IOTA 1999 TRIMESTER NO. 1
                   FINAL -- OBSERVING SCHEDULE 
 
Dates Nights Observers (PI & CoIs)   Inst.   Project
----- ------ ----------------------- ------- -----------------------
Jan 1    1   Open

Jan     11   Carleton,Lacasse,       3rd telescope work
2-12         Pras,Morel

Jan      9   Corporon, et al.        Nicmos  HAeBe binaries
13-21        (tbd)                   & lens
            
Jan 22  19   Morel                   Nicmos  Fringe packet tracker
-Feb 9                               & lens

Feb      5   Bregman,Witteborn,      Nicmos  Fringe packet tracker 
10-14        Morel                   & lens  & star tracker 

Feb     10   Porro,Schuller,         Nicmos  MIDI calibrator stars
15-24        Ligori,Leinert          & lens  & YSO disks

Feb      2   Morel                   Nicmos  Fringe packet tracker
25-26                                & lens

Feb 27   7   Millan-Gabet,Traub,     Nicmos  AeBe, symbiotics, CI Cam,
-Mar 5       Schloerb,Kanbur,        & lens  & Mira diameters
             Karovska

Mar     15   Foresto,Ruilier,        Nicmos  Fast-scan, binaries,
6-20         Ridgway,Mennesson,      & Fluor & Miras
             Perrin

Mar      7   Schoeller,Tokovinin,    Nicmos  Multiple star systems
21-26        Kervella,Foresto        & Fluor  

Mar 27  15   Mennesson,Chagnon,      Tisis   Supergiants
-Apr 10      Foresto,Ridgway,        M-band  & Miras
             Ruilier,Perrin

Apr     14   Segransan,Forveille,    Nicmos  Low mass binaries
11-24        Perrier,Traub,          & lens
             Milan-Gabet

Apr      2   Morel,Bregman,          Nicmos  Fringe packet tracker
25-26        Witteborn               & lens

Apr 27  18   Millan-Gabet,Traub,     Nicmos  AeBe, symbiotics,
-May 14      Schloerb,Kanbur,        & lens  & Mira diameters
             Karovska

Notes:
1.  People may wish to come a few days early to familiarize themselves with
the detector system to be used;  observers should cooperate by passing on 
their acquired wisdom about the current state of the instruments.
2.  The Nicmos detector may in fact be a Picnic detector, which should be a
somewhat better detector, but this switch is not settled as of this writing.
3.  The 4mm lens inside the Nicmos dewar reduces the plate scale nicely for
the classical beamsplitter setup, but is too strong for the 2x2 fiber-end 
image, and will need to be removed for fiber (Fluor) work, or else the 
standard InSb Fluor detectors should be used.  The lens removal/insertion is
not difficult for dexterous people, but it should be approached with caution. 
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