We have conducted a systematic search for stellar disk truncations in disk-like galaxies at intermediate redshift (z<1.1) using the Hubble Ultra Deep Field (UDF) data. We use the position of the truncation as a direct estimator of the size of the stellar disk. After accounting for the surface brightness evolution of the galaxies, our results suggest that the radial position of the truncations has increased with cosmic time by ~1-3 kpc in the last ~8 Gyr. This result indicates a small to moderate (~25%) inside-out growth of the disk galaxies since z~1
We determine the abundance of i'-band drop-outs in the recently-released HST/ACS Hubble Ultra Deep F...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dime...
Aims. Galaxy scaling relations such as the Tully-Fisher relation (between the maximum rotation veloc...
We have conducted a systematic search for stellar disk truncations in disklike galaxies at intermedi...
We have conducted a systematic search for stellar disk truncations in disklike galaxies at intermedi...
We report here the first evidence for stellar disk truncation at high redshift, based on surface pho...
We report here the first evidence for stellar disk truncation at high redshift, based on surface pho...
We report here the first evidence for stellar disk truncation at high redshift, based on surface ph...
We report here the finding that some stellar disks at high redshift are truncated at a shorter radiu...
In the light of several recent developments we revisit the phenomenon of galactic stellar disk-trunc...
The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular momen...
Thin and thick disks are found in most spiral galaxies, yet their formation scenarios remain uncerta...
<p>The stellar disk size of a galaxy depends on the fraction of the dark-halo mass settled as disk s...
The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular momen...
We analyze the redshift- and luminosity-dependent sizes of dropout galaxy candidates in the redshift...
We determine the abundance of i'-band drop-outs in the recently-released HST/ACS Hubble Ultra Deep F...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dime...
Aims. Galaxy scaling relations such as the Tully-Fisher relation (between the maximum rotation veloc...
We have conducted a systematic search for stellar disk truncations in disklike galaxies at intermedi...
We have conducted a systematic search for stellar disk truncations in disklike galaxies at intermedi...
We report here the first evidence for stellar disk truncation at high redshift, based on surface pho...
We report here the first evidence for stellar disk truncation at high redshift, based on surface pho...
We report here the first evidence for stellar disk truncation at high redshift, based on surface ph...
We report here the finding that some stellar disks at high redshift are truncated at a shorter radiu...
In the light of several recent developments we revisit the phenomenon of galactic stellar disk-trunc...
The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular momen...
Thin and thick disks are found in most spiral galaxies, yet their formation scenarios remain uncerta...
<p>The stellar disk size of a galaxy depends on the fraction of the dark-halo mass settled as disk s...
The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular momen...
We analyze the redshift- and luminosity-dependent sizes of dropout galaxy candidates in the redshift...
We determine the abundance of i'-band drop-outs in the recently-released HST/ACS Hubble Ultra Deep F...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dime...
Aims. Galaxy scaling relations such as the Tully-Fisher relation (between the maximum rotation veloc...