Table 5.
Summary of the Herschel photometry for Psyche.
Instrument | OBS_ID | Epoch | Photometry (Jy) |
||||
---|---|---|---|---|---|---|---|
F70 | F160 | F250 | F350 | F500 | |||
PACS | 1342202250 | 2010-08-07T17:30:40 | 19.49 ± 1.00 | 4.58 ± 0.28 | |||
PACS | 1342202251 | 2010-08-07T18:54:57 | 18.98 ± 0.98 | 4.59 ± 0.34 | |||
SPIRE | 1342202250 | 2010-08-07T17:22:05 | 1.47 ± 0.10 | 0.61 ± 0.05 | 0.42 ± 0.03 | ||
SPIRE | 1342202251 | 2010-08-07T18:46:39 | 1.63 ± 0.10 | 0.90 ± 0.06 | 0.61 ± 0.04 |
Notes. The total flux densities at 70, 160, 250, 350, and 500 μm in Janskys. The epochs of the peak flux detection of the source when it was scanned by the detectors are provided in the column marked “Epoch”. We note that the PACS and SPIRE scans in Parallel mode are separated by ∼20′, and that is why the asteroid is not seen at the same time, but with an 8 min offset.
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