CONSTRAINING STELLAR PROPERTIES OF INTERVENING DAMPED Lyα AND Mg II ABSORBING GALAXIES TOWARD GRB 050730

We performed multiband deep imaging of the field around GRB 050730 to identify the host galaxies of intervening absorbers, which consist of a damped Lyα absorption (DLA) system at zabs = 3.564, a sub-DLA system at zabs = 3.022, and strong Mg II absorption systems at zabs = 1.773 and 2.253. Our observations were performed after the gamma-ray burst afterglow had disappeared. Thus, our imaging survey has a higher sensitivity to the host galaxies of the intervening absorbers than the normal imaging surveys in the direction of QSOs, for which the QSO glare tends to hide the foreground galaxies. In this deep imaging survey, we could not detect any unambiguous candidates for the host galaxies of the intervening absorbers. Using the 3σ upper limit of the flux in the optical to mid-infrared observing bands, which corresponds to the UV to optical bands in the rest frame of the intervening absorbers, we constrained the star formation rates and stellar masses of the hosts. We estimated the star formation rates for the intervening absorbers to be ∼< 2.5 M☉ yr–1 for z > 3 DLAs and ∼< 1.0 M☉ yr–1 for z ∼ 2 Mg II systems. Their stellar masses are estimated to be several times 109 M☉ or smaller for all intervening galaxies. These properties are comparable to dwarf galaxies, rather than the massive star-forming galaxies commonly seen in the z > 2 galaxy surveys based on emission-line selection or color selection.