H. E. Bond 7/29/04 SMARTS 1.5m Service Observing Program Night of Thursday 2004 July 29-30 Times are UT-4 Sunset: 18:08 Twilight: 6:07 Twilight: 19:31 Sunrise: 7:30 Duration of night: 10:36 Moon age 12 days. RA/Dec: 19 06 50, -27 09.7 Sets 06:52 Sidereal time evening twilight: 15:20 midnight: 19:49 morning twilight: 01:58 .............................................................................. Civil date Setup Program(s) Jul 29 56/II Observing plan: http://www.stsci.edu/~bond/s15m040729.plan STSI 04a-08/BondPNN STSI 04a-11/BondV838Mon STSI 04a-05/Walborn SUNY 04a-11/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 two times: near 20:15 local time (0:15 UT) near 2:30 local time (6:30 UT) IC 4593 Try to observe two times: at about 19:25 local time (as soon as sky is dark enough) at about 22:30 local time S CrA observe twice: at about 2010 CST at about 0210 CST (when the star is at - and + 3 hours HA). ASAS 164647 Get one good observation. If it has strong emission lines, make sure they are not saturated. LSIV -12.111 Try to observe two times approx 6 hours apart: at or before 21:10 local time, and again at or after 3:10 local time NGC 6891 Try to observe two times: at about 22:30 local time at about 2:30 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 SUNY 04a-11 2 LTT 4364 11 45 37.7 -64 50 25 11.5 3x240 1 STSI 04a-08 3 HD 107369 12 20 45.0 -32 33 26 9.5 3x90 2 PAGB STSI 04a-08 1 NGC 4361 12 24 30.8 -18 47 06 13.2 3x500 2 STSI 04a-08 2 DY Cen 13 25 34.2 -54 14 45 12 3x400 2 STSI 04a-08 1 Lo 8 13 25 37.4 -37 36 16 12.9 3x450 2 STSI 04a-08 3 Omega Cen 24 13 26 26.3 -47 16 27 10.8 3x150 2 PAGB STSI 04a-08 1 A 36 13 40 41.3 -19 52 55 11.5 3x200 2 STSI 04a-08 1 LSE 153 13 53 08.2 -46 43 42 11.4 3x150 2 sdO STSI 04a-08 3 SuWt 2 13 55 43.2 -59 22 41 12.2 3x400 2 STSI 04a-08 1 HD 127493 14 32 21.5 -22 39 26 10.0 3x150 2 sdO STSI 04a-08 1+ 5 Ser 15 19 18.8 +01 45 55 5.0 3x30 2 RV std STSI 04a-08 1 LSE 125 15 43 05.0 -39 18 15 12.4 3x350 2 STSI 04a-08 3 NGC 5986-W 15 46 03.3 -37 46 38 12 3x300 2 PAGB STSI 04a-08 3 NGC 5986-E 15 46 05.5 -37 47 01 12 3x300 2 PAGB STSI 04a-08 1 Cn 1-1 15 51 16.0 -48 45 00 11.1 3x180 2 STSI 04a-08 1 He 2-138 15 56 01.9 -66 09 09 10.9 3x120 2 STSI 04a-08 1+ NGC 6026 16 01 21.0 -34 32 36 13.2 3x500 2 STSI 04a-08 1+ IC 4593 16 11 44.5 12 04 16 11.2 3x150 2 STSI 04a-08 2 He 2-151 16 15 42.4 -59 54 01 13.0 3x400 2 STSI 04a-08 1 LS IV -12 1 16 23 44.0 -12 12 34 11.1 3x150 2 sdO STSI 04a-08 3 BD +14 3061 16 29 48.6 +14 