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Daniel J. Mortlock works on statistical inference in astrophysics. He led the 2011 report of the quasar ULAS J1120+0641 at cosmological redshift $z=7.085$.

The observation connected two questions about the early universe: how a very massive black hole could already have grown, and how much of the surrounding intergalactic gas remained neutral. The paper interpreted the small ionized region and the absorption profile as evidence about cosmic reionization. Its quoted age and black hole mass are inferences within the adopted physical model, alongside the measured radiation spectrum.^[ref]

Distinguish the rest-mass supply ${\dot{M}}_{\mathrm{in}}$ from the actual black-hole mass growth. With the usual radiative-efficiency definition,At the Eddington limit the growth is exponential:The available time is the difference of the supplied ages, $\Delta t=650\mathrm{Myr}$; no new cosmological age-redshift relation is needed.

Using the printed ${\sigma }_e=6.6\times 10^{-29}{\mathrm{m}}^2$, together with $G=6.67430\times 10^{-11}{\mathrm{m}}^3\mathrm{k}{\mathrm{g}}^{-1}{\mathrm{s}}^{-2}$, $m_p\simeq 1.67262\times 10^{-27}\mathrm{kg}$, $c=299792458\mathrm{m}{\mathrm{s}}^{-1}$ and a Julian year of $31557600\mathrm{s}$, givesThereforeThis is about $13.09$ e-folds. The constants just listed are evaluation constants, not additional observational inputs asserted to be on the paper.

Sometimes an elementary growth convention identifies ${\dot{M}}_{\mathrm{BH}}$ directly with $L/(ϵc^2)$ and drops the radiated fraction of the incoming rest mass. That approximation instead gives $t_{\mathrm{Sal}}\simeq 44.69\mathrm{Myr}$ and $M_0\simeq 9.7\times 10^2{M}_{\odot }$. The first result retains the physically distinct supplied and retained masses; the convention must be stated because exponential growth magnifies this difference.

The main implication is already severe in the optimistic calculation: a low-mass stellar-remnant seed has insufficient time under the specified efficiency and strictly Eddington-limited accretion. A heavier seed, earlier formation, a different efficiency, mergers or episodes beyond that idealized luminosity limit can relax the inference. Any duty cycle below unity or sub-Eddington episodes require a larger initial mass within the adopted model. The reported high-redshift quasar motivating this calculation was identified spectroscopically at $z=7.085$; its published age estimate need not replace the ages supplied here.^[ref]