Publication

The first ground-based detection of the 752 GHz water line in local ultra-luminous infrared galaxies using APEX-SEPIA, D. Quinatoa, C. Yang, E. Ibar, 2024, MNRAS, 527, 6321; (student's paper)
SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys, C. Yang, A. Omont, ; S. Martín et al., 2023, A&A, 680, 95;
First detection of the 448 GHz ortho-H $_\mathsf{\mathit{2}}$ O line at high redshift: probing the structure of a starburst nucleus at z = 3.6, C. Yang, E. González-Alfonso et al. 2020, A&A, 634, L3;
Etching glass in the early Universe: Luminous HF and water emission in a QSO-SMG pair at z=4.7, M. D. Lehnert, C. Yang, B. H. C. Emomonts et al. 2020, A&A, 641, 124;
CO, H $_\mathsf{\mathit{2}}$ O, H $_\mathsf{\mathit{2}}$ O $^+$ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales, C. Yang, R. Gavazzi et al. 2019, A&A ,624, 138.
Planck's dusty GEMS. VI. Multi-J CO excitation and interstellar medium conditions in dusty starburst galaxies at z = 2-4, R. Cañameras; C. Yang; N. P. H. Nesvadba, et al. 2018, A&A, 620, 61.