FM Walter 8/14/03 SMARTS 1.5m Service Observing Program 030819 --- EPHEMERIS INFORMATION --- For the night of: Tue, 2003 Aug 19 ---> Wed, 2003 Aug 20 Local midnight = 2003 Aug 20, 4 hr UT, or JD 2452871.667 Local Mean Sidereal time at midnight = 21 09 05.1 Sunset ( 2215 m horizon): 18 28 CST; Sunrise: 7 05 CST Evening twilight: 19 41 CST; LMST at evening twilight: 16 50 Morning twilight: 5 52 CST; LMST at morning twilight: 3 02 Moonrise: 1 19 CST Moon at civil midnight: illuminated fraction 0.480 0.1 days after last quarter, RA and dec: 3 46 47, 20 25.7 The sun is down for 12.6 hr; 10.2 hr from eve->morn 18 deg twilight. .............................................................................. Civil date Setup Program(s) Aug 19 26/I CHIL 03b-01/Mennickent STSI 03b-02/Valenti STSI 03b-03/Reid STSI 03b-04/Bond V838Mon STSI 03b-10/Bond FGS STSI 03b-11/Bond PNN SUNY 03b-10/Walter TTau SUNY 03a-15/Walter Galaxies SUNY 03b-01/Walter PolarBears YALE 03b-08/Woo .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. 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 UT 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 30 minutes for a change in the grating tilt/filter. If you start late, pick up the timeline with the first priority 1 target observable. .............................................................................. In afternoon or during dinner: - Install 26/I grating setup - obtain at least 10 Zero frames - obtain at least 5, preferably 10, flat-field frames (projector or dome) Get well-exposed twilight spectrum at zenith at beginning (or end) of night. Aim for 3 spectra, with 5000-30000 counts/pixel. Do not overexpose the long wavelength end of the chip. .............................................................................. Observing Timeline Program Pri Target RA (J2000) Dec mag Exp Cmp T UT remark SUNY 03a-15 1 IC 4212 13 12 03.0 -06 59 29 14.5 3x500 1 34 1935 STSI 03b-11 3 DY Cen 13 25 34.2 -54 14 45 12 3x300 2 24 2006 STSI 03b-04 2 V4745 Sgr 18 40 02.5 -33 26 55 ~11 3x400 1 26 2027 STSI 03b-04 1 V4743 Sgr 19 01 09.4 -22 00 06 ~12 3x500 1 34 2053 STSI 03b-10 2 HD 132475-R7 14 59 30.0 -22 00 28 14.6 3x550 1 36 2124 STSI 03b-10 3 HD 140283-R4 15 42 46.8 -10 57 17 14.1 3x450 1 29 2158 CHIL 03b-01 1 LTT 7987 20 10 57.4 -30 13 01 12.2 3x 40 1 8 2227 SUNY 03b-10 1 RU Lup 15 56 42.3 -37 49 15.5 3x300 1 24 2235 SUNY 03b-10 1 V1121 Oph 16 49 15.3 -14 22 08.6 3x300 1 24 2256 SUNY 03b-10 2 V4046 Sgr 18 14 10.5 -32 47 34.5 3x300 1 24 2317 SUNY 03b-10 1 S CrA 19 01 08.7 -36 57 19.8 3x300 1 24 2338 SUNY 03b-01 1 QS Tel 19 38 35.7 -46 12 56.5 16 3x400 1 26 2359 2 cal 1 Feige 110 23 19 58.4 -05 09 56 11.8 3x240 1 21 025 1 YALE 03b-08 1 CTS 407 00 38 28.0 -36 24 26 17.5 3x1200 1 69 043 CHIL 03b-01 1 OGLE 0053125 00 53 12.6 -72 55 34 16.0 3x300 1 24 149 YALE 03b-08 2 CTS 607 00 44 59.3 -55 08 10 17.3 3x1200 1 69 210 SUNY 03b-01 2 BL Hyi 01 41 00.3 -67 53 27.7 14.9 3x400 1 26 316 2 SUNY 03b-01 1 EF Eri 03 14 13.0 -22 35 41.4 14.5 3x400 1 26 342 2 STSI 03b-02 1 GJ 841 A 21 57 41.2 -51 00 22 10.4 3x300 1 24 408 STSI 03b-02 2 FL Aqr 22 38 45.2 -20 36 49 11.4 3x400 1 26 429 STSI 03b-02 2 FK Aqr 22 38 45.6 -20 37 16 9.1 3x200 1 16 455 CHIL 03b-01 1 OGLE 0515533 05 15 53.3 -69 25 58 15.5 3x300 1 24 511 CHIL 03b-01 1 LTT 2415 05 56 24.3 -27 51 29 12.2 3x 40 1 9 532 STSI 03b-02 1 BL Cet 01 39 01.5 -17 57 02 12.6 3x600 1 39 540 Note: if a target is too faint to see on the TV monitor, skip it and go to the next target. Astronomical twilight begins at 0552 local time, so if all goes well this is as far as you are likely to get. If you skip targets and need more, select from the following: YALE 03b-08 2 CTS 230 03 10 02.0 -37 23 38 17.7 3x1200 1 69 4 STSI 03b-10 3 alpha PsA 22 57 39.0 -29 37 20 1.2 3x 4 1 8 STSI 03b-03 1 CSSGP-1-00042 1 0 31.3 -30 12 27 14.86 1x900 1 22 STSI 03b-03 1 CSSGP-1-00149 0 46 5.4 -30 11 24 15.51 1x900 1 22 STSI 03b-03 1 CSSGP-1-00283 1 2 9.1 -30 10 35 15.10 1x900 1 22 STSI 03b-03 1 CSSGP-1-00315 0 47 3.7 -30 10 4 15.21 1x900 1 22 STSI 03b-03 1 CSSGP-1-00421 0 51 14.8 -30 8 57 14.58 1x900 1 22 STSI 03b-03 1 CSSGP-1-00450 0 52 44.5 -30 8 44 13.85 1x900 1 22 SUNY 03b-02 2 NY Ori 05 35 37 -05 12 24 15.0 3x600 1 39 YALE 03b-08 3 CTS 256 04 43 14.3 -36 46 24 17.2 3x1200 1 69 SUNY 03b-02 3 UZ Tau E 04 32 43.06 25 52 31.3 13.0 3x500 1 34 3 SUNY 03b-02 3 VY Tau 04 39 17.4 +22 47 54 14.5 3x600 1 39 3 SUNY 03b-02 3 T Tau 04 21 59.4 +19 32 06.4 9.5 3x200 1 16 3 SUNY 03b-02 3 DR Tau 04 47 05.48 16 58 42.1 11.5 3x400 1 26 3 Shortly before sunrise, get well-exposed twilight spectrum at zenith, if you were unable to get them at dusk. Aim for 3 spectra, with 5000-30000 counts/pixel. Do not overexpose the long wavelength end of the chip. .............................................................................. Remarks: 1: moon within 10 degrees. Skip if you do not see the star in the acquisition TV 2: cataclysmic variable. May be fainter than in finding chart. Skip if not visible. If visible but much fainter than on chart, increase exposure times to 3x600. 3: Far northern target. Hour angle must be less than ~2h. 4: consider only if there is at least an hour left before twilight. .............................................................................. 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 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 were prepared at telescope in February and should be available. STSI 03b-02: Most of the stars have large proper motions, so charts may be necessary to find them. A complete set of charts has been posted at http://www.stsci.edu/~bond/valenti_finding_charts.pdf , which you should download and print out (12 MB pdf file). The charts mark where the stars will be in 2003. Some of the stars are binaries, and the remarks give the separations. If both components are listed, try to obtain separate spectra of each component. STSI 03b-03: The finding charts are in two binders at the telescope. SUNY 03b-02: Finding charts are available at http://www.astro.sunysb.edu/fwalter/SMARTS/2003B/suny03b-02.tar.gz CHIL 03b-01: Charts are at http://www.stsci.edu/~bond/Ogle005312.jpg and http://www.stsci.edu/~bond/Ogle051553.jpg , but Dr. Mennickent has been asked to send you better ones. YALE 03b-08: These are galaxies, but they may look almost stellar. .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (other STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs) Jeff Valenti valenti@stsci.edu (program STSI 03b-10) Jong-Hak Woo jhwoo@astro.yale.edu (YALE programs) Ronald Mennickent rmennick@stars.cfm.udec.cl (CHIL programs)