H. E. Bond 8/21/04 SMARTS 1.5m Service Observing Program Night of Sunday 2004 August 22-23 Times are UT-4 Sunset: 18:22 Twilight: 5:47 Twilight: 19:42 Sunrise: 7:08 Duration of night: 10:05 Moon 0.3 days before first quarter, RA and dec: 15 33 19, -20 57.8 Moonset : 1 16 CST Sidereal time evening twilight: 17:06 midnight: 21:24 morning twilight: 03:13 .............................................................................. Civil date Setup Program(s) Aug 22 56/II Observing plan: http://www.stsci.edu/~bond/s15m040729.plan STSI 04b-11/BondPNN STSI 04b-14/STScI TOO STSI 04b-04/Walborn SUNY 04b-13/Walter .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. Res (A) 56/II 83.0 CuSO4 620 56 22.90 He-Ar 60 225 280 4900 4017-4938 2.2 .............................................................................. In afternoon or during dinner: - Install 56/II grating setup - CONFIRM THAT THE GRATING TILT IS SET TO EXACTLY 22.90 - check focus - obtain at least 10 Zero frames - obtain at least 5, preferably 10, flat-field frames (projector or dome) Try to get a few good twilight spectra at the beginning (or end) of the night, but only if it would not interfere with observations of target stars. NOTE NOTE NOTE: Highest priority: NGC 6026 Observe one time: near 21:45 local time (1:45 UT) IC 4593 Try to observe two times: at about 19:25 local time (as soon as sky is dark enough) at about 21:00 local time S CrA Observe twice: at about 1930 (after IC 4593) at about 0100 CST LSIV -12.111 Try to observe two times: at or before 20:00 local time, and again at or after 1:45 local time NGC 6891 Try to observe two times: at about 21:30 local time at about 0:30 local time PHL 932 Try to observe two times: at about 02:30 local time at about 04:30 local time Make sure to observe the 1++ and 1+ targets. During the rest of the night, select targets according to the listed priorities. There are more targets than can be observed during the night. Stars marked "sdB" can be observed several times during the night, separated by ~2 hours or more. Pgm Pri Target RA (J2000) Dec mag Exp Cmp Remarks STSI 04b-11 1+ DY Cen 13 25 34.2 -54 14 45 12 3x400 2 STSI 04b-11 1 Lo 8 13 25 37.4 -37 36 16 12.9 3x450 2 STSI 04b-11 1 Omega Cen 24 13 26 26.3 -47 16 27 10.8 3x150 2 PAGB STSI 04b-11 1 A 36 13 40 41.3 -19 52 55 11.5 3x200 2 STSI 04b-11 1 LSE 153 13 53 08.2 -46 43 42 11.4 3x150 2 sdO STSI 04b-11 3 SuWt 2 13 55 43.2 -59 22 41 12.2 3x400 2 STSI 04b-11 1 HD 127493 14 32 21.5 -22 39 26 10.0 3x150 2 sdO STSI 04b-11 1+ 5 Ser 15 19 18.8 +01 45 55 5.0 3x30 2 RV std STSI 04b-11 1 LSE 125 15 43 05.0 -39 18 15 12.4 3x350 2 STSI 04b-11 1 NGC 5986-W 15 46 03.3 -37 46 38 12 3x300 2 PAGB STSI 04b-11 1 NGC 5986-E 15 46 05.5 -37 47 01 12 3x300 2 PAGB STSI 04b-11 1 Cn 1-1 15 51 16.0 -48 45 00 11.1 3x180 2 STSI 04b-11 1 He 2-138 15 56 01.9 -66 09 09 10.9 3x120 2 STSI 04b-11 1+ NGC 6026 16 01 21.0 -34 32 36 13.2 3x500 2 STSI 04b-11 1+ IC 4593 16 11 44.5 12 04 16 11.2 3x150 2 STSI 04b-11 2 He 2-151 16 15 42.4 -59 54 01 13.0 3x400 2 STSI 04b-11 1 LS IV -12 1 16 23 44.0 -12 