All Tables

Table 1: Log of the observations. The instruments and telescopes, filter names and central wavelengths, full width at half-maximum ( FWHM) of point sources, final useful field of view, total integration times and the dates of the observations are given.
Table 2: Catalogue of the dark globules and their estimated properties. Their assigned number, H-band surface brightness difference inside and outside of the globule, the derived extinction, approximate dimensions and axis ratio together with additional notes are given. For their location and orientation see Fig. 5.
Table 3: Summary of the observed fluxes of objects in the vicinity of the UC H II region G268.42-0.85. Only objects that are detected in more than one band are given; for the nomenclature, see Fig. 12. Due to the extended nebulosity the objects can not be distinguished in the Js-band and therefore no fluxes in this band are provided here. At wavelengths longwards of the M-band only object D is visible. Photometry on object G is omitted in this table because the object lacks definable boundaries and extends outside the image. ^a - See Table 4 for the complete list of measurements.
Table 4: Summary of the observed fluxes and errors of the UC H II region G268.42-0.85. As the error of the NIR photometry, we give the statistical error of the PSF fit. The last but one column indicates if the given flux density was included in the SED fitting (see Sect. 3.5). Notes: ^a PSF-Fit; ^b filter centered on Br $\alpha$ ; ^c narrow-band filter; ^d flux standard star not detected, only lower limit can be given. References: ¹ this paper; ² Egan et al. (1999); ³ Ghosh et al. (2000); ⁴ Walsh et al. (1998).