Suppose we choose to observe a source with a declination of +12o10'35" while it is on the meridian. We choose an azimuth angle of 360. What zenith angle would we use?
The ALFALFA survey is using the ALFA detector. But we plan to followup exciting ALFALFA detections using the L-Band Wide (LBW) detector. Why don't we use ALFA?
What is the frequency range covered by the L-Band Wide (LBW) detector? What wavelengths does this correspond to? Assuming that you were observing the 21-cm line, what range of velocities and redshifts does this correspond to? Compare to the coverage of ALFA.
What is the difference between Code 1, 2, and 9 targets in the ALFALFA cataloging scheme?
How are the optical counterparts of ALFALFA sources determined?