FM Walter 8/20/04 SMARTS 1.5m Service Observing Program 040821 --- EPHEMERIS INFORMATION --- For the night of: Sat, 2004 Aug 21 ---> Sun, 2004 Aug 22 Local midnight = 2004 Aug 22, 4 hr UT, or JD 2453239.667 Local Mean Sidereal time at midnight = 21 19 57.4 Sunset ( 2215 m horizon): 18 30 CST; Sunrise: 7 02 CST Evening twilight: 19 43 CST; LMST at evening twilight: 17 02 Morning twilight: 5 49 CST; LMST at morning twilight: 3 10 Moonset : 0 09 CST Moon at civil midnight: illuminated fraction 0.353 1.3 days before first quarter, RA and dec: 14 38 37, -16 03.3 The sun is down for 12.5 hr; 10.1 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) Aug 21 47/II AMNH 04b-01 47/Ib STSI 04a-03 STSI 04b-04 STSI 04b-14 STSI 04b-99 SUNY 04a-10 SUNY 04b-02 SUNY 04b-10 SUNY 04b-11 SUNY 04b-13 SUNY 04b-17 .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 47/II 83.0 CuSO4 620 47 27.39 He-Ar 45 200 280 TBD 3550 3878-4552 1.6 47/Ib 110.5 GG495 595 47 22.64 Neon 20 200 280 164 7100 5652-6972 3.1 .............................................................................. New notes: 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. .............................................................................. In afternoon or during dinner: - Install 47/II 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 CDT Rem STSI 04b-99 1 BZ Cru 12 42 50.3 -63 03 31 5.3 3x 10 2 10 18 58 cal 1 LTT 4364 11 45 37.70 -64 50 25.1 11.5 3x240 1 21 19 8 SUNY 04b-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x600 1 39 19 29 S SUNY 04b-10 2 RU Lup 15 56 42.3 -37 49 15.5 11 3x600 1 39 20 8 SUNY 04b-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 9: 3x300 1 24 20 47 N STSI 04a-03 2 V2574 Oph 17 38 45.5 -23 28 18 11: 3x600 1 39 21 11 N SUNY 04b-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 9 3x600 1 39 21 50 N SUNY 04b-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x300 1 24 22 29 end 47/II 22 53 ****************** 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 04b-10 1 Oph 118 16 31 15.8 -24 34 02.1 13 3x300 1 24 23 18 STSI 04b-04 1 HD 148937 16 33 52.2 -48 06 40 6.7 3x 60 1 12 23 42 SUNY 04b-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 9: 3x100 1 14 23 54 N STSI 04a-03 2 V2574 Oph 17 38 45.5 -23 28 18 11: 3x200 1 19 0 8 N SUNY 04b-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 9 3x200 1 19 0 27 N SUNY 04b-11 1 V475 Sct 18 49 37.7 -9 33 52.7 3x600 1 39 0 46 STSI 04b-14 1 V4745 Sgr 18 40 02.5 -33 26 55 ~11 3x500 1 34 1 25 SUNY 04b-10 1 S CrA 19 01 08.7 -36 57 19.8 11 3x300 1 24 1 59 cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x200 1 19 2 23 AMNH 04b-01 1 J2127-3844 21 27 4.53 -38 44 50.8 13.4 2x 75 1 10 2 42 AMNH 04b-01 2 J2205-7240 22 05 9.00 -72 40 47.1 12.7 2x150 1 13 2 52 AMNH 04b-01 1 J2209-7855 22 09 27.70 -78 55 37.0 10.4 2x 40 1 9 3 5 AMNH 04b-01 2 J2212-8512 22 12 3.15 -85 12 2.8 12.4 2x150 1 13 3 14 AMNH 04b-01 1 J2219-4123 22 19 13.11 -41 23 59.5 11.2 2x 75 1 10 3 27 AMNH 04b-01 2 J2219-6529 22 19 48.35 -65 29 16.9 14.3 2x600 1 28 3 37 AMNH 04b-01 1 J2221-6547 22 21 37.00 -65 47 28.4 14.8 2x300 1 18 4 5 AMNH 04b-01 2 J2227-5044 22 27 55.83 -50 44 22.9 15.9 2x600 1 28 4 23 AMNH 04b-01 1 J2240-4931 22 40 18.75 -49 31 