12 34 11.1 3x150 2 sdO STSI 04b-11 1 BD +14 3061 16 29 48.6 +14 15 44 9.5 3x75 2 PAGB STSI 04b-04 1 HD 148937 16 33 52.2 -48 06 40 6.7 3x30 1 (Walborn) STSI 04b-11 1+ HD 149382 16 34 23.3 -04 00 52 9.0 3x75 2 RV std/sdOB STSI 04b-11 2 PC 11 16 37 42.9 -55 42 27 12.6 3x400 2 STSI 04b-11 3 ASAS 164647 16 46 46.8 -55 42 40 12.5 3x400 1 STSI 04b-11 2 He 2-187 17 01 37.1 -50 22 59 12.7 3x500 2 STSI 04b-11 2 SaSt 2-12 17 03 03.0 -53 55 55 11.5 3x300 2 STSI 04b-11 1 IC 4637 17 05 10.5 -40 53 10 12.5 3x600 2 STSI 04b-11 2 Tc 1 17 45 35.4 -46 05 24 11.3 3x180 2 STSI 04b-11 2 M 1-26 17 45 57.8 -30 12 01 12.7 3x500 2 STSI 04b-11 1 Sp 3 18 07 15.9 -51 01 09 12.5 3x400 2 STSI 04b-11 1+ Cn 3-1 18 17 34.1 10 09 04 12.3 3x180 2 STSI 04b-11 2 NGC 6629 18 25 42.4 -23 12 11 12.9 3x500 2 STSI 04b-11 2 M 1-46 18 27 56.4 -15 32 57 12.8 3x400 2 STSI 04b-11 2 VV 3-5 18 36 32.4 -19 19 29 13.3 3x500 2 STSI 04b-11 1 M 1-55 18 36 33.9 -21 49 04 13.9 3x700 2 STSI 04b-11 1 HD 171858 18 37 56.7 -23 11 35 9.9 3x100 2 sdB STSI 04b-11 2 Sa 3-151 18 58 51.7 -00 32 55 14 3x600 2 SUNY 04b-13 1++ S CrA 19 01 08.7 -36 57 20 11 3x600 1 STSI 04b-11 2 Sh 2-71 19 02 00.3 2 09 10 13.4 3x500 2 STSI 04b-11 2 LSE 263 19 02 11.8 -51 30 10 11.7 3x200 2 sdO STSI 04b-11 3 IRAS 1912+17 19 14 59.8 17 22 45 13.4 3x400 2 STSI 04b-11 2 LSE 21 19 55 38.2 -23 13 42 11.8 3x200 2 sdO STSI 04b-11 1+ LSIV -12.111 20 01 49.8 -12 41 18 11.3 3x200 2 STSI 04b-11 1+ NGC 6891 20 15 08.9 +12 42 14 12.4 3x400 2 STSI 04b-11 1 CRBB 1 20 19 28.7 -41 31 28 10.6 3x200 2 STSI 04b-11 1 HD 205805 21 39 10.6 -46 05 52 10.2 3x120 2 sdB STSI 04b-11 1++ Feige 110 23 19 58.4 -05 09 56 11.8 3x300 2 sdO/RV std STSI 04b-11 1 CD -35 15910 23 44 22.0 -34 27 00 11.0 3x200 2 sdB STSI 04b-11 1+ 6 Cet 00 11 15.9 -15 28 05 4.9 3x10 2 RV std STSI 04b-11 1 CD -38 222 00 42 58.3 -38 07 37 10.5 3x120 2 sdB STSI 04b-11 1 NGC 246 00 47 03.4 -11 52 19 11.8 3x300 2 STSI 04b-11 1 HD 4539 00 47 29.2 +09 58 56 10.3 3x120 2 sdB STSI 04b-11 1 BD -11 162 00 52 15.1 -10 39 46 11.1 3x200 2 STSI 04b-11 1+ PHL 932 00 59 56.7 +15 44 13 12.1 3x300 2 sdB/PNN STSI 04b-11 1 NGC 1360 03 33 14.6 -25 52 18 11.3 3x180 2 STSI 04b-11 1 NGC 1535 04 14 15.5 -12 44 24 12.1 3x360 2 For the 3 novae, also take a shorter exposure if any part of the spectrum is saturated. But, increase exposure time if the first exposure is very weak. ONLY ONE SET OF 3 SPECTRA NEEDED PER EACH NOVA DURING THE NIGHT. SUNY 04b-11 3 V5114 Sgr 18 19 32.3 -28 36 36 ~11 3x300 1 nova STSI 04b-14 2 V4745 Sgr 18 40 02.5 -33 26 55 ~12? 3x450 1 nova STSI 04b-14 1 V4743 Sgr 19 01 09.4 -22 00 06 ~13? 3x700 1 nova General Notes: Pri: Target priority. 1 = observe object if possible 2 = extra targets; observe only if no Priority 1 target is available 3 = backup targets; low priority RA & Dec: all coordinates are accurate to 1"; charts can be generated by operator as necessary using LEDAS or DSS. Charts for many objects were prepared at telescope in February 2003 and should be available. Cmp: 1 means take comparison spectrum only before target exposures; 2 means before and after