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Close Major Merger Pairs at $z=0$: Bulge-to-Total Ratio and Star Formation Enhancement
Free accessArXiv | 2022| -
CO observations of major merger pairs at z=0: Molecular gas mass and star formation
Free accessArXiv | 2019| -
CO observations of major merger pairs at z = 0: molecular gas mass and star formation⋆
Free accessEDP Sciences | 2019| -
Close Major-merger Pairs at $z=0$: Star-forming Galaxies with Pseudobulges
Free accessArXiv | 2024| -
UV and NIR size of the low-mass field galaxies: the UV compact galaxies
Free accessEDP Sciences | 2020| -
Herschel Observations of Major Merger Pairs at z=0: Dust Mass and Star Formation
Free accessArXiv | 2015| -
Spectral energy distribution similarity of the local galaxies and the 3.6 μm selected galaxies from the Spitzer Extended Deep Survey
IOP Institute of Physics | 2021| -
The atomic gas of star-forming galaxies at z ∼ 0.05 as revealed by the Five-hundred-meter Aperture Spherical Radio Telescope
Free accessEDP Sciences | 2020| -
ALMA [N \i\i ] 205 \mu m Imaging Spectroscopy of the Lensed Submillimeter galaxy ID 141 at redshift 4.24
Free accessArXiv | 2020|
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