Towards a unified scheme of blazar evolution
E. Oukacha, Y. Becherini

TL;DR
This paper uses machine learning to classify blazars, study their evolution, and reveal a continuum between different types, supporting a gradual transition in their accretion states.
Contribution
It introduces a novel ML-based classification and visualization approach that uncovers the continuous nature of blazar evolution and transitional objects.
Findings
Revealed a continuum between FSRQs and BL Lacs.
Identified Changing-Look Blazars as transitional sources.
Supported a gradual evolution scenario in blazar accretion states.
Abstract
Machine learning (ML) and deep learning (DL) techniques are increasingly used across astrophysics, enabled by the growing availability of data and improved acquisition methods. These approaches now support tasks from redshift estimation to source classification. In this work, we aim to (i) classify blazars from the Fermi 4LAC-DR3 catalogue, in particular to identify the likely origin of blazars of uncertain type (BCUs), and (ii) investigate the full blazar sample to study their structure and redshift-luminosity evolution. We focus especially on the transition region between Flat Spectrum Radio Quasars (FSRQs) and BL Lacertae objects (BL Lacs), which may yield insights into accretion disk evolution. We examine Changing-Look Blazars (CLBs) as potential intermediates in this transition. We implement a classification pipeline using both a strong benchmark model (XGBoost) and a foundation…
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