FM Walter 3/8/05 rev 0313 SMARTS 1.5m Service Observing Program 050313 --- EPHEMERIS INFORMATION --- For the night of: Sun, 2005 Mar 13 ---> Mon, 2005 Mar 14 Local midnight = 2005 Mar 14, 4 hr UT, or JD 2453443.667 Local Mean Sidereal time at midnight = 10 44 14.7 Sunset ( 2215 m horizon): 19 09 CST; Sunrise: 6 36 CST Evening twilight: 20 23 CST; LMST at evening twilight: 7 07 Morning twilight: 5 23 CST; LMST at morning twilight: 16 08 Moonset : 21 14 CST Moon at civil midnight: illuminated fraction 0.165 3.6 days before first quarter, RA and dec: 2 33 24, 17 24.0 The sun is down for 11.4 hr; 9.0 hr from eve->morn 18 deg twilight. .............................................................................. Civil date Setup Program(s) Mar 13 13/I STSI 05a-02 SUNY 05a-02 SUNY 05a-11 .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 13/I 110.5 clear 585 13 11.58 He-Ar 120 200 280 TBD 4450 3146-9374 17.2 .............................................................................. In afternoon or during dinner: - Install 13/I grating setup - check focus if necessary - obtain at least 25 Zero frames - obtain at least 5, 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 05a-02 1 V1118 Ori 5 34 44.66 -05 33 41.3 16.5 3x 300 1 24 19 44 STSI 05a-02 1 V838 Mon-15 7 04 01.1 -03 50 33 16.53 4x1800 1 130 20 8 SUNY 05a-11 1 YY Dor 5 56 42.5 -68 54 35 13 4x1800 1 130 22 18 N SUNY 05a-11 1 V574 Pup 7 41 53.8 -27 6 37 12: 3x 600 1 39 0 28 N cal 1 LTT 4364 11 45 37.70 -64 50 25.1 11.5 3x 240 1 21 1 7 SUNY 05a-11 1 DE Cir 15 17 52.5 -61 57 16.4 3x1800 1 99 1 28 N SUNY 05a-11 1 V1187 Sco 17 29 18.81 -31 46 01.5 15: 3x1000 1 59 3 7 N SUNY 05a-11 1 V5114 Sgr 18 19 32.3 -28 36 35.7 15: 3x1000 1 59 4 6 N SUNY 05a-11 1 V475 Sct 18 49 37.7 -9 33 52.7 3x1000 1 59 5 5 N end 13/I 6 04 If any of the targets are too faint to acquire, or if there is any time left before dawn, select from among the following: SUNY 04a-09 3 HD 93308 10 45 03.6 -59 41 04 6.2 6x 2 1 12 SUNY 04b-01 3 V834 Cen 14 09 07.5 -45 17 17.1 14 3x 400 1 29 C SUNY 05a-10 3 RU Lup 15 56 42.3 -37 49 15.5 11 3x 300 1 24 STSI 04b-14 3 V4745 Sgr 18 40 02.5 -33 26 55 15: 3x 600 1 39 N SUNY 05a-13 3 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 Just before sunrise, get well-exposed TWILIGHT SPECTRA at zenith, if you did 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 deg. Skip if you do not see the star in the acquisition TV M*: moon within 5 deg. Skip if you do not see the star in the acquisition TV C: cataclysmic variable: may be fainter than on finding chart. If any emission lines are overexposed in the first spectrum, shorten the exposure time and take 3 more. F: Faint supernova may be difficult to see with moon up. Use offset coordinates, and complete full integration. G: galaxy. Center on nucleus. N: fading nova S1: set slit width to 2.0 arcsec. observing sequence is: comparison lamp 1 observation centered on target 1 observation centered 30" East of target 1 observation centered 30" West of target remember to reset the slit width following observation. S2: set slit width to 10.0 arcsec use same observing sequence as in note S1. remember to reset the slit width following observation. -------------------------------------------------------------------- General Notes: Astronomical ephemerides are from SKYCAL,by John Thorstensen Pri: Target 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 local 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. For now I am allotting the nominal overheads, plus 20-25 minutes for changes 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. Charts for many objects should be available at the telescope. STSI 04b-02: see http://www.stsci.edu/~bond/v838mon_field.jpg or http://www.astro.sunysb.edu/fwalter/SMARTS/FC/v838mon_field.jpg 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 05a-02: Finding charts are available at http://www.astro.sunysb.edu/fwalter/SMARTS/2003B/suny03b-02.tar.gz Chart for V1118 Ori is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/FC_V1118_Ori.jpg Chart for EX Lup is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/exlup_fc.ps SUNY 05a-11: Finding chart for DE Cir: http://www.astro.sunysb.edu/fwalter/SMARTS/FC/decir_fc.ps Finding chart for V475 Sct (Nova Sct 2003): http://www.astro.sunysb.edu/fwalter/SMARTS/FC/v475sct.jpg Finding chart for V2574 Oph: http://www.astro.sunysb.edu/fwalter/SMARTS/FC/FC_V2574_Oph.gif Finding chart for YY Dor: http://www.astro.sunysb.edu/fwalter/SMARTS/FC/yydor.jpg Finding chart for V574 Pup: http://www.astro.sunysb.edu/fwalter/SMARTS/FC/FC_V574_Pup.jpg SUNY 05a-12: Finding chart for V1647 Ori (IRAS05436) is at http://www.astro.sunysb.edu/fwalter/SMARTS/FC/iras05436.jpg .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)