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Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA
We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.2   1.5 consistent with the expected uncertainties. We also develop a new method
The Chandra Deep Field-South: Optical Spectroscopy. I.*
We present the results of our spectroscopic follow-up program of the X-ray sources detected in the 942 ks exposure of the Chandra Deep Field-South (CDFS). A total of 288 possible counterparts were
Chandra Deep Field South: The 1 Ms Catalog
In this paper we present the source catalog obtained from a 942 ks exposure of the Chandra Deep Field South (CDFS), using the Advanced CCD Imaging Spectrometer (ACIS-I) on the Chandra X-ray
The Chandra Deep Field-South: The 1 Million Second Exposure*
We present the main results from our 940 ks observation of the Chandra Deep Field-South using the source catalog described in an accompanying paper by Giacconi et al. We extend the measurement of
The size evolution of galaxies since z~3: combining SDSS, GEMS, and FIRES
We present the evolution of the luminosity-size and stellar mass-size relations of luminous ( L-V greater than or similar to 3.4 x 10(10) h(70)(-2) L-circle dot) and massive ( M-* greater than or
New Results from the X-Ray and Optical* Survey of the Chandra Deep Field-South: The 300 Kilosecond Exposure. II.
We present results from 300 ks of X-ray observations of the Chandra Deep Field-South. The field of the four combined exposures is now 0.1035 deg2, and we reach a flux limit of 10-16 ergs s-1 cm-2 in
RECENT STRUCTURAL EVOLUTION OF EARLY-TYPE GALAXIES : SIZE GROWTH FROM z = 1 TO z = 0
Strong size and internal density evolution of early-type galaxies between -->z ~ 2 and the present has been reported by several authors. Here we analyze samples of nearby and distant ( -->z ~ 1)
Tracing the Large-Scale Structure in the Chandra Deep Field South
We report the discovery of large-scale structures of X-ray sources in the 1 Ms observation of the Chandra Deep Field South. Two main structures appear as narrow (?z 0.02) spikes in the source
Hubble space telescope and Spitzer imaging of red and blue galaxies at z 2.5: a correlation between size and star formation activity from compact quiescent galaxies to extended star-forming galaxies
We present HST NICMOS+ACS and Spitzer IRAC+MIPS observations of 41 galaxies at 2 < z < 3.5 in the FIRES MS 1054 field with red and blue rest-frame optical colors. About half of the galaxies are very
A classic type 2 QSO
In the Chandra Deep Field-South 1 Ms exposure, we have found, at redshift 3.700 ± 0.005, the most distant type 2 active galactic nucleus ever detected. It is the source with the hardest X-ray
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