Tsan-Ming Wang

most citedA

^{3}

COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time

49 citations · 49 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024

A $^{3}$ COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$

Benjamin Magnelli, Sylvia Adscheid, Tsan-Ming Wang +14

[Abridged] In recent years, conflicting results have provided an uncertain view of the dust-attenuated properties of $z > 4$ star-forming galaxies (SFGs). To solve this, we used the…

astro-ph.GA2023

A $^{3}$ COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 $\leq z$ < 1.6

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +5

We aim to understand the physical mechanisms that drive star formation in a sample of mass-complete (>10 $^{9.5} M_{⊙}$ ) star-forming galaxies (SFGs) at 1.2 $\leq z$ < 1.6. We se…

astro-ph.GA2022★ 49 cited

A $^{3}$ COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +6

To constrain for the first time the mean mass and extent of the molecular gas of a mass-complete sample of $> 1 0^{10}$ M $_{⊙}$ main-sequence (MS) galaxies at $0.4 < z < 3.6$ . We appl…

A3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4<z<5

A3COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 ≤z < 1.6

A3COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time

A $^{3}$ COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4 < z < 5$

A $^{3}$ COSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 $\leq z$ < 1.6

A $^{3}$ COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time