most citedLong-term Mid-infrared Color Variations of Narrow-Line Seyfert 1 Galaxies

1 citations · 2 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

A systematic study of the long-term mid-infrared color variations of Seyfert 1 galaxies

Jiahua Wu, Liming Dou, Zhining Chen +7

We present a comparative analysis of long-term mid-infrared (MIR) color variations (MCVs) for 1,977 narrow-line Seyfert 1 (NLSy1) and 4,113 broad-line Seyfert 1 (BLSy1) galaxies at…

astro-ph.HE2026

Mrk 382: A Narrow-line Seyfert 1 Galaxy with Recurrent X-ray State Transitions

Yanli Ai, Wenfeng Wen, Liming Dou +10

We report recurrent X-ray state transitions in the nearby narrow-line Seyfert~1 galaxy Mrk~382 using multi-epoch observations from \textit{Swift}, \textit{Chandra}, \textit{XMM-New…

astro-ph.HE2026★ 1 cited

A Radio Changing-state Jet in the Narrow-line Seyfert 1 Galaxy J1105+1452

Liming Dou, Zhining Chen, Jiahua Wu +9

We report the discovery of a radio-quiet to radio-loud transition in the narrow-line Seyfert 1 galaxy J1105+1452. The source has undergone a long-term evolution from a radio-quiet…

astro-ph.GA2026

X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state

Xiaohui Yang, Yanli Ai, Liming Dou +8

We present a multi-epoch study of the extreme X-ray variability of the type~1 quasar SDSS~J000532.84+200717.4 using archival observations from \textit{XMM-Newton}, \textit{Swift}/X…

astro-ph.GA2025★ 1 cited

Long-term Mid-infrared Color Variations of Narrow-Line Seyfert 1 Galaxies

Jiahua Wu, Huifang Xie, Liming Dou +6

We present a systematic investigation of long-term mid-infrared (MIR) color variability in 1,718 Narrow-Line Seyfert 1 galaxies (NLSy1s) using 14-year \textit{WISE}/NEOWISE monitor…

astro-ph.GA2025

AGNs in the extremely overdense galaxy region BOSS 1441: A Chandra observation

Jiahua Wu, Liming Dou, Zheng Cai +6

We present a Chandra/ACIS-I study of X-ray sources in BOSS 1441, a protocluster at that exhibits a prominent overdensity of Ly emitters (LAEs). Using a 45 ks obs…