${{\mathit N}}$ BARYONS
($\mathit S$ = 0, $\mathit I$ = 1/2)
${{\mathit p}}$, ${{\mathit N}^{+}}$ = ${\mathit {\mathit u}}$ ${\mathit {\mathit u}}$ ${\mathit {\mathit d}}$; ${{\mathit n}}$, ${{\mathit N}^{0}}$ = ${\mathit {\mathit u}}$ ${\mathit {\mathit d}}$ ${\mathit {\mathit d}}$		 INSPIRE search

${{\mathit N}{(1710)}}$ $I(J^P)$ = $1/2(1/2^{+})$ 

Older and obsolete values are listed and referenced in the 2014 edition, Chinese Physics C38 070001 (2014).
${{\mathit N}{(1710)}}$ POLE POSITION
REAL PART   $1650\text{ to }1750\text{ }(\approx1700) $ MeV 
$-2{\times }$IMAGINARY PART   $80\text{ to }160\text{ }(\approx120) $ MeV 
${{\mathit N}{(1710)}}$ ELASTIC POLE RESIDUE
MODULUS $\vert \mathit r\vert $   $4\text{ to }10\text{ }(\approx7) $ MeV 
PHASE $\theta $   $120\text{ to }270\text{ }(\approx190) $ $^\circ{}$ 
${{\mathit N}{(1710)}}$ INELASTIC POLE RESIDUE
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \eta}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit \Lambda}}{{\mathit K}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit \Sigma}}{{\mathit K}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit N}{(1535)}}{{\mathit \pi}}$
${{\mathit N}{(1710)}}$ BREIT-WIGNER MASS   $1680\text{ to }1740\text{ }(\approx1710) $ MeV 
${{\mathit N}{(1710)}}$ BREIT-WIGNER WIDTH   $80\text{ to }200\text{ }(\approx140) $ MeV 
${{\mathit N}{(1710)}}$ PHOTON DECAY AMPLITUDES AT THE POLE
${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
${{\mathit N}{(1710)}}$ BREIT-WIGNER PHOTON DECAY AMPLITUDES
${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
${{\mathit N}{(1710)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
The following branching fractions are our estimates, not fits or averages.
$\Gamma_{1}$ ${{\mathit N}}{{\mathit \pi}}$  $5 - 20\%$ 588
$\Gamma_{2}$ ${{\mathit N}}{{\mathit \eta}}$  $10 - 50\%$ 412
$\Gamma_{3}$ ${{\mathit N}}{{\mathit \omega}}$  $1 - 5\%$ -1
$\Gamma_{4}$ ${{\mathit \Lambda}}{{\mathit K}}$  $5 - 25\%$ 269
$\Gamma_{5}$ ${{\mathit \Sigma}}{{\mathit K}}$  seen 138
$\Gamma_{6}$ ${{\mathit N}}{{\mathit \pi}}{{\mathit \pi}}$  $14 - 48$ $\%$ 557
$\Gamma_{7}$ ${{\mathit \Delta}{(1232)}}{{\mathit \pi}}$ , ${\mathit P}{\mathrm -wave}$  $3 - 9$ $\%$ 394
$\Gamma_{8}$ ${{\mathit N}}{{\mathit \rho}}$ , $\mathit S$=1/2, ${\mathit P}{\mathrm -wave}$  $11 - 23$ $\%$ -1
$\Gamma_{9}$ ${{\mathit N}}{{\mathit \sigma}}$  $<$16 $\%$
$\Gamma_{10}$ ${{\mathit N}{(1535)}}{{\mathit \pi}}$  $9 - 21\%$ 113
$\Gamma_{11}$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity=1/2  $0.002 - 0.08\%$ 598
$\Gamma_{12}$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity=1/2  $0.0 - 0.02\%$ 597