FM Walter 8/09/04 SMARTS 1.5m Service Observing Program 040810 --- EPHEMERIS INFORMATION --- For the night of: Tue, 2004 Aug 10 ---> Wed, 2004 Aug 11 Local midnight = 2004 Aug 11, 4 hr UT, or JD 2453228.667 Local Mean Sidereal time at midnight = 20 36 35.3 Sunset ( 2215 m horizon): 18 23 CST; Sunrise: 7 13 CST Evening twilight: 19 37 CST; LMST at evening twilight: 16 13 Morning twilight: 5 59 CST; LMST at morning twilight: 2 37 Moonrise: 4 09 CST Moon at civil midnight: illuminated fraction 0.206 3.2 days after last quarter, RA and dec: 5 37 25, 27 15.1 The sun is down for 12.8 hr; 10.4 hr from eve->morn 18 deg twilight. .......................................................................... Civil date Setup Program(s) Aug 10 47/II STSI 04a-03/Bond 47/Ib SUNY 03b-16 SUNY 04a-09 SUNY 04b-01 SUNY 04b-02 SUNY 04b-10 SUNY 04b-11 SUNY 04b-13 .............................................................................. 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 SUNY 03b-16 1 HD 93308 10 45 03.6 -59 41 04 6.2 3x 20 1 10 18 58 cal 1 LTT 4364 11 45 37.70 -64 50 25.1 11.5 3x240 1 21 19 8 S SUNY 04b-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x600 1 39 19 29 SUNY 04b-10 1 RU Lup 15 56 42.3 -37 49 15.5 11 3x600 1 39 20 8 SUNY 04b-02 1 EX Lup 16 03 05.48 -40 18 25.9 11.4 3x600 1 39 20 47 SUNY 04b-10 1 Oph 118 16 31 15.8 -24 34 02.1 13 3x600 1 39 21 26 SUNY 04b-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 9: 3x300 1 24 22 5 NN STSI 04a-03 1 V2574 Oph 17 38 45.5 -23 28 18 11 3x400 1 29 22 29 N SUNY 04b-10 1 V4046 Sgr 18 14 10.5 -32 47 34.5 11 3x600 1 39 22 58 SUNY 04b-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 9 3x400 1 29 23 37 N SUNY 04b-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x600 1 39 0 6 end 47/II 0 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 04b-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 9: 3x120 1 15 1 10 NN SUNY 04b-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 9 3x200 1 19 1 25 N STSI 04a-03 1 V4743 Sgr 19 01 09.4 -22 00 06 12 3x300 1 24 1 44 N SUNY 04b-13 1 S CrA 19 01 08.7 -36 57 19.8 11 3x300 1 24 2 8 SUNY 04b-01 1 QS Tel 19 38 35.73 -46 12 56.5 16 3x300 1 34 2 32 C cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x240 1 21 3 6 standard 1 HD224618 23 59 27.9 -16 56 41 8.9 3x150 1 17 3 27 SUNY 04a-09 1 CF Tuc 0 53 07.77 -74 39 05.6 7.6 3x100 1 14 3 44 SUNY 04b-01 1 BL Hyi 1 41 00.3 -67 53 27.7 14.9 3x300 1 34 3 58 C SUNY 04a-09 1 BQ Hyi 2 18 00.84 -71 28 02.8 8.3 3x150 1 17 4 32 SUNY 04b-01 1 EF Eri 3 14 13.0 -22 35 41.4 14.5 3x600 1 39 4 49 C standard 1 HD 10476 1 42 29.7 +20 16 06.6 5.2 3x 20 1 11 5 28 standard 1 HD 10700 1 44 04.1 -15 56 14.9 3,5 3x 5 1 9 5 39 SUNY 04a-09 1 AB Dor 5 28 44.8 -65 26 54.8 7.0 3x100 1 14 5 48 SUNY 04b-02 1 NY Ori 05 35 37 -05 12 24 15.0 3x300 1 24 6 2 cal 1 pflats -- -- -- -- -- -- 6 26 cal 1 twilight -- -- -- -- -- -- 7 05 end 47/Ib 7 10 ---------------------------------------------------------------------------- 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: standard 3 Gl 9066 02 00 13.1 +13 03 05 12.3 3x200 1 19 PM standard 3 CC Eri 02 34 22.6 -43 47 47 8.9 3x200 1 19 PM standard 3 HD 18331 02 56 37.4 -03 42 44.4 5.2 3x 10 1 9 SUNY 04a-09 3 V471 Tau 3 50 11.8 17 15 17 9.7 3x150 1 16 SUNY 04a-10 3 T Tau 04 21 59.43 +19 32 06.4 9.5 3x300 1 24 SUNY 04b-17 3 HD 45166 06 26 19.15 +07 58 28 9.8 3x 60 1 12 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 try to observe Feige 110 before changing to 47/Ib. PM: may have significant proper motion. -------------------------------------------------------------------- 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. SUNY 04a-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 04a-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 04a-10: VSST 14 is 45 arcsec SW of S CrA SUNY 04a-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 SUNY 04a-12: Finding charts for MN Lup and R88 are in http://www.astro.sunysb.edu/fwalter/SMARTS/FC/suny-012a.tar.gz YALE 04a-99: Finding charts is at http://www.astro.yale.edu/buxton/smarts/find_charts/J1628.html .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (STSI programs) Nolan Walborn walborn@stsci.edu (program STSI 04a-05) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)