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@INPROCEEDINGS{2021IAUS..356...77P, author = {{Panda}, Swayamtrupta and {Marziani}, Paola and {Czerny}, Bo{\.Z}ena}, title = "{FeII emission in NLS1s - originating from denser regions with higher abundances?}", keywords = {accretion, accretion disks, radiation mechanisms: thermal, radiative transfer, galaxies: active, (galaxies:) quasars: emission lines, galaxies: Seyfert, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies}, booktitle = {Nuclear Activity in Galaxies Across Cosmic Time}, year = 2021, editor = {{Povi{\'c}}, Mirjana and {Marziani}, Paola and {Masegosa}, Josefa and {Netzer}, Hagai and {Negu}, Seblu H. and {Tessema}, Solomon B.}, volume = {356}, month = jan, pages = {77-81}, doi = {10.1017/S1743921320002616}, archivePrefix = {arXiv}, eprint = {1912.03119}, primaryClass = {astro-ph.HE}, adsurl = {https://ui.adsabs.harvard.edu/abs/2021IAUS..356...77P}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }
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