| Dates | Nights | Observers (PI & CoIs) | Instrument | Project |
| April 24-30 | 7 | Carleton, Lacasse | .... | 3rd telescope; sidewalks |
| May 1-9 | 9 | Debernardi | Nicmos/Fluor | Am stars in SB systems |
| May 10-24 | 15 | Perrin,Foresto | Nicmos/Fluor | Narrow-band obs of pulsing stars |
| May 25 -June 1 | 8 | Segransan, Haguerauer, Forveille, Perrier, Millan-Gabet, Traub | Nicmos/Fluor
or Nicmos/Class |
M/L for low-mass stars |
| June 2-8 | 7 | Papaliolios, Karovska, Sasselov, Marengo | APD/Visible | Cepheid program |
| June 9-12 | 4 | Monnier, CfA IOTA team, Tuthill, Danchi | Nicmos/Fluor | Keck-IOTA synthesis |
| June 13-15 | 3 | Monnier, CfA IOTA team | Nicmos/Fluor | Sources unresolved by Keck |
| June 16-22 | 7 | Millan-Gabet, Traub, Monnier, Porro, Schloerb, Kanbur, Hofmann, Weigelt | Nicmos/Fluor | Mira diameters |
| June 20 | 0.5 | Ratner, Porro, Traub | Nicmos/Fluor | IM Peg GP-B star |
| June 23 -July 2 | 10 | Schloerb, Brewer, Souccar, Morel, Lacasse | .... | 3rd telescope VxWorks test |
| July 2 | 0.5 | Ratner, Porro, Traub | Nicmos/Fluor | IM Peg GP-B star |
| July 3 -Aug 31 | 60 | Lacasse, More | .... | 3rd telescope Engineering |
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Notes:
1. This is the final schedule.
2. Scientific requests totaled 60 nights; 53.5 nights are assigned.
3. The two half-nights are the last half of each night.
4. The VxWorks test now occurs at the end of June, so as to not interrupt
the science program, and so that there is no great need
to restore
science capability at the end, except we would like to
operate the
instrument for the last half-night of July 2nd.
5. Send comments to: wtraub@cfa.harvard.edu