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astro-ph.GA2026
Testing [O II] as a Star Formation Rate Tracer in Quasar Host Galaxies
Xiaotong Feng, Xue-Bing Wu, Yuming Fu +3
The [O II] emission line is a widely used star formation rate (SFR) tracer. However, its application to type I quasars is not straightforward, because the line can be…
astro-ph.GA2026
Far-Infrared Star Formation Rates of Quasar Host Galaxies from Multiwavelength Spectral Energy Distribution Decomposition
Xiaotong Feng, Xue-Bing Wu, Yuming Fu +3
Reliable star formation rates (SFRs) are essential for studying the connection between black hole growth and quasar host galaxies. We study the far-infrared (FIR) SFRs and the host…