Diversity of chemistry and excitation conditions in the high-mass star forming complex W33

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Table 4

Resolutions and sensitivities of the infrared to submillimeter observations that were used for the construction of the SEDs in Sect. 4.

Survey	Telescope/Instrument	Wavelength [μm]	Resolution [″]	Sensitivity


MSX	MSX	8.3	18.3	1 MJy sr^-1
MSX	MSX	12.1	18.3	16 MJy sr^-1
MSX	MSX	14.7	18.3	11 MJy sr^-1
MSX	MSX	21.3	18.3	35 MJy sr^-1
Hi-GAL	Herschel/PACS	70	9.0^a	20.2 mJy beam^-1^b
Hi-GAL	Herschel/PACS	160	13.5^a	45.2 mJy beam^-1^b
Hi-GAL	Herschel/SPIRE	250	18.1^c	12.1 mJy beam^-1^b
Hi-GAL	Herschel/SPIRE	350	25.2^c	10.0 mJy beam^-1^b
Hi-GAL	Herschel/SPIRE	500	36.6^c	14.4 mJy beam^-1^b
ATLASGAL	APEX/LABOCA	870	19.2	40−60 mJy beam^-1

Notes.

^(a)

Poglitsch et al. (2010).

^(b)

Spectral and Photometric Imaging Receiver (SPIRE) Photodetector Array Camera and Spectrometer (PACS) Parallel Mode Observers’ Manual (http://herschel.esac.esa.int/Docs/PMODE/html/parallel_om.html).

^(c)

Griffin et al. (2010).

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