template redlog file of all fall A2707 observations. Use this file
to log the reduction of the LBW data from Fall 2012.
links to SDSS/SkyView/DSS2/NED for each targeted position.
The first step is to identify which sources
are detected and which ones are not; the two classes will
be treated differently.
Non-detections:
We want to measure the rms noise in
the baseline-subtracted, smoothed spectrum.
Detections:
We want to measure the HI line flux,
systemic velocity and velocity width
and their errors, as well as the rms noise.
In both cases, we want to store the output in an IDL-readable
file (akin to a "src" file in IDL_ALFA) and also to an ASCII
version so that we can archive the output once and for all time.
Once we get everything in place, reduction should go quickly.
More to come here as time permits and we think through the process.
Last modified: Wed Jan 23 08:15:01 EST 2013
by Martha
