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- Publications
- Influence
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies
- K. Noeske, B. Weiner, +40 authors Spitzer Science Center
- Physics
- 31 January 2007
We analyze star formation (SF) as a function of stellar mass (M☉) and redshift z in the All-Wavelength Extended Groth Strip International Survey. For 2905 field galaxies, complete to 10^10(10^10.8 )M… Expand
Mid-Infrared Selection of Active Galaxies
- D. Stern, P. Eisenhardt, +15 authors Noao
- Physics
- 21 October 2004
Mid-infrared photometry provides a robust technique for identifying active galaxies. While the ultraviolet to mid-infrared (λ 5 μm) continuum of stellar populations is dominated by the composite… Expand
Black Hole Masses and Eddington Ratios at 0.3 < z < 4
- J. Kollmeier, C. Onken, +12 authors Jpl
- Physics
- 30 August 2005
We study the distribution of Eddington luminosity ratios, Lbol/LEdd, of active galactic nuclei (AGNs) discovered in the AGN and Galaxy Evolution Survey (AGES). We combine Hβ, Mg II, and C IV line… Expand
A SPITZER-SELECTED GALAXY CLUSTER AT z = 1.62
- C. Papovich, I. Momcheva, +26 authors C. Saclay
- Physics
- 16 February 2010
We report the discovery of a galaxy cluster at z = 1.62 located in the Spitzer Wide-Area Infrared Extragalactic survey XMM-LSS field. This structure was selected solely as an overdensity of galaxies… Expand
Star Formation in AEGIS Field Galaxies since z = 1.1: Staged Galaxy Formation and a Model of Mass-dependent Gas Exhaustion
We analyze star formation (SF) as a function of stellar mass (M☉) and redshift z in the All-Wavelength Extended Groth Strip International Survey, for star-forming field galaxies with M* ≳ 10^10 M☉… Expand
UBIQUITOUS OUTFLOWS IN DEEP2 SPECTRA OF STAR-FORMING GALAXIES AT z = 1.4
Galactic winds are a prime suspect for the metal enrichment of the intergalactic medium (IGM) and may have a strong influence on the chemical evolution of galaxies and the nature of QSO… Expand
The Hubble Deep Field-North SCUBA Super-map - IV. Characterizing submillimetre galaxies using deep Spitzer imaging
We present spectral energy distributions (SEDs), Spitzer colours, and infrared (IR) luminosities for 850-μm selected galaxies in the Great Observatories Origins Deep Survey Northern (GOODS-N) field.… Expand
CANDELS: The Progenitors of Compact Quiescent Galaxies at z ~ 2
We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to track the evolution of structure and activity of massive (M > 1010 M ?) galaxies at redshifts z =… Expand
The Major and Minor Galaxy Merger Rates at z < 1.5
- J. Lotz, P. Jonsson, +11 authors Jpl
- Physics
- 11 August 2011
Calculating the galaxy merger rate requires both a census of galaxies identified as merger candidates, and a cosmologically-averaged‘observability’ timescale hTobs(z)ifor identifying galaxy mergers.… Expand
The Stellar Mass Tully-Fisher Relation to z=1.2
- S. Kassin, B. Weiner, +17 authors U. Berkeley
- Physics
- 1 December 2006
We combine newly measured rotation velocities, velocity dispersions, and stellar masses to construct stellar mass Tully-Fisher relations (M*TFRs) for 544 galaxies with strong emission lines at 0.1 <… Expand
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