Deb, Narayan C.2025-02-202025-03-312025-02-202012-11-05https://doi.org/10.1088/1742-6596/388/15/152005https://dspacenew8-imu.refread.com/handle/123456789/2219Recently Meléndez & Barbuy [1] reported accurate log(gf) values for 142 important astrophysical lines within the 4000Å to 8000Å wavelength range. We compare these log(gf) values with our calculated values in a large scale CI calculation involving the lowest 262 fine structure levels of Fe II.enlog(<i>gf</i>) values for astrophysically important transitions in Fe II /Article