FM Walter 8/15/06 rev 0816 SMARTS 1.5m Service Observing Program 060819 --- EPHEMERIS INFORMATION --- For the night of: Sat, 2006 Aug 19 ---> Sun, 2006 Aug 20 Local midnight = 2006 Aug 20, 4 hr UT, or JD 2453967.667 Local Mean Sidereal time at midnight = 21 10 09.8 Sunset ( 2215 m horizon): 18 28 CST; Sunrise: 7 05 CST Evening twilight: 19 42 CST; LMST at evening twilight: 16 51 Morning twilight: 5 52 CST; LMST at morning twilight: 3 03 Moonrise: 5 15 CST Moon at civil midnight: illuminated fraction 0.120 3.6 days before new moon, RA and dec: 7 15 05, 27 22.7 The sun is down for 12.6 hr; 10.2 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) August 19 47/IIb CHIL 06b-921 47/Ib STSI 06b-13 47/II SUNY 06b-03 SUNY 06b-10 SUNY 06b-12 SUNY 06b-22 .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 47/IIb 83.0 CuSO4 620 47 28.22 He-Ar 45 200 280 3550 4058-4732 1.6 47/Ib 110.5 GG495 595 47 22.64 Neon 20 200 280 164 7100 5652-6972 3.1 47/II 83.0 CuSO4 620 47 27.39 He-Ar 45 200 280 3550 3878-4552 1.6 .............................................................................. In afternoon or during dinner: - Install 47/IIb grating setup - check focus if necessary - obtain at least 25 Zero frames - obtain at least 10, preferably 25, flat-field frames (projector or dome) Get well-exposed TWILIGHT SPECTRA at zenith at beginning of night. Aim for three spectra, each with between 5,000 and 30,000 counts per pixel. ---------------------------------------------------------------------------- Program Pri Target RA (J2000) Dec mag Exp Cmp T CST Rem cal 1 LTT 4364 11 45 37.70 -64 50 25.1 11.5 3x 240 1 21 19 3 SUNY 06b-12 1 HD 109962 12 39 07.89 -45 33 44 9.7 3x 400 2 30 19 24 STSI 06b-08 1 HD 148937 16 33 52.2 -48 06 40 6.7 3x 60 1 12 19 54 SUNY 06b-10 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 600 1 39 20 6 end 47/IIb 20 45 ****************** GRATING TILT, FILTER, etc., CHANGE ****************** When the above list has been finished, change the grating tilt, filter, slit, comparison source, possibly the collimator focus, etc., to the 47/Ib setup. SUNY 06b-10 2 ScoPMS 51 16 12 20.9 -19 9 3.5 15.4 3x 600 1 39 21 10 SUNY 06b-22 1 LuHa-33 16 08 01.11 -39 02 51.6 15.7 3x1420 1 80 21 49 SUNY 06b-10 2 Oph 118 16 31 15.8 -24 34 02.1 12 3x 300 1 24 23 9 STSI 06b-08 1 HD 148937 16 33 52.2 -48 06 40 6.7 3x 60 1 12 23 33 NOAO6A-4030 2 2U_12993238 17 38 40.3 -44 17 42.8 10.3 3x 300 1 24 23 45 NOAO6A-4030 2 2U_12993290 17 38 46.3 -44 06 00.8 8.1 3x 90 1 14 0 9 NOAO6A-4030 2 2U_14065576 18 03 50.1 -41 33 25.0 12.6 3x 300 1 24 0 23 SUNY 06b-10 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 0 47 CHIL 6b-921 1 NGC7213 22 09 16.25 -47 10 00.0 --- 3x 360 1 27 1 11 S2 CHIL 6b-921 2 CD-47-14075 22 09 45.89 -47 13 15.9 9.8 1x 60 0 7 1 38 S10 cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 240 1 21 1 45 NOAO 6b-909 1 chs-43-5615 3 27 46.55 -28 10 04.3 12.0 3x 300 1 24 2 6 E1 cal 1 pflat --- --- --- 0 10 2 30 end 47/Ib 2 40 ****************** GRATING TILT, FILTER, etc., CHANGE ****************** When the above list has been finished, change the grating tilt, filter, slit, comparison source, possibly the collimator focus, etc., to the 47/II setup. cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 240 1 21 3 5 STSI 06b-13 1 6 Cet 0 11 15.9 -15 28 05 4.9 3x 15 2 11 3 26 R STSI 06b-13 1 CD -38 222 0 42 58.3 -38 07 37 10.5 3x 150 2 18 3 37 STSI 06b-13 1 NGC 246 0 47 03.4 -11 52 19 11.8 3x 300 2 25 3 55 STSI 06b-13 1 HD 4539 0 47 29.2 +09 58 56 10.3 3x 120 2 16 4 20 STSI 06b-13 2 PHL 932 0 59 56.7 +15 44 13 12.1 3x 300 2 25 4 36 STSI 06b-13 2 BD -11 162 0 52 15.1 -10 39 46 11.1 3x 200 2 20 5 1 STSI 06b-13 2 NGC 1360 3 33 14.6 -25 52 18 11.3 3x 200 2 20 5 21 STSI 06b-13 2 NGC 1535 4 14 15.5 -12 44 24 12.1 3x 360 2 