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Black Hole Growth in a Cosmological Context and the Associated Cosmic Star Formation History
Based on a co-evolution scenario of massive black holes (MBH) and their host spheroids, we trace the BH growth and the joint cosmic star formation... -
Radiative Feedback from Quasars and the Growth of Supermassive Black Holes
We discuss the role of feedback via photoionization and Compton heating in the co-evolution of massive black holes at the center of spheroidal... -
The Influence of Black Hole Mass and Accretion Rate on the FRI/FRII Radio Galaxy Dichotomy
We use medium resolution optical spectra of 3CR radio galaxies to estimate their black hole masses and accretion rates. Black hole masses are found... -
When Supermassive Black Holes Were Growing: Clues from Deep X–ray Surveys
Merging the Chandra and XMM–Newton deep surveys with the previously identified ROSAT surveys a unique sample of almost 1000 AGN–1 covering five... -
The Art and Science of Black Hole Mergers
The merger of two black holes is one of the most extraordinary events in the natural world. Made of pure gravity, the holes combine to form a single... -
Galaxies of 1012 M⊙ at z ≥ 4 Along the K-z Sequence
Stellar masses of galaxies are derived from the K-band (2.2 μm) photometry by taking into account evolution and cosmological effects with the code... -
The CDF-S Viewed with SIMBA
Observations of the Chandra Deep Field South (CDF-S) with the bolometer array SIMBA on the SEST 15m telescope is presented. SIMBA operates at 1250 μm... -
The TESIS Project: Are Type 2 QSO Hidden in X-Ray Emitting EROs?
X-ray selected EROs are, on average, the hardest X-ray sources in medium and deep X-ray fields. This coupled with their extremely red colors... -
The Deepest Near-Infrared View of the Universe
We present very deep near-infrared imaging in the J s , H and K s -bands of the HDF-S and... -
A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B
We present spectroscopic identifications for a sample of 85 millimeter and submillimeter galaxies detected with the SCUBA/JCMT and MAMBO/IRAM30m... -
The Evolution of Evolved Galaxies
The plethora of high redshift multifrequency surveys currently under way, that were extensively illustrated at this meeting will shortly provide us... -
The First 1–2 Gyrs of Galaxy Formation: Dropout Galaxies from z~ 3–6
The unique high–resolution wide–field imaging capabilities of HST with ACS have allowed the characterization of galaxies at redshift 6, less than 1... -
COSMOS 2 $\square^\circ$ Survey
The Cosmic Evolution Survey (COSMOS) will provide complete multi-wavelength imaging and spectroscopy of a 2... -
Nuclei of Galaxy Bulges Through HST NIR Imaging
We have analyzed the structure of bulges of early-to intermediate-type spirals, on nuclear and global scales, using HST NIR imaging together with... -
On the Dearth of Low-Luminosity, High-Redshift Quasars
The GOODS Team [2] presented a sample of 17 high-redshift QSO candidates from the GOODS fields with 3.5 < z < 5.2. The number counts of their z > 4... -
Large Scale Structure in the Two Micron All Sky Survey
The unprecedented sky coverage and photometric uniformity of the Two Micron All Sky Survey (2MASS) [1] provides a rich resource for obtaining an... -
Tracing the Evolution of Massive Galaxies up to z ~ 3
Objects with unusual red near-IR color J-K > 3 are extremely rare at magnitude brighter than K=20, while their surface density increases at fainter... -
T-ReCS and Michelle: The Mid-Infrared Spectroscopic Capabilities of the Gemini Observatory
Gemini Observatory’s northern and southern telescopes are both presently being outfitted with facility mid-infrared imagers/spectrometers. This will... -
Infrared Spectroscopy of H+3 in the Interstellar Medium
Long a subject of laboratory and theoretical studies, H+3indexAH+3 is now recognized to be a fundamental ingredient of interstellar space, as the... -
High-Resolution Infrared Spectroscopy of Protoplanetary Disks
High-resolution spectroscopy at near and mid-infrared wavelengths can provide important and unique information about protoplanetary disks around...