Talks

Invited colloquia, contributed talks, posters, and upcoming travel.

Upcoming

  • August 24–28, 2026 · 12th Galaxy Evolution Workshop, Seoul National University, Korea — Contributed talk: From Structural Growth to Quenching: Bulge–Disk Decomposition Across Cosmic Time and the Local Resolved ISM.
  • October 15, 2026 · Kavli IPMU, University of Tokyo, Japan — Invited APEC Seminar: Contrasting UV and Optical Evolution: The Structural Transformation of Galaxies Since z ~ 1. (Visit Oct 13–19, host: Prof. John Silverman.)

Invited Colloquia

  • Contrasting UV and Optical Evolution: The Structural Transformation of Galaxies Since z~1. Kavli IPMU (APEC Seminar), University of Tokyo, Kashiwa, Japan, October 15, 2026. Upcoming.
  • Contrasting UV and Optical Evolution: The Structural Transformation of Galaxies Since z~1. National Central University, Taoyuan, Taiwan, April 10, 2026.
  • Two Wavelengths, One Story: UV and Optical Views of 7 Billion Years of Galaxy Growth. National Tsing Hua University, Hsinchu, Taiwan, March 6, 2026.
  • Two Wavelengths, Two Perspectives: UV and Optical Views of the Structural Evolution of Galaxies over the Last 7 Billion Years. Indian Institute of Astrophysics, Bengaluru, India, February 10, 2026.

Invited Lunch Talks / Seminars

  • Two Wavelengths, Two Perspectives: UV and Optical Views of Galaxy Structure and Growth Since z ~ 1. ASIAA Lunch Talk, Taipei, Taiwan, 2025.

Contributed Oral Talks

  • Two Wavelengths, Two Components: A New View of Galaxy Growth. CASCA 2026, Montréal, Canada, June 2026.
  • Contributed talk on galaxy quenching with KILOGAS. KILOGAS Workshop 2026, Victoria, BC, Canada, May 2026.
  • Two Wavelengths, Two Stories: How Bulges and Disks Grow. APRIM 2026 (Asia–Pacific Regional IAU Meeting), Hong Kong, May 2026.
  • Structural Evolution of Galaxies: UV vs. Optical. Symposium for Early Career Astronomers, ASIAA, Taipei, 2025.
  • Evolution of Massive Quiescent Galaxies in Clusters and Field. ICA Symposium, Halifax, Canada, 2025.
  • From UV to Visible Light: Unveiling the Secrets of Galaxy Size Evolution in the COSMOS Field. CASCA-TO, Toronto, Canada, 2024.
  • From UV to Visible Light: Galaxy Size Evolution in the COSMOS Field Since z ~ 1. ICA Symposium, Halifax, Canada, 2024.

Posters

  • Environmental Effects on the Size Growth of Quiescent Galaxies from UV–Optical Perspectives in Clusters vs. the Field. APRIM 2026, Hong Kong, May 2026.
  • Unveiling the Size Growth of Quiescent Galaxies: Environmental Effects from UV–Optical Perspectives in Clusters vs. the Field. CL2025 — 1st East Asian Workshop on Galaxy Clusters, ASIAA, Taipei, 2025.
  • Galaxy Size Evolution in Field vs Clusters. DEEP24, Sintra, Portugal, 2024.
  • Evolution of Galaxy Morphology Since z ~ 1. CASCA 2022, Waterloo, Canada, 2022.

Research Visits

  • Kavli IPMU, University of Tokyo, Japan — October 13–19, 2026 (host: Prof. John Silverman). Upcoming.
  • Saint Mary’s University, Halifax, Canada — June 1–5, 2026.

Observing Programs

  • Gemini South / GS-2026B-Q-104 — Testing Molecular Gas Scaling Relations in z ~ 1.4 Galaxy Clusters with ALMA and Gemini. Co-PI (PI: R. Monteiro-Oliveira). 5.4 hr awarded, Band 1.
  • Magellan / ROSIE (Baade 6.5 m), 2026B — Galaxy Cluster Selection via Emission Line Galaxies: Preparing for the Prime Focus Spectrograph Cosmology Survey. PI. 1.0 night.
  • Magellan / ROSIE (Baade 6.5 m), 2026B — Beyond Field Gas Scaling Laws: Empirical CO Predictions versus Actual CO Observations in Cluster Environments Over Cosmic Time. PI. 0.5 nights.