Blazar research with AstroGenesis
Blazars are the first source class covered by AstroGenesis. The Blazar research module is active; modules for gamma-ray bursts, tidal disruption events and fast radio bursts are in development.
Why blazars first
Blazars are relativistic jet systems in which variability and emission processes are strongly coupled. Studying them means combining data from radio to gamma rays, following how a source changes in time, and fitting physically consistent models to its spectral energy distribution (SED). These steps usually happen in separate tools. AstroGenesis keeps them in one research session.
What the agents do for a blazar
The literature agent searches published work on the source and the physics in question, and returns a synthesis with citations. Its retrieval was benchmarked on about 21,000 blazar papers: for 76.6% of 209 single-paper questions and 79.2% of 154 multi-paper questions, at least one relevant paper was in the top five results (arXiv:2609.28579, Table 1).
The data agent retrieves science-ready multi-wavelength and multi-messenger data from the Markarian Multiwavelength Data Center (MMDC) and runs temporal and spectral analyses. The modeling agent compares emission models with the data using neural networks trained on radiative simulations. The ideation agent looks for tensions between the literature, the data and the models.
What the examples show
The examples below are real answers, abridged: where gamma rays are produced in 3C 279 during flares, the 2009 to 2015 SED of Mrk 421, a one-zone SSC fit to PKS 2155-304, and what is still open in the association of IceCube-170922A with TXS 0506+056.
AstroGenesis works on science-ready data products, not raw instrumental data. You can ask about your own source in plain language; the free plan allows 10 messages per day.
Worked examples
- 3C 279: where are the flare gamma rays produced?Where flare gamma rays are produced in the jet, from 8 cited papers.
- Mrk 421: multi-epoch SED data, 2009 to 201522,608 measurements from radio to gamma rays, with plot and CSV.
- PKS 2155-304: one-zone SSC fit, August 2013Best-fit Doppler factor, magnetic field, region size and electron index.
- TXS 0506+056 and IceCube-170922A: what remains openWhat the neutrino association does and does not establish, from 9 cited papers.
Other topics
- Literature analysis for astrophysics questionsPublished papers synthesised into one answer, with evidence, disagreements and ADS-linked citations.
- Multi-wavelength and multi-messenger data retrievalScience-ready radio to gamma-ray data from MMDC, with instrument and epoch metadata.
- SED modeling with neural networks trained on radiative simulationsEmission models fitted to SEDs with neural networks trained on radiative simulations.
- Research ideation from literature, data and modelsOpen questions found where literature, data and models disagree.
Ask about your own source
Ask in plain language: literature, data, or a model fit. Free plan: 10 messages per day.