FM Walter 8/27/05 SMARTS 1.5m Service Observing Program 050912 --- EPHEMERIS INFORMATION --- For the night of: Mon, 2005 Sep 12 ---> Tue, 2005 Sep 13 Local midnight = 2005 Sep 13, 4 hr UT, or JD 2453626.667 Local Mean Sidereal time at midnight = 22 45 44.4 Sunset ( 2215 m horizon): 18 41 CST; Sunrise: 6 37 CST Evening twilight: 19 54 CST; LMST at evening twilight: 18 39 Morning twilight: 5 24 CST; LMST at morning twilight: 4 11 Moonset : 3 39 CST Moon at civil midnight: illuminated fraction 0.681 1.7 days since first quarter, RA and dec: 18 52 57, -27 50.9 The sun is down for 11.9 hr; 9.5 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) Sep 12 26/Ib LANL 05b-01 SUNY 05b-01 SUNY 05b-02 SUNY 05b-10 .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 26/Ib 110.5 clear 565 26 16.50 He-Ar 30 214 280 " 3550 3800-5575 4.3 .............................................................................. 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 26/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 CST Rem SUNY 05b-10 2 RU Lup 15 56 42.3 -37 49 15.5 11 3x 300 1 24 19 15 SUNY 05b-02 3 EX Lup 16 03 05.5 -40 18 25.9 11.4 3x 400 1 29 19 39 LANL 05b-01 1 MCT_2019 63 20 23 19.6 -43 32 57.1 14.79 3x 130 1 16 20 8 LANL 05b-01 1 MCT_2019 64 20 22 34.8 -43 30 24.1 14.90 3x 130 1 16 20 24 LANL 05b-01 1 MCT_2019 65 20 22 24.0 -43 35 15.3 15.09 3x 150 1 17 20 40 LANL 05b-01 2 MCT_2019 66 20 23 06.7 -43 23 29.4 14.94 3x 150 1 17 20 57 LANL 05b-01 2 MCT_2019 68 20 22 34.2 -43 31 55.9 15.05 3x 160 1 17 21 14 LANL 05b-01 2 MCT_2019 69 20 22 25.9 -43 23 31.9 15.25 3x 180 1 18 21 31 LANL 05b-01 1 220000-595900 60 22 00 05.5 -60 01 14.5 14.42 3x 90 1 14 21 49 LANL 05b-01 1 220000-595900 61 22 00 33.5 -60 03 05.4 14.53 3x 100 1 14 22 3 LANL 05b-01 2 220000-595900 64 22 00 17.2 -60 02 44.5 14.82 3x 120 1 15 22 17 LANL 05b-01 2 220000-595900 65 22 00 14.7 -59 57 49.3 14.76 3x 120 1 15 22 32 cal 1 Feige 110 23 19 58.4 -05 09 56 11.8 3x 200 1 19 22 47 SUNY 05b-01 2 BL Hyi 1 41 00.3 -67 53 27.7 14.9 3x 400 1 29 23 6 LANL 05b-01 1 020000-300600 45 1 59 45.6 -30 11 02.7 14.58 3x 110 1 15 23 35 LANL 05b-01 1 020000-300600 44 2 00 06.2 -30 06 01.4 14.58 3x 100 1 14 23 50 LANL 05b-01 2 020000-300600 46 2 00 09.5 -30 07 36.4 15.18 3x 130 1 16 0 4 LANL 05b-01 2 020000-300600 47 2 00 08.1 -30 08 57.4 14.93 3x 140 1 16 0 20 LANL 05b-01 1 040020-600200 72 3 59 37.7 -60 01 01.2 14.79 3x 130 1 16 0 36 LANL 05b-01 1 040020-600200 47 3 59 38.8 -60 00 33.8 13.20 3x 30 1 11 0 52 LANL 05b-01 1 040020-600200 56 3 59 45.0 -60 02 46.3 14.08 3x 70 1 13 1 3 LANL 05b-01 1 040020-600200 76 3 59 55.4 -60 06 26.2 15.01 3x 160 1 17 1 16 LANL 05b-01 1 040020-600200 73 4 00 31.9 -60 03 08.2 15.14 3x 160 1 17 1 33 LANL 05b-01 2 040020-600200 61 4 00 43.2 -60 05 30.8 14.67 3x 90 1 14 1 50 LANL 05b-01 2 040020-600200 58 4 00 48.1 -60 05 37.6 14.13 3x 80 1 13 2 4 LANL 05b-01 2 040020-600200 70 4 00 56.5 -60 00 03.9 14.98 3x 130 1 16 2 17 LANL 05b-01 2 040020-600200 74 4 01 02.2 -59 56 12.8 14.99 3x 160 1 17 2 33 LANL 05b-01 1 040004-295900 27 3 59 33.6 -29 57 05.7 13.69 3x 50 1 12 2 50 LANL 05b-01 1 040004-295900 29 4 00 17.1 -29 58 49.0 14.37 3x 70 1 13 3 2 LANL 05b-01 1 040004-295900 30 4 00 02.2 -30 01 36.1 14.16 3x 70 1 13 3 15 LANL 05b-01 1 040004-295900 32 4 00 26.6 -29 