Observing Experience

Optical

Yerkes Observatory

1.05m reflector (many nights)
--- photographic photometry of globular cluster stars (investigating possible variability of asymptotic giant branch stars)
--- high-resolution interferometric spectroscopy of planetary nebulae and symbiotic stars (velocity profiles of H-alpha and O III] emission)
--- experiments in ccd astrometry

Kitt Peak National Observatory

coude feed + coude spectrograph (18 runs, >100 nights)
--- high-resolution (1.2-1.5 km/s or 2.5-3.0 km/s) spectroscopy of interstellar absorption lines toward many Galactic stars (surveys, regional studies, detailed line of sight studies)

McDonald Observatory

2.7m + coude spectrograph (4 runs, 15 nights)
--- high-resolution (0.5-0.6 km/s) spectroscopy of interstellar absorption lines (Na I, K I, Ca I)

Anglo-Australian Observatory

3.9m AAT + UHRF (2 runs, 7 nights)
--- high-resolution (0.3 km/s) spectroscopy of interstellar absorption lines (Na I, Ca II, Ca I, Fe I)
3.9m AAT + UCLES (1 run, 5 nights)
--- moderately high resolution (5 km/s) spectroscopy of interstellar Na I and K I absorption in the LMC and SMC

European Southern Observatory

3.6m + CES (3 runs, 9 nights)
--- high-resolution (1.25-2.0 km/s) spectroscopy of interstellar Na I and Ca II absorption in the LMC and SMC
VLT + UVES (1 run, 3 nights)
--- moderately high resolution (5 km/s) spectroscopy of interstellar absorption in the Magellanic Clouds

Las Campanas Observatory

Magellan + MIKE (1 run, 2 nights)
--- moderately high resolution (6 km/s) spectroscopy of interstellar absorption (Galactic and extragalactic targets)

Ultraviolet

International Ultraviolet Explorer

high- and low-resolution UV spectra to study interstellar absorption lines and UV extinction in high-latitude molecular clouds (PI for five observing programs; co-I for several other observing and archival programs)

Hubble Space Telescope

GHRS (Goddard High-Resolution Spectrograph)
--- high-resolution spectra of interstellar absorption lines toward one SMC star (PI)
--- high-resolution spectra of high-velocity gas toward three disk stars (PI)
--- high-resolution spectra of interstellar lines toward 12 disk stars (co-I)
STIS (Space Telescope Imaging Spectrograph)
--- high-resolution spectra of interstellar absorption lines toward one SMC star (PI)
--- high-resolution spectra monitoring variable interstellar absorption toward one halo star (PI)
--- high-resolution spectra of interstellar absorption lines toward three LMC stars (PI)
--- high-resolution spectra of interstellar absorption lines toward HD 62542 (PI)
--- high-resolution spectra of interstellar absorption lines toward HD 204827 (co-I)
--- high-resolution spectra of interstellar absorption lines toward two Magellanic Clouds stars (PI)

IMAPS (Interstellar Medium Absorption Profile Spectrograph)

spectra of interstellar absorption lines toward one disk star (PI)

Far Ultraviolet Spectroscopic Explorer

spectra of interstellar absorption lines toward two SMC stars (PI)

Radio

CARMA (Combined Array for Research in Mm-wave Astronomy)

3 week-long stints as observer -- scheduling projects, monitoring array performance, minor trouble-shooting

PI for two projects aimed at detecting high-z molecular absorption (corresponding to damped Lyman-alpha systems) toward quasars


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Dan Welty / dwelty@oddjob.uchicago.edu

Last modified 22 Jan 2013