FM Walter 8/27/05 rev 0905 SMARTS 1.5m Service Observing Program 050907 --- EPHEMERIS INFORMATION --- For the night of: Wed, 2005 Sep 7 ---> Thu, 2005 Sep 8 Local midnight = 2005 Sep 8, 4 hr UT, or JD 2453621.667 Local Mean Sidereal time at midnight = 22 26 01.6 Sunset ( 2215 m horizon): 18 39 CST; Sunrise: 6 43 CST Evening twilight: 19 51 CST; LMST at evening twilight: 18 16 Morning twilight: 5 31 CST; LMST at morning twilight: 3 57 Moonset : 22 22 CST Moon at civil midnight: illuminated fraction 0.170 3.3 days before first quarter, RA and dec: 14 06 10, -14 28.8 The sun is down for 12.1 hr; 9.7 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) Sep 07 47/II SUNY 05b-01 47/Ib SUNY 05b-02 SUNY 05b-09 SUNY 05b-10 SUNY 05b-11 SUNY 05b-12 .............................................................................. 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 3550 3878-4552 1.6 47/Ib 110.5 GG495 595 47 22.64 Neon 20 200 280 164 7100 5652-6972 3.1 .............................................................................. In afternoon or during dinner: - Install 47/Ib 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 SUNY 05b-11 1 N Cen 2005 13 20 49.74 -62 37 50.5 9 3x 100 1 14 19 12 NN SUNY 05b-10 1 RU Lup 15 56 42.3 -37 49 15.5 11 3x 300 1 24 19 26 SUNY 05b-02 2 EX Lup 16 03 05.48 -40 18 25.9 11.4 3x 300 1 24 19 50 SUNY 05b-10 2 Oph 118 16 31 15.8 -24 34 02.1 13 3x 300 1 24 20 11 STSI 05b-07 1 HD 148937 16 33 52.2 -48 06 40 6.7 3x 60 1 12 20 35 SUNY 05b-11 2 V1663 Aql 19 05 12.50 +05 14 12.0 15 3x 400 1 29 20 47 N SUNY 05b-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 9 3x 900 1 54 21 16 N SUNY 05b-10 1 V4046 Sgr 18 14 10.5 -32 47 34.5 11 3x 300 1 24 22 10 SUNY 05b-10 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 22 34 SUNY 05b-01 2 QS Tel 19 38 35.73 -46 12 56.5 16 3x 600 1 39 22 58 C SUNY 03b-01 2 HU Aqr 21 07 58.3 -05 17 39.4 15.3 3x 900 1 54 23 37 C cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 240 1 21 0 16 standard 3 HD 224618 23 59 27.9 -16 56 41 8.7 3x 300 1 24 0 37 SUNY 05b-09 2 CF Tuc 0 53 7.7 -74 39 5.6 7.6 3x 90 1 14 1 1 SUNY 05b-01 1 BL Hyi 1 41 00.3 -67 53 27.7 14.9 3x 600 1 39 1 15 C standard 3 HD 4628 0 48 23.0 +05 16 50.2 5.8 3x 15 1 10 1 54 standard 3 HD 10647 1 42 29.3 -53 44 27.0 5.5 3x 15 1 10 2 4 standard 3 HD 16046A 2 33 50.7 -28 13 56.4 5.0 3x 10 1 9 2 14 SUNY 05b-01 1 EF Eri 3 14 13.0 -22 35 41.4 14.5 3x1200 1 69 2 23 C standard 3 HD 26407 3 52 46.3 -42 50 12 7.8 3x 90 1 14 3 32 SUNY 05b-02 + V1118 Ori 5 34 44.66 -05 33 41.3 16.5 3x 500 1 34 3 46 X,E end 47/Ib 4 20 ****************** 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 mu Col 5 45 59.9 -32 18 23.4 5.2 3x 8 1 9 4 45 SUNY 05b-09 2 CF Tuc 0 53 7.7 -74 39 5.6 7.6 3x 240 1 21 4 54 SUNY 05b-02 + V1118 Ori 5 34 44.66 -05 33 41.3 16.5 3x 900 1 54 5 15 X cal 1 pflats -- -- 10 6 09 end 47/II 6 19 ---------------------------------------------------------------------------- If you get ahead and have to wait for V1118 Ori to rise, or if some targets are too faint to acquire, please select from among the following 47/Ib targets: standard 3 HD 222095 23 37 50.9 -45 29 33 4.7 3x 10 1 9 standard 3 HD 7526 1 14 34 -48 15 9 9.8 3x 600 1 39 standard 3 HD 16582 2 39 28.9 0 19 43 4.1 3x 15 1 10 standard 3 HD 19285 3 03 27.7 -58 55 37 7.3 3x 90 1 14 If there is any time left before dawn, 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 05b-02 3 NY Ori 5 35 37 -05 12 24 15.0 3x 600 1 39 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 E: may be below the east limit if you get to it early. EF: star immediately to the west of EF Eri. The coordinates are those of EF Eri F: faint target may be hard to see with moon up. R: radial velocity stardard for STSI programs. N: Nova. Will be fainter than on finding chart. NN: possible new nova. Should be the brightest star within 1 arcminute. C: cataclysmic variable. May be fainter than in finding chart. Skip if not visible. TC: time critical W: A: target reaches 2 air masses at end of exposure. Do not start late; do the calibration lamp at the end if it helps. X: Contemporaneous with XMM observation that begins at 0825UT on 9/8 Y: 5 arcsec SE of brighter star -------------------------------------------------------------------- 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 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) Nolan Walborn walborn@stsci.edu (program STSI 05b-07) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)