Vision-language models underperform specialized astronomical methods on real observational data, with accuracy improving when physical explanations are provided in prompts and when raw numerical measurements replace rendered plots.
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5 Pith papers cite this work. Polarity classification is still indexing.
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FRB dispersion measures directly constrain suppression of the matter power spectrum due to feedback at k ~ 0.1-3 h/Mpc, reduce posterior variance by a factor of ~8 at k~1 h/Mpc, and exclude extreme large-scale feedback scenarios at ~2 sigma.
In M83 the efficiency of turning molecular gas and dense gas into stars is suppressed by factors of about 2 and 0.35 in the bar versus spiral arms, with higher CO line widths suggesting turbulence as the cause.
Metal abundance discontinuities at cold fronts and a shock in IC 1262 link sloshing and AGN activity to metal transport in the intragroup medium.
DIXE NXB averages 4.46e-2 counts s^-1 cm^-2 keV^-1 at the geomagnetic equator under solar minimum, dominated by cosmic-proton-induced particles, rising to 1.55e-1 at higher latitudes, with SAA delayed background negligible after ~5 minutes.
citing papers explorer
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A systematic evaluation of vision-language models for observational astronomical reasoning tasks
Vision-language models underperform specialized astronomical methods on real observational data, with accuracy improving when physical explanations are provided in prompts and when raw numerical measurements replace rendered plots.
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Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts
FRB dispersion measures directly constrain suppression of the matter power spectrum due to feedback at k ~ 0.1-3 h/Mpc, reduce posterior variance by a factor of ~8 at k~1 h/Mpc, and exclude extreme large-scale feedback scenarios at ~2 sigma.
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The Impact of the Bar on Dense Gas and Star Formation in M83
In M83 the efficiency of turning molecular gas and dense gas into stars is suppressed by factors of about 2 and 0.35 in the bar versus spiral arms, with higher CO line widths suggesting turbulence as the cause.
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Metal enrichment in the galaxy group IC 1262
Metal abundance discontinuities at cold fronts and a shock in IC 1262 link sloshing and AGN activity to metal transport in the intragroup medium.
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Simulation of non X-ray background for the DIffuse X-ray Explorer (DIXE) mission
DIXE NXB averages 4.46e-2 counts s^-1 cm^-2 keV^-1 at the geomagnetic equator under solar minimum, dominated by cosmic-proton-induced particles, rising to 1.55e-1 at higher latitudes, with SAA delayed background negligible after ~5 minutes.