Table 4: Solar phosphorus abundances from the various observed spectra, adopting the (corrected) \ensuremath{\log\ensuremath{gf}} of Berzinsh et al. (1997).

Spectrum		 Wave EW A(P) from EW $\sigma$ 3D- \ensuremath{{\rm 1D}_{{\rm LHD}}} 3D- \ensuremath{\left\langle{\rm 3D}\right\rangle}
  [nm] [pm] [dex] [dex] [dex] [dex] [dex] [dex] [dex] [dex] [dex] [dex]
      3D ATLAS HM          
        1.0 1.5 1.0 1.5   1.0 1.5 1.0 1.5
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

KF		 1051.2 0.674 5.482 5.476 5.471 5.480 5.475 0.015 0.015 0.019 0.005 0.010
NF 1051.2 0.734 5.523 5.517 5.512 5.521 5.516 0.013 0.015 0.020 0.005 0.010
NI 1051.2 0.811 5.502 5.476 5.473 5.498 5.493 0.012 0.028 0.032 0.022 0.026
DI 1051.2 0.822 5.508 5.483 5.479 5.504 5.500 0.012 0.028 0.032 0.022 0.027

KF		 1053.0 1.330 5.431 5.421 5.412 5.427 5.417 0.010 0.019 0.028 0.005 0.015
NF 1053.0 1.340 5.435 5.424 5.416 5.431 5.421 0.010 0.019 0.028 0.005 0.015
NI 1053.0 1.520 5.425 5.392 5.382 5.417 5.408 0.010 0.036 0.044 0.025 0.034
DI 1053.0 1.550 5.436 5.402 5.392 5.427 5.418 0.010 0.036 0.044 0.025 0.034

KF		 1058.2 2.280 5.480 5.463 5.448 5.473 5.456 0.012 0.027 0.042 0.006 0.023
NF 1058.2 2.120 5.436 5.421 5.406 5.429 5.414 0.013 0.025 0.039 0.005 0.021
NI 1058.2 2.330 5.407 5.363 5.346 5.393 5.379 0.012 0.047 0.059 0.029 0.043
DI 1058.2 2.330 5.407 5.363 5.346 5.393 5.379 0.012 0.047 0.059 0.029 0.043

KF		 1059.7 0.684 5.482 5.475 5.471 5.480 5.475 0.014 0.015 0.019 0.005 0.010
NF 1059.7 0.660 5.464 5.458 5.454 5.462 5.458 0.014 0.015 0.019 0.005 0.010
NI 1059.7 0.748 5.456 5.431 5.427 5.452 5.448 0.012 0.027 0.030 0.022 0.026
DI 1059.7 0.751 5.458 5.433 5.429 5.454 5.450 0.012 0.027 0.031 0.022 0.026

KF		 1068.1 0.670 5.370 5.364 5.360 5.368 5.364 0.014 0.015 0.019 0.005 0.010
NF 1068.1 0.617 5.330 5.324 5.320 5.328 5.324 0.015 0.015 0.019 0.006 0.010
NI 1068.1 0.699 5.322 5.297 5.294 5.318 5.314 0.013 0.027 0.030 0.022 0.026
DI 1068.1 0.731 5.343 5.319 5.315 5.340 5.336 0.013 0.027 0.030 0.022 0.026
Column (1) spectrum identification: DI: Delbouille intensity, NI: Neckel intensity, NF: Neckel flux, KF: Kurucz flux. Column (2) wavelength of the line. Column (3) measured equivalent width. Column (4) phosphorus abundance, A(P), according to the ${{\rm CO}^5{\rm BOLD}}$ 3D model. Columns (5)-(8) provide A(P) from 1D models, odd numbered columns correspond to a micro-turbulence $\xi$ of 1.0 km s-1, even numbered columns to $\xi=1.5$ km s-1. Column (9) uncertainty in A(P) due to the uncertainty in the measured EWs. Column (10)-(13) provide 3D corrections, even numbered columns for $\xi=1.0$  ${\rm km~ s^{-1}}$, and odd numbered columns for 1.5  ${\rm km~ s^{-1}}$, respectively.

Source LaTeX | All tables | In the text