Recent DSLC.club meetings:
🔵 R4DS: Numbers youtu.be/b6Q7UfReAuY
From the DSLC.video aRchives:
🔵 Advanced R: Functions - part I youtu.be/UD4DCDuUpg0
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#dataBS #RStats #R4DS
youtu.be
R for Data Science: Numbers (r4ds12 13)
YouTube video by Data Science Learning Community Videos
![Scatter plot showing the emission-line flux ratios of nearly 500 nearby galaxies, with both axes on logarithmic scales. Each circle represents a galaxy; colour indicates whether its nucleus is powered by young stars, an active galactic nucleus (AGN), or both, while transparency represents uncertainty in the classification. The plot shows that galaxies with AGN-powered nuclei are more common than previously recognised, with most AGN-hosting galaxies clustered at higher [O III]/Hβ ratios. It also highlights that AGN-hosting galaxies moving towards and away from us occupy different regions of the plot, and that smaller circles indicate galaxies with lower central stellar velocity dispersion and therefore lower central mass.](https://cdn.bsky.app/img/feed_thumbnail/plain/did:plc:jiushxoiyvgcw2tgsjyvd2mc/bafkreief3g5nhmrfb4gykdpoqvft4fkoid6sm2vmn6jdgdbnafaul2kydi)
