Herschel images of NGC 6720: H2 formation on dust grains

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Table B.1:

Aperture photometry of NGC 6720 in various photometric bands.
$\lambda$	Aperture	Flux	Pixel size	Beam size	Source
$\mu$ m	$^{\prime\prime}$	Jy	$^{\prime\prime}$	$^{\prime\prime}$
12		$0.82\pm0.07$			IRAS
25		$10.1\pm0.5$			IRAS
60		$52.\pm6.$			IRAS
65		$55.\pm5.$			AKARI
70	150	$59.\pm7.\pm6.$	1	${\sim}5.2$	PACS
90		$70.\pm7.$			AKARI
100		$55.\pm5.$			IRAS
140		$37.\pm4.$			AKARI
160	150	$30.\pm3.\pm6.$	2	${\sim}12$	PACS
160	152	$28.\pm7.$	8	${\sim}40$	Spitzer
160		$37.\pm14.$			AKARI
250	168	$13.\pm6.\pm4.$	6	18.1	SPIRE
350	150	$8.\pm4.\pm2.$	10	25.2	SPIRE
500	154	$2.2\pm1.5\pm0.7$	14	36.6	SPIRE

Notes. The apertures are elliptical and the semimajor axis is listed in the second column. The fluxes are listed with their measurement and calibration uncertainties, respectively. For the Spitzer data no measurement uncertainties were obtained. The AKARI data were taken from Izumiura et al. (in prep.). The pixel and beam sizes in the Herschel and Spitzer maps are also given.

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