28 5 41 SUNY 06b-03 + HD 37468 5 38 44.77 -02 36 00.2 3.7 3x 30 1 10 6 9 SUNY 06b-03 2 HD 35079 5 21 58.28 -02 57 49.4 7.0 3x 150 1 16 6 19 cal 1 pflat --- --- --- 0 10 6 35 end 47/II 6 45 If there is any time left before dawn, or you get ahead and have to wait for targets to rise, or if some targets are too faint to acquire, please select from among the following 47/II targets: SUNY 05b-09 3 AB Dor 5 28 44.8 -65 26 54.8 7.0 3x 120 1 15 SUNY 06b-03 3 HD 34238 5 15 46.40 -01 16 40.4 8.77 3x 180 1 18 SUNY 06b-03 3 HD 34280 5 16 14.54 -03 28 59.2 7.76 3x 150 1 16 SUNY 06b-03 3 HD 34582 5 18 24.33 -02 32 07.5 8.72 3x 180 1 18 SUNY 06b-03 3 HD 34595 5 18 29.97 -01 08 17.7 9.34 3x 200 1 19 SUNY 06b-03 1 HD 35153 5 22 38.82 -01 02 33.9 9.0 3x 200 1 19 SUNY 06b-03 1 HD 35259 5 23 19.76 -03 6 6.3 9.7 3x 200 1 19 SUNY 06b-03 3 HD293959 5 19 33.47 -02 19 20.4 9.23 3x 240 1 21 SUNY 06b-03 3 HD294046 5 25 55.87 -02 20 07.9 8.28 3x 200 1 19 SUNY 06b-03 3 HD294054 5 23 34.18 -02 48 18.7 9.64 3x 240 1 21 Just before sunrise, get well-exposed TWILIGHT SPECTRA at zenith. Aim for 3-5 spectra, each with between 5,000 and 30,000 counts per pixel. -------------------------------------------------------------------- Remarks: M: moon within 10 degrees. Skip if the star is not seen in the acquisition TV B: very bright star: best observed through clouds. C: cataclysmic variable. May be fainter than in finding chart. Skip if not visible. E: may be below the east limit if you get to it early. E1: if target is too far to the east to reach, insert the following target(s): standard 3 BD+19 5116 23 31 52.2 +19 56 14 10.3 3x 200 1 19 standard 3 HD222661 23 42 43.3 -14 32 41.7 4.5 3x 10 1 9 F: faint target may be hard to see with moon up. N: Nova. Will be fainter than on finding chart. R: radial velocity standard. S2: set slit width to 2.0 arcsec. Be sure to center on the nucleus of the galaxy. S10: set slit width to 10.0 arcsec. Please reset at the end of the observation. No wavecal is necessary with this exposure. TC: time critical. maintain spacing between the 3 images W: target reaches 2 air masses at end of exposure. Do not start late; do the calibration lamp at the end. X: If running 10 minutes or more ahead at this point, increase exposure lengths to 600 seconds. Y: 5 arcsec SE of brighter star. Skip if not clearly resolved. -------------------------------------------------------------------- General Notes: Astronomical ephemerides are from SKYCAL,by John Thorstensen Pri: Target priority. + = absolute highest priority 1 = observe object if possible 2 = extra targets; skip if running behind and Priority 1 targets remain unobserved. 3 = backup/filler targets; low priority Cmp: 1 means take comparison spectrum only before target exposures; 2 means before and after The T column lists the approximate time in minutes for this line. This includes 5 minutes acquisition plus 1 minute for the comparison. The CDT column is the approximate start time assumed for scheduling purposes. If you fall too far behind, you may need to drop some priority 2 or 3 targets, but otherwise don't pay too much attention to it. As I get experience with scheduling, I will try to make it more accurate. For now I am allotting the nominal overheads, plus 25 minutes for a change in the grating tilt/filter. .............................................................................. Notes about finding charts: RA & Dec: all coordinates are accurate to 1"; charts can be generated by operator as necessary using LEDAS or DSS. Most charts are available via the link from the main 1.5m scheduling page. Charts for most objects should be available at the telescope. .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs) Eric Mamajek emamajek@cfa.harvard.edu (NOAO 06a-4030)