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Research
my ORCID record: http://orcid.org/0000-0002-8899-4673
click to view My publications on ADS
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MALATANG (MApping the dense moLecular gAs in the sTrongest stAr-formiNg Galaxies)

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The scientific goals of MALATANG
Resolved dense gas star formation relations
especially at Intermediate scales/luminosities
diagnose the SF properties in different environments: nuclear vs. disk
obtain the radial distribution of dense gas and SF efficiency
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I am actively working on one of the JCMT large program MALATANG, dealing with observerving preparation, data reduction, telecon orgnization and project Wiki maintanence:
project page: http://www.eaobservatory.org/jcmt/science/large-programs/malatang/
project Wiki : https://www.eao.hawaii.edu/MALATANG/ (need registration to access)
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Status
The observations has been completed in 2017, and the overall sensitivity came out as we expected; But the signals of most of the galaxies are much weaker than predicted. Affected by ozone features NGC 1097 and NGC 1365 were non-detections in either HCN or HCO+ line. HCN was not detected in NGC 2146, NGC 2903 & NGC 3521.
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CCH in the ISM (Astrochemistry)**
- I am particularly interested in the new and open topic: Astrochemistry, as chemistry is a new way to understand the composition, properties of the interstellar medium, hence the secret of star formation.