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Table 1

Observational geometry of all data sets used in this study.

UT date Observing Filter(s)/ R h Δ α References Aspect angle
facility wavelength [AU] [AU] [degrees] [degrees]

Optical data
11/03/03 HST V,R 2.503 1.522 4.70 L06 100
26/02/04 NTT B,V,R 4.481 3.959 11.47 This work*
15/04/04 VLT R 4.670 3.679 2.13 T08 70
16/06/04 VLT R 4.889 4.296 10.33 T08 73
10/05/05 NTT V,R,I *,* 5.599 4.592 0.87 This work 61
12/05/05 NTT V,R,I * 5.601 4.592 0.47 This work 61
14/05/05 NTT V,R,I *,* 5.603 4.593 0.10 This work 61
26/05/06 VLT R 5.620 4.614 1.32 T08 55
30/05/06 VLT R 5.614 4.602 0.57 T08 55
31/05/06 VLT R 5.613 4.601 0.53 T08 55
18/07/06 VLT R 5.511 5.268 10.46 T08*
19/07/06 VLT R 5.509 5.283 10.49 T08*
23/07/06 VLT R 5.503 5.341 10.57 T08*
24/07/06 VLT R 5.501 5.355 10.58 T08*
17/07/07 VLT R 4.635 3.717 6.00 T08 53
17/07/07 NTT V,R 4.635 3.717 6.00 This work 53
20/07/07 NTT R *,* 4.624 3.729 6.64 This work 53
14/09/07 NTT V,R,I *,* 4.398 4.247 13.22 This work*
08/08/07 VLT R 4.549 3.854 10.11 S12*
11/10/07 VLT R 4.279 4.546 12.52 S12*
Thermal-IR data
25/02/04 SST 24 μm 4.477 4.041 12.10 L08*
17/05/07 SST μm 4.851 4.401 11.20 K09*
18/05/07 SST 24 μm 4.848 4.382 11.13 K09*

Notes. Aspect angle is given for the rotation pole orientation determined in Sect. 3. Reference Key: L06 – Lamy et al. (2006), T08 – Tubiana (2008), S12 – Snodgrass et al. (in prep.), L08 – Lamy et al. (2008), K09 – Kelley et al. (2009).

(*)

These data sets were used in the phase-darkening curve fitting and ATPM modelling only. All other data sets were incorporated into our shape and spin state model.

(†)

Comet-spacecraft distance.

(‡)

Spacecraft–comet–Sun angle.

(*,*)

While colour data was taken on these runs, we present just the R-filter data here.

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