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The EDGE-CALIFA Survey: Star Formation Efficiency and Galaxy Quenching across 62 Main-sequence, Green Valley, and Red Galaxies

  • Authors: Yu-Hsuan Teng, Alberto D. Bolatto, Peter J. Teuben, Erik Rosolowsky, David T. Frayer, Amanda A. Kepley, Sebastian F. Sanchez, Tony Wong, Adam K. Leroy, Dario Colombo, Serena A. Cronin, K. Decker French, Veselina Kalinova, Rebecca C. Levy, Karin M. Sandstrom, Vicente Villanueva, Jorge K. Barrera-Ballesteros, Zein Bazzi, Yixian Cao, Alex Green, Rodrigo Herrera-Camus, Eduardo A. D. Lacerda, Jialu Li, Alejandra Z. Lugo-Aranda, Jocabed Martinez-Lopez, Elizabeth Tarantino, Akshat Tripathi, Carolyn G. Volpert, Di Wen

Yu-Hsuan Teng et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

The relation between global SFR and stellar mass (Mstar) for our GBT sample (black points; 62 galaxies), the CARMA sample (gray stars; A. D. Bolatto et al. 2017), and the full CALIFA sample (contours; S. F. Sánchez et al. 2016a). The blue (upper) and red (lower) dashed lines indicate best linear fits from M. Cano-Díaz et al. (2016) for the MS galaxies and RGs, respectively. The GBT-EDGE sample is representative of the z = 0 galaxy population with Mstar = 108.5−11.5 M⊙.

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