Table 3: Photometry of the Vela pulsar (PSR) and the nearby objects o1, o2, and o3, marked in Fig. 1. The offsets of the objects from the pulsar position are given in the second column. Each spectral band cell for the PSR and o1 consists of two pairs of magnitude/flux values, divided by lines: upper pair are measured values, lower pair are dereddened values. Dereddening was performed with E_B-V=0.055(5). Each pair consists of the magnitude (upper value) and the flux in Jy (lower value). Only measured magnitudes/fluxes are presented for o2 and o3. All magnitudes are measured via aperture photometry, except for the pulsar magnitudes in the and H bands, which are measured with PSF fitting (see Sect. 2.3 for details). No magnitudes for  HST bands are calculated. Empty cells mean that the object is not measurable in this band.

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