${{\mathit N}}$ 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

${{\mathit N}{(1675)}}$ $I(J^P)$ = $1/2(5/2^{-})$ 

Older and obsolete values are listed and referenced in the 2014 edition, Chinese Physics C38 070001 (2014).
${{\mathit N}{(1675)}}$ POLE POSITION
REAL PART   $1650\text{ to }1660\text{ }(\approx1655) $ MeV 
$-2{\times }$IMAGINARY PART   $120\text{ to }150\text{ }(\approx135) $ MeV 
${{\mathit N}{(1675)}}$ ELASTIC POLE RESIDUE
MODULUS $\vert \mathit r\vert $   $22\text{ to }32\text{ }(\approx26) $ MeV 
PHASE $\theta $   $-27\text{ to }-17\text{ }(\approx-22) $ $^\circ{}$ 
${{\mathit N}{(1675)}}$ INELASTIC POLE RESIDUE
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit \Delta}}{{\mathit \pi}}$, ${\mathit D}{\mathrm -wave}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \eta}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit \Lambda}}{{\mathit K}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit \Sigma}}{{\mathit K}}$
Normalized residue in ${{\mathit N}}$ ${{\mathit \pi}}$ $\rightarrow$ ${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit N}}{{\mathit \sigma}}$
${{\mathit N}{(1675)}}$ BREIT-WIGNER MASS   $1665\text{ to }1680\text{ }(\approx1675) $ MeV 
${{\mathit N}{(1675)}}$ BREIT-WIGNER WIDTH   $130\text{ to }160\text{ }(\approx145) $ MeV 
${{\mathit N}{(1675)}}$ PHOTON DECAY AMPLITUDES AT THE POLE
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-3/2 amplitude A$_{3/2}$
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-3/2 amplitude A$_{3/2}$
${{\mathit N}{(1675)}}$ BREIT-WIGNER PHOTON DECAY AMPLITUDES
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$   $0.010\text{ to }0.025\text{ }(\approx0.018) $ GeV${}^{−1/2}$ 
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity-3/2 amplitude A$_{3/2}$   $0.015\text{ to }0.030\text{ }(\approx0.022) $ GeV${}^{−1/2}$ 
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-1/2 amplitude A$_{1/2}$   $-0.065\text{ to }-0.055\text{ }(\approx-0.060) $ GeV${}^{−1/2}$ 
${{\mathit N}{(1675)}}$ $\rightarrow$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity-3/2 amplitude A$_{3/2}$   $-0.095\text{ to }-0.075\text{ }(\approx-0.085) $ GeV${}^{−1/2}$ 
The following branching fractions are our estimates, not fits or averages.
$\Gamma_{1}$ ${{\mathit N}}{{\mathit \pi}}$  $38 - 42\%$ 564
$\Gamma_{2}$ ${{\mathit N}}{{\mathit \eta}}$  $<$ 1$\%$ 376
$\Gamma_{3}$ ${{\mathit \Lambda}}{{\mathit K}}$  $<$0.04 $\%$ 216
$\Gamma_{4}$ ${{\mathit N}}{{\mathit \pi}}{{\mathit \pi}}$  $25 - 45\%$ 532
$\Gamma_{5}$ ${{\mathit \Delta}{(1232)}}{{\mathit \pi}}$ , ${\mathit D}{\mathrm -wave}$  $23 - 37\%$ 366
$\Gamma_{6}$ ${{\mathit N}}{{\mathit \rho}}$  $0.1 - 0.9$ $\%$ -1
$\Gamma_{7}$ ${{\mathit N}}{{\mathit \rho}}$ , $\mathit S$=1/2  $<$0.2 $\%$ -1
$\Gamma_{8}$ ${{\mathit N}}{{\mathit \rho}}$ , $\mathit S$=3/2 , ${\mathit D}{\mathrm -wave}$  $0.1 - 0.7$ $\%$ -1
$\Gamma_{9}$ ${{\mathit N}}{{\mathit \sigma}}$  $3 - 7\%$
$\Gamma_{10}$ ${{\mathit p}}{{\mathit \gamma}}$  $0 - 0.02\%$ 575
$\Gamma_{11}$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity=1/2  $0 - 0.01\%$ 575
$\Gamma_{12}$ ${{\mathit p}}{{\mathit \gamma}}$ , helicity=3/2  $0 - 0.01\%$ 575
$\Gamma_{13}$ ${{\mathit n}}{{\mathit \gamma}}$  $0 - 0.15\%$ 574
$\Gamma_{14}$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity=1/2  $0 - 0.05\%$ 574
$\Gamma_{15}$ ${{\mathit n}}{{\mathit \gamma}}$ , helicity=3/2  $0 - 0.10\%$ 574