H. E. Bond 4/17/03 SMARTS 1.5m Service Observing Program Night of Sunday 2003 April 20-21 Times are UT-4 Sunset: 18:18 Twilight: 5:45 Twilight: 19:39 Sunrise: 7:06 Moon age -11 days. RA/Dec: 1754-26 Rises 21:41 Sidereal time evening twilight: 08:50 morning twilight: 18:57 .............................................................................. Civil date Setup Program(s) Apr 20 56/II Observing plan: http://www.stsci.edu/~bond/s15m030420.plan STSI 03a-02/Bond [1.00] STSI 03a-04/Walborn [0.00] .............................................................................. 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: - obtain at least 10 Zero frames - obtain at least 5, preferably 10, flat-field frames (projector or dome) No twilight spectrum needed Observe at beginning of night: Pgm Pri Target RA (J2000) Dec mag Exp Cmp Remarks STSI 03a-02 1 mu CMa 06 56 06.6 -14 02 36 5.0 3x10 2 Main observing program; observe as many of these as possible. If exposure time is not given, make an estimate based on the magnitude: STSI 03a-02 1 NGC 1360 03 33 14.6 -25 52 18 11.3 3x180 2 Airmass may be too high STSI 03a-02 1 NGC 1535 04 14 15.5 -12 44 24 12.1 3x360 2 " " " " " STSI 03a-02 3 J 320 05 05 34.4 10 42 21 13.7 3x600 2 STSI 03a-02 1 LoTr 1 05 55 07.1 -22 54 02 14 3x600 2 STSI 03a-02 1 K 2-2 06 52 23.2 9 57 56 14.3 3x600 2 STSI 03a-02 1 NGC 2392 07 29 10.8 20 54 42 10.5 3x200 2 STSI 03a-02 1 EGB 5 08 11 12.8 10 57 17 13.8 3x600 2 STSI 03a-02 1 He 2-36 09 43 25.9 -57 16 57 11.3 3x250 2 STSI 03a-02 1 LSS 1362 09 52 44.6 -46 16 50 12.4 3x400 2 STSI 03a-02 2 NGC 3242 10 24 46.2 -18 38 34 12.3 3x400 2 STSI 03a-02 1 HD 107369 12 20 45.0 -32 33 26 9.5 3x90 2 STSI 03a-02 1 NGC 4361 12 24 30.8 -18 47 06 13.2 3x500 2 STSI 03a-02 1 Lo 8 13 25 37.4 -37 36 16 12.9 3x450 2 STSI 03a-02 1 Omega Cen 24 13 26 26.3 -47 16 27 10.8 3x150 2 STSI 03a-02 1 A 36 13 40 41.3 -19 52 55 11.5 3x200 2 STSI 03a-02 3 NGC 5315 13 53 57.1 -66 30 50 14.4 3x600 2 STSI 03a-02 3 SuWt 2 13 55 43.2 -59 22 41 12.2 3x400 2 STSI 03a-02 2 He 2-108 14 18 09.0 -52 10 41 12.7 3x400 2 STSI 03a-02 1 NGC 5882 15 16 49.9 -45 38 59 13.4 2 STSI 03a-02 2 He 2-131 15 37 11.4 -71 54 52 11.0 3x150 2 STSI 03a-02 1 LSE 125 15 43 05.0 -39 18 15 12.4 3x400 2 STSI 03a-02 1 NGC 5986-W 15 46 03.3 -37 46 38 12 3x300 2 STSI 03a-02 1 NGC 5986-E 15 46 05.5 -37 47 01 12 3x300 2 STSI 03a-02 1 Cn 1-1 15 51 16.0 -48 45 00 11.1 3x180 2 STSI 03a-02 1 He 2-138 15 56 01.9 -66 09 09 10.9 3x120 2 STSI 03a-02 1 NGC 6026 16 01 21.0 -34 32 36 13.2 2 STSI 03a-02 1 IC 4593 16 11 44.5 12 04 16 11.2 3x150 2 STSI 03a-02 1 He 2-151 16 15 42.4 -59 54 01 13.0 3x360 2 STSI 03a-02 2 He 2-162 16 27 51.0 -54 01 30 13.4 3x450 2 STSI 03a-02 1 BD +14 3061 16 29 48.6 +14 15 44 9.5 3x75 2 STSI 03a-02 2 PC 11 16 37 42.9 -55 42 27 12.6 3x500 2 STSI 03a-02 2 He 2-182 16 54 35.3 -64 14 29 13.4 3x600 2 STSI 03a-02 1 IC 4634 17 01 33.7 -21 49 34 13.9 2 STSI 03a-02 1 H 2-1 17 04 36.3 -33 59 20 13.2 2 STSI 03a-02 2 Tc 1 17 45 35.4 -46 05 24 11.3 3x180 2 STSI 03a-02 1 M 1-26 17 45 57.8 -30 12 01 12.7 2 STSI 03a-02 1 Sp 3 18 07 15.9 -51 01 09 12.5 2 STSI 03a-02 1 NGC 6629 18 25 42.4 -23 12 11 12.9 2 STSI 03a-02 1 M 1-55 18 36 33.9 -21 49 04 13.9 2 STSI 03a-02 1 Hb 7 18 55 37.8 -32 15 49 13.9 2 Observe all 3 of these at end of night. (HD 148937 can be omitted tonight.) For the nova, also take a shorter exposure if any part of the spectrum is saturated at 300 sec. STSI 03a-04 3 HD 148937 16 33 52.2 -48 06 40 6.7 3x30 1 STSI 03a-02 1 5 Ser 15 19 18.8 +01 45 55 5.0 3x10 2 STSI 03a-05 1 V4743 Sgr 19 01 09.4 -22 00 06 11 3x300 1 nova, very faint on sky survey STSI 03a-02 1 LSIV -12.111 20 01 49.8 -12 41 18 11.3 3x200 2 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 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 03a-02) Nolan Walborn walborn@stsci.edu (program STSI 03a-04)