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Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies

  • Authors: Vaidik Prasal, Yogesh Wadadekar, Pralay Biswas, Rashi Jain

Vaidik Prasal et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 11.

SFHs for all galaxies in our sample from BAGPIPES SED modeling. Each panel shows the posterior SFH for one galaxy, with the blue vertical line indicating the formation time (t50, BG) and the red vertical line indicating the quenching time (tq, BG). The SFHs indicate rapid early mass assembly followed by quenching in ≈1.4 Gyr.

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