  The upcoming second release of PBJam -- a software instrument for fitting
normal modes ("peakbagging") -- supplements the simple power-spectrum model
used in the first version to additionally constrain other features. Dipole
($\ell = 1$) modes, which had been excluded in the initial version of the tool,
are now specifically included. The primary samples of the PLATO mission consist
mainly of main-sequence and subgiant stars, so PBjam implements a single
parameterisation of dipole mixed-mode frequencies that reduces to pure p-modes
in the former, and is suitable for use with the latter, outside the red-giant
"asymptotic" regime. In keeping with the overall philosophy of PBjam's design,
PBjam 2 will specify prior distributions on these parameters empirically,
through predetermined values found for existing samples of solar-like
oscillators. While the red-giant asymptotic regime has been extensively
characterised observationally, the nonasymptotic construction for subgiants
here has not, requiring us to construct this prior sample ourselves. To assist
in this task, we built a tool -- Reggae -- to manually fine-tune and fit the
dipole-mode model, and check the quality of both our initial guesses and fitted
solutions. We have found it very helpful both for these tuning and
visualisation tasks, and also as a didactic aid to understanding the dipole
mixed-mode parameters. Moreover, no other tools currently exist for performing
these tasks in the nonasymptotic parameterisation considered here. As such, we
release Reggae publicly in advance of this update to PBjam, as we believe the
community will benefit from access to such a visualisation tool. This will also
assist future users of PBjam in devising ad-hoc prior constraints on the
mixed-mode parameters, should they wish to perform mode identification for
anomalous stars.
