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Table 4

Spitzer observations summary.

Object AORKEY Dur. Mid-time r Δ α MIPS flux densities (mJy) Ref.
(min) (UT) (AU) (AU) (°) 24 μm 70 μm

1996 TP66 8805632 38.4 04-01-23 03:31 26.4913 26.2500 2.1 0.689 ± 0.038  <5.87 1
12659456 40.8 05-09-24 15:54 26.6292 26.1132 1.9 0.426 ± 0.029  <2.30 1
1999 TC36 9039104 62.4 04-07-12 11:04 31.0977 30.9436 1.9 1.233 ± 0.022 25.30 ± 2.53 1
2000 GN171 9027840 25.1 04-06-21 00:01 28.5040 28.0070 1.8 0.258 ± 0.031 5.60 ± 4.00 2
2002 VE95 17766912/...7168 18.0 07-09-18 21:28 28.2291 28.2962 2.1 0.476 ± 0.044 3
2002 XV93 17768704/...8960 227.4 07-10-28 04:30 40.0092 39.6962 1.4 0.321 ± 0.018 3
2003 AZ84 10679040 28.9 06-03-30 09:22 45.6674 45.218 1.1 0.291 ± 0.023 17.8 ± 2.66 1
2003 VS2 10680064 11.7 05-08-27 10:08 36.4298 36.5344 1.6 0.304 ± 0.051 25.7 ± 7.34 1
Huya 8808192 21.3 04-01-27 09:40 29.3261 29.2503 1.9 3.630 ± 0.052 57.2 ± 5.25 1
8937216 43.1 04-01-29 17:55 29.3252 29.2100 1.9 3.400 ± 0.050 52.9 ± 1.86 1

Notes. Column headings are: object name; Spitzer AORKEY identification; total duration of all AORs; observation mid-time of the 24 and 70 μm measurements (20YY-MM-DD UT); r: heliocentric distance; Δ: Spitzer-target distance; α: solar phase angle; color-corrected flux density values at MIPS photometer reference wavelengths 23.68 and 71.42 μm, upper limits are 1σ; references. Geometric data were extracted from NASA Horizons (http://ssd.jpl.nasa.gov/horizons.cgi) for the indicated mid-time of the observations.

References. 

(1)

Stansberry et al. (2008), uncertainties derived as flux density/SNR;

(2)

revised 70 μm data from Stansberry et al. (2008);

(3)

previously unpublished data.

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