FM Walter 7/22/05 rev 0730 SMARTS 1.5m Service Observing Program 050730 --- EPHEMERIS INFORMATION --- For the night of: Sat, 2005 Jul 30 ---> Sun, 2005 Jul 31 Local midnight = 2005 Jul 31, 4 hr UT, or JD 2453582.667 Local Mean Sidereal time at midnight = 19 52 15.9 Sunset ( 2215 m horizon): 18 17 CST; Sunrise: 7 22 CST Evening twilight: 19 32 CST; LMST at evening twilight: 15 24 Morning twilight: 6 07 CST; LMST at morning twilight: 2 00 Moonrise: 4 03 CST Moon at civil midnight: illuminated fraction 0.208 3.0 days after last quarter, RA and dec: 4 48 07, 26 45.9 The sun is down for 13.1 hr; 10.6 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) Jul 30 26/I STSI 04b-14 STSI 05a-03 SUNY 05a-01 SUNY 05a-02 SUNY 05a-10 SUNY 05a-11 SUNY 05a-13 .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 26/I 110.5 clear 565 26 15.93 He-Ar 30 214 280 " 3550 3532-5300 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/I 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 04a-09 3 HD 93308 10 45 03.6 -59 41 04 6.2 3x 5 1 9 18 53 cal 1 LTT 4364 11 45 37.7 -64 50 25.1 11.5 3x 240 1 21 19 2 SUNY 05a-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 19 23 Z SUNY 04a-01 2 V834 Cen 14 09 07.5 -45 17 17.1 14 3x 400 1 29 19 47 C SUNY 05a-10 1 RU Lup 15 56 42.3 -37 49 15.5 11 3x 300 1 24 20 16 SUNY 05a-02 2 EX Lup 16 03 05.48 -40 18 25.9 11.4 3x 400 1 29 20 40 SUNY 05a-11 1 V475 Sct 18 49 37.7 -9 33 52.7 16 3x1200 1 69 21 9 N SUNY 05a-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 12: 3x1200 1 69 22 18 N SUNY 05a-11 1 V1188 Sco 17 44 22 -34 16 30 9 3x 120 1 15 23 27 NN SUNY 05a-10 1 V4046 Sgr 18 14 10.5 -32 47 34.5 11 3x 300 1 24 23 42 SUNY 05a-11 2 V5114 Sgr 18 19 32.3 -28 36 35.7 13: 3x1200 1 69 0 6 N STSI 05a-03 1 V1216 Sgr 18 49 49.4 -23 50 10 10.5 3x 300 1 24 1 15 STSI 05a-03 2 AY Ind 21 49 05.8 -72 06 09 9.8 3x 200 1 19 1 39 STSI 05a-03 1 GJ 841 A 21 57 41.2 -51 00 22 10.4 3x 300 1 24 1 58 STSI 05a-03 1 GJ 865 22 38 29.8 -65 22 43 11.5 3x 400 1 29 2 22 SUNY 05a-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 2 51 Z STSI 05a-03 1 FL Aqr 22 38 45.2 -20 36 49 11.4 3x 400 1 29 3 15 STSI 05a-03 1 FK Aqr 22 38 45.6 -20 37 16 9.1 3x 200 1 19 3 44 STSI 05a-03 2 BL/UV Cet 1 39 01.5 -17 57 02 12.6 3x 600 1 39 4 3 STSI 05a-03 2 CC Eri 2 34 22.6 -43 47 47 8.9 3x 200 1 19 4 42 STSI 05a-03 2 40 Eri C 4 15 18.5 -07 39 07 11.2 3x 300 1 24 5 1 STSI 05a-03 1 GJ 2036 A 4 53 31.2 -55 51 37 11.1 3x 300 1 24 5 25 STSI 05a-03 1 GJ 2036 B 4 53 30.8 -55 51 34 12.2 3x 500 1 31 5 49 SUNY 05a-02 1 V1118 Ori 5 34 44.66 -05 33 41 16.5 3x 400 1 29 6 20 E,V end 26/I 6 49 ---------------------------------------------------------------------------- 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/I targets: standard 3 HD209290 22 02 10.3 +01 24 01 9.2 3x300 1 24 standard 3 HD219688 23 17 54.2 -09 10 57.0 4.4 3x 7 1 9 standard 3 HD222368 23 39 57.0 +05 37 34.7 4.1 3x 10 1 9 SUNY 05b-09 3 CF Tuc 0 53 07.77 -74 39 05.6 7.6 3x 60 1 12 SUNY 04a-01 3 BL Hyi 1 41 00.3 -67 53 27.7 14.9 3x 400 1 29 standard 3 HD 10476 1 42 29.7 +20 16 06.6 5.2 3x 20 1 10 standard 3 HD 11636 1 54 38.4 +20 48 28.9 2.6 3x 1 1 9 standard 3 HD 19285 3 03 27.7 -58 55 37 7.3 3x240 1 21 SUNY 04a-09 3 AB Dor 5 28 44.8 -65 26 54.8 7.0 3x 60 1 12 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. NN: also known as Nova Sco 2005 R: radial velocity standard for STSI programs. PM: may have significant proper motion. V: If running early, lengthen exposures up to 3x600. If target is too far east, go to AB Dor in the secondary target list, then return to V1118 Ori. 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: Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)