All Tables

Table 1: Available photometric data for the 15 $\mu$ m sources in the HDF-S observed spectroscopically in the optical and near-infrared. Data are from the EIS Deep survey, but in highlighted cases for which the Teplitz et al. (1998) photometry is used. All magnitudes are in the AB system; ISOCAM LW2 and LW3 fluxes and uncertainties are reported in the last four columns. In the case only an upper limit is available, it is specified.
Table 2: Summary of ISAAC/VLT observations. Slits have been rotated (anti-clockwise with respect to the North direction by the angle in column PA) in order to include the most interesting features of the sources.
Table 3: Summary of results of spectroscopic observations. We report the source name, the instrument, the exposure time, spectroscopic redshift, the measured fluxes (in units of 10^-17 erg cm^-2 s^-1) and equivalent widths (EW, in Å) of [O II] $\lambda 3727$ , H $\beta$ ( $\lambda$ 4861), [O III] $\lambda \lambda 4959, 5007$ , and H $\alpha$ ( $\lambda$ 6563). H $\alpha$ fluxes and EW of H $\alpha$ + [N II] are from Rigopoulou et al. (2000). These measured line fluxes are not corrected for aperture.
Table 4: Widths of relevant emission lines from ISAAC Low-Res and optical spectroscopy. The source name, reference line used for the measure, FWHM in Å, FWHM in km s^-1, and the threshold resolving power in km s^-1 are reported.
Table 5: Relevant spectroscopic data: aperture-corrected H $\alpha$ luminosities, rates of star formation based on H $\alpha$ , and extinction estimates from the Balmer decrement. In the fourth column we report extinction values based on photometric fits with spectral synthesis codes (see Sect. 4.1) and values of SFR corrected for slit-aperture and reddening (from Balmer lines when available). SFRs are in $M_\odot$ yr^-1.
Table 6: Values of the baryonic masses, SFRs and bolometric IR ( $8 \div 1000~\mu$ m) luminosities of the 15 $\mu$ m sources in the HDF-S, as derived from the analysis of their spectral energy distributions (see Sects. 4.3 and 4.4).
Table 7: Radio estimate of the SFR of 15 $\mu$ m sources in both HDF's and FF's. In the first column objects named n are from the HDF-N sample, those with s in the HDF-S. The ISOCAM LW3 sources in HDF-N refer to the catalogue by Aussel et al. (1999). Third column specifies the frequency at which the fluxes in the fourth were measured. Data are from Richards (2000) and Mann (2002).