Multi-agent systems (MAS) utilizing multiple Large Language Model agents with Retrieval Augmented Generation and that can execute code locally may become beneficial in cosmological data analysis.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics Computational Physics Data Analysis, Statistics and Probability
We have built a reliable and robust system that takes as input an astronomical image, and returns as output the pointing, scale, and orientation of that image (the astrometric calibration or WCS information).
Instrumentation and Methods for Astrophysics
The majority of these are clusters older than log(age/yr)=8. 0, and are located in the inner disk with $|b|<5^\circ$.
Astrophysics of Galaxies
IceCube DeepCore, the existing low-energy extension of the IceCube Neutrino Observatory, was designed to lower the neutrino detection energy threshold to the GeV range.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Experiment Instrumentation and Detectors
The halo model is a successful framework for describing the distribution of matter in the Universe -- from weak lensing observables to galaxy 2-point correlation functions.
Cosmology and Nongalactic Astrophysics
We use X-ray observations of quasar microlensing (sensitive to smaller compact objects than in the optical) to study the possible presence of a population of low mass black holes (from $\sim$ $10^{-3}M_{\odot}$ to $10^{-1}M_{\odot}$) in lens galaxies.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
anesthetic is a Python package for processing nested sampling runs, and will be useful for any scientist or statistician who uses nested sampling software.
Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics
The 21\, cm line and the patchy kinetic Sunyaev-Zel'dovich (kSZ) effect are promising and complementary probes of the Epoch of Reionization (EoR).
Cosmology and Nongalactic Astrophysics
We present new frontiers in the modelling of the spectral energy distributions (SED) of active galaxies by introducing the radio-to-X-ray fitting capabilities of the publicly available Bayesian code AGNfitter.
Astrophysics of Galaxies
From data collection to photometric fitting and analysis of white dwarfs to generating a white dwarf luminosity function requires numerous Astrophysical, Mathematical and Computational domain knowledge.
Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
