While the nuclide $^{148}\mathrm{Gd}$ is only known to undergo $\alpha$ decay, with a half-life of $86.9$ years, I noticed that it has higher energy than its isobar $^{148}\mathrm{Eu}$: $m_{^{148}\mathrm{Gd}}=147.9181214(16)\,\mathrm{amu}$, $m_{^{148}\mathrm{Eu}}=147.918086(11)\,\mathrm{amu}$, which means that $$ ^{148}\mathrm{Gd}+e^-\to\,^{148}\mathrm{Eu}+\nu_e $$ is energetically possible, with $Q_{\mathrm{EC}}$ lying between $21.2\,\mathrm{keV}$ and $44.7\,\mathrm{keV}$. Such an energetically allowed but unobserved $\beta$ decay mode occurs also for $^{222}\mathrm{Rn}$, but the latter only has an $\alpha$ half-life of $3.8$ days, so seeing $^{148}\mathrm{Gd}$ undergoing electron capture should have been easier.
So I was wondering: Have experiments been carried out to try to observe this decay mode? Is there any experimentally known lower limit on the EC half-life?
If not, could there be any prediction based on the value of $Q_{\mathrm{EC}}$ on the half-life of electron capture of $^{148}\mathrm{Gd}$ that would help me to get a picture of the order to magnitude of the EC half-life? In other words, would you expect the half-life to be too long to make the decay mode observable, compared with its short $\alpha$ half-life?
Thank you in advance for any information/references/suggestions.