CCD: FULL 13'x13'armin READOUT: ONE AMP GAIN INDEX: 3: Read Noise ~ 3.5 ADU = 3.5 e- FILTER SET: UBVRI (using R filter only) ----------------------------------------------------------------------- NOTES FOR TARGET FIELDS ----------------------------------------------------------------------- Our program is to observe bright Kuiper Belt objects (KBOs) to 0.01 arcsecond precision in order to obtain very precise astrometry. We will also observe some field stars to determine their astrometry. Some objects can only be observed at the very beginning or end of the night. The observations are simple direct imaging in the R-band. Images of the KBOs should be no more than about 10 minutes each to prevent trailing losses of the moving KBOs. Field star images are 60 or 80 seconds each. 15 arcsecond dithering between successive images is requested. All objects should be observed on both nights. If time is short or weather is bad please observe only the high priority targets. ----------------------------------------------------------------------- NOTES FOR CALIBRATION FIELDS ----------------------------------------------------------------------- No standards are needed. Only flats and biases are needed in the R-band. Epoch is J2000 ----------------------------------------------------------------------- OBSERVING SEQUENCE ----------------------------------------------------------------------- KBO/Starfield #exposures Total time Priority x seconds for object each night 136108 5x600sec (60 minutes) 1 Ixion 5x600sec (60 minutes) 1 119951 5x600sec (60 minutes) 3 Quaoar 5x600sec (60 minutes) 1 55636 5x600sec (60 minutes) 3 Eris 5x600sec (60 minutes) 2 55638 5x600sec (60 minutes) 1 Starfield1 5x80sec (10 minutes) 1 Starfield2 5x60sec (10 minutes) 2 Priority: 1=Highest, 2=Medium, 3=Low Please image all objects listed for the required time on both nights. If extra time is available repeat objects but only after all objects have been observed at least once in good conditions. No finder charts. Airmass less than 1.5 preferred if possible. R-band filter for all observations. All Kuiper Belt Object integrations 600 seconds. Field star integrations are 60 or 80 seconds. Please dither about 15 arcseconds between images. The proper RA and Dec for each KBO for late July is put below. Please observe the object for the full amount of time as stated. KBO (136108) 2003EL61 => R-filter, 5 exposures of 600 seconds each Highest Priority Date R.A. (J2000) Decl. July2008 13 32 44.5 +19 25 00 KBO (28978) Ixion => R-filter, 5 exposures of 600 seconds each Highest Priority Date R.A. (J2000) Decl. July2008 16 43 43.7 -23 14 30 KBO (119951) 2002KX14 => R-filter, 5 exposures of 600 seconds each Low Priority Date R.A. (J2000) Decl. July2008 16 03 02.0 -21 00 10 KBO (50000) Quaoar => R-filter, 5 exposures of 600 seconds Highest Priority Date R.A. (J2000) Decl. July2008 17 06 30.0 -15 15 00 KBO (55636) 2002TX300 => R-filter, 5 exposures of 600 seconds Low Priority Date R.A. (J2000) Decl. July2008 00 37 18.6 +27 31 50 KBO (136199) Eris => R-filter, 5 exposures of 600 seconds Medium Priority Date R.A. (J2000) Decl. July2008 01 40 52.3 -04 33 25 KBO (55638) 2002VE95 => R-filter, 5 exposures of 600 seconds Highest Priority Date R.A. (J2000) Decl. July2008 04 25 12.0 +10 04 40 Starfield1 => R-filter, 5 exposures of 80 seconds Highest Priority Date R.A. (J2000) Decl. July2008 04 26 11.00 +10 01 50 Starfield2 => R-filter, 5 exposures of 60 seconds Medium Priority Date R.A. (J2000) Decl. July2008 04 25 47.00 +10 03 00