pith:FIORR7UL
Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering
High-redshift quasars at z>5 reside in dark matter halos of roughly 10^12 solar masses, with duty cycles low enough to imply most black hole growth is obscured.
arxiv:2602.02778 v3 · 2026-02-02 · astro-ph.GA
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Claims
The dark matter halo mass of quasars estimated from the projected auto correlation function is log(M_h/M_⊙)=12.13 ± 0.07 (12.45 ± 0.14), with the bias parameter b of 14.80 ± 0.84 (24.18 ± 3.11) for the redshift interval of 5.0 ≤ z <5.6 (5.6 ≤ z <6.2). The duty cycle is 0.0002 ± 0.0001 (0.0021^{+0.0049}_{-0.0014}) aligning with the f_duty - M_halo scaling relation.
The photometric quasar candidates selected via machine learning are sufficiently pure and the standard halo bias model from lower-redshift simulations applies without modification at z>5.
High-redshift quasars at 5<z<6.2 reside in dark matter halos of log(M_h/M_sun) ~12.1-12.5 with duty cycles of 0.0002-0.002 indicating obscured black hole growth.
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| First computed | 2026-05-28T01:05:11.630701Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
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