We investigate dust-unbiased star formation rates (SFR) as a function of the environment in 20 massive clusters ($M_{200}>4\times10^{14} {\rm M}_{\odot}$) between $0.15<z<0.35$ using radio luminosities ($L_{\rm 1.4GHz}$) from the recently released MeerKAT Galaxy Cluster Legacy Survey catalogue. We use optical data from the Dark Energy Camera Legacy Survey to estimate photo-$z$s and assign cluster membership. We observe a steady decline in the fraction ($f_{\rm SF}$) of star-forming galaxies from $2R_{200}$ to the cluster centres in our full cluster sample, but notice a significant difference in $f_{\rm SF}$ gradients between clusters hosting large-scale extended radio emission in the form of haloes and relics (associated with ongoing merger...
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
We present first results of a study aimed to constrain the star formation rate (SFR) and dust conten...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluster...
Analyzing 24 μm MIPS/Spitzer data and the [O II]3727 line of a sample of galaxies at 0.4 ≤ z ≤ 0.8 f...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluster...
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluste...
We quantify the star formation (SF) in the inner cores (R/R200 ≤0.3) of 24 massive galaxy clusters ...
We present Spitzer MIPS 24 μm observations of sixteen 0.4 5 Å, and ~75% exhibit optical signatures ...
We measure star formation rates (SFRs) and specific SFRs (SSFRs) of Ks-selected galaxies from the VI...
We investigate the role of environment on star formation rates (SFRs) of galaxies at various cosmic ...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
We present first results of a study aimed to constrain the star formation rate (SFR) and dust conten...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluster...
Analyzing 24 μm MIPS/Spitzer data and the [O II]3727 line of a sample of galaxies at 0.4 ≤ z ≤ 0.8 f...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluster...
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We quantify the star formation (SF) in the inner cores (R/R_(200) ≤0.3) of 24 massive galaxy cluste...
We quantify the star formation (SF) in the inner cores (R/R200 ≤0.3) of 24 massive galaxy clusters ...
We present Spitzer MIPS 24 μm observations of sixteen 0.4 5 Å, and ~75% exhibit optical signatures ...
We measure star formation rates (SFRs) and specific SFRs (SSFRs) of Ks-selected galaxies from the VI...
We investigate the role of environment on star formation rates (SFRs) of galaxies at various cosmic ...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
We present first results of a study aimed to constrain the star formation rate (SFR) and dust conten...