============================================================================== File: 1995_S9_jones_nsdc.data.txt =============================== Contents: - 7 observations of S-9 Phoebe made from 1995 Aug. 31 to 1997 Oct. 22 References: Observations communicated to NSDC by : | Derek Jones | Work: +44 (0)1223 766661 | | Institute of Astronomy | Fax: +44 (0)1223 337523 | | Madingley Road, | Home: +44 (0)1954 210314 | | Cambridge CB3 0HA | email: dhpj@ast.cam.ac.uk | | United Kingdom | | Comments: The observations were taken by David Harper and Kevin Beurle with the 1-metre Jacobus Kapteyn Telescope on La Palma. The pixels were 0.33 arcsec and the CCD chip size 330 arcsec on the side. A red (R) filter was used and the exposure was 64 sec. It is straightforward to measure the position of Phoebe and about ten reference stars on each exposure. The positions of the reference stars were measured on the Digital Sky Survey (DSS-II with 1 arcsec pixels) together with about ten stars from the USNO ACT catalogue, all within 0.7 degrees of the CCD fields. The goodness of fit was 0.12 arcsec, rms in one co-ordinate. The goodness of fit of the reference stars to the positions measured on the CCD was smaller. Phoebe was measured relative to the same reference stars within each night but relative to a different set of reference stars on different nights. The scatter of the residuals relative to the JPL Horizons ephemeris within nights was much smaller than from night to night. This indicates that the accuracy is simply the accuracy of the star positions, i.e. 0.12 arcsec. The observations have been combined into one normal place for each of the seven nights with an rms scatter of 0.04 arcsec within nights. Format: The data are: julian date in MJD (JD - 2400000.5) UTC F14.5 hours R.A. J2000 I3 minutes " I3 seconds " F7.3 degrees Declination J2000 I5 minutes " I3 seconds " F6.2 4X Obs F3.2 Hor F5.2 n I6 `Obs - Hor' are the residuals in arcsec from the JPL Horizons ephemeris. `n' is the number of CCD exposures. ==============================================================================