text:   quiescent galaxies in different environments",9,"['New paper just accepted in ApJ📡:💫The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0💫: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments:  <LINK>  🌌 <LINK>', 'Galaxy evolution is driven by a variety of physical processes that proceed at different rates for different dark matter haloes and environments. A record of this evolution is preserved in galaxy stellar populations, which we can access using absorption-line spectroscopy 🔭:👇 https://t.co/3UQyD2BxE5', 'In this paper we explore the outstanding LEGA-C survey (DR3; see https://t.co/VN78t0MsMl) to investigate the role of the environment and stellar mass on stellar populations (using D4000 and H-delta) at z~0.6-1.0 in the COSMOS field, from poor fields to some rich clusters 👇 https://t.co/8Cq2Mm4l3s', 'We separate galaxies in terms of star-forming and quiescent, and also centrals and satellites, and leverage the statistical power and depth of LEGA-C to investigate the roles of stellar mass and environment in setting the quiescent fraction, 7 Gyrs ago: https://t.co/RMJXYA4peM', 'We reveal significant gradients  in D4000 and H-delta equivalent width (EW) distributions over the stellar mass vs environment 2D spaces at z~0.6-1.0. D4000 and H-delta EWs primarily depend on mass, but they also *depend on environment at fixed stellar mass* for massive galaxies: https://t.co/oijL6AA2xY', 'By splitting the sample into star-forming galaxies and quiescent galaxies we reveal that the significant environmental trends of D4000 and H-delta EW when controlling for stellar mass are *fully* driven by quiescent galaxies 😲👇 https://t.co/Cfw7wIam9u', 'Perhaps surprisingly: 🤔 regardless of being centrals or satellites, star-forming galaxies reveal D4000 and H-delta EWs which depend strongly on their stellar mass and are completely independent of the environment at 0.6&lt;z&lt;1.0: https://t.co/fvn1vVlY3X', 'Interestingly, the *environmental trends seen for satellite galaxies are fully driven by the trends that hold only for quiescent galaxies*, combined with the strong environmental dependency of the quiescent fraction at fixed stellar mass 🌌 https://t.co/F7lwhXnYL4', 'What next? LEGA-C allows to go beyond just 2 indicators. By modelling the full star formation histories of each galaxy we will be able to gain a much deeper insight, so stay tuned and check out other recent LEGA-C papers (+ download the public catalogue https://t.co/VN78t0MsMl) https://t.co/4FOxqXiyv0']",21,12,2320