The MALATANG Survey: The L<sub>GAS</sub>–L<sub>IR</sub>Correlation on Sub-kiloparsec Scale in Six Nearby Star-forming Galaxies as Traced by HCN J = 4 → 3 and HCO<sup>+</sup>J = 4 → 3Qinghua Tan, Ming Zhu, Yu Gao et al.|The Astrophysical Journal|2018Cited by 52
JWST and ALMA Imaging of Dust-obscured, Massive Substructures in a Typical z ∼ 3 Star-forming Disk GalaxyW. Rujopakarn, J. D. Silverman, Christina C. Williams et al.|The Astrophysical Journal Letters|2023Cited by 26
Fitting pseudo-Sérsic (Spergel) light profiles to galaxies in interferometric data: The excellence of the <i>uυ</i>-planeQinghua Tan, Shaobo Zhang, Carlos Gómez-Guijarro et al.|Astronomy and Astrophysics|2024Cited by 8
Under the glare of a luminous quasar, the FIR continuum is still an excellent tracer of the ISM down to the central kiloparsecJohn D Silverman, W. Rujopakarn, E. Daddi et al.|Monthly Notices of the Royal Astronomical Society|2026Cited by 2
JWST and ALMA imaging of dust-obscured, massive substructures in a typical $z \sim 3$ star-forming disk galaxyW. Rujopakarn, J. D. Silverman, Christina C. Williams et al.|arXiv (Cornell University)|2023Cited by 0