Table 2: Summary of the photometric results.
  Object Amplitude Photometric
    (mag) period (hrs)
TNOs      
  1999 TD10 $0.65\pm0.05$ $7.71\pm0.02$
  1999 TC36 0.06? Several possibilities?
  2000 EB173 <0.1 $6.75^{c}\pm0.01$
  Varuna $0.41\pm0.02$ $3.1718^{a}\pm0.0001$
  Ixion <0.15 None detected
  2002 CR46 <0.15 3.66b or $4.35^{b}\pm0.02$
Centaurs      
  2000 QC243 $0.75\pm0.09$ $4.57 \pm0.02$
  2001 PT13 $0.16\pm0.02$ $4.1546 \pm0.0001$
  2002 PN34 $0.18\pm0.04$ 4.23 or $5.11\pm0.03$
  2002 GO9 0.14$\pm0.04$ 6.97 or $9.67\pm0.04$
a Combining our data with those by Jewitt & Sheppard (2002).
b Confidence level below 50%.
c Possible alternate periods are 6.68 h and 6.82 h.

Source LaTeX | All tables | In the text