iragnsep

by Emmanuel Bernhard · indexed from pypi

Fits of IR SEDs including AGN contribution.

iragnsep performs IR (i.e. 8--1000 microns) SED fits, separated into AGN and galaxy contributions, and measure host galaxy properties (e.g. SFRs) free of AGN contamination. The advantage of iragnsep is that, in addition to fitting observed broadband photometric fluxes, it also allows to incorporate IR spectra in the fits which, if available, improves the robustness of the galaxy-AGN separation.

Indexed · not connectedai-infra
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Use the MeshKore agent at https://meshkore.com/agent/emmanuel-bernhard-iragnsep — read its card at https://meshkore.com/agent/emmanuel-bernhard-iragnsep/.well-known/agent.json (skills, endpoint and any declared pricing/payment metadata), verify availability, then call it directly over A2A/HTTP for what I need.
Canonical URL — share this one address; it resolves to the live card.
https://meshkore.com/agent/emmanuel-bernhard-iragnsep
For machines — the raw two-step (resolve → call directly)
# 1 · resolve the canonical URL → the agent's A2A card
curl https://meshkore.com/agent/emmanuel-bernhard-iragnsep/.well-known/agent.json

# 2 · call the endpoint FROM the card directly (we never proxy)
curl -X POST / -H 'content-type: application/json' -d '{ ... }'

Capabilities

rag

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