Short-term variability of 29 minor planets (Thirouin+, 2010)

Details Short-term variability of 29 minor planets (Thirouin+, 2010) Short-term variability of 29 minor planets (Thirouin+, 2010)

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35229093t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/522/A93. Originally published in: 2010A&A...522A..93T

Physics

Minor Planets, Photometry

Scientific paper

The time series photometry of all the objects is provided as Table 3. We highlighted in bold face the times corresponding to the images that we used to obtain an R magnitude calibration. The rest of the R magnitudes in the table was obtained by using the relative magnitude information. Also, in table 1 are geometric data such as geocentric and heliocentric distances. The R magnitudes that the TNOs would have if they were at 1AU from the Earth and the Sun (mR(1,1)) are also shown. No phase corrections were applied.
In table 3, we present our photometric results: the name of the object and for each image we specify the Julian date (not corrected for travel time), the Relative magnitude [mag] and the 1-sigma error associated [mag], the R magnitude [mag], the filter used during observational runs, the phase angle (phi) [deg], topocentric (rh) and heliocentric (Delta) distances [AU] and the magnitude [mag] at 1AU from the Earth and at 1AU from the Sun. We highlight in bold face the date of the image in which we performed a crude absolute calibration.
(4 data files).

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