Wuji Wang
@wujiwang.bsky.social
Postdoc @Caltech | PhD @Heidelberg University ｜explore high-ish universe | web: https://wujiwang-astro.github.io/
**Paper day**
My PI JWST+ALMA data finally published after 547 days (JWST) + 931 days (ALMA)! Also a new VLA data(54days)
We find ubiquitous companions around radio AGN at z=3.5. Maybe the trigger of the most powerful radio jets. arxiv.org/pdf/2502.20442
My PI JWST+ALMA data finally published after 547 days (JWST) + 931 days (ALMA)! Also a new VLA data(54days)
We find ubiquitous companions around radio AGN at z=3.5. Maybe the trigger of the most powerful radio jets. arxiv.org/pdf/2502.20442
March 3, 2025 at 5:08 AM
**Paper day**
My PI JWST+ALMA data finally published after 547 days (JWST) + 931 days (ALMA)! Also a new VLA data(54days)
We find ubiquitous companions around radio AGN at z=3.5. Maybe the trigger of the most powerful radio jets. arxiv.org/pdf/2502.20442
My PI JWST+ALMA data finally published after 547 days (JWST) + 931 days (ALMA)! Also a new VLA data(54days)
We find ubiquitous companions around radio AGN at z=3.5. Maybe the trigger of the most powerful radio jets. arxiv.org/pdf/2502.20442
Paper Day! Check our JWST NIRSpec/IFU view of a powerful z=3.59 radio AGN 👉 arxiv.org/abs/2401.02479
Despite being a luminous AGN, it is inefficient in outflow at <5kpc. The resolved fascinating ISM still needs more analysis. This is only 1/4 of my sample. More will come soon!
Despite being a luminous AGN, it is inefficient in outflow at <5kpc. The resolved fascinating ISM still needs more analysis. This is only 1/4 of my sample. More will come soon!
JWST discovers an AGN ionization cone but only weak...
We present the first results from a JWST program studying the role played by powerful radio jets in the evolution of the most massive galaxies at the onset of Cosmic Noon. Using NIRSpec integral...
arxiv.org
January 8, 2024 at 8:55 AM
Paper Day! Check our JWST NIRSpec/IFU view of a powerful z=3.59 radio AGN 👉 arxiv.org/abs/2401.02479
Despite being a luminous AGN, it is inefficient in outflow at <5kpc. The resolved fascinating ISM still needs more analysis. This is only 1/4 of my sample. More will come soon!
Despite being a luminous AGN, it is inefficient in outflow at <5kpc. The resolved fascinating ISM still needs more analysis. This is only 1/4 of my sample. More will come soon!
Hello! First post: Paper Day🥳 We mapped the intrinsic Ly-alpha nebulae around eight of some of the most powerful radio AGN (type-2 quasars) at 2.9Check it on arxiv: arxiv.org/abs/2309.15144
arxiv.org
September 28, 2023 at 7:25 AM
Hello! First post: Paper Day🥳 We mapped the intrinsic Ly-alpha nebulae around eight of some of the most powerful radio AGN (type-2 quasars) at 2.9Check it on arxiv: arxiv.org/abs/2309.15144