FM Walter 8/22/09 SMARTS 1.5m Service Observing Program 090829 --- EPHEMERIS INFORMATION --- For the night of: Fri, 2009 Aug 21 ---> Sat, 2009 Aug 22 Local midnight = 2009 Aug 22, 4 hr UT, or JD 2455065.667 Local Mean Sidereal time at midnight = 21 19 07.5 Sunset ( 2215 m horizon): 18 29 CST; Sunrise: 7 03 CST Evening twilight: 19 43 CST; LMST at evening twilight: 17 01 Morning twilight: 5 49 CST; LMST at morning twilight: 3 09 Moonset : 20 08 CST Moonrise: 8 12 CST Moon at civil midnight: illuminated fraction 0.042 1.7 days since new moon, RA and dec: 11 26 54, -0 40.8 The sun is down for 12.6 hr; 10.1 hr from eve->morn 18 deg twilight. ........................................................................... Civil date Setup Program(s) Aug 29 26/Ia GSU 09b-05 STSI 09a-05 SUNY 09a-02 SUNY 09b-10 SUNY 09b-11 YALE 09b-10 YALE 09b-41 The queue program starts at 1900 LST (21:10 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 21:41 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 SUNY 09b-11 + V2672 Oph 17 38 19.68 -26 44 14.0 11 3x1200 1 69 21 30 NN SUNY 09a-11 1 V1280 Sco 16 57 40.91 -32 20 36.4 13 3x 500 1 34 22 39 N Yale 09b-41 2 HIP 90604 18 29 16.79 -38 51 04.7 6.6 3x 60 1 12 23 13 SUNY 09a-10 2 S CrA 19 01 08.7 -36 57 19.8 11 3x 300 1 24 23 25 Yale 09b-41 2 HIP 105779 21 25 23:47 -45 09 42.9 6.8 3x 60 1 12 23 49 Yale 09b-41 2 HD 210934 22 14 18.75 -27 46 00.9 5.4 3x 60 1 12 0 1 Yale 09b-41 2 HIP 108626 22 00 24.25 -55 53 00.6 6.0 3x 60 1 12 0 13 GSU 09b-05 1 IRAS20051-11 20 07 51.3 -11 08 35 14.4 3x 900 1 54 0 25 S4 cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 240 1 21 1 19 GSU 09b-05 1 NGC 7590 23 18 54.8 -42 14 21 12.1 3x 900 1 54 1 40 S4 Yale 09b-10 1 ASAS_232246 23 22 46 -46 41 32 12.5 3x 60 2 13 2 34 STSI 09a-05 2 NGC 246 0 47 03.4 -11 52 19 11.8 3x 300 1 25 2 47 Yale 09b-10 1 ASAS_002443 0 24 43 -69 49 42 11.1 3x 30 2 12 3 12 Yale 09b-10 1 ASAS_023020 2 30 20 -59 08 06 12.1 3x 30 2 12 3 24 Yale 09b-10 1 ASAS_031346 3 13 46 -14 12 42 12.9 3x 90 2 14 3 36 Yale 09b-10 1 BD-17 484 2 31 25.76 -16 59 05.0 10.4 3x 300 1 24 3 50 R Yale 09b-10 1 ASAS_040312 4 03 12 -19 51 12 12.1 3x 30 2 12 4 14 Yale 09b-10 1 ASAS_042716 4 27 16 -48 28 00 11.9 3x 30 2 12 4 26 Yale 09b-10 1 ASAS_044203 4 42 03 -51 33 36 12.2 3x 30 2 12 4 38 SUNY 09a-02 2 NY Ori 5 35 37 -05 12 24 15.0 3x 400 1 30 4 50 Y SUNY 09b-02 1 V1143 Ori 5 38 03.8 -04 16 42 16.8 3x 900 1 54 5 20 SUNY 08a-05 2 AB Dor 5 28 44.8 -65 26 54.8 7.0 3x 60 1 12 6 14 end 26/Ia 6 26 ---------------------------------------------------------------------------- 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 09b-11 3 V598 Pup 7 05 42.7. -38 14 42 15 3x 900 1 54 STSI 09b-02 3 V838 Mon 7 04 04.8 -03 50 50 15.6 3x1000 1 59 SUNY 09b-11 3 V574 Pup 7 41 53.8 -27 6 37 12 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: 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)