English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We investigate the relationship between environment and the galaxy mainsequence (the relationship between stellar mass and star formation rate) andalso the relationship between environment and radio luminosity (P$_{\rm1.4GHz}$) to shed new light on the effects of the environments on galaxies. Weuse the VLA-COSMOS 3 GHz catalogue that consists of star-forming galaxies(SFGs) and quiescent galaxies (AGN) in three different environments (field,filament, cluster) and for three different galaxy types (satellite, central,isolated). We perform for the first time a comparative analysis of thedistribution of SFGs with respect to the main sequence (MS) consensus regionfrom the literature, taking into account galaxy environment and using radioobservations at 0.1 $\leq$ z $\leq$ 1.2. Our results corroborate that SFR isdeclining with cosmic time which is consistent with the literature. We findthat the slope of the MS for different $z$ and M$_{*}$ bins is shallower thanthe MS consensus with a gradual evolution towards higher redshift bins,irrespective of environments. We see no SFR trends on both environments andgalaxy type given the large errors. In addition, we note that the environmentdoes not seem to be the cause of the flattening of MS at high stellar massesfor our sample.

Effect of the environment on star formation activity and stellar mass for star-forming galaxies in the COSMOS field