All Tables

Table 1: Summary of observations: each mask is named with the identification number of its primary target. The number of slitlets, of IR-peakers included, and of measured spectroscopic redshifts are reported.
Table 2: Data for IR-peak sources included in slit, sorted by field: basic photometric information, photometric flag, spectroscopic classification and redshift are listed. See Table 5 for more details on flags.
Table 3: Detected lines for IR-peak targets, sorted by mask (first night). For each source, we report the observed wavelength, equivalent width (EW), full width at half maximum (FWHM, corrected for the instrumental resolution) and identification of the detected spectral features. For each detected line, the spectroscopic redshift is computed (last column).
Table 4: Detected lines for IR-peak targets, sorted by mask (second night).
Table 7: Results of spectro-photometric fitting for sources with no AGN component. The five columns on the right contain the stellar masses of galaxies, their ongoing (within the last 10⁸ yr) star formation rate, two values of the intrinsic extinction, and the IR (8-1000 $\mu$ m restframe) luminosity produced by the ongoing starburst, estimated assuming an M 82-like template. The two $A_{\rm V}$ values are computed by averaging over the whole galaxy life and over the last 10⁸ yr (representing the amount of dust affecting the ongoing burst). In parenthesis the 3 $\sigma$ ranges derived from the exploration of the parameter space are reported.
Table 8: Results of SED fitting for IR-peakers requiring an AGN component. The fit consists in the combination of a simple stellar population and a torus model (Fritz et al. 2006). The 3 $\sigma$ ranges for the main geometrical and dust properties of the torus are reported, as well as stellar population ages, extinctions and masses.
Table 9: Summary of results.
Table 5: Results for first night. For each target, the number of detected absorption and emission lines is reported, as well as a photometric and spectroscopic (see footnotes) classification. The measured spectroscopic redshift is in Col. 6, while Col. 7 lists the photometric estimate of z, as obtained with the Hyper-z code (Bolzonella et al. 2000).
Table 6: Results for second night.