• Home
  • About
    • Overview
    • Mission
    • History
    • Governance
    • Facilities
    • Location / Map
    • FAQ
    • Contact
  • Research
    • Overview
    • Research Groups
    • Training
    • Courses
    • Publications
    • Research Labs
    • Collaborations
    • Visitor Program
  • People
    • Full Directory
    • Faculty
    • Research Associates
    • Graduate Students
    • Research Recognition
    • Teaching Awards
    • Visitor Program
    • Former Students
  • Outreach
    • Outreach
    • Mitchell Institute Physics Enhancement Program (MIPEP)
    • Star Parties
    • Observatory
    • Departmental Programs
    • Contact
  • Events
    • Seminars
    • Meetings
    • Outreach
  • News
    • Video Library
    • Contact
    • Open Positions
  • Support
    • Support the Mitchell Institute
    • Ways to Give
    • Donor Profiles
    • Contact

Mitchell Institute

The George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy

The George P. and Cynthia Woods
Mitchell Institute for Fundamental Physics and Astronomy

Casey Papovich

Are you a human? What is 5 + 4 ?



Phone: 979-862-2704

Email: papovich@tamu.edu

Office: M325

Websites

Homepage

 

Research Team

  • Sijie Chen (Graduate Student)
  • Vincent Estrada-Carpenter (Graduate Student)
  • Peter Ferguson (Graduate Student)
  • Taylor Hutchison (Graduate Student)

Biography

Casey Papovich's research is in the areas of observational cosmology, the formation and evolution of the most distant galaxies, and the growth of large scale structures of galaxies. His recent work focuses on observations of the properties of the first galaxies, constraints on cosmological reionization, quantifying the growth and assembly of stellar mass in galaxies in the early universe, the formation of galaxy clusters and their properties, and using satellite galaxies to test of the nature of dark matter and feedback mechanisms in galaxy evolution.

Dr. Papovich's research utilizes data from all of NASA's space-based Great Observatories (Hubble, Spitzer, and Chandra), the NASA/ESA Herschel Space Observatory, and the largest terrestrial telescopes, including the Gemini Observatory, Magellan Telescopes, Keck Observatory, and the ALMA Observatory). He is the project scientist for GMACS, the primary wide-field spectrograph being built for the Giant Magellan Telescope. He is involved in multiple international collaborations, including the ZFOURGE, CANDELS, HETDEX, HerS, DES, and LSST projects.

» Astronomy Group
 

News Highlights

  • Texas A&M-Led Study Helps Prove Galaxy Evolution Theory
  • Our Sun Came Late to the Milky Way's Star-Birth Party
  • Four Texas A&M Science Faculty Among Thomson Reuters Highly Cited Researchers 2016
 

Recent Publications

2015

An Increasing Stellar Baryon Fraction in Bright Galaxies at High Redshift

2015

ZFIRE: Galaxy Cluster Kinematics, H alpha SFRs and Gas Phase Metallicities of XMM-LSS J02182-05102 at z=1.6232

2015

The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years

2015

A Critical Assessment of Stellar Mass Measurement Methods

2015

The Sizes of Massive Quiescent and Star-forming Galaxies at z~4 with ZFOURGE and CANDELS


Update

Contact the Mitchell Institute • Phone: (979) 845-7778 • Fax: (979) 845-8674 • Map / Directions
  • Report Ethics Violations
  • Statewide Search
  • Texas Homeland Security
  • State of Texas
  • Download Adobe Reader
  • Privacy and Security
  • Policies & Legal Notices
  • Web Accessibility
Copyright © 2021. All Rights Reserved. Texas A&M University Trademark | Texas A&M University, College Station, Texas 77843