/schedule/obs.01-3b IOTA 2001 TRIMESTER NO. 3 10 September 2001 REVISED FINAL OBSERVING SCHEDULE Dates Nights Observers (PI, CoIs) Inst. Project --------- ------ ---------------------- ----------- ------------------------- Sept 1-15 15 Ahearn, Lacasse Star tracker Rapid acquisition, 3 tel. Sept 16-30 15 Traub, Millan-Gabet, 3-beam comb. Phase-closure engineering; Monnier, Berger, & PICNIC star-tracker engineering Pedretti, Carleton, Schloerb, Ragland, Lacasse, Ahearn Oct 1-7 7 Monnier, Berger, visible Cepheid pulsation diameters CfA team fibers, APDs Oct 8-14 7 Schloerb, Pedretti, 3-beam comb. Capella and Betelgeuse IOTA team PICNIC Oct 15-29 15 Pedretti, IOTA Team 3-beam comb. Betelgeuse and Capella (as above) PICNIC Oct 30- 10 Perrin, Mennesson, FLUOR/NICMOS Mira stars: K' narrow-band; Nov 8 Foresto, Ridgway; (IM Peg on Nov 1, 7 +/-1); Ragland Mira synoptic program Nov 9-12 4 Gerbaldi, Foresto, FLUOR/NICMOS Lambda Boo stars; Perrin, Borde, Mk III G/SG stars Faraggiana, Lai; Safizadeh Nov 13-22 10 Borde, Foresto; FLUOR/NICMOS Short-period binary stars; Safizadeh Mk III G/SG stars Nov 23- 14 Berger, Haguenauer, Integ Optic Phase-closure meas. Dec 6 Kern, Malbet, Traub, PICNIC Millan-Gabet, Perraut Dec 7-27 21 Pedretti, Traub, 3-beam comb. Betelgeuse Millan-Gabet, Berger, Integ Optic IOTA team PICNIC Dec 28- 12 Ragland, Traub, FLUOR/NICMOS Mira stars Jan 8 IOTA team ________________________________________________________________________________ 1. This is a REVISED FINAL fall 2001 schedule; the main difference from before is that 3-beam work is moved to the last 3 weeks of October, and FLUOR work is moved to the first 3 weeks of November. 2. The single-CCD star-tracker acquisition sequence using VxWorks control will be perfected by Ahearn and Lacasse this summer, and will be used for both 2- and 3-telescope observations starting in September. 3. Telescopes and delay lines will also be controlled by the VxWorks system. 4. Data acquisition and Short Delay (SD1) for FLUOR will be controlled by FLUOR as usual. 5. FLUOR observers are requested to look at IM Peg on the approximate dates shown with ~38 m baseline, in exchange for collaboration rights with M. Ratner. 6. FLUOR observers are requested to help Michelson Summer School IOTA-time winner Neda Safizadeh with her Mk III giant, supergiant K-band program, also collab. ________________________________________________________________________________