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Object ID | Object | na | Typeb | Elem.c | ad | ee | if | ![]() |
Hh | UT Datei | Tel.j | Rk | ![]() |
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mRp |
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tr | S/Ns |
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20030929_01 | 48821 (1997 WK35) | 1 | Them | P | 3.193 | 0.191 | 2.28 | 3.17 | 14.5 | 20030929 | UH 2.2 | 2.82 | 2.62 | 20.8 | 0.0 | 299.2 | 19.6 | 0.1 | 1500 | 147 | 25.9 | 0.0009 |
20030929_02 | 68899 (2002 JL95) | 1 | Them | P | 3.091 | 0.146 | 1.48 | 3.21 | 15.3 | 20030929 | UH 2.2 | 2.68 | 1.69 | 3.5 | 0.1 | 45.5 | 19.0 | 0.1 | 1200 | 215 | 25.9 | 0.0011 |
20030929_03 | 69839 (1998 SJ10) | 1 | Them | P | 3.047 | 0.157 | 1.81 | 3.22 | 15.2 | 20030929 | UH 2.2 | 2.61 | 1.61 | 1.0 | -0.2 | 317.9 | 18.1 | 0.1 | 900 | 327 | 25.5 | 0.0008 |
20030930_01 | 66065 (1998 RB13) | 1 | Them | P | 3.115 | 0.147 | 1.47 | 3.20 | 15.2 | 20030930 | UH 2.2 | 2.56 | 1.90 | 19.7 | 0.1 | 358.4 | 18.7 | 0.1 | 900 | 155 | 25.7 | 0.0008 |
20030930_02 | 69220 (3030 T-3) | 1 | Them | P | 3.053 | 0.157 | 1.57 | 3.22 | 15.3 | 20030930 | UH 2.2 | 2.50 | 2.06 | 22.9 | 0.2 | 344.1 | 19.4 | 0.1 | 1200 | 106 | 25.3 | 0.0020 |
20030930_03 | 71552 (2000 DR7) | 1 | Them | P | 3.185 | 0.152 | 1.47 | 3.18 | 15.0 | 20030930 | UH 2.2 | 2.80 | 1.86 | 8.3 | 0.1 | 57.5 | 18.4 | 0.1 | 900 | 316 | 26.0 | 0.0005 |
20030930_04 | 155387 (1994 AC9) | 1 | Them | P | 3.165 | 0.152 | 1.09 | 3.18 | 16.0 | 20030930 | UH 2.2 | 2.63 | 1.69 | 9.7 | 0.9 | 332.7 | 19.3 | 0.1 | 1500 | 140 | 26.0 | 0.0014 |
20031212_01 | 47085 (1999 AW2) | 1 | Them | P | 3.110 | 0.152 | 1.01 | 3.20 | 14.5 | 20031212 | UH 2.2 | 2.68 | 1.71 | 4.8 | -0.4 | 44.5 | 17.9 | 0.1 | 600 | 206 | 25.3 | 0.0007 |
20031212_02 | 68451 (2001 SZ31) | 2 | Them | P | 3.161 | 0.157 | 0.95 | 3.19 | 14.7 | 20031212 | UH 2.2 | 2.71 | 2.79 | 20.6 | 0.2 | 1.2 | 19.6 | 0.1 | 2100 | 83 | 25.9 | 0.0008 |
20031212_03 | 139964 (2001 SH7) | 2 | Them | P | 3.095 | 0.144 | 1.10 | 3.21 | 15.0 | 20031212 | UH 2.2 | 2.70 | 2.46 | 21.3 | 0.6 | 18.1 | 20.5 | 0.1 | 2100 | 37 | 25.7 | 0.0025 |
20031213_01 | 112407 (2002 NU39) | 1 | Them | P | 3.074 | 0.151 | 1.05 | 3.21 | 15.5 | 20031213 | UH 2.2 | 2.90 | 1.93 | 3.9 | -0.4 | 82.5 | 20.1 | 0.1 | 1500 | 63 | 26.1 | 0.0019 |
* Excerpt only; full Table 3 available online at the
CDS (http://cdsweb.u-strasbg.fr/A+A.htx) a Number of independent times an object was observed during the course of this survey. b Target category of object (see Sect. 1.3) where ``Them'' indicates a Themis family asteroid, ``Koro'' indicates a Koronis family asteroid, ``Veri'' indicates a Veritas family asteroid, ``Kari'' indicates a Karin cluster asteroid, and ``Low-i'' indicates a low-inclination outer-belt asteroid. c Type of orbital elements used, where ``P'' indicates proper elements from the AstDyS website were used, and ``O'' indicates osculating elements from JPL's Solar System Dynamics Group's Small-Body Database (http://ssd.jpl.nasa.gov/sbdb.cgi) were used. d Orbital semimajor axis in AU. e Orbital eccentricity. f Orbital inclination in degrees. g Tisserand parameter, computed from listed orbital elements. h Absolute magnitude (V-band); from JPL's Small-Body Database. i UT date in year, month, and day (YYYYMMDD). jTelescope used (CT1m: CTIO 1.0 m telescope; Gemn: Gemini North 8.1 m telescope; Keck: Keck I 10 m telescope; Lulin: Lulin 1.0 m telescope; SOAR: southern astrophysical research 4.1 m telescope; Subr: Subaru 8.2 m telescope; UH 2.2: University of Hawaii 2.2 m telescope). k Median heliocentric distance in AU; from JPL's Solar System Dynamics Group's Horizons ephemeris generator (http://ssd.jpl.nasa.gov/horizons.cgi). l Median geocentric distance in AU; from JPL's Horizons ephemeris generator. m Solar phase angle in degrees; from JPL's Horizons ephemeris generator. n Orbit plane angle (between the observer and object orbit plane as seen from the object) in degrees; from JPL's Horizons ephemeris generator. o True anomaly in degrees; from JPL's Horizons ephemeris generator. p Approximate mean R-band magnitude of nucleus as measured from observations. q Estimated magnitude uncertainty, where uncertainties of 0.1 mag are assigned to observations obtained during clear conditions, and uncertainties of 0.5 mag are assigned to observations obtained with cirrus present (observing conditions listed in Table 2). r Total effective exposure time in seconds. s Measured signal-to-noise ratio for composite image. t Surface brightness detection limit for activity, in mag arcsec-1, as measured in a 1 arcsec2 sampling aperture. u Fractional scattering surface area of dust with respect to the nucleus cross-section, in 106 km-1 at the geocentric distance of the nucleus, that is represented by ![]() |
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