Known astrometry of S/2000 S 8

Astrometric entries have been preserved as submitted to the MPC.
Therefore the naming nomenclature may slightly vary;
some are internal designation before the discovery IAU Circulars were issued.
Note that the CORRECT nomenclature has a space before and after the 'S'!



OBS B. Gladman, J. Kavelaars
TEL CFHT 3.6-m reflector + CCD
NET USNO-A2.0
CON B. Gladman            
CON gladman@obs-nice.fr
     S5c6n1 * C2000 09 23.47373 03 57 42.41 +18 33 04.5                      568
     S5c6n1   C2000 09 23.52979 03 57 42.16 +18 33 03.6                      568
     S5c6n1   C2000 09 23.61053 03 57 41.82 +18 33 02.2          23.5 R      568
     S5c6n1   C2000 09 24.48641 03 57 38.41 +18 32 46.7          23.5 R      568
     S5c6n1   C2000 09 24.54793 03 57 38.13 +18 32 45.5          23.6 R      568
     S5c6n1   C2000 09 24.61033 03 57 37.83 +18 32 44.4          23.9 R      568
 
TEL ESO VLT-UT1 8-m reflector + CCD
OBS UT1 Science team (Service observing)
MEA B. Gladman
CAT USNO A2.0
CON B. Gladman, Obs. de la Cote d'Azur
CON gladman@obs-nice.fr
     S5c6n1   C2000 11 04.24298 03 49 30.02 +18 04 58.1                      309
     S5c6n1   C2000 11 04.28701 03 49 29.21 +18 04 55.6                      309

OBS P.D. Nicholson, JJ Kavelaars
COD 675
TEL Hale 5m + CCD
CAT USNO A2.0
CON JJ Kavelaars
CON kavelaars@physics.mcmaster.ca
        Position measured on shifted 675 images, astrometry poor ( +/- 0.75'')
     s5c6n1   C2000 11 27.28907 03 42 10.70 +17 41 28.9                      675
     s5c6n1   C2000 11 27.39100 03 42 08.72 +17 41 22.4                      675

     S2000S8  C2000 12 18.17633 03 36 04.67 +17 22 20.3                      695
     S2000S8  C2000 12 18.25217 03 36 03.49 +17 22 16.8          23.5 R      695
     S2000S8  C2000 12 18.30313 03 36 02.71 +17 22 14.0                      695

    SK00S080  C2001 01 21.11472 03 30 58.65  17 08 23.0                      675
    SK00S080  C2001 01 21.19989 03 30 58.43  17 08 23.4                      675

! Absence of S 8 on Sep 18 imaging understood as being due to crowding.
     S00s8    C2001 09 19.37675 04 53 04.98 +20 25 38.1          24   R      675
     S00s8    C2001 09 20.44765 04 53 07.62 +20 25 35.5                      675
     S00s8    C2001 09 20.45591 04 53 07.61 +20 25 35.8                      675
     S00s8    C2001 09 20.49846 04 53 07.73 +20 25 35.3          24   R      675
     S00s8    C2001 09 20.50674 04 53 07.72 +20 25 35.2                      675

Following were corrected after Brian noted discrepancy.
     S8       C2002 11 05.29568 05 56 15.94 +22 29 49.3                      675
     S8       C2002 11 06.36738 05 56 03.86 +22 29 46.9                      675
     S8       C2002 11 06.39575 05 56 03.52 +22 29 47.2                      675

+ Nice detection on all images
     S8       C2002 12 31.18427 05 38 50.49 +22 24 09.1                      675
     S8       C2002 12 31.18927 05 38 50.39 +22 24 09.0                      675
     S8       C2002 12 31.19416 05 38 50.28 +22 24 08.9                      675
     S8       C2002 12 31.19912 05 38 50.19 +22 24 08.9                      675
     S8       C2002 12 31.20495 05 38 50.04 +22 24 09.1                      675
     S8       C2002 12 31.21009 05 38 49.94 +22 24 09.1                      675