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Table 1

Summary of observations.

Obs. ID Instrument/Mode Filter Start time Tobs Δ a Longitudeb Fluxc
(2012-) (s) (mJy)
1342239786 SPIREPhoto 250/350/500 02-29 20:08:23 1421 32.649 28.0 179.9 ± 2.7/107.9 ± 2.9/ 58.4 ± 3.5
1342239900 SPIREPhoto 250/350/500 03-01 13:04:38 1421 32.638 347.5 176.8 ± 2.0/105.8 ± 3.0/ 56.0 ± 3.5
1342239979 SPIREPhoto 250/350/500 03-02 06:30:10 1421 32.627 306.8 174.8 ± 3.0/106.2 ± 2.9/ 57.7 ± 3.5
1342240025 SPIREPhoto 250/350/500 03-02 22:44:11 1421 32.617 268.8 175.5 ± 2.9/104.9 ± 3.1/ 58.6 ± 3.5
1342241087 SPIREPhoto 250/350/500 03-03 16:21:25 1421 32.606 227.4 171.9 ± 2.8/106.0 ± 3.1/ 59.4 ± 3.6
1342241158 SPIREPhoto 250/350/500 03-04 09:17:02 1421 32.596 187.6 170.7 ± 2.9/106.2 ± 3.0/ 56.5 ± 3.5
1342240277 SPIREPhoto 250/350/500 03-05 02:18:31 1421 32.585 147.6 174.9 ± 2.9/106.3 ± 3.0/ 56.5 ± 3.5
1342240315 SPIREPhoto 250/350/500 03-05 19:12:47 1421 32.574 107.9 184.9 ± 2.9/111.9 ± 3.0/ 59.8 ± 3.5
1342240318 SPIREPhoto 250/350/500 03-06 11:44:14 1421 32.563 69.1 186.9 ± 3.0/116.6 ± 2.9/ 63.9 ± 3.5
1342241381-2 PACSPhoto 70/160 03-14 03:02:01 2 × 286 32.442 358.7 321.9 ± 8.6/ /331.0 ± 10.1
1342241383-4 PACSPhoto 100/160 03-14 03:13:39 2 × 286 32.442 358.2 /393.3 ± 4.0/331.0 ± 10.1
1342241418-9 PACSPhoto 70/160 03-14 19:54:46 2 × 286 32.431 319.1 316.5 ± 2.7/ /317.3 ± 20.9
1342241420-1 PACSPhoto 100/160 03-14 20:06:24 2 × 286 32.431 318.6 /406.1 ± 7.9/317.3 ± 20.9
1342241471-2 PACSPhoto 70/160 03-15 12:58:39 2 × 286 32.419 279.0 312.2 ± 7.3/ /313.3 ± 20.0
1342241473-4 PACSPhoto 100/160 03-15 13:10:17 2 × 286 32.419 278.6 /380.4 ± 13.4/ 313.3 ± 20.0
1342241509-0 PACSPhoto 70/160 03-16 06:33:59 2 × 286 32.407 237.6 295.0 ± 7.1/ /314.8 ± 13.6
1342241511-2 PACSPhoto 100/160 03-16 06:45:37 2 × 286 32.407 237.2 /377.2 ± 3.6/314.8 ± 13.6
1342241620-1 PACSPhoto 70/160 03-17 00:10:12 2 × 286 32.395 196.3 299.8 ± 3.5/ /309.9 ± 10.5
1342241622-3 PACSPhoto 100/160 03-17 00:21:50 2 × 286 32.395 195.8 /371.1 ± 7.1/309.9 ± 10.5
1342241655-6 PACSPhoto 70/160 03-17 17:31:54 2 × 286 32.384 155.5 311.5 ± 4.5/ /307.5 ± 16.6
1342241657-8 PACSPhoto 100/160 03-17 17:43:32 2 × 286 32.384 155.1 /379.3 ± 9.3/307.5 ± 16.6
1342241699-0 PACSPhoto 70/160 03-18 11:04:14 2 × 286 32.372 114.3 342.1 ± 2.8/ /329.7 ± 12.6
1342241701-2 PACSPhoto 100/160 03-18 11:15:52 2 × 286 32.372 113.9 /418.3 ± 2.9/329.7 ± 12.6
1342241865-6 PACSPhoto 70/160 03-19 04:42:46 2 × 286 32.360 72.9 347.6 ± 12.4/ /338.7 ± 25.7
1342241867-8 PACSPhoto 100/160 03-19 04:54:24 2 × 286 32.360 72.4 /426.9 ± 6.2/338.7 ± 25.7
1342241928-9 PACSPhoto 70/160 03-19 20:44:31 2 × 286 32.349 35.2 349.1 ± 4.4/ /353.0 ± 18.5
1342241930-1 PACSPhoto 100/160 03-19 20:56:09 2 × 286 32.349 34.8 /413.9 ± 3.9/353.0 ± 18.5

Notes. .

(a)

Observer-centric distance.

(b)

Subobserver east longitude at mid-point. We adopt the same orbital conventions as, e.g., Buie et al. (1997) and Lellouch et al. (2011). Zero longitude on Pluto is the sub-Charon point. The subobserver point longitude decreases with time.

(c)

Color-corrected fluxes. PACS 160-μm fluxes are given for the average over four consecutive Obs. IDs (see text)

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