FM Walter 8/5/09 SMARTS 1.5m Service Observing Program 090813 --- EPHEMERIS INFORMATION --- For the night of: Thu, 2009 Aug 13 ---> Fri, 2009 Aug 14 Local midnight = 2009 Aug 14, 4 hr UT, or JD 2455057.667 Local Mean Sidereal time at midnight = 20 47 35.1 Sunset ( 2215 m horizon): 18 25 CST; Sunrise: 7 11 CST Evening twilight: 19 39 CST; LMST at evening twilight: 16 26 Morning twilight: 5 57 CST; LMST at morning twilight: 2 45 Moonrise: 1 41 CST Moon at civil midnight: illuminated fraction 0.451 0.4 days after last quarter, RA and dec: 3 34 47, 24 17.1 The sun is down for 12.8 hr; 10.3 hr from eve->morn 18 deg twilight. ........................................................................... Civil date Setup Program(s) Aug 13 26/Ia GSU 09b-05 STSI 09a-05 SUNY 09a-02 SUNY 09b-10 SUNY 09b-11 YALE 09b-41 The queue program starts at 1900 LST (22:12 CST), .............................................................................. Name Slit Filter Coll Grating Tilt & Comp,exp Ystart Ysize Yspec Blaze w.l. cov. (sec) Res (A) 26/Ia 110.5 clear 565 26 16.14 He-Ar 30 214 280 " 3550 3532-5300 4.3 .............................................................................. In afternoon or during dinner, set up the echelle: Please set the chip readout to read out the full CCD. Please obtain at least 10, and preferably 25, bias and projector flat (quartz) frames. Then, set up the RC - Install 26/Ia grating setup - check focus if necessary - obtain at least 25 Zero frames - obtain at least 10, preferably 25, flat-field frames (projector or dome) .............................................................................. Start with the alpha Cen echelle program At 22:12 CST, please set up the 26/Ia RC mode. I assume 20 minutes for the switchover. ---------------------------------------------------------------------------- Program Pri Target RA (J2000) Dec mag Exp Cmp T CST Rem Yale 09b-41 + V4641 Sgr 18 19 21.6 -25 24 25.1 13.5 3x 900 2 55 22 32 A Yale 09b-41 + V4641 Sgr 18 19 21.6 -25 24 25.1 13.5 3x 900 1 49 23 27 A SUNY 09b-11 + N Sgr 2009 18 7 7.67 -33 46 33.9 8.3 3x 200 1 18 0 16 NN SUNY 09a-11 2 V5558 Sgr 18 10 18.27 -18 46 52.1 8 4x 600 1 50 0 34 SUNY 09a-10 1 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 1 24 SUNY 09a-01 1 HU Aqr 21 7 58.22 -05 17 40.1 16 3x 300 1 24 1 48 C GSU 09b-05 1 ESO 602-G031 22 36 55.9 -22 13 15 14.9 3x1200 1 69 2 12 S4 cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 240 1 21 3 21 GSU 09b-05 1 IRAS00317-21 0 34 13.8 -21 26 21 14.0 3x 900 1 54 3 42 S4 STSI 09a-05 1 NGC 246 0 47 03.4 -11 52 19 11.8 3x 300 1 25 4 36 SUNY 08a-01 2 BL Hyi 1 41 00.3 -67 53 27.7 14.9 3x 300 1 24 5 1 C SUNY 08a-05 2 AB Dor 5 28 44.8 -65 26 54.8 7.0 3x 60 1 12 5 25 SUNY 07b-02 1 V1118 Ori 5 34 44.66 -05 33 41.3 16.5 3x1000 1 59 5 37 end 26/Ia 6 36 ---------------------------------------------------------------------------- If time remains at the end of the night, please select from among the following targets: SUNY 04a-09 3 HD 22468 3 36 47.3 +00 35 16 5.9 3x 100 1 14 SUNY 09a-02 3 NY Ori 5 35 37 -05 12 24 15.0 3x 400 1 30 Y SUNY 09b-02 3 V1143 Ori 5 38 03.8 -04 16 42 16.8 3x 600 1 39 SUNY 09b-11 3 V598 Pup 7 05 42.7. -38 14 42 15 3x 900 1 54 ---------------------------------------------------------------------------- At the end of the night, please obtain at least 10, and preferably 25, projector flat (quartz) frames with the full chip readout. if you did not take them earlier. ---------------------------------------------------------------------------- Remarks: A: The sequence for V4641 Sgr is: ThAr 3 exposures on target ThAr 3 exposures on target ThAr C: cataclysmic variable: may be fainter than on finding chart. H: target is far to the north. It must be observed within +/- 20 minutes of transit to keep the zenith distance <60 degrees. M: moon within 10 degrees. Skip if the star is not seen in the acquisition TV E: may be below the east limit if you get to it early. N: Nova. Will be fainter than on finding chart. R: radial velocity standard. S4: Please set RC slit width to 4 arcsec S10: Please set RC slit width to 10 arcsec S6: Please set slit width to 60 microns (echelle) ST: If you cannot observe LTT 4364 early in the evening, please be sure to observe Feige 10 (in the backup list) as the specroscopic calibrator. TC: time critical. maintain spacing between the images W: target reaches 2 air masses at end of exposure. Do not start late; do the calibration lamp at the end. -------------------------------------------------------------------- General Notes: Astronomical ephemerides are from SKYCAL,by John Thorstensen Pri: Target priority. + = absolute highest priority 1 = observe object if possible 2 = extra targets; skip if running behind and Priority 1 targets remain unobserved. 3 = backup/filler targets; low priority Cmp: 1 means take comparison spectrum only before target exposures; 2 means before and after; 3 means before, after, and between each exposure. 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. .............................................................................. Notes about finding charts: RA & Dec: all coordinates are accurate to 1"; charts can be generated by operator as necessary using LEDAS or DSS. Most charts are available via the link from the main 1.5m scheduling page. .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs) Thomas Rivinius triviniu@eso.org (CN-23 program)