Adam M. Ritchey


Department of Physics and Astronomy
University of Toledo
2801 West Bancroft Street
Toledo, OH 43606
McMaster Hall 4004
(419) 205-0124
adam.ritchey@utoledo.edu

Education

  • Ph.D. in Physics (2009), University of Toledo
  • M.S. in Physics (2007), University of Toledo
  • B.S. in Astronomy (2002), Case Western Reserve University

Positions

  • Visiting Assistant Professor, University of Toledo (Aug 2024 - Present)
  • Adjunct Instructor, University of Toledo (Jan 2024 - Aug 2024)
  • Research Scientist, Eureka Scientific (Nov 2017 - May 2023)
  • Adjunct Instructor, Terra State Community College (Aug 2021 - Dec 2022)
  • Research Scientist, University of Washington (Dec 2014 - Oct 2017)
  • Adjunct Instructor, Seattle University (Sep 2015 - Jun 2016)
  • Postdoctoral Research Associate, University of Washington (Jan 2011 - Nov 2014)
  • Postdoctoral Research Associate, University of Toledo (Aug 2009 - Dec 2010)
  • Adjunct Instructor, Northwest State Community College (Jan 2010 - May 2010)
  • Research Assistant, University of Toledo (Aug 2007 - Jul 2009)
  • Teaching Assistant, University of Toledo (Aug 2004 - Jul 2007)

Observing

  • Hubble Space Telescope (HST)
    • Space Telescope Imaging Spectrograph (STIS)
      • High and medium-resolution UV spectra of stars probing the Galactic ISM (111 orbits; Co-I)
      • High-resolution far-UV spectra of stars in the Vela supernova remnant (12 orbits; PI)
      • High-resolution far-UV spectra of stars near pointings from the GOT C+ survey (12 orbits; Co-I)
      • High-resolution far-UV spectra of stars in the supernova remnant IC 443 (10 orbits; PI)

  • McDonald Observatory
    • Harlan J. Smith 2.7-meter Telescope
      • Tull Spectrograph: high-resolution optical spectra of stars for studies of interstellar absorption lines (90+ nights)
    • Hobby Eberly Telescope (HET)
      • High Resolution Spectrograph (HRS): high-resolution optical spectra to study Li isotope ratios in interstellar clouds (19.3 hours)
      • Habitable-zone Planet Finder (HPF): moderate-resolution near-IR spectra to study chemical fractionation in diffuse molecular clouds (13.5 hours)

  • Apache Point Observatory (APO)
    • Astrophysical Research Consortium (ARC) 3.5-meter Telescope
      • ARC Echelle Spectrograph (ARCES): moderate-resolution optical spectra of stars for studies of stellar and interstellar absorption lines (50+ nights)

  • Ritter Observatory
    • Ritter 1-meter Telescope: echelle spectra of variable stars for long-term monitoring

Publications

Service

  • NASA Astrophysics Data Analysis Program (ADAP) Review Panel (2022)
  • Hubble Space Telescope (HST) Mid-Cycle Review Panel (Cycle 25)
  • Referee for ApJ, A&A, MNRAS, and PASP

Outreach

  • Hosted a Special Viewing Night at the Harlan J. Smith 2.7-meter Telescope at McDonald Observatory (2018)

Memberships

  • International Astronomical Union (Since 2015)
  • American Astronomical Society (Since 2009)
  • Sigma Pi Sigma, Society of Physics Students (Since 2005)


Adam Ritchey / adam.ritchey@utoledo.edu

Last Modified: 08 Aug 2024