g clumps selected from the Millimetre Astronomy Legacy Team 90Hz (MALT90) survey, but not found in ATLASGAL. Ref:=2016Ap&SS.361..191Z byZHANG Y.-J. , ZHOU J.-J., ESIMBEK J., HE Y.-X., LI D.-L., TANG X.-D., JI W.-G., YUAN Y., GUO W.-H. Ap&SS, 361, 191 (2016) The global chemical properties of high-mass star forming clumps at different evolutionary stages. o<[ZZE2016] GLLL.lll+BB.bbb> (Nos G354.207-00.036, G354.206-00.038, G350.687-00.491, G350.688-00.489, G342.822+00.382, G342.824+00.381, G341.034-00.114, G341.038-00.113). =E=Catalogue in electronic form as <J/other/ApSS/361.191/>
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