All Tables
- Table 1:
Log of the observations relevant to this paper.
- Table 2:
Optical broad-band imaging photometric calibration parameters.
- Table 3:
Averaged local background values for the H II regions of the bar. Values were
corrected for Galactic extinction (Schlegel et al. 1998).
- Table 4:
Column 1: identification number of the H II regions (from the
NGC 1530 H II region catalogue, Relaño et al. 2005); Col. 2: decimal
logarithm of the H
luminosity (in erg s-1). The errors represent
uncertainties in the H
luminosity due to the image noise and the
uncertainties in the determination of the H II region area
(as described in Zurita 2001); Col. 3: decimal logarithm
of the H
equivalent width of the H II regions; Cols. 4 to 7:
broad band magnitudes of the H II regions corrected for Galactic
extinction (Schlegel et al. 1998); Cols. 8 to 11: number of
data points used for the determination of the broad band colour in the
corresponding band (see Sect. 3.2.3 for more details). The
errors in the broad band magnitudes include uncertainties due to the
determination of the local background for each H II region (see
Sect. 3.2.1 for details), which dominate the error bars. The
asterisks highlight the H II regions data which rely on only one measurement of
the local background, and which are therefore more uncertain.