Exploring the Sensitivity Limit:
21-cm Observations of Low Surface Brightness Galaxies with the Arecibo Telescope

Authors: Karen O'Neil, Jo Ann Eder, G. Bothun, J. Shcombert

Published: "The NAIC/NRAO School on Single Dish Radio Astronomy " Salter, et.al eds. (San Francisco:ASP) (2001).


The wide bandwidth, high sensitivity, and flat baselines of the Arecibo Gregorian telescope make it an excellent instrument to probe the HI content of LSB systems. In this paper we briefly describe a few of the results to come out of Arecibo observations of these enigmatic systems.

Entire paper (oneil_post.ps.gz - 35kb)