activity
20142022
most citedInefficient Star Formation In Extremely Metal Poor Galaxies

210 citations · 721 across the 14 of their papers we have counts for

collaborators

25 papers

astro-ph.GA202417 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

Molecular gas excitation in the circumgalactic medium of MACS1931-26

L. Ghodsi, J. Zhou, P. Andreani +6

The evolution of galaxies is largely affected by exchanging material with their close environment, the circumgalactic medium (CGM). In this work, we investigate the CGM and the int…

astro-ph.GA2023

The \ion{H}{I}-rich Ultra-diffuse Galaxies follow the Extended Schmidt Law

Sai Zhai, Yong Shi, Zhi-Yu Zhang +7

The \ion{H}{I}-rich ultra-diffuse galaxies (HUDGs) offer a unique case for studies of star formation laws (SFLs) as they host low star formation efficiency (SFE) and low-metallicit…

astro-ph.GA2023

The first ground-based detection of the 752 GHz water line in local ultra-luminous infrared galaxies using APEX-SEPIA

Daysi Quinatoa, Chentao Yang, Edo Ibar +10

We report the first ground-based detection of the water line p-H2O (211-202) at 752.033 GHz in three z < 0.08 ultra-luminous infrared galaxies (ULIRGs): IRAS 06035-7102, IRAS 17207…

astro-ph.GA20232 cited

Opacities of dense gas tracers in galactic massive star-forming regions

Shu Liu, Junzhi Wang, Fei Li +5

Optical depths of dense molecular gas are commonly used in Galactic and extragalactic studies to constrain the dense gas mass of the clouds or galaxies. The optical depths are ofte…

astro-ph.HE20235 cited

Molecular environment of the thermal composite supernova remnant G352.70.1

Qian-Qian Zhang, Ping Zhou, Yang Chen +5

Galactic supernova remnants (SNRs) play an important role in our understanding of supernovae and their feedback on the interstellar environment. SNR G352.70.1 is special for its…