begin.tex

 \documentclass[fleqn,usenatbib]{article}
 \usepackage[left=2cm,right=2cm,top=2cm,bottom=2cm,paperwidth=22cm,paperheight=32cm]{geometry}% Easy control of page dimensions
% paperwidth=100cm,paperheight=300cm
\usepackage{changepage}%Alter page layout
\usepackage{xr} 
%\usepackage{xr-hyper} 
%\usepackage{hyperref} 
\usepackage{caption}
\usepackage{subcaption}

\usepackage[T2A]{fontenc}    % кириллица на выходе
\usepackage[utf8]{inputenc}  % utf8 на входе
%\usepackage[cp866]{inputenc}
% \usepackage[russian]{babel}   % for Russian documents

\usepackage{mathptmx}
\usepackage{ae,aecompl}
\usepackage{graphicx}	% Including figure files
\usepackage{amsmath}	% Advanced maths commands
\usepackage{amssymb}	% Extra maths symbols
\usepackage{multicol}        % Multi-column entries in tables
\usepackage{bm}         % Bold maths symbols, including upright Greek
\usepackage{pdflscape}  % Landscape pages
\usepackage{enumitem}
\usepackage{xspace}
\usepackage{hhline}
\usepackage{cprotect}

\def\beq#1{\begin{equation}\label{#1}}
\def\eeq{\end{equation}}

\usepackage{color}
\newcommand{\red}[1]{\textcolor{red}{#1}}
\newcommand{\blue}[1]{\textcolor{blue}{#1}}
\newcommand{\green}[1]{\textcolor{green}{#1}}
\usepackage[maxfloats=256]{morefloats}  % to mend an error caused by too many unprocessed floats.

\usepackage{alphalph}
% \renewcommand*{\thesubfigure}{\alphalph{\value{subfigure}}}
\renewcommand*{\thesubfigure}{(\thefigure.\arabic{subfigure})}


\maxdeadcycles=1000 %to mend ---100 consecutive dead cycles.

\date{}

\begin{document}
\def\Fin{F_\mathrm{in}}
\def\Fm{F_\mathrm{m}}

\def\hout{h_\mathrm{hot}}
\def\mag{\mathrm{mag}}

\def\vem{ViDEM}
%\renewcommand{\star}{\mathrm{x}}
\def\vem{model of viscous disc evolution}
\def\Ledd{L_\mathrm{Edd}}
\def\ledd{L_\mathrm{Edd}}
\def\dMed{\dot M_\mathrm{Edd}}
\def\dMin{\dot M_\mathrm{in}}
\def\dMout{\dot M_\mathrm{out}}
\def\Fd{F_\mathrm{dead}}
\def\Rc{R_\mathrm{cor}}
\def\Rg{R_\mathrm{s}}  % 2GM/c^2
\def\rg{r_\mathrm{g}}  % GM/c^2
\def\Rd{R_\mathrm{dead}}
\def\Rmso{R_\mathrm{mso}}
\def\Rcor{R_\mathrm{cor}}
\def\Rin{R_\mathrm{in}}
\def\Rhot{R_\mathrm{hot}}
\def\Rm{R_\mathrm{m}}
\def\Rms{R_\mathrm{ms}}
\def\sigmat{\sigma_{\scriptsize\mbox{\textsc{t}}}}
\def\xinner{\xi_\mathrm{mag}}
\newcommand{\vis}{\mathrm{vis}}
\newcommand{\scr}{\mathrm{scr}}
\newcommand{\Wrf}{W_{r\varphi}}
\newcommand{\rc}{R_{\mathrm{cor}}}
\newcommand{\rin}{R_{\mathrm{in}}}
\newcommand{\rscr}{R_\mathrm{scr}}
\newcommand{\hin}{h_\mathrm{in}}
\newcommand{\Fvis}{F_\mathrm{vis}}
\newcommand{\Fmag}{F_\mathrm{mag}}
\newcommand{\mns}{M_{\rm x}}
\newcommand{\Msun}{M_\odot}
\newcommand{\ksu}{K_\mathrm{su}}
\newcommand{\ksd}{K_\mathrm{sd}}
\newcommand{\kappat}{\kappa_\mathrm{t}}
\newcommand{\kappatd}{\kappa_\mathrm{td}}
\newcommand{\irr}{\mathrm{irr}}
\newcommand{\eff}{\mathrm{eff}}

\title{HACOL
}
\author{Supplement Material}

\maketitle

\section*{}
% Each figure presents a particular fit and observed light curves. The fit parameters are shown at the top of a figure and in Table~3 of the paper.  From left to right, from top to bottom, the panels show:

% \begin{enumerate}
% \item
% \end{enumerate}
%{\bf (1)} The inner accretion rate $\dMin$ (thin line), the accretion rate onto the neutron star $\dot M_\star = f_\star \times \dMin$ (thick green line), and the propelled accretion rate $\dot M_p = \dMin-\dot M_\star$ (thicker grey line).


%\section{Supplement Figures}