One of the major unresolved questions in astronomy is: how do galaxies form and evolve? In the local universe we can distinguish between actively star-forming and quiescent galaxies. Quiescent galaxies are typically the most massive, with elliptical morphologies and red optical colors. The mechanisms that cause star-formation in galaxies to be turned off, so that star-forming galaxies become quiescent, are not yet well understood. Using the FourStar Galaxy Evolution Survey (ZFOURGE), comprising near-infrared data of over seventy thousand galaxies, we aim to find and study the first quiescent galaxies. First we describe the data products of ZFOURGE. Then we present the discovery of 15 very massive quiescent galaxies over 12 billion years ago...
In this thesis, we measure for the first time the projected shapes of large samples of distant early...
This thesis explores the theoretical and observational properties of distant massive galaxies that h...
Galaxies in the local Universe are characterized by blue, star-forming disk galaxies, and red, massi...
Galaxies are systems in which stars are formed out of gas and dust. In each galaxy, millions to hund...
One of the major unresolved questions in astronomy is: how do galaxies form and evolve? In the local...
This thesis is devoted to the study of the properties of high-redsfhit galaxies in the epoch 1 < z <...
We investigate the buildup of galaxies from various vantage points. The first two chapters focus on ...
Galaxy clusters mainly grow through mergers with other clusters and groups. Major mergers give rise ...
One of the important properties of galaxies is their sizes which correlate with their stellar masses...
This thesis investigates the nature of distant red galaxies in the early universe in search for mass...
Galaxies grow by accreting gas, which they need to form stars, from their surrounding haloes. These ...
We constrain the stellar population properties of a sample of 52 massive galaxies - with stellar mas...
While galaxies formed stars most actively around z=2, or ~3 Gyr after the Big Bang, when the univers...
Stars, and collections of stars, encode rich signatures of stellar physics and galaxy evolution. Wit...
Deep surveys have allowed us to precisely chart the evolution of galaxies from billions of years ago...
In this thesis, we measure for the first time the projected shapes of large samples of distant early...
This thesis explores the theoretical and observational properties of distant massive galaxies that h...
Galaxies in the local Universe are characterized by blue, star-forming disk galaxies, and red, massi...
Galaxies are systems in which stars are formed out of gas and dust. In each galaxy, millions to hund...
One of the major unresolved questions in astronomy is: how do galaxies form and evolve? In the local...
This thesis is devoted to the study of the properties of high-redsfhit galaxies in the epoch 1 < z <...
We investigate the buildup of galaxies from various vantage points. The first two chapters focus on ...
Galaxy clusters mainly grow through mergers with other clusters and groups. Major mergers give rise ...
One of the important properties of galaxies is their sizes which correlate with their stellar masses...
This thesis investigates the nature of distant red galaxies in the early universe in search for mass...
Galaxies grow by accreting gas, which they need to form stars, from their surrounding haloes. These ...
We constrain the stellar population properties of a sample of 52 massive galaxies - with stellar mas...
While galaxies formed stars most actively around z=2, or ~3 Gyr after the Big Bang, when the univers...
Stars, and collections of stars, encode rich signatures of stellar physics and galaxy evolution. Wit...
Deep surveys have allowed us to precisely chart the evolution of galaxies from billions of years ago...
In this thesis, we measure for the first time the projected shapes of large samples of distant early...
This thesis explores the theoretical and observational properties of distant massive galaxies that h...
Galaxies in the local Universe are characterized by blue, star-forming disk galaxies, and red, massi...