Note: Once again, we were in the highest-ranked proposals at the WIYN, so we should be given high priority to get our observations in the queue scheduling mode. Also, note that the HST DD time should have been following up our March SNe, but they are too busy running tests of the new instruments -- we will still try to get a few nights on one supernova, if we can convince them. The two search runs of Jan and March 1997 are scheduled so far as follows: Dec 13,14 CTIO references, and test search using old references Jan 4,5 CTIO search Jan 8,10,12 WIYN check candidates and follow up: Brad Schaefer (Yale time) Jan 13-18 WIYN check candidates and follow up -- queue scheduled Jan 9,10 CTIO further searching and follow-up photometry Jan 11,12 Keck follow-up spectroscopy Jan 12,13 ESO follow-up spectroscopy or photometry (whichever is needed) Jan 29,31 WHT S/D time first half of both these nights. Jan 30 WHT Pilar can get one or so SN this night. Jan 31 CTIO follow-up photometry Feb 2-7 WIYN queue scheduled follow-up Feb 6 ESO follow-up spectroscopy or photometry (whichever is needed) Feb 9,10 CTIO references, and test search using old references Feb 12-16 WIYN (Yale, not yet confirmed) photometry (38--77% moon) Feb 13 AAT service spectroscopy (if useful for R<22 mag?) Feb18-18,24-26 WIYN queue photometry BUT bright time Feb 28?? INT CAT time [proposed, but 64% moon] Mar 3-7 AAT photometry? Brian Boyle(0.4 arcsec/pix x1000 pixel field) Mar 5,6 CTIO search Mar 9,10 CTIO further searching and follow-up photometry Mar 9-14 WIYN queue Mar 11-17 AAT 2-degree-field (2DF) Mar 11,12 INT CAT time [12th possible] Mar 11,12,13 Keck follow-up spectroscopy Mar 12-18 MDM Possible 2.5m spectroscopy of very bright SN Mar 15-18 OCIW Possible Los Companos 2.5m spectroscopy of very bright SN Mar 19-23 WHT IS/UES service/discretionary (Benn,et al) Mar 24-30 WHT WYFFOSmultiobject spectrograph(1 S/D night+7commisioning) Mar 24-28 WIYN (Yale, not confirmed) BUT bright time Mar 29-Apr 3 WIYN queue photometry [two nights may be taken out of this] Apr 1 WHT WYFFOSmultiobject spectrograph S/D night (Chris Benn) Apr 3 INT Prime-focus service/discretionary night (Mike Irwin on) Apr 2-11 AAT 2-degree-field (2DF) spectroscopy Apr 6,7 ESO follow-up photometry (or spectroscopy, if still needed) Apr 11 INT CAT time Apr 13-18 WIYN queue BUT grey-to-bright time Apr 28,29 INT Prime-focus service/discretionary night (Nic Walton on) Apr 28-May 2 WIYN (Yale, not yet confirmed) Apr 30 WHT Prime-focus service/discretionary night May 3-8 WIYN queue photometry May 8 WHT Prime-focus service/discretionary HALF night May 4 INT CAT time May 4,6 ESO follow-up photometry time May 18, 24-26 WIYN queue BUT bright time May 28,29 INT Prime-focus service/discretionary night (Nic Walton on) June 2-7 WIYN (Yale, not yet confirmed) June 8-12 WIYN queue [two nights may be taken out of this] June 27-July 2 WIYN queue July 7-11 WIYN (Yale, not yet confirmed) July 22 WIYN queue BUT bright time NB: We will request that our HST director's discretionary time be scheduled approximately every 8 days for 5 points over the peak of the lightcurve, beginning approximately March 12 (the earliest they will allow us to start), and then one final point 9 -- 12 months later.