IV. Gaffey Meteorite Spectra

1. Observer full name should be Mike Gaffey. Remove "data provider full 
name" from data set catalog as this is an obsolete keyword.

2. Dan Britt will contact Gaffey to make sure he knows his data are
being archived.

3. In the index, meteorite names should be capitalized.

4. Many meteorite classifications have been updated since Gaffey compiled
them. Update the meteorite classifications to current classifications.
Dan Britt has voluteered to do this.

5. Change microns to nanometers in the data label.

6. Add information to the data set catalog about how the data
were taken, the instrument used, how the samples were prepared, particles
sizes, etc. Dan Britt will recapture this information from 
Gaffey or other sources and provide to Carol for inclusion in the 
data set.

7. Add description to the column objects in the index label.

Note: Dan Britt offered to take the lead in gathering meteorite spectra
for archiving in PDS. He plans to start by doing the work outlined here
for the Gaffey spectra, as well as producing a list of potential data 
providers.

VI. Asteroid Lightcurve Parameters (Update) //Completed

Check with Al Harris to find out what appears in the sidereal period 
flag in the case of a trojan or other orbit type with a long rotation
information. Also confirm that 'A' always stands for Aten and not 
Apollo or Amor.

Note: Reviewers noted that this is a very useful data set and should be 
updated each year that an update is available.

VII. Asteroid Taxonomy (Update) //Completed

Add the asteroid Pholus to the table.

Two entries at the end of the table are in reverse chronological order.
Reverse them to chronological order.

Note: Reviewers made several suggestions for future updates to this data set.
They recommend collecting asteroid taxonomies from additional sources 
including Wisniewski's classifications and Hammergren's. Totally, for 
each asteroid spectrum archived in PDS there should be a taxonomic classification 
in this table. Dan Britt also asked Dave Tholen to create an additional
taxonomy file with his personal assignment of taxonomic classifications. Mark
Sykes asked for a piece of code which could take a spectrum in the 
appropriate wavelength range and resolution and produce a taxonomic classification.
Rick Binzel may already have such a program. This program could be available as a
resource to users of PDS. The Winsniewski classifiactions were orginally assigned 
"by eye". What would be best would be to reclassify them from W's spectra by Dave's 
method.

VIII. Radar detections (Update) //Completed.