53 32.2 14.45 3x 90 1 14 3 28 LANL 05b-01 2 040004-295900 33 3 59 38.7 -29 58 21.0 14.54 3x 110 1 15 3 42 LANL 05b-01 2 040004-295900 37 4 00 21.8 -30 04 41.8 14.90 3x 140 1 16 3 57 LANL 05b-01 2 040004-295900 40 3 59 43.1 -30 02 41.2 14.89 3x 150 1 17 4 13 SUNY 05b-02 1 V1118 Ori 5 34 44.7 -05 33 41.3 16.5 3x 400 1 29 4 30 LANL 05b-01 1 DLS_0520-49 61 5 20 29.6 -48 58 28.5 13.33 3x 30 1 11 4 59 LANL 05b-01 1 DLS_0520-49 64 5 19 27.3 -48 57 29.1 13.42 3x 40 1 10 5 09 LANL 05b-01 1 DLS_0520-49 65 5 19 44.4 -48 57 37.8 13.55 3x 40 1 10 5 19 LANL 05b-01 2 DLS_0520-49 70 5 19 26.6 -49 05 16.4 14.15 3x 60 1 11 5 29 LANL 05b-01 2 DLS_0520-49 71 5 20 08.4 -48 54 55.0 14.12 3x 70 1 12 5 40 LANL 05b-01 2 DLS_0520-49 77 5 20 36.4 -49 05 08.5 14.36 3x 90 1 13 5 51 end 26/Ib 6 04 ---------------------------------------------------------------------------- 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 26/Ib targets: LANL 05b-01 2 DLS_0520-49 111 5 20 33.2 -48 59 14.6 15.27 3x 190 1 19 LANL 05b-01 2 DLS_0520-49 114 5 19 34.9 -49 03 59.7 15.25 3x 200 1 19 LANL 05b-01 2 DLS_0520-49 119 5 20 16.3 -49 00 32.7 15.43 3x 220 1 20 LANL 05b-01 2 DLS_0520-49 126 5 20 06.2 -49 01 38.2 15.44 3x 230 1 21 LANL 05b-01 2 DLS_0520-49 128 5 19 25.6 -48 53 21.8 15.50 3x 250 1 22 LANL 05b-01 2 DLS_0520-49 134 5 19 44.9 -49 01 46.9 15.87 3x 310 1 25 LANL 05b-01 2 DLS_0520-49 137 5 20 31.5 -48 54 25.9 15.76 3x 320 1 25 LANL 05b-01 2 DLS_0520-49 140 5 19 48.1 -48 56 25.4 15.86 3x 340 1 26 LANL 05b-01 2 DLS_0520-49 147 5 20 27.9 -48 54 54.0 16.06 3x 390 1 29 LANL 05b-01 2 DLS_0520-49 149 5 19 45.0 -49 02 16.0 16.13 3x 400 1 29 LANL 05b-01 2 DLS_0520-49 150 5 20 23.4 -48 55 32.5 15.99 3x 400 1 29 LANL 05b-01 2 DLS_0520-49 151 5 20 12.3 -49 04 57.7 16.07 3x 440 1 31 Just before sunrise, get well-exposed TWILIGHT SPECTRA at zenith IF you could not obtain them at dusk. Aim for 3-5 spectra, each with between 5,000 and 30,000 counts per pixel. -------------------------------------------------------------------- Remarks: M: moon within 10 degrees. Skip if not visible in the acquisition TV A: target reaches 2 air masses at end of exposure. Do not start late; do the calibration lamp at the end if it helps. B: very bright target. C: cataclysmic variable. May be fainter than in finding chart. Skip if not visible. E: target far to the east at twilight. Don't go there too early. F: faint target may be hard to see with moon up. N: Nova. Will be fainter than on finding chart. R: radial velocity standard for STSI programs. PM: may have significant proper motion. W: star very close to 2 air masses at end of observation. Don't start late. Y: 5 arcsec SE of brighter star. Try to keep the brighter star out of the slit. Skip if the seeing is really bad. Z: monitoring target. Try to maintain spacing between observations. -------------------------------------------------------------------- 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. Many charts are available via the link from the main 1.5m scheduling page. Charts for many objects should be available at the telescope. .............................................................................. Questions may be addressed to: Douglas Tucker dtucker@fnal.gov (LANL programs) Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)