Submillimeter galaxies (SMGs) are high-redshift galaxies (z = 1 − 4) with very bright flux densities in the submillimeter waveband. To study their nature and their role in the galaxies evolution history, we present an angular clustering measurement of SMGs in the GOODS-North and GOODS-South. We make a 2.0 mJy and 0.5 mJy cut on 850 µm flux density and noise. The total available SMG sources are 141, with 75 in North and 66 in South. Due to the large uncertainties induced from small size target autocorrelation, we conduct a cross-correlation between target and tracer with larger size to effectively reduce the uncertainties. We use ∼ 2500 Ks-selected normal galaxies from deep infrared observations in each field. We derive the clustering lengths and linear galaxy biases of both populations, which lead to the estimation of the SMG clustering length of r0 ∼ 4−5 h−1 Mpc. We find that SMGs do not cluster strongly as reported in previous studies, occupying dark matter halo mass of Mhalo ∼ 1012 M⊙.
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