15 44 9.5 3x75 2 PAGB STSI 04a-05 3 HD 148937 16 33 52.2 -48 06 40 6.7 3x30 1 (Walborn) STSI 04a-08 1+ HD 149382 16 34 23.3 -04 00 52 9.0 3x75 2 RV std/sdOB STSI 04a-08 2 PC 11 16 37 42.9 -55 42 27 12.6 3x400 2 STSI 04a-08 1 ASAS 164647 16 46 46.8 -55 42 40 12.5 3x400 1 STSI 04a-08 2 He 2-187 17 01 37.1 -50 22 59 12.7 3x500 2 STSI 04a-08 2 SaSt 2-12 17 03 03.0 -53 55 55 11.5 3x300 2 STSI 04a-08 1 IC 4637 17 05 10.5 -40 53 10 12.5 3x600 2 STSI 04a-08 2 Tc 1 17 45 35.4 -46 05 24 11.3 3x180 2 STSI 04a-08 2 M 1-26 17 45 57.8 -30 12 01 12.7 3x500 2 STSI 04a-08 1 Sp 3 18 07 15.9 -51 01 09 12.5 3x400 2 STSI 04a-08 1+ Cn 3-1 18 17 34.1 10 09 04 12.3 3x180 2 STSI 04a-08 2 NGC 6629 18 25 42.4 -23 12 11 12.9 3x500 2 STSI 04a-08 2 M 1-46 18 27 56.4 -15 32 57 12.8 3x400 2 STSI 04a-08 2 VV 3-5 18 36 32.4 -19 19 29 13.3 3x500 2 STSI 04a-08 1 M 1-55 18 36 33.9 -21 49 04 13.9 3x700 2 STSI 04a-08 1 HD 171858 18 37 56.7 -23 11 35 9.9 3x100 2 sdB STSI 04a-08 2 Sa 3-151 18 58 51.7 -00 32 55 14 3x600 2 SUNY 04a-10 1++ S CrA 19 01 08.7 -36 57 20 11 3x600 1 STSI 04a-08 2 Sh 2-71 19 02 00.3 2 09 10 13.4 3x500 2 STSI 04a-08 2 LSE 263 19 02 11.8 -51 30 10 11.7 3x200 2 sdO STSI 04a-08 3 IRAS 1912+17 19 14 59.8 17 22 45 13.4 3x400 2 STSI 04a-08 2 LSE 21 19 55 38.2 -23 13 42 11.8 3x200 2 sdO STSI 04a-08 1+ LSIV -12.111 20 01 49.8 -12 41 18 11.3 3x200 2 STSI 04a-08 1+ NGC 6891 20 15 08.9 +12 42 14 12.4 3x400 2 STSI 04a-08 1 CRBB 1 20 19 28.7 -41 31 28 10.6 3x200 2 STSI 04a-08 1 HD 205805 21 39 10.6 -46 05 52 10.2 3x120 2 sdB STSI 04a-08 1++ Feige 110 23 19 58.4 -05 09 56 11.8 3x300 2 sdO/RV std STSI 04a-08 1 CD -35 15910 23 44 22.0 -34 27 00 11.0 3x200 2 sdB STSI 04a-08 1+ 6 Cet 00 11 15.9 -15 28 05 4.9 3x10 2 RV std STSI 04a-08 1 CD -38 222 00 42 58.3 -38 07 37 10.5 3x120 2 sdB STSI 04a-08 1 NGC 246 00 47 03.4 -11 52 19 11.8 3x300 2 STSI 04a-08 1 HD 4539 00 47 29.2 +09 58 56 10.3 3x120 2 sdB STSI 04a-08 1 BD -11 162 00 52 15.1 -10 39 46 11.1 3x200 2 STSI 04a-08 1 PHL 932 00 59 56.7 +15 44 13 12.1 3x300 2 sdB/PNN STSI 04a-08 1 NGC 1360 03 33 14.6 -25 52 18 11.3 3x180 2 STSI 04a-08 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 04a-11 2 V5114 Sgr 18 19 32.3 -28 36 36 ~11 3x240 1 nova STSI 04a-11 3 V4745 Sgr 18 40 02.5 -33 26 55 ~12? 3x450 1 nova STSI 04a-11 3 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 .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (program STSI 04a-08) Nolan Walborn walborn@stsci.edu (program STSI 04a-05) Fred Walter (program SUNY 04a-11)