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THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OF z ∼ 2 STAR-FORMING GALAXIES
- N. F. Förster Schreiber, R. Genzel, M. Onodera
- Physics
- 10 March 2009
We present the Spectroscopic Imaging survey in the near-infrared (near-IR) with SINFONI (SINS) of high-redshift galaxies. With 80 objects observed and 63 detected in at least one rest-frame optical…
Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe
- M. Vogelsberger, S. Genel, Stsci
- Physics
- 12 May 2014
We introduce the Illustris Project, a series of large-scale hydrodynamical simulations of galaxy formation. The highest resolution simulation, Illustris-1, covers a volume of $(106.5\,{\rm Mpc})^3$,…
Properties of galaxies reproduced by a hydrodynamic simulation
- M. Vogelsberger, S. Genel, L. Hernquist
- PhysicsNature
- 6 May 2014
TLDR
CONSTRAINTS ON THE ASSEMBLY AND DYNAMICS OF GALAXIES. II. PROPERTIES OF KILOPARSEC-SCALE CLUMPS IN REST-FRAME OPTICAL EMISSION OF z ∼ 2 STAR-FORMING GALAXIES
- N. F. Förster Schreiber, A. Shapley, L. Tacconi
- Physics
- 1 April 2011
We study the properties of luminous stellar “clumps” identified in deep, high-resolution Hubble Space Telescope NIC2/F160W imaging at 1.6 μm of six z ∼ 2 star-forming galaxies with existing…
Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor
- L. Tacconi, R. Genzel, A. Baker
- Physics
- 23 January 2008
We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z ∼ 2 submillimeter galaxies (SMGs), and sensitive CO(3-2) flux limits toward three z ∼ 2 UV/optically selected…
From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution at z ~ 2 from Integral Field Spectroscopy in the SINS Survey
- R. Genzel, A. Burkert, S. Lilly
- Physics
- 8 July 2008
We present Hα integral field spectroscopy of well-resolved, UV/optically selected z ∼ 2 star-forming galaxies as part of the SINS survey with SINFONI on the ESO VLT. Our laser guide star adaptive…
THE SINS SURVEY OF z ∼ 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPS
- R. Genzel, S. Newman, G. Zamorani
- Physics, Geology
- 24 November 2010
We have studied the properties of giant star-forming clumps in five z ∼ 2 star-forming disks with deep SINFONI AO spectroscopy at the ESO VLT. The clumps reside in disk regions where the Toomre…
THE IMPACT OF COLD GAS ACCRETION ABOVE A MASS FLOOR ON GALAXY SCALING RELATIONS
- N. Bouché, A. Dekel, L. Tacconi
- Physics
- 10 December 2009
Using the cosmological baryonic accretion rate and normal star formation (SF) efficiencies, we present a very simple model for star-forming galaxies that accounts for the mass and redshift…
First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- A. Pillepich, D. Nelson, M. Vogelsberger
- Physics
- 11 July 2017
The IllustrisTNG project is a new suite of cosmological magneto-hydrodynamical simulations of galaxy formation performed with the Arepo code and updated models for feedback physics. Here we introduce…
Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- S. Genel, M. Vogelsberger, L. Hernquist
- Physics
- 15 May 2014
We present an overview of galaxy evolution across cosmic time in the Illustris Simulation. Illustris is an N-body/hydrodynamical simulation that evolves 2*1820^3 resolution elements in a (106.5Mpc)^3…
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