pith:C7B6TJOI
The impact of strong feedback on galaxy group scaling relations
Highly ejective AGN feedback models underpredict the X-ray luminosity of galaxy groups at fixed mass.
arxiv:2512.04203 v2 · 2025-12-03 · astro-ph.CO · astro-ph.GA · astro-ph.HE
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Claims
highly ejective models under-predict the luminosity of galaxy groups at fixed mass at high significance (5.7σ). This conclusion is robust against selection effects and is obtained from directly measurable and minimally correlated quantities.
That the observed X-ray luminosity-temperature relation in the heterogeneous sample of 44 groups can be compared directly to simulation predictions without substantial biases from selection effects, measurement uncertainties, or differences in how groups are identified.
Highly ejective feedback models under-predict the X-ray luminosity of galaxy groups at fixed mass at 5.7 sigma significance.
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| First computed | 2026-05-20T02:05:38.823216Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
17c3e9a5c8f2353f381cad9288d76c7bcf55c1a6cdf5c88ddcf09445259fe259
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· · · · ·Agent API
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/C7B6TJOI6I2T6OA4VWJIRV3MPP \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 17c3e9a5c8f2353f381cad9288d76c7bcf55c1a6cdf5c88ddcf09445259fe259
Canonical record JSON
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