activity
20192026
most citedJWST/CEERS sheds light on dusty star-forming galaxies: forming bulges, lopsidedness and outside-in quenching at cosmic noon

31 citations · 218 across the 28 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.GA2024

PGC 44685: A Dwarf Star-forming Lenticular Galaxy with Wolf-Rayet Population

Shiying Lu, Qiusheng Gu, Yulong Gao +8

Lenticular galaxies (S0s) are formed mainly from the gas stripping of spirals in the cluster. But how S0s form and evolve in the field is still untangled. Based on spatially resolv…

astro-ph.GA2024★ 1 cited

Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535

Jiantong Cui, Qiusheng Gu, Shiying Lu +3

Lenticular galaxies (S0s) in the local universe are generally absent of recent star formation and lack molecular gas. In this paper, we investigate one massive (5$\times…

astro-ph.GA2024★ 17 cited

NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at in the COSMOS field

Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +41

The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at in six deep fields. We report spectroscopic confirmation of eight g…

astro-ph.GA2024★ 7 cited

PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5

Yipeng Lyu, Benjamin Magnelli, David Elbaz +9

The stellar structures of star-forming galaxies (SFGs) undergo significant size growth during their mass assembly and must pass through a compaction phase as they evolve into quies…

astro-ph.GA2024★ 12 cited

Strong spectral features from asymptotic giant branch stars in distant quiescent galaxies

Shiying Lu, Emanuele Daddi, Claudia Maraston +27

Dating the ages and weighting the stellar populations in galaxies are essential steps when studying galaxy formation through cosmic times. Evolutionary population synthesis models…

astro-ph.GA2024★ 15 cited

JWST's first glimpse of a z > 2 forming cluster reveals a top-heavy stellar mass function

Hanwen Sun, Tao Wang, Ke Xu +11

Clusters and their progenitors (protoclusters) at z = 2-4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves a…