From Fragmentation to Scientific Continuity
AstroGenesis integrates literature, multiwavelength data, and physics-based modeling into a unified research workflow. Instead of navigating fragmented tools and archives, you work within a continuous, traceable scientific environment.
Domain-Specific Research Modules
Each module is designed around the physical regimes, data characteristics, and analysis workflows of a specific astrophysical source class.
DSRM: Blazar
DSRM: Blazar
Relativistic jet systems with strongly coupled variability and emission processes, demanding coordinated multiwavelength analysis and physically consistent spectral modeling.
DSRM: GRB
DSRM: GRB
Explosive transient phenomena characterized by rapid spectral evolution, extreme luminosities, and tightly constrained temporal windows across high-energy observatories.
DSRM: TDE
DSRM: TDE
Rare nuclear transients tracing accretion onset and disk formation, observed through sparse, heterogeneous data spanning months to years.
DSRM: FRB
DSRM: FRB
Fast radio bursts exhibiting extreme transient behavior and uncertain physical origins, requiring coordinated multiwavelength observations and integrated temporal and spectral analyses.
DSRM: to be added
DSRM: to be added
A new domain-specific research module is currently in development. Stay tuned for updates.
Start a research session in AstroGenesis
Open the chat and start from your source, your epoch, your model. AstroGenesis connects literature, multiwavelength data, and modeling in a traceable workflow.
AstroGenesis is described in
AstroGenesis: A Domain-Specific Multi-Agent Research Infrastructure for Astrophysics
N. Sahakyan et al.
The Astrophysical Journal, 2026
DOI: 10.xxxx/xxxxx