Star Formation Rate versus Stellar Mass
The Pan-STARRS1 medium-deep survey : the role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to z ~ 0.8.
... We thank the anonymous referee for constructive suggestions that further improve this paper. We also thank M. Kriek for re- leasing her SED fitting code “FAST,” and O. Ilbert and the COS- MOS team for the usage of the ...
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The origin of scatter in the star formation rate-stellar mass relation
... the mass de- pendence, evolution and origin of scatter in the SFR-M star ...with stellar mass from 0.35 dex at M star ≈ 10 9 M to ...M star & 10 ...M star & 10 10 M and by ...
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Brightest Group Galaxies : Stellar Mass and Star Formation Rate (paper I)
... the stellar mass distribution of the BGGs versus the mean redshift of each subsample and linear ...the stellar mass distribution tends to decrease with ...the stellar mass ...
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Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function
... the stellar absorption may in general be a luminosity- dependent quantity, the required correction could be higher for high SFR ...and stellar absorption ...luminosity-dependent stellar absorption ...
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Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function
... the mass range of interest (Salpeter 1955; Baldry & Glazebrook ...From star counts of local resolved stellar populations, the IMF is measured to have a high-mass (m > ...the star ...
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Star formation and stellar mass assembly in galaxy formation models
... the stellar mass assembly histories pre- dicted by models and simulations have been made recently in the literature, typ- ically focusing on reducing the fraction of stars that form at high ...early ...
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Galaxy and mass assembly: group and field galaxy morphologies in the star formation rate stellar mass plane
... halo mass changes. For the quiescent galaxies and the star-forming central galaxies, the maximum and minimum C remain approximately constant, im- plying that the ratio between r 20 and r 80 remains ...halo ...
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Quenching or Bursting:the Role of Stellar Mass, Environment, and Specific Star Formation Rate to z ~ 1
... of star-formation happens in mas- sive, high sSFR galaxies, particularly those in the field (and among group galaxies, satellites more than centrals), whereas most of the quenching of ...
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The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8–2.2, with HiZELS.
... halo mass via the two-point correlation function as we have done for HiZELS galaxies, we identify the halo masses of EAGLE galaxies ...(FOF) mass of the galaxy’s halo, labelled as GroupMass in the EAGLE FOF ...
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VIS3COS I:Survey overview and the role of environment and stellar mass on star formation
... of star formation activity we find that our typical complete- ness is lower for quiescent galaxies (∼ 30%) when compared to star-forming ones (∼ ...
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Galaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growth
... and stellar mass, since the inclusion or not of the quiescent population greatly affects the ...detected star-forming ...SSFR versus stellar mass for all redshift bins, for the ...
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Black hole growth is mainly linked to host-galaxy stellar mass rather than star formation rate.
... Figure 6 . As expected, both SFR and M * display positive correlations with á BHAR . ñ We perform partial correlation (PCOR) analyses on the results using “ PCOR ” in R. 28 The PCOR analyses are deployed to measure the ...
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The dependence of galaxy clustering on stellar mass, star formation rate and redshift at z = 0 8 − 2 2, with HiZELS
... as stellar mass functions, luminosity functions and the detailed properties of individual galaxies such as sizes, bulge/disk masses and star-formation histories were poorly matched (see ...
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The star formation rate and stellar content contributions of morphological components in the EAGLE simulations.
... of stellar and halo mass. Beyond stellar mass and environment, A third property that shows strong redshift evolution and could influence cir- cularities is galaxy ...for star-forming ...
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Constraining Star Formation Histories of Blue Galaxies using the Scatter between Stellar Mass and Halo Mass
... Often in the literature, an empirical color-color or SFR–M ∗ cut that separates the two main modes (red/blue or star-forming/quiescent) in the distribution is chosen to classify galaxies (e.g. Baldry et al. 2006; ...
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VIS^3COS - I. Survey overview and the role of environment and stellar mass on star formation
... of star-forming galax- ies) seem to be invariant to their environment (but it is still a debated issue, see ...of star-forming galax- ies are independent of ...that star-forming galaxies have ...
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Galaxy Zoo : the dependence of the star formation-stellar mass relation on spiral disk morphology
... the stellar mass–star formation rate (SFR) relation in star-forming disc galaxies at z ≤ ...in star formation at a constant mass, only boost the SFR above ...
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Linking galaxies to dark matter halos at z ~ 1 : dependence of galaxy clustering on stellar mass and specific star formation rate.
... halo mass as a function of sSFR for the M M M 10 10 ⊙ < * < 10 ...halo mass on the y-axis rather than the bias factor. From both stellar mass bins, we con firm the anti-correlation in the ...
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The Role of Stellar Feedback in Star Cluster Formation
... massive star clusters spanning ∼ 10 4 − 10 8 M in mass have been observed to have similar surface brightness ...of star cluster formation have also produced star clusters with this ...
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Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
... halo mass, we compare the AGN model (blue curve), which includes AGN feedback, to the REF ...the stellar ejecta are deposited, we again expect a low recycling-fuelled SFR if the AGN feedback is strong ...
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