# Popularity Evolution of Professional Users on Facebook

**Authors:** Samin Mohammadi, Reza Farahbakhsh, Noel Crespi

arXiv: 1705.02156 · 2017-05-08

## TL;DR

This study analyzes the popularity growth patterns of 8,000 professional Facebook users over 14 months, revealing that activity and fame levels positively influence popularity trends.

## Contribution

It provides a large-scale empirical analysis of popularity evolution patterns among professional social media users, with insights into factors affecting growth.

## Key findings

- Active users tend to gain more followers.
- Famous users generally experience positive popularity trends.
- Different popularity evolution patterns are characterized and analyzed.

## Abstract

Popularity in social media is an important objective for professional users (e.g. companies, celebrities, and public figures, etc). A simple yet prominent metric utilized to measure the popularity of a user is the number of fans or followers she succeed to attract to her page. Popularity is influenced by several factors which identifying them is an interesting research topic. This paper aims to understand this phenomenon in social media by exploring the popularity evolution for professional users in Facebook. To this end, we implemented a crawler and monitor the popularity evolution trend of 8k most popular professional users on Facebook over a period of 14 months. The collected dataset includes around 20 million popularity values and 43 million posts. We characterized different popularity evolution patterns by clustering the users temporal number of fans and study them from various perspectives including their categories and level of activities. Our observations show that being active and famous correlate positively with the popularity trend.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/1705.02156/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1705.02156/full.md

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Source: https://tomesphere.com/paper/1705.02156