http://arxiv.org/abs/2208.11668
In this paper we estimate the “star formation change parameter”, SFR${79}$, which characterizes the current SFR relative to the average during the last 800 Myr, for $\sim$ 300’000 galaxies selected from the Sloan Digital Sky Survey (SDSS). The goals are to examine, in a much larger and independent sample, the trends previously reported in a sample of star-forming MaNGA galaxies, and also to search for spectroscopic signatures of ongoing quenching in the so-called “Green Valley”, which is generally believed to contain galaxies that are migrating from the star-forming (SF) population to the quenched population of galaxies. Applying SFR${79}$ to our large sample of SDSS galaxies, we first confirm the basic results of SF galaxies published by Wang & Lilly. We then discuss in detail the calibration and meaning of SFR${79}$ for galaxies that are well below the SFMS and establish what would be the expected signatures of systematic ongoing quenching within the population. We conclude that it is not possible at present to establish unambiguous observational evidence for systematic ongoing quenching processes with the data at hand, due to limitations of noise in the observational data, in particular in the measurements of H$\delta$ absorption, and in the calibration of SFR${79}$, as well as biases introduced by the necessity of selecting objects with significant amounts of H$\alpha$ emission. We do however see plausible indications of ongoing quenching, which are quantitatively consistent with expectations from pertinent “growth+quenching” models of galaxy evolution and a typical e-folding timescale for quenching of order $\sim500$ Myr.
A. Weibel, E. Wang and S. Lilly
Thu, 25 Aug 22
9/43
Comments: 29 pages, 18 figures, submitted to AAS/ApJ