0.7 13.3 2x 75 1 10 4 51 AMNH 04b-01 2 J2246-6905 22 46 10.45 -69 05 42.9 14.6 2x600 1 28 5 1 AMNH 04b-01 1 J2331-4240 23 31 45.82 -42 40 10.5 15.4 2x300 1 18 5 29 SUNY 04b-02 1 NY Ori 05 35 37 -05 12 24 15.0 3x400 1 29 5 47 SUNY 04b-17 1 HD 45166 06 26 19.15 +07 58 28 9.8 3x 90 1 14 6 16 cal 1 pflats -- -- -- -- -- -- 6 30 cal 1 twilight -- -- -- -- -- -- 6 57 end 47/Ib 7 02 ---------------------------------------------------------------------------- If there is any time left before dawn, or you get ahead and have to wait for targets to rise, select from among the following 47/Ib targets: AMNH 04b-01 3 J0122-8403 01 22 0.77 -84 03 54.4 10.8 2x 75 1 10 AMNH 04b-01 3 J0247-6855 02 47 4.45 -68 55 38.0 10.5 2x 40 1 9 AMNH 04b-01 3 J0302-6952 03 02 30.61 -69 52 2.0 12.8 2x 75 1 10 AMNH 04b-01 3 J0306-6106 03 06 33.72 -61 06 23.5 13.9 2x300 1 18 AMNH 04b-01 3 J0310-8432 03 10 39.88 -84 32 37.0 9.8 2x 20 1 9 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 you do not see the star in the acquisition TV M*: moon within 5 degrees. Skip if you do not see the star in the acquisition TV F: faint target may be hard to see with full moon up. R: radial velocity stardard for STSI programs. N: Nova. Will be fainter than on finding chart. C: cataclysmic variable. May be fainter than in finding chart. Skip if not visible. S spectrophotometric standard. If you cannot observe LTT4364, please observe Feige 110 (3x240) before changing to 47/Ib. -------------------------------------------------------------------- General Notes: Astronomical ephemerides are from SKYCAL,by John Thorstensen Pri: Target priority. + = absolute highest priority 1 = observe object if possible 2 = extra targets; observe only if no Priority 1 target is available 3 = backup/filler targets; low priority Cmp: 1 means take comparison spectrum only before target exposures; 2 means before and after .............................................................................. Notes about finding charts: RA & Dec: all coordinates are accurate to 1"; charts can be generated by operator as necessary using LEDAS or DSS. Charts for many objects should be available at the telescope. AMNH 04b-01: No finding charts supplied. Proper motions are typically 0.5-1 arcsec/year, so positions are good to better than 5 arcsec. SUNY 04b-01: Finding charts are available at http://www.astro.sunysb.edu/fwalter/SMARTS/2003B/suny03b-01.tar.gz Chart for V834 Cen is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/V834_Cen.jpg SUNY 04b-02: Finding charts are available at http://www.astro.sunysb.edu/fwalter/SMARTS/2003B/suny03b-02.tar.gz Chart for EX Lup is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/exlup_fc.ps Chart for IRAS05436 is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/iras05436.jpg SUNY 04b-11: Finding chart for DE Cir is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/decir_fc.ps Finding chart for V475 Sct (Nova Sct 2003) is at http://www.astro.sunysb.edu/fwalter/FC/v475sct.jpg .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (STSI programs) Nolan Walborn walborn@stsci.edu (program STSI 04b-04) Fred Walter fwalter@astro.sunysb.edu (SUNY programs) Sebastien Lepine lepine@amnh.org (AMNH 04b-01)