pith. sign in

Yuanze Luo

Identifiers

  • name variant Yuanze Luo 0.60 · backfill

Papers (16)

  1. Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon astro-ph.GA · 2026 · author #12
  2. Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE astro-ph.GA · 2026 · author #9
  3. SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies astro-ph.GA · 2025 · author #12
  4. Quenching Through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ~ 0.7 Post-Starburst Galaxies astro-ph.GA · 2025 · author #8
  5. Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector astro-ph.GA · 2025 · author #6
  6. Cold gas in a post-starburst pair at z ~ 1.4: major mergers as a pathway to quenching in the HeavyMetal survey astro-ph.GA · 2025 · author #9
  7. Shocked POststarburst Galaxy Survey. IV. Outflows in Shocked Post-Starburst Galaxies Are Not Responsible For Quenching astro-ph.GA · 2024 · author #9
  8. Measuring the ISM Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C II] astro-ph.GA · 2024 · author #1
  9. Pulling back the curtain on shocks and star-formation in NGC 1266 with Gemini-NIFS astro-ph.GA · 2024 · author #11
  10. Characterizing the Molecular Gas in Infrared Bright Galaxies with CARMA astro-ph.GA · 2024 · author #11
  11. SDSS-IV MaNGA: how do star-formation histories affect gas-phase abundances? astro-ph.GA · 2023 · author #5
  12. Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past astro-ph.GA · 2022 · author #6
  13. A Multiwavelength view of IC 860: What Is in Action inside Quenching Galaxies astro-ph.GA · 2022 · author #1
  14. Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs astro-ph.GA · 2021 · author #9
  15. Evidence for the Accretion of Gas in Star-Forming Galaxies: High N/O Abundances in Regions of Anomalously-Low Metallicity astro-ph.GA · 2020 · author #1
  16. Characterization of Optical Light Curves of Extreme Variability Quasars Over a ~16-yr Baseline astro-ph.GA · 2020 · author #1

Mentions

  • 2509.00148 #12 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2506.19162 #6 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2507.21249 #8 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2506.14361 #9 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2410.04641 #1 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2412.06621 #9 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2409.17319 #11 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2409.09116 #11 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2312.06196 #5 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2210.12199 #6 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2208.08379 #1 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2105.09956 #9 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2012.04073 #1 · arxiv_oai · confidence 0.70 Yuanze Luo
  • 2004.04774 #1 · arxiv_oai · confidence 0.70 Yuanze Luo

Frequent Coauthors