H. E. Bond 7/26/03 SMARTS 1.5m Service Observing Program Night of Thursday 2003 August 7-8 Times are UT-4 Sunset: 18:13 Twilight: 6:01 Twilight: 19:35 Sunrise: 7:23 Duration of night: 10:26 Moon age +9 days. RA/Dec: 1718-25 Setss 04:22 Sidereal time evening twilight: 15:57 midnight: 20:22 morning twilight: 02:23 .............................................................................. Civil date Setup Program(s) Aug 7 26/I Observing plan: http://www.stsci.edu/~bond/s15m030807.plan STSI 03b-02/Valenti STSI 03b-04/BondV838Mon STSI 03b-10/BondFGS STSI 03b-11/BondPNN SUNY 03b-10/WalterTTau SUNY 03a-15/WalterGalaxies SUNY 03b-01/WalterPolarBears 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 .............................................................................. 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. Try for 5000-30000 counts/pixel. Main observing programs are in several lists below; observe as many of these as possible. Intermix programs as appropriate, and generally try to observe in order of RA. Get all of the Priority 1 if possible, and then Priority 2+, 2, and 3 if there is time. The objects in SUNY 03a-15 are galaxies. The objects in Yale 03b-08 are also galaxies, but they may look almost stellar. Most of the stars in STSI 03b-02 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 below, try to obtain separate spectra of each component. Charts for the CHIL program are at http://www.stsci.edu/~bond/Ogle005312.jpg and http://www.stsci.edu/~bond/Ogle051553.jpg, but I have asked Dr. Mennickent to send you better ones. Pgm Pri Target RA (J2000) Dec mag Exp Cmp Remarks SUNY 03a-15 1+ IC 4212 13 12 03.0 -06 59 29 14.5 3x500 1 SUNY 03a-15 1+ IC 0971 14 03 52.7 -10 08 25 13.3 3x500 1 SUNY 03a-15 1+ MCG-01-38-01214 58 30.0 -06 49 14 14.6 3x500 1 YALE 03b-08 1 CTS 582 22 40 18.8 -52 31 52 17.8 3x1200 1 calib 1+ Feige 110 23 19 58.4 -05 09 56 11.8 3x240 1 phot.std YALE 03b-08 1 CTS 487 23 22 10.9 -34 47 57 16.5 3x1200 1 YALE 03b-08 1 CTS 407 00 38 28.0 -36 24 26 17.5 3x1200 1 YALE 03b-08 1 CTS 607 00 44 59.3 -55 08 10 17.3 3x1200 1 YALE 03b-08 1 CTS 631 02 45 11.7 -27 53 08 17.3 3x1200 1 YALE 03b-08 1 CTS 230 03 10 02.0 -37 23 38 17.7 3x1200 1 YALE 03b-08 1 CTS 256 04 43 14.3 -36 46 24 17.2 3x1200 1 STSI 03b-11 1 DY Cen 13 25 34.2 -54 14 45 12 3x300 2 STSI 03b-10 1 HD 132475-R6 14 59 56.4 -22 00 18 14.2 3x500 1 STSI 03b-10 1 HD 132475-R7 14 59 30.0 -22 00 28 14.6 3x550 1 STSI 03b-10 1 HD 140283-R3 15 43 00.0 -10 55 27 13.8 3x400 1 STSI 03b-10 1 HD 140283-R4 15 42 46.8 -10 57 17 14.1 3x450 1 STSI 03b-10 3 lambda Ser 15 46 26.6 +07 21 11 4.4 3x10 1 G0 V STSI 03b-04 2 V4745 Sgr 18 40 02.5 -33 26 55 ~11 3x400 1 nova STSI 03b-04 1 V4743 Sgr 19 01 09.4 -22 00 06 ~12 3x500 1 nova STSI 03b-10 3 mu Aql 19 34 05.4 +07 22 44 4.4 3x10 1 K3 IIIb STSI 03b-10 3 alpha PsA 22 57 39.0 -29 37 20 1.2 3x4 1 A3 V STSI 03b-04 3 NGC 246 00 47 03.4 -11 52 19 11.8 3x500 1 STSI 03b-10 2 psi-3 Psc 01 09 49.2 +19 39 30 5.6 3x10 1 G0 III STSI 03b-10 2 theta Cet 01 24 01.4 -08 10 59 3.6 3x10 1 K0 IIIb STSI 03b-10 2 o Psc 01 45 23.6 +09 09 28 4.2 3x10 1 G8 III STSI 03b-10 2 HR 856 02 53 11.7 +16 29 00 6.3 3x10 1 F5 III STSI 03b-10 2 kappa Cet 03 19 21.7 +03 22 13 4.8 3x10 1 G5 V STSI 03b-10 2 epsilon Eri 03 32 55.8 -09 27 30 3.7 3x8 1 K2 V STSI 03b-02 1 V1216 Sgr 18 49 49.4 -23 50 10 10.5 3x300 1 STSI 03b-02 1 AY Ind 21 49 05.8 -72 06 09 9.8 3x200 1 STSI 03b-02 1 GJ 865 22 38 29.8 -65 22 43 11.5 3x400 1 STSI 03b-02 2+ UV Cet 01 39 01.5 -17 57 04 12.7 3x600 1 1.5" STSI 03b-02 1 CC Eri 02 34 22.6 -43 47 47 8.9 3x200 1 STSI 03b-02 1 40 Eri C 04 15 18.5 -07 39 07 11.2 3x300 1 SUNY 03b-10 1 RU Lup 15 56 42.31 -37 49 15.5 3x300 1 SUNY 03b-10 1 V866 Sco 16 11 31.40 -18 38 24.5 3x300 1 SUNY 03b-10 2 Oph 118 16 31 15.77 -24 34 02.1 3x300 1 SUNY 03b-10 1 V1121 Oph 16 49 15.31 -14 22 08.6 3x300 1 SUNY 03b-10 2 V4046 Sgr 18 14 10.47 -32 47 34.5 3x300 1 SUNY 03b-10 1 S CrA 19 01 08.69 -36 57 19.8 3x300 1 SUNY 03b-01 2 QS Tel 19 38 35.7 -46 12 56 16 3x400 1 SUNY 03b-01 1 HU Aqr 21 07 58.3 -05 17 39 15.3 3x400 1 SUNY 03b-01 1 BL Hyi 01 41 00.2 -67 53 27 14.9 3x400 1 SUNY 03b-01 1 EF Eri 03 14 13.0 -22 35 41 14.5 3x400 1 CHIL 03b-01 1 LTT 7987 20 10 57.4 -30 13 01 12.2 3x40 1 CHIL 03b-01 1+ OGLE 0053125 00 53 12.6 -72 55 34 16.0 3x300 1 CHIL 03b-01 1+ OGLE 0515533 05 15 53.3 -69 25 58 15.5 3x300 1 CHIL 03b-01 1 LTT 2415 05 56 24.3 -27 51 29 12.2 3x40 1 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 RA & Dec: all coordinates are accurate to 1". Cmp: 1 means take comparison spectrum only before target exposures; 2 means before and after .............................................................................. Questions may be addressed to: Howard Bond bond@stsci.edu Jeff Valenti valenti@stsci.edu Fred Walter fwalter@astro.sunysb.edu Jong-Hak Woo jhwoo@astro.yale.edu Ronald Mennickent rmennick@stars.cfm.udec.cl CHIL program