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Fig. 5
IR SOFI blue and red grism spectroscopy of H 1743-322 on April 19, 2003 (left) and July 31, 2004 (right). Both parts around 1.3 and 1.8 μm are not shown due to high level of atmospheric absorption. We indicate the position of the lines that we could detect and identify, reported in Table 2.
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