Shoe Hopes And Goals

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It is likely that this observed turnover in the spectra at low frequencies is due synchrotron self-absorption. 3358 indicate that it is a massive system with a long-term intensive star formation process rather than a low massive system which harbors a star formation burst. 3358 is not detected at the X-ray energies (0.5-7.0 keV) with 30 ks Chandra observation (P.I. 3358 is triggered by galaxy major mergers or fueled by rapid accretion of cold gas from the intergalactic medium (IGM). 3358 does not show any other redshift systems that could be from the lensing galaxy. 3358 is not a lensed galaxy. 3358 is similar to the dust extinction in the typical LBGs. We adopt the dust extinction law proposed by Calzetti et al. The other interpretation is that most of the galaxies that form stars at high intensity are dusty and highly obscured, e.g., SMGs (Chapman et al., 2005) or DOGs (dust-obscured galaxies) (Dey et al., 2008; Fiore et al., 2008), and only small fraction of galaxies that show high SFR is unobscured by dust. Typically, the systemic redshift can be derived from absorption lines that are clearly associated with photospheric features (e.g., S v 1502, C iii 1176, O vi 1343, etc) (e.g., Dey et al., 1997; Shapley et al., 2003), but we can not identify these lines from the spectrum at current S/N level

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