James O. Chibueze

TL;DR: Based on sub-arcsecond Atacama Large Millimeter/submillimeter Array (ALMA) and SMA 1.3 mm continuum images of the massive protocluster NGC 6334I obtained in 2015 and 2008, the authors found that the dust emission from MM1 has increased by a factor of 4.0±0.3 during the intervening years, and undergone a significant change in morphology.

TL;DR: The FOREST Unbiased Galactic plane Imaging Survey (FUGIN) as mentioned in this paper was the first project to investigate the distribution, kinematics, and physical properties of both diffuse and dense molecular gas in the Galaxy at once by observing 12CO, 13CO, and C18O J=1-0 lines simultaneously.

TL;DR: In this article, the Atacama Large Millimeter/submillimeter Array (ALMA) and SMA 1.3 mm continuum images of the massive protocluster NGC 6334I obtained in 2015 and 2008 were used to find that the dust emission from MM1 has increased by a factor of 4.0$\pm$0.3 during the intervening years, and undergone a significant change in morphology.

TL;DR: The Long Baseline Campaign (LBC) was carried out from 2014 September to late November, culminating in end-to-end observations, calibrations, and imaging of selected Science Verification (SV) targets as discussed by the authors.

TL;DR: The FOREST Unbiased Galactic plane Imaging Survey (FUGIN) as discussed by the authors was the first project to investigate the distribution, kinematics, and physical properties of both diffuse and dense molecular gas in the Galaxy at once by observing 12CO, 13CO, and C18O J=1-0 lines simultaneously.