Peng, B., Lamarche, C., Stacey, G. J., Nikola, T., Vishwas, A., Ferkinhoff, C., Rooney, C., Ball, C., Brisbin, D., Higdon, J., and Higdon, S. J. Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies. Retrieved from https://par.nsf.gov/biblio/10274906. The Astrophysical Journal 908.2 Web. doi:10.3847/1538-4357/abd4e2.

Peng, B., Lamarche, C., Stacey, G. J., Nikola, T., Vishwas, A., Ferkinhoff, C., Rooney, C., Ball, C., Brisbin, D., Higdon, J., & Higdon, S. J. Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies. The Astrophysical Journal, 908 (2). Retrieved from https://par.nsf.gov/biblio/10274906. https://doi.org/10.3847/1538-4357/abd4e2

Peng, B., Lamarche, C., Stacey, G. J., Nikola, T., Vishwas, A., Ferkinhoff, C., Rooney, C., Ball, C., Brisbin, D., Higdon, J., and Higdon, S. J. "Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies". The Astrophysical Journal 908 (2). Country unknown/Code not available. https://doi.org/10.3847/1538-4357/abd4e2. https://par.nsf.gov/biblio/10274906.

@article{osti_10274906,
place = {Country unknown/Code not available}, title = {Far-Infrared Line Diagnostics: Improving N/O Abundance Estimates for Dusty Galaxies}, url = {https://par.nsf.gov/biblio/10274906}, DOI = {10.3847/1538-4357/abd4e2}, abstractNote = {}, journal = {The Astrophysical Journal}, volume = {908}, number = {2}, author = {Peng, B. and Lamarche, C. and Stacey, G. J. and Nikola, T. and Vishwas, A. and Ferkinhoff, C. and Rooney, C. and Ball, C. and Brisbin, D. and Higdon, J. and Higdon, S. J.}, editor = {null} }