survey (COSMOS) is an astronomical survey designed to probe the formation and evolution of galaxies as a function of both cosmic time (redshift) and the local galaxy environment. The survey covers a 2 square degree equatorial field with spectroscopy and X-ray to radio imaging by most of the major space-based telescopes and a number of large ground based telescopes. Over 2 million galaxies are detected, spanning 75% of the age of the Universe. COSMOS is led by Caitlin Casey, Jeyhan Kartaltepe, and Vernesa Smolcic and involves more than 200 scientists in a dozen countries. More information on the COSMOS team members can be found here.
Galaxy groups and clusters are important systems for cosmology and galaxy evolution. The COSMOS survey has offered a unique data set to study the evolution of galaxy groups and clusters as well as their constituent galaxies.
In the latest contribution to this project, Dr. Gozaliasl and his collaborators provide a catalog of X-ray selected groups and clusters based on XMM and deep Chandra observations which offer an unprecedented spatial resolution in X-ray.
The brightest and most massive galaxies in the universe, the Brightest Cluster Galaxies (BCGs), tell a unique story of galaxy evolution. Today, BCGs are quiescent ellipticals hosted in relaxed galaxy clusters, with pasts fraught with mergers and high star formation rates (SFRs).
In a recent publication, Cooke et al. investigate how this active past may depend on local environment by estimating star formation in BCG progenitors in the COSMOS field out to a redshift of z ~ 3 (more than 11 billion years in the past). To estimate star formation rates, they fit progenitor observations with various models from the far-ultraviolet to far-infrared wavelengths. They find that BCG progenitors gain stellar mass in three phases, with effects due to local environment manifesting at z < 1.25 (9 billion years in the past).
The image shows the stellar mass growth of of galaxies in the field (meaning isolated) in blue and dense environments (meaning in clusters) in red.
For more information, check out the full paper!
The Hyper Suprime-Cam (HSC) team made the second data release public!
The HSC on the 8-meter Subaru telescope in Hawaii also covers the COSMOS field. The increased depth in the g, r, i, z, and Y-band in DR2 is crucial for the study of the first galaxies in our universe. But it doesn't stop there - also galaxies that cease their star-formation can be studied in detail with these data.
The increase in depth is stunning - between 0.7 and 1.7 AB magnitudes with new limiting magnitudes of (depth of old observations in parenthesis) 28.4 (27.6) , 28.0 (27.0), 27.7 (26.9), 27.1 (26.4), and 26.6 (24.9) in g, r, i, z, and Y-band, respectively.
The image shows a comparison of the previous Suprime-Cam data (right) vs. HSC DR2 data(left) in I-band on a small field of COSMOS. Note the much deeper imaging of HSC DR2 (also compare the insets).
More information on the HSC data release 2: https://hsc-release.mtk.nao.ac.jp/doc/index.php/tools-2/