FM Walter 10/10/08 rev 10/12 SMARTS 1.5m Service Observing Program 081013 --- EPHEMERIS INFORMATION --- For the night of: Mon, 2008 Oct 13 ---> Tue, 2008 Oct 14 Local midnight = 2008 Oct 14, 3 hr UT, or JD 2454753.625 Local Mean Sidereal time at midnight = 23 48 52.4 Sunset ( 2215 m horizon): 19 59 CDT; Sunrise: 6 59 CDT Evening twilight: 21 15 CDT; LMST at evening twilight: 21 03 Morning twilight: 5 43 CDT; LMST at morning twilight: 5 33 Moonrise: 18 47 CDT Moonset : 6 43 CDT Moon at civil midnight: illuminated fraction 0.992 0.7 days until full moon, RA and dec: 0 37 02, 9 02.6 The sun is down for 11.0 hr; 8.5 hr from eve->morn 18 deg twilight. .............................................................................. Civil date Setup Program(s) Oct 13 13/I CN 08b-06 STSI TOO SUNY 08b-02 YALE 08b-01 .............................................................................. 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 30 200 280 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) Program Pri Target RA (J2000) Dec mag Exp Cmp T CST Rem YALE 08A-01 1 1730-130 17 33 02.7 -13 04 50 18.5 4x 900 2 71 20 36 W YALE 08A-01 1 PKS 2155-304 21 58 52.0 -30 13 32 ~12 3x 300 2 25 21 47 YALE 08A-01 1 3C 454.3 22 53 57.7 +16 08 13 ~14 9x 300 2 58 22 12 cal 1 Feige 110 23 19 58.39 -05 09 55.8 11.8 3x 100 1 14 23 10 ST YALE 08A-01 2 3C 454.3 22 53 57.7 +16 08 13 ~14 13x 300 2 85 23 24 CN 08B-06 1 CSS080922 23 16 16.60 11 42 47.5 17 3x1500 1 84 0 49 STSI TOO 1 NGC 300 0 54 34.16 -37 38 28.6 ~18 3x1200 1 69 2 13 TR YALE 08A-01 1 0208-512 2 10 46.2 -51 01 02 ~18 3x 900 2 55 3 22 YALE 08A-01 1 0235+164 2 38 38.9 +16 36 59 ~18 3x 300 2 25 4 17 YALE 08A-01 1 0528+134 5 30 56.4 +13 31 55 ~18 6x 900 2 103 4 42 end 13/I 6 25 If there is any time left before dawn, or sky conditions preclude acquisition of the faint targets, select from among the following: cal 3 mu Col 5 45 59.9 -32 18 23.4 5.2 3x 5 1 9 ST SUNY TOO 1 V1647 Ori 5 46 13.14 -00 06 04.8 17 3x1200 1 69 standard 3 HD 6953 1 10 19.4 25 27 33.7 5.8 3x 10 1 9 standard 3 Gl 9066 2 00 13.1 +13 03 05 12.3 3x 300 1 24 PM standard 3 HD 16160 2 36 04.9 +06 53 12.7 5.8 3x 10 1 9 standard 3 HD 23249 3 43 14.9 -09 45 48.2 3.5 3x 2 1 9 standard 3 HD 22049 3 32 55.8 -09 27 30 3.7 3x 10 1 9 standard 3 HD 29712 4 36 45.6 -62 04 37.8 5.7 3x 10 1 9 standard 3 HD 30501 4 45 38.6 -50 04 27.2 7.6 3x 30 1 11 standard 3 HD 33894 5 10 57.6 -48 30 43 7.2 3x 30 1 11 SUNY 04a-09 3 HD 93308 10 45 03.6 -59 41 04 6.2 5x 2 1 10 Just before sunrise, get well-exposed TWILIGHT SPECTRA at zenith, if you did not obtain then 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. C: cataclysmic variable: may be fainter than on finding chart. EF Eri is the easternmost star of the pair, and may be 3 mag fainter than the start to its west. G: galaxy. Center on nucleus. N: fading nova o: check finding chart. 40 Eri B is the SE component of a triple system. PP: if not done at the start of the night. Be sure to get one set of bias frames either at the start of end of the night. PM: may have appreciable proper motion. ST: Photometric standard. Please observe only if you could not observe the primary standard Feige 110. X: Insert a wavelength calibration lamp exposure after the 6th 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 .............................................................................. Notes about finding charts: Charts are at www.astro.yale.edu/buxton/smarts/find_charts/blazars/blazars.html RA & Dec: all coordinates are accurate to 1"; charts can be generated by operator as necessary using LEDAS or DSS. .............................................................................. Questions may be addressed to: Michelle Buxton michelle.buxton@yale.edu (YALE program) Howard Bond bond@stsci.edu (STSI programs) Fred Walter fwalter@astro.sunysb.edu (SUNY programs)