Relation between sSFR and galaxy mass - No significant galaxy
Comparing the Relation Between Star Formation and Galaxy Mass in Different Environments
... stellar mass in galaxy clusters and groups, and compare these with results from field ...in SSFR as galaxy stellar mass increases, showing that the current SF contributes more to the ...
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The temperature mass relation in magnetized galaxy clusters
... temperature-mass relation depends on the cho- sen radius within which the mean temperature is ...the mass-weighted ...simulated galaxy clusters to velocity ...tionship between cluster ...
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CLASH: The Concentration-Mass Relation of Galaxy Clusters
... correlation between mass and concentration for dark matter structures, although with signi ficant ...(c–M) relation which is a mild function of formation redshift and halo mass (Bullock et ...
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A mass-dependent slope of the galaxy size-mass relation out to z ∼ 3 : further evidence for a direct relation between median galaxy size and median halo mass
... –mass relation point of view, the pivot marks the stellar mass at which the galaxy population transitions from being dominated by star-forming galaxies to being dominated by quiescent ...the ...
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Galaxy And Mass Assembly (GAMA) : the sSFR M* relation part I σsSFR M* as a function of sample, SFR indicator, and environment
... σ sSFR –M ∗ relation with no selection applied to the population (other than those previously ...σ sSFR –M ∗ relation derived from this distribution is most directly comparable to the previous ...
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Galaxy Zoo:major galaxy mergers are not a significant quenching pathway
... same mass bin. The horizontal dashed lines show the best fitting relation if we assume a constant ...each mass bin at the bottom of each ...stellar mass functions, ...clear mass ...
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Bent by baryons: the low-mass galaxy-halo relation
... The relation between galaxies and dark matter haloes is of vital importance for evaluating theoretical predictions of structure formation and galaxy formation ...visible galaxy, and baryon ...
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Galaxy and mass assembly (GAMA): projected galaxy clustering
... with mass is stronger in our data than the fitting ...median mass of the ...no significant differences between the original and deeper ...
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CiteSeerX — Bent by baryons: the low mass galaxy-halo relation
... The relation between galaxies and dark matter halos is of vital importance for evalu- ating theoretical predictions of structure formation and galaxy formation ...low mass end because two of ...
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Galaxy and Mass Assembly (GAMA): the stellar mass budget of galaxy spheroids and discs
... spheroid mass divided by total mass of indi- vidual galaxies in both isolated and grouped ...individual galaxy spheroid-to-total-mass ratios within each halo mass ...spheroid ...
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Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions
... 0.1 M r for GAMA galaxies, µ 50,r = 22.42 + 0.029 0.1 M r with 1-sigma scatter of 0.76 mag. Target completeness is obtained using the empirically observed completeness shown in Fig. 2. Note that we do not attempt to ...
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Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small scale galaxy clustering
... The sSFR cuts used to select the 30% highest sSFR galaxies from M f and M ∗ samples are shown by the dashed ...The significant overlap between the high sSFR and optically red M ∗ ...
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Galaxy and Mass Assembly (GAMA) : the environmental dependence of the galaxy main sequence.
... halo mass between 10 12 and 10 14 M ...log SSFR distribution is clearly bimodal (consis- tent with the bimodality discovered in the colour-mass diagram in Taylor et ...higher SSFR and ...
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Galaxy And Mass Assembly (GAMA) : the environmental dependence of the galaxy main sequence
... In Fig. 6, we plot the fraction of SFG F(SFG) as a function of stellar mass and examine how it depends on halo mass, redshift and galaxy type. Note that the di ff erence between Figs. 4 and 6 ...
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Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations.
... of galaxy environment on their star formation rates (SFRs) using galaxies observed in the Galaxy And Mass Assembly (GAMA) ...stellar mass and ...passive galaxy population along with the ...
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Galaxy and Mass Assembly (GAMA) : impact of the group environment on galaxy star formation.
... nearby galaxy groups (z ∼ ...and sSFR for the whole galaxy population in 22 groups in the redshift range 0 ...−local galaxy density relation is only visible when both the passive and ...
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Galaxy and Mass Assembly (GAMA) : Impact of the Group Environment on Galaxy Star Formation
... analyze sSFR histograms since the median distills a lot of information about the distribu- tions of the sSFRs at a given radius into one ...the sSFR distribution of group galaxies can be different with ...
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Galaxy And Mass Assembly (GAMA) : the galaxy luminosity function within the cosmic web
... the galaxy luminosity function on geometric environment within the Galaxy And Mass Assembly (GAMA) ...evenly between environments. We find a significant variation in the luminosity ...
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Evolution of galaxy size-stellar mass relation from the Kilo-Degree Survey
... This is clearly shown in Fig. 7, which displays more exam- ples of galaxy images and residual maps in the r-band. Here, galaxies with χ ′ 2 < 1.3 are shown on the left two columns and examples of χ ′ 2 > 1.3 ...
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The SAMI Galaxy Survey : mass as the driver of the kinematic morphology density relation in clusters
... each galaxy in Figure 3, we show the velocity map to highlight the stellar ...overlap between the galaxy velocity maps, the data are fi rst placed on a regular grid with a spacing of ...each ...
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