activity
19982023
most citedThe Chandra Deep Field-South Survey: 4 Ms Source Catalogs

581 citations · 3.6k across the 83 of their papers we have counts for

collaborators

83 papers

astro-ph.GA2023★ 3 cited

Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449

Xiaotong Guo, Qiusheng Gu, Jun Xu +5

We presented the multiwavelength analysis of a heavily obscured active galactic nucleus (AGN) in NGC 449. We first constructed a broadband X-ray spectrum using the latest NuSTAR an…

astro-ph.GA2022

Diagnosing deceivingly cold dusty galaxies at 3.5<z<6: a substantial population of compact starbursts with high infrared optical depths

Shuowen Jin, Emanuele Daddi, Georgios E. Magdis +9

Using NOEMA and ALMA 3mm line scans, we measure spectroscopic redshifts of six new dusty galaxies at 3.5<z<4.2 by solidly detecting [CI](1-0) and CO transitions. The sample was sel…

astro-ph.GA2022★ 23 cited

Systematic biases in determining dust attenuation curves through galaxy SED fitting

Jianbo Qin, Xian Zhong Zheng, Min Fang +16

While the slope of the dust attenuation curve () is found to correlate with effective dust attenuation () as obtained through spectral energy distribution (SED) fitting, it…

astro-ph.GA2021★ 3 cited

Observations of cold gas and star formation in dwarf S0 galaxies

Xue Ge, Qiu-Sheng Gu, Ruben Garcıa-Benito +3

Very little work has been done on star formation in dwarf lenticular galaxies (S0s). We present 2D-spectroscopic and millimetre observations made by Centro Astronomico Hispano Alem…

astro-ph.HE2021★ 14 cited

The origin of the soft X-ray excess in the narrow-line Seyfert 1 galaxy SBS 1353+564

Xinpeng Xu, Nan Ding, Qiusheng Gu +2

We present for the first time the timing and spectral analyses for a narrow-line Seyfert 1 galaxy, SBS 1353+564, using \it{XMM-Newton} and \it{Swift} multi-band observations from 2…

astro-ph.GA2021★ 5 cited

PGC 38025: A Star-forming Lenticular Galaxy With an Off-nuclear Star-forming Core

Zhengyi Chen, Qiu-Sheng Gu, Rubén García-Benito +4

Lenticular galaxies (S0s) were considered mainly as passive evolved spirals due to environmental effects for a long time; however, most S0s in the field cannot fit into this common…