Volume 518, July-August 2010
Herschel: the first science highlights
Article Number L140
Number of page(s) 5
Section Letters
Published online 16 July 2010

Online Material

Table 1:   Herschel-PACS total flux measurements.

\end{figure} Figure 3:

PHT22 ISO-PHOT observation of AQ And. A red circle denotes the shell (radius of 52 $^{\prime \prime }$) observed with Herschel-PACS discussed below. ISOs FWHM resolution is 35-40 $^{\prime \prime }$ at 60 $\mu $m.

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\end{figure} Figure 4:

SED fitting results. The dashed black line is the observed ISO short wavelength spectrum (SWS) and the long wavelength spectrum (LRS) (Sloan et al. 2003), the black symbols are literature photometry points, the red diamonds the PACS photometry, and the continuous red line is the model. From bottom to top: TT Cyg, U Ant, and AQ And, which was shifted by up by 102 Jy for clarity.

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\end{figure} Figure 5:

Extended field of U Ant: Left: HIRAS image at 100 $\mu $m (Izumiura et al. 1997); right: Herschel-PACS image at 70 $\mu $m rebinned to 30 $\hbox {$^{\prime \prime }$ }/ $pixel.

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