[PDF] Top 20 An empirical model for the galaxy luminosity and star formation rate function at high redshift
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An empirical model for the galaxy luminosity and star formation rate function at high redshift
... UV luminosity function evolution towards higher ( z ≈ 8) redshifts has been the focus of several past studies, in the form of both hydrodynamical simulations ...Lyman-break galaxy (LBG) population at ... See full document
10
The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type
... the galaxy rest-frame spectrum and hence is a useful indicator of the present star ...of high signal-to- noise ratio, low redshift galaxies observed before January ...1.50) star-forming ... See full document
14
The dependence of galaxy clustering on stellar mass, star formation rate and redshift at z = 0 8 − 2 2, with HiZELS
... at high stellar masses, which flattens at low stellar masses, just like we found for the HiZELS ...with star-formation rate at fixed stellar mass. At high stellar masses (M ∗ & 10 ... See full document
17
Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA
... lensing model by Dye et al. (2015). This model was used in the image plane with the semilinear inversion method (Warren & Dye 2003) developed by Nightingale & Dye ...average ... See full document
11
Submillimeter evidence for the coeval growth of massive black holes and galaxy bulges
... the formation of these two components must be ...accretion luminosity in the ...skewed rate of submillimeter detection with redshift is consistent with a high redshift epoch of ... See full document
8
The Hα luminosity dependent clustering of star forming galaxies from z ∼ 0 8 to z ∼ 2 2 with HiZELS
... and high redshifts has provoked a flurry of recent work aiming to understand the relationships between stellar mass, star- formation rate and environment ...colour, ... See full document
21
GAMA/H ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters
... our galaxy samples selected at different wavelengths and con- struct a joint UV-H α -IR ...a function of galaxy physical parameters, such as stellar mass, redshift, UV continuum slope, BD, ... See full document
19
A Physical Model for the Luminosity Function of High‐Redshift Quasars
... the high-redshift quasar lumi- nosity function that are based on the Press-Schechter (1974) mass function of dark matter halos (including the modifica- tion of Sheth & Tormen 1999) and the ... See full document
10
Campisi, Maria Angela (2009): Gamma-ray Bursts and their Host Galaxies from Cosmological Simulation. Dissertation, LMU München: Fakultät für Physik
... large luminosity, GRBs represent “cosmological” events, which have been detected up to z ∼ ...in star-forming galaxies, predominantly irregular dwarf ...use galaxy catalogues constructed by combining ... See full document
124
The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN
... and star formation looks very similar; (2) growing SMBHs may be pref- erentially located in star-forming galaxies and (3) SMBH mass is tightly correlated with galaxy bulge mass and stellar ... See full document
26
Guo, Qi (2009): Galaxy Formation and Evolution in a LCDM Universe. Dissertation, LMU München: Fakultät für Physik
... to model this in cosmological semi-analytic models because the inner structure of galaxies is not well ...slab model is assumed, which acts as a screen in front of the stars (Kauffmann et ...a model ... See full document
141
7-30-2014 12:00 AM The X-ray View of Galaxies in Compact Groups and the Coma Cluster Infall Region
... the high-mass stars exhaust their fuel and end in supernovae, while the low-mass stars remain on the main sequence for longer than 10 ...a galaxy is obviously an oversimplifi- cation, as galaxies are better ... See full document
290
The Luminosity Function of Galaxies as Modeled by a Left Truncated Beta Distribution
... new luminosity function of galaxies can be built starting from a left truncated beta proba- bility density function, which is characterized by four ...new galaxy luminosity ... See full document
10
A Chandra Observation of the Globular Cluster Terzan 1: The Neutron Star X‐Ray Transient X1732−304 in Quiescence
... However, the detection of either source is statistically not significant and those sources could be due to chance super- position of background photons. Longer Chandra observa- tions are needed to confirm the presence of ... See full document
5
Righi, Mattia (2008): CO lines and dust emission from merging star-forming galaxies as CMB foregrounds. Dissertation, LMU München: Fakultät für Physik
... cosmic star formation history (the aforementioned Madau plot) shows that the bulk of the star formation activity in the universe takes place in a very broad redshift ...the ... See full document
131
NOEMA complementarity with NIKA2
... The high angular resolution of interferometers make them sensitive to small scale temperature gradients and suitable to char- acterize pressure substructures in the ICM up to scales ∼ λ/2D (see ... See full document
6
Pfuhl, Oliver (2012): The GRAVITY interferometer and the Milky Way’s nuclear star cluster. Dissertation, LMU München: Fakultät für Physik
... reduced star formation, while during the last few 100 Myrs the star formation rate was ...The formation of the cluster might coincide with the formation of the bulge ... See full document
169
The KMOS Redshift One Spectroscopic Survey (KROSS):the origin of disc turbulence in z~0 9 star forming galaxies
... given redshift there is no strong correlation between dispersion and stellar mass, however higher redshift galaxies appear to have larger ...versus star formation rate. While there is ... See full document
30
Analytic Approximation of Luminosity Distance in Cosmology via Variational Iteration Method
... For instance, a simple algebraic approximation for the lu- minosity distance in a flat universe with pressureless matter and a cosmological constant is considered in [7]. In [8], the so-called Pad´ e approximant is ... See full document
7
Accretion by the Galaxy
... that star formation will drive a circulation of gas in galaxies goes back a long way and has been explored by many authors Bregman (1980); Collins et ...this model was able to account for most ... See full document
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