Attention: Nick Scoville
The array of six telescopes, each of 10.4 m diameter is used primarily for aperture synthesis mapping of molecular lines and dust continuum emission at wavelengths observable in the 1.3 and 3 mm atmospheric windows. Baseline to 400 m provides sub-arcsecond (0.5") spatial resolution. Typical large-scale observational programs include studies of nearby regions of star formation and mapping of the molecular gas in external galaxies. We seek candidates with ambitious observational programs for the array and/or those wishing to work on technical aspects of millimeter-wave interferometry.
Applications (including a brief statement of research interests, curriculum vitae, and three letters of reference) should reach Caltech before 31 January 2001, but later applications will be considered.
Women, minorities, veterans and disabled persons are encouraged to apply. AAE/EOE.
to Job Register Table of Contents.
aas